2024-03-28T23:20:16Z
http://cds.unistra.fr:443/reg-bin/vizier/oai.pl
ivo://CDS.VizieR/J/other/Obs/116.382
2019-06-21T18:30:00Z
J.other
ivo_managed
BVRI Photometry of Spectroscopic Binaries (Miller+ 1996)
Miller R., Osborn W.
BVRI photometry has been obtained for 82 of the spectroscopic binaries with orbits published in The Observatory by Griffin and his collaborators. The observations were obtained on nineteen nights during 1994-95. Given here are the star name, Griffin's paper number for the spectroscopic orbit, the abbreviated calendar date and heliocentric Julian Date (HJD) of the observation, the derived V, (B-V), (V-R)c, and (R-I)c values, and the phase in the spectroscopic orbit. The mean photometric values are listed in the final entry for each star. One night of poor quality, 950128, was given half weight in forming the means. The rms error of a single observation is about 0.025 mag. for all indices.
CDS
1997-12-09T21:49:59
ivo://CDS.VizieR/J/other/Obs/116.382
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/PBeiO/16.18
2019-06-21T18:30:00Z
J.other
ivo_managed
Physical data of the FK stars (Luo+ 1990)
Luo D., Zhang B.
The precise positions and proper motions (J2000.0) of 1535 Basic FK5 (FK4) stars in FK5 system (Cat. <I/149>) have been used in the reduction of local vertical monitoring and catalog observations at the Beijing Astronomical Observatory. The same data of 1987 FK4Sup stars, in which 980 stars denoted with "F" will be included in FK5, are also available recently from Heidelberg by courtesy of Prof Tong Fu, the Director of the Purple Mountain Observatory. The positions and proper motions of the other 1007 FK4Sup stars in FK5 system have been given by the Astronomisches Rechen-Institut in Heidelberg with comparatively low accuracy. However, the physical data, such as the visual magnitudes and the spectral types of these stars with rather larger uncertainties are originated from the Henry Draper Catalogue since the compilation of FK4 and FK4Sup (Cat. <I/143>). The more accurate visual magnitudes are available in the well-defined photoelectric system and the spectral types in MK-system that may be found, for example, in the Bright Star Catalogue (Cat. <V/50>) and a Supplement to this catalogue (Cat. <V/36>).
CDS
1997-12-09T21:50:37
ivo://CDS.VizieR/J/other/PBeiO/16.18
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/PNAOJ/2.561
2019-06-21T18:30:00Z
J.other
ivo_managed
Binaries speckle observations. IV. (Miura+ 1992)
Miura N., Baba N., Ni-Ino M., Ohtsubo J., Noguchi M., Isobe S.
This is the fourth paper of this series giving results of speckle observations for 22 visual and 161 spectroscopic binaries. The observation was carried out by using the 212 cm telescope of San Pedro Martir Observatory in Mexico at 7 nights from July 20 to July 26, 1991. We obtained fringes in power spectra of i 19 visual and 11 spectroscopic binaries (6 newly resolved ones) with angular separation larger than 0.06". We introduced a new ICCD TV camera in this observation, and were able to achieve the diffraction-limit resolution of the 212 cm telescope.
CDS
1997-12-09T21:51:32
ivo://CDS.VizieR/J/other/PNAOJ/2.561
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/SAAOC/14.11
2019-06-21T18:30:00Z
J.other
ivo_managed
UBVRI photometry of GSPC stars (Kilkenny+ 1990)
Kilkenny D., Laing J.D.
Photoelectric UBVRI observations are given for 336 stars brighter than 11.5mag from the Hubble Space Telescope Guide Star Photometric Catalogue (GSPC). Apart from a Declination-dependent effect in the V magnitudes there are no systematic differences between GSPC (Cat. <II/143>) and SAAO (Menzies et al., 1989SAAOC..13....1M) data which are significantly greater than differences between the Landolt and E-region standard systems. The Declination effect might be due to the occurrence of unusually high atmospheric extinction coefficients at CTIO following the eruption of the Mexican volcano, El Chichon.
CDS
1997-12-09T21:51:57
ivo://CDS.VizieR/J/other/SAAOC/14.11
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/PBeiO/18.7
2019-06-21T18:30:00Z
J.other
ivo_managed
Far infrared Seyfert galaxies (Liu 1991)
Liu Y.-L.
Confusing sources of Seyfert and HII galaxies in IRAS point source catalogue may be caused by companion objects of those galaxies. Comparison between confused galaxies and non-confused galaxies have been made. The preliminary comparison shows that confused galaxies are fainter than nonconfused galaxies generally, and colour diagrams illustrate that confused Seyferts are separated from nonconfused Seyferts obviously.
CDS
1998-02-24T17:27:15
ivo://CDS.VizieR/J/other/PBeiO/18.7
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/RMxAA/32.143
2019-06-21T18:30:00Z
J.other
ivo_managed
uvby photometry in Baade's Window (Ruelas-Mayorga+ 1996)
Ruelas-Mayorga A., Garcia-Ruiz G.
We have obtained uvby data of a sample of 232 stars in Baade's Window. These observations are presented along with the corresponding diagrams. For a description of the uvby photometric system, see e.g. <GCPD/04>
CDS
1998-03-02T20:22:40
ivo://CDS.VizieR/J/other/RMxAA/32.143
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/KFNT/12.20
2019-06-21T18:30:00Z
J.other
ivo_managed
Nearby stars metallicities (Zakhozhaj+ 1996)
Zakhozhaj V.A., Shaparenko E.F.
The catalogue for nearby stars' metallicities has been compiled. The catalogue contains 558 values obtained from photometric UBV data
CDS
1998-06-08T10:28:28
ivo://CDS.VizieR/J/other/KFNT/12.20
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/BSAO/38.152
2019-06-21T18:30:00Z
J.other
ivo_managed
Effective temperatures of CP stars (Glagolevskij 1994)
Glagolevskij Yu.V.
A new list is presented of effective temperatures estimated for about 700 chemically peculiar stars from the photometric parameters, calibrated with the temperatures determined by Shallis Blackwell (Blackwell et al., 1980A&A....82..249B) method from the total flux of the energy emitted by the stars.
CDS
1999-01-16T15:51:26
ivo://CDS.VizieR/J/other/BSAO/38.152
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/PBeiO/17.105
2019-06-21T18:30:00Z
J.other
ivo_managed
Third preliminary catalogue of stars (PPCP3; Lu 1990)
Lu L.-Z.
On the basis of the data observed with the Photoelectric Transit Instrument, of the Beijing Astronomical Observatory during the period from 1980 through 1984, the third preliminary catalogue of stars on right ascension observed with the Photoelectric Transit Instrument (PPCP3) have been compiled. The relations between the residuals V and the magnitude M, and the spectral type S of FK4 stars are discussed. There are 411 stars in this catalogue. The mean precisions of {DELTA}alpha's is +/-2.3ms. Finally systematic corrections of PPCP3-FK4 are given.
CDS
1999-02-25T08:14:02
ivo://CDS.VizieR/J/other/PBeiO/17.105
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/PBeiO/17.120
2019-06-21T18:30:00Z
J.other
ivo_managed
Fourth preliminary catalogue of stars (PPCP4; Wang+ 1991)
Wang R., Lu L.
On the photon counter data observed with Photoeleetric Transit Instrument of Beijing Astronomical Observatory during the period from 1988 to 1990, corrections of right ascensions of 324 stars are given. The mean precision (<m_{DELTA}{alpha}cos{delta}_>) is 4.7ms. The mean observational epoch is 1989.7. The relations of residuals with magnitudes and spectral types are discussed and given respectively. Finally the systematic corrections (PPCP4-FK4) are also analysed.
CDS
1999-02-25T08:14:53
ivo://CDS.VizieR/J/other/PBeiO/17.120
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/SAAOC/15.30
2019-06-21T18:30:00Z
J.other
ivo_managed
DDO photometry of E-region stars (Cousins 1993)
Cousins A.W.J.
This paper describes the observations and gives the results of a series of observations of bright E-region stars (Cousins A.W.J. and Stoy R.H., 1962RGOB...49....3C) for use as zero point stars for DDO photometry in the southern hemisphere. The list comprises 45 stars, all brighter than V=6.0, and gives the colours in the instrumental system with internal s.e. +/-0.001mag and m_48_ with s.e. +/-0.002mag. The observed m_48_ is indistinguishable from McClure's system and has the same zero point (+/-0.002mag). The individual E-region zero points have been established with s.e. +/-0.001 relative to the instrumental system, but the colour equations (and zero point corrections) to transform the instrumental colours to McClure's system have still to be finalised. For a description of the DDO photometric system, see e.g. <GCPD/12>
CDS
1999-02-25T08:18:02
ivo://CDS.VizieR/J/other/SAAOC/15.30
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/SAAOC/15.40
2019-06-21T18:30:00Z
J.other
ivo_managed
Southern reddened luminous stars. I. (Kilkenny+ 1993)
Kilkenny D., Whittet D.C.B.
Stroemgren uvby photometry has been obtained for 270 reddened and very reddened OB stars selected from the Stephenson & Sanduleak (1971) catalogue of Luminous Stars in the Southern Milky Way (LSS), Cat. <III/43>. Corrections have been applied to convert the data as closely as possible to the reddened O stars observed by Crawford (1975PASP...87..481C). Uncorrected and corrected data ar presented in Tables 1 and 3, respectively.
CDS
1999-02-25T08:18:46
ivo://CDS.VizieR/J/other/SAAOC/15.40
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/SAAOC/15.53
2019-06-21T18:30:00Z
J.other
ivo_managed
Southern reddened luminous stars. II. (Kilkenny 1993)
Kilkenny D.
H{beta} photometry is given for 263 reddened and very reddened stars from the Stephenson & Sanduleak (1971, Cat. <III/43>) catalogue of Luminous Stars in the Southern Milky Way (LSS). The results are combined with the uvby photometry presented in Paper I to determine reddenings, E(b-y), and distances for the stars and to estimate the spectral types and luminosity classes from derived T_eff_ and M_V_ values.
CDS
1999-02-25T08:19:24
ivo://CDS.VizieR/J/other/SAAOC/15.53
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/SAAOC/15.65
2019-06-21T18:30:00Z
J.other
ivo_managed
Southern reddened luminous stars. III. (Kilkenny+ 1993)
Kilkenny D., van Wyk F., Marang F., Spencer Jones J.H., Whittet D.C.B.
V(RI)C photometry has been obtained for 262 reddened and very reddened stars selected from the Stephenson & Sanduleak (1971, Cat. <III/43>) catalogue of Luminous Stars in the Southern Milky Way (LSS). This photometry, together with data from earlier papers in this series, is used to identify a number of probable variable stars.
CDS
1999-02-25T08:22:32
ivo://CDS.VizieR/J/other/SAAOC/15.65
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/SAAOC/15.73
2019-06-21T18:30:00Z
J.other
ivo_managed
Southern reddened luminous stars. IV. (Spencer Jones+ 1993)
Spencer Jones J.H., Whittet D.C.B., He L.
Infrared JHK measurements are presented for 232 reddened and very reddened stars selected from the Stephenson & Sanduleak (1971, Cat. <III/43>) catalogue of Luminous Stars in the Southern Milky Way (LSS).
CDS
1999-02-25T08:23:37
ivo://CDS.VizieR/J/other/SAAOC/15.73
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/SAAOC/15.78
2019-06-21T18:30:00Z
J.other
ivo_managed
UBV photometry of HD stars (Kilkenny+ 1993)
Kilkenny D., Barrett P.E., Marang F., van Wyk F., Roberts G., Winkler H.
Photoelectric UBV photometry is presented for over 400 HD stars which lie within about a degree of selected cataclysmic variables. The data will be combined with polarimetry to determine the distances of the CVs.
CDS
1999-02-25T08:24:10
ivo://CDS.VizieR/J/other/SAAOC/15.78
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/PASAu/10.310
2019-06-21T18:30:00Z
J.other
ivo_managed
Parkes-Tidbinbilla radio sources (Duncan+ 1993)
Duncan R.A., White G.L., Wark R., Reynolds J.E., Jauncey D.L., Norris R.P., Taaffe L., Savage A.
We have measured the 2.3GHz total and correlated flux densities on a baseline of 275km of all sources in the Parkes catalogue which : (i) are south of declination +10deg, (ii) have a catalogued 2.7GHz total flux density exceeding 0.5Jy, and (iii) have a 2.7/5.0GHz spectral index flatter than -0.5. More than 14% of the sample showed visibility amplitudes greater than 0.9, and more than 72% showed visibility amplitudes greater than 0.5. Of the sources with optical or other identifications 79% were quasars. In this paper we briefly summarise the results of this survey.
CDS
1999-02-25T08:57:32
ivo://CDS.VizieR/J/other/PASAu/10.310
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/PBeiO/24.71
2019-06-21T18:30:00Z
J.other
ivo_managed
CPASJ1 position corrections (Lu+, 1994)
Lu L., Manrique W.T., Perdomo R.
Using the data observed with the Photoelectric Astrolabe Mark II (PA II) of the Beijing Astronomical Observatory during the period from Feb. 1992 to Oct. 1993 in San Juan of Argentina, the first catalogue of stars (PASJ1, Cat. <J/A+AS/118/1>) have been compiled. It consists of 1400 stars included 682 FK5/FK4 Supp stars. 433 FK5 Ext stars and 285 CAMC stars (1, 1989). The mean precisions of delta alpha's and delta delta's are +/-3.2ms and 0.055", respectively. The mean epoch is 1992.9. Finally, systematic corrections of (PASJ1-FK5) are given.
CDS
1999-12-23T10:50:33
ivo://CDS.VizieR/J/other/PBeiO/24.71
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/PASAu/10.140
2019-06-21T18:30:00Z
J.other
ivo_managed
Southern radio sources catalog (White, 1992)
White G.L.
A list of 900 radio sources with positional accuracies better than 0.5" has been prepared from seventeen lists of radio source positions found in the literature. This compilation includes all such sources south of declination +48{deg} (the northern declination limit of the Compact Array of the Australia Telescope National Facility). Where available, optical identifications, optical magnitudes and redshifts are given as well as total-power flux densities.
CDS
2000-03-11T12:57:42
ivo://CDS.VizieR/J/other/PASAu/10.140
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/KFNT/15.483
2019-06-21T18:30:00Z
J.other
ivo_managed
Positions of Thebe and Amalthea (Ledovskaya+ 1999)
Ledovskaya I.V., Jockers K., Karpov N.V., Sergeev A.V.
The file jovsat.dat contains 35 intersatellite positions of inner Jovian moons Thebe and Amalthea, derived from the observations made with the 2-m Zeiss RCC telescope of Terskol Observatory (Terskol peak, Northern Caucasus, long=42.50083{deg}, lat= 43.27427{deg}, h=3100m) in 1998. The Two-Channel Focal Reducer of the Max-Planck Institute for Aeronomy (MPAe,Germany) was used for acquisition of the images. We provide delta(alpha) and delta(delta) of Thebe and Amalthea with respect to the Galilean satellites, that were used as the reference points forming the reference direction on the frames. Astrometric topocentric coordinates J2000.0 of the Galilean satellites were used for scale and orientation angle determination. The array scale was corrected for differential refraction and differential aberration to first-order. All observed positions are compared with the theoretical ones.
CDS
2001-12-29T13:32:44
ivo://CDS.VizieR/J/other/KFNT/15.483
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/PNAOJ/6.1
2019-06-21T18:30:00Z
J.other
ivo_managed
KUG survey, second series. II (Miyauchi-Isobe+ 2000)
Miyauchi-Isobe N., Maehara H.
The catalogue list of ultraviolet(UV)-excess galaxies (KUG) which have been detected on two-color Kiso Schmidt plates is presented for the 10 Schmidt fields. Catalogued are 644 objects, down to the photographic magnitude 17 in the sky area of some 300 square degrees.
CDS
2002-05-10T09:23:04
ivo://CDS.VizieR/J/other/PNAOJ/6.1
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/RMxAA/38.129
2019-06-21T18:30:00Z
J.other
ivo_managed
Stellar Spectral Classification. II. (Stock+, 2002)
Stock J., Stock M., Garcia J., Sanchez N.
The following tables contains the 10 best linear and quadratic solutions to calculate the absolute magnitudes and the intrinsic colors, using two or three equivalent widths of some absorption lines. Also, their average residual, the number of used and eliminated stars for each combination are given, as well as the coefficients obtained for the respective terms.
CDS
2003-01-06T20:09:55
ivo://CDS.VizieR/J/other/RMxAA/38.129
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/PASA/19.455
2019-06-21T18:30:00Z
J.other
ivo_managed
Damped Lyman alpha absorption of QSOs (Curran+, 2002)
Curran S.J., Webb J.K., Murphy M.T., Bandiera R., Corbelli E., Flambaum V.V.
We present a catalogue of the 322 damped Lyman alpha absorbers taken from the literature. All damped Lyman alpha absorbers are included, with no selection on redshift or quasar magnitude. Of these, 123 are candidates and await confirmation using high resolution spectroscopy. For all 322 objects we catalogue the radio properties of the background quasars, when known. Around 60 quasars have radio flux densities above 0.1Jy and approximately half of these have optical magnitudes brighter than V=18. This compilation should prove useful in several areas of extragalactic/cosmological research.
CDS
2003-02-13T23:26:21
ivo://CDS.VizieR/J/other/PASA/19.455
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/Ap/45.322
2019-06-21T18:30:00Z
J.other
ivo_managed
FBS 13th list of late M and carbon stars (Gigoyan+, 2002)
Gigoyan K.S., Abrahamyan H.V., Azzopardi M., Russeil D.
The thirteenth list of faint late M and carbon type stars detected on the plates of the First Byurakan Spectral Sky Survey in zone +1{deg}<={delta}<=+13{deg} covering about 3118 sq. degrees is presented. From 285 stars, 161 are newly detected objects: they are 17 carbon stars, 25 carbon star candidates, and 117 M-type stars. The spectral type of two objects is assumed to be between M8 - M9 or late N-subtypes. Among 161 objects, 85 (66 PSC + 19 FSC) are unclassified IRAS sources. Accurate positions, spectral classes, red magnitudes, and color indices are given using several astronomical databases. Finding charts from DSS are given for the most interesting objects.
CDS
2003-03-21T22:41:54
ivo://CDS.VizieR/J/other/Ap/45.322
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/RMxAA/39.39
2019-06-21T18:30:00Z
J.other
ivo_managed
CCD Photometry of NGC 2658, 2849, 3247 (Ahumada, 2003)
Ahumada J.A.
CCD photometry of the galactic open clusters NGC 2658, NGC 2849, and NGC 3247 is presented. For the first two clusters, BV(RI)_c data are given, and for NGC 3247 the data are BV(I)_c. The observations were carried out from the Complejo Astronomico El Leoncito (Argentina), and from Las Campanas (Chile). Each cluster was observed on two different nights; when possible, measurements for a given star were averaged. NGC 2658 observations were carried out from CASLEO on the nights of 8-9 January 1997 and 18-19 April 2001, in the BVRI filters. NGC 2849 data in the BVRI filters were obtained at Las Campanas on the night 10-11 April 1996, and at CASLEO on 19-20 April 2001. NGC 3247 was observed at CASLEO on the nights 16-17 January 1996 (BV) and 1-2 April 1998 (BVI). The given star coordinates are relative to the corresponding cluster center.
CDS
2003-05-04T21:29:13
ivo://CDS.VizieR/J/other/RMxAA/39.39
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/BASI/30.911
2019-06-21T18:30:00Z
J.other
ivo_managed
BVRI CCD photometry of 4 galaxy clusters (Sharma+, 2002)
Sharma M., Prabhu T.P.
We acquired optical imaging observations at the prime focus of the 2.34-m Vainu Bappu Telescope (VBT), at the Vainu Bappu Observatory (VBO), Kavalur, India. The observatory (longitude 78.8{deg}E, latitude 12.5{deg}N, altitude 730m above sea level) is operated by the Indian Institute of Astrophysics, Bangalore. We employed the following filters in our observations: broad-band blue, visual, red and near infra-red (approximating the standard B, V, R and I photometric bands). We chose to transform our instrumental magnitudes to the standard Johnson-Morgan BV and Kron-Cousins R_c_I_c_ broadband systems using the old Galactic cluster M67 for which many studies are available.
CDS
2003-08-10T11:23:14
ivo://CDS.VizieR/J/other/BASI/30.911
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/Sci/292.2290
2019-06-21T18:30:00Z
J.other
ivo_managed
Chandra compact binaries in 47 Tuc (Grindlay+, 2001)
Grindlay J.E., Heinke C., Edmonds P.D., Murray S.S.
We have obtained high-resolution (<~1") deep X-ray images of the globular cluster 47 Tucanae (NGC 104) with the Chandra X-ray Observatory to study the population of compact binaries in the high stellar density core. A 70-kilosecond exposure of the cluster reveals a centrally concentrated population of faint (L_X_~10^30-33^ergs/s) X-ray sources, with at least 108 located within the central 2'x2.5' and >~half with L_X_<~10^30.5^ergs/s. All 15 millisecond pulsars (MSPs) recently located precisely by radio observations are identified, though 2 are unresolved by Chandra. The X-ray spectral and temporal characteristics, as well as initial optical identifications with the Hubble Space Telescope, suggest that >~50 percent are MSPs, about 30 percent are accreting white dwarfs, about 15 percent are main-sequence binaries in flare outbursts, and only two to three are quiescent low-mass X-ray binaries containing neutron stars, the conventional progenitors of MSPs. An upper limit of about 470 times the mass of the sun is derived for the mass of an accreting central black hole in the cluster. These observations provide the first X-ray ``color-magnitude'' diagram for a globular cluster and census of its compact object and binary population. Observations were made on UT 16.31 - 17.22 March, 2000.
CDS
2003-11-11T20:38:15
ivo://CDS.VizieR/J/other/Sci/292.2290
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/NewA/5.137
2019-06-21T18:30:00Z
J.other
ivo_managed
Supersoft X-ray sources catalog (Greiner+, 2000)
Greiner J.
This catalog comprises an up-to-date (December 1999) list of luminous (>10^36^erg/s), binary supersoft X-ray sources.
CDS
2004-05-16T14:42:20
ivo://CDS.VizieR/J/other/NewA/5.137
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/IBVS/5493
2019-06-21T18:30:00Z
J.other
ivo_managed
2003 CCD minima of eclipsing binaries (Nelson+, 2004)
Nelson R.H.
- Observatory and telescope: Sylvester Robotic Observatory (SRO): 33cm f/4.5 Newtonian on Paramount GT-1100s mount - Detector: SRO: SBIG ST7e, 1.24 pixels, 15.8x10.5 FOV, cooled -10<T<-30{deg}C - Method of data reduction: Aperture photometry using MIRA, by Axiom Research - Method of minimum determination: Digital tracing paper method, bisection of chords, curve fitting, and (occasionally) Kwee and van Woerden (1956BAN....12..327K)
CDS
2006-05-22T19:00:25
ivo://CDS.VizieR/J/other/IBVS/5493
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/BASI/32.295
2019-06-21T18:30:00Z
J.other
ivo_managed
CCD UBVRI photometry of 3 open clusters (Sujatha+, 2004)
Sujatha S., Babu G.S.D., Ananthamurthy S.
The clusters were observed on 13 and 14 December 2001, with the 1.02m telescope at the Vainu-Bappu Observatory of Indian Institute of Astrophysics at Kavalur. Standard UBVRI filters along with 1k CCD were used at the Cassegrain focus of the telescope, the image scale being 0.315arcsec/pixel. The well-known open cluster M67 (NGC 2682) was also observed on each of the above-mentioned dates for the calibration of the instrument.
CDS
2006-05-23T12:45:55
ivo://CDS.VizieR/J/other/BASI/32.295
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/IBVS/5526
2019-06-21T18:30:00Z
J.other
ivo_managed
BVRI photometry of stars in BZ UMa field (Price+, 2004)
Price A., Vanmunster T., Starkey D., Boyd D., Zissell R., Gary B., Graham K., Macdonald II W., Aquino B., West D., Blackwell J., Walker G., Simonsen M., Henden A., Templeton M.R., Mattei J.A.
The AAVSO has received 4270 CCD measurements of BZ UMa over four nights during its March, 2004 outburst. Analysis of the measurements reveals rapid flickering and quasiperiodic behaviour but no coherent periodicity (beyond the orbital period) and the notable absence of superhumps
CDS
2006-05-30T22:01:52
ivo://CDS.VizieR/J/other/IBVS/5526
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/Ap/46.46
2019-06-21T18:30:00Z
J.other
ivo_managed
FBS. Blue stellar objects. XII (Abrahamyan+, 2003)
Abrahamyan G.V., Sinamyan P.K., Gigoyan K.S.
The twelfth list of blue stellar objects in the second part of the First Byurakan Spectral Sky Survey (FBS) is presented. This list contains 143 objects in the region -3{deg}<DE<+1{deg} at high latitudes with an area of approximately 992 square degrees (62 fields). The objects have magnitudes V of 11.8-18.1 and B-V colors ranging from -0.82 to +0.81. Of the 143 objects, 51 have been discovered for the first time. Equatorial coordinates, V magnitudes, color indices, and preliminary classifications of the objects are given. DSS identification charts are given for the newly discovered objects.
CDS
2006-08-08T13:05:21
ivo://CDS.VizieR/J/other/Ap/46.46
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/JApA/25.143
2019-06-21T18:30:00Z
J.other
ivo_managed
High galactic latitude HI absorption survey (Mohan+, 2004)
Mohan R., Dwarakanath K.S., Srinivasan G.
We have used the Giant Meterwave Radio Telescope (GMRT) to measure the Galactic HI 21-cm line absorption towards 102 extragalactic radio continuum sources, located at high (|b|>15{deg}) Galactic latitudes. The Declination coverage of the present survey is DE~-45{deg}. With a mean rms optical depth of ~0.003, this is the most sensitive Galactic HI 21-cm line absorption survey to date. To supplement the absorption data, we have extracted the HI 21-cm line emission profiles towards these 102 lines of sight from the Leiden Dwingeloo Survey of Galactic neutral hydrogen. We have carried out a Gaussian fitting analysis to identify the discrete absorption and emission components in these profiles. In this paper, we present the spectra and the components. A subsequent paper will discuss the interpretation of these results.
CDS
2006-09-10T12:52:08
ivo://CDS.VizieR/J/other/JApA/25.143
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/NewA/10.325
2019-06-21T18:30:00Z
J.other
ivo_managed
2MASS observations of Be stars (Zhang+, 2005)
Zhang P., Chen P.S., Yang H.T.
A catalogue of almost all known Galactic Be stars in the 2MASS (<II/246>) database (1185 in total) and in the MSX (<V/114>) database (225 in total) is presented in this paper. From the color-color diagrams and spectral indexes, it is found that the IR excesses for many samples are due to free-free and free-bound emission from the ionized material around a Be star as suggested previously and that the mean spectral index derived for the samples is 1.50+/-0.34 between J to K bands and 1.14+/-0.42 between K to A bands, respectively. However, it is also found that there are eight Be stars that have large near infrared excess emission with spectral index values outside the range expected for freefree and freebound emission. This is likely attributed to circumstellar dust emission.
CDS
2006-09-10T13:11:04
ivo://CDS.VizieR/J/other/NewA/10.325
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/P+SS/53.925
2019-06-21T18:30:00Z
J.other
ivo_managed
CCD photometry of 23 minor planets (Szekely+, 2005)
Szekely P., Kiss L.L., Szabo Gy.M., Sarneczky K., Csak B., Varadi M., Meszaros Sz.
We carried out CCD observations on 39 nights from September, 1999 to February, 2003. Standard Johnson R filtered and unfiltered data were obtained, using the 60/90/180cm Schmidt-telescope of the Konkoly Observatory.
CDS
2006-11-28T13:51:00
ivo://CDS.VizieR/J/other/P+SS/53.925
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/Ap/48.344
2019-06-21T18:30:00Z
J.other
ivo_managed
New galaxies with UV excess. VI. (Kazarian+, 2005)
Kazarian M.A., Petrosian G.V.
A list is presented of 122 new galaxies with UV excess observed on plates obtained using the 40 Schmidt telescope at the Byurakan Observatory with a 1.5{deg} objective prism. It is shown that the relative number of galaxies with a strong UV excess (classes 1 and 2) listed in Table 1 is roughly 55.7%. This is 6.7% higher than for the previously observed galaxies. These samples also differ in terms of the morphology of the spectra. The largest deviation, approximately 9.9%, occurs for type sd.
CDS
2006-12-08T08:52:10
ivo://CDS.VizieR/J/other/Ap/48.344
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/NewA/11.262
2019-06-21T18:30:00Z
J.other
ivo_managed
BVIc photometry in Lynga 11 (Piatti+, 2006)
Piatti A.E., Claria J.J., Ahumada A.V.
CCD images of the cluster field were obtained with the Johnson B and V and Kron-Cousins I filters during the same night in which they were obtained for NGC 6318, whose analysis was published by Piatti et al. (2005, Cat. <J/PASP/117/22>, hereafter Paper I).
CDS
2006-12-23T16:35:42
ivo://CDS.VizieR/J/other/NewA/11.262
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/BASI/29.519
2019-06-21T18:30:00Z
J.other
ivo_managed
VI CCD photometry in NGC 6631 (Sagar+, 2001)
Sagar R., Naidu B.N., Mohan V.
The VI CCD photometric observations were obtained during May 8 to 10, 2001.
CDS
2007-06-17T11:35:35
ivo://CDS.VizieR/J/other/BASI/29.519
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/GCN/1070.1
2019-06-21T18:30:00Z
J.other
ivo_managed
HETE Trigger Information (Ricker+, 2001)
Ricker G., Lamb D., Woosley S., et al.
At 15:54:53.123 UT on 23 June, the HETE FREGATE and WXM instruments detected and localized an intense burst from SGR1806-20, a soft gamma-ray repeater. This event, disseminated in near real time as a GCN Alert (HETE BID_1566; see http://gcn.gsfc.nasa.gov/gcn/hete_grbs.html ), is the second burst localized from this source in the past week. (The first burst was reported in GCN Circular #1068). The coordinates (J2000) of the 23 June burst are: RA=272.1460{deg} (18:08:35.02), DE=-20.3658{deg} (-20:21:56) The error circle for this localization is 6 arcmin in radius. SGR1806-20 lies 3.1arcmin from the HETE position. The burst duration in the 8-40keV band was ~200ms, comprised of two peaks each <100ms in duration. A total of 2250 counts were detected during that interval, corresponding to a fluence of ~4x10^-7^ergs/cm^2^. The peak flux was >6x10^-6^erg/cm^2^/s (i.e. >200Crab-flux). Follow-up observations of this transient are encouraged. Additional information on this burst detection (including light curves), as well as for the HETE mission, will be available at: http://space.mit.edu/HETE/
CDS
2007-06-17T11:36:02
ivo://CDS.VizieR/J/other/GCN/1070.1
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/IBVS/5633
2019-06-21T18:30:00Z
J.other
ivo_managed
Miras in Scorpius (Roslund+, 2005)
Roslund C., Larsson A., Schalander P., Radbo M.
In the recent IBVS 5633, Roslund et al. give a list of new red variable stars. The work evidently was done in the early 1970s, but no effort was made to match the star-list with recent data available from modern on-line resources in this late publication. Johnson R magnitudes at maximum are shown for all stars and spectral classifications for about half. The authors warn that the magnitudes could have a systematic error, such that they are perhaps a magnitude too bright overall. Similarly, the coordinates, given to arcsecond precision, are noted as being poorly determined with "a simple, unpretentious plate-measuring machine of unproven accuracy." I confirm here both of these problems. I have gone through the list to recover the stars in modern catalogues. I matched the source-list in the Strasbourg VizieR utility against UCAC2 and 2MASS, searching a 20" radius and _assuming_ the brightest red star in the region is the variable (typical J-K>>1.0). There are no identification charts published, so misidentifications are possible. However, the candidates are all very similar in near-IR brightness (commonly 7<J<10), so it seemed the choices were limited. The original positions are indeed semi-accurate, being typically 5"-15" in error. I show improved coordinates in the table below. Nearly all thepositions come from 2MASS, but a few appear in UCAC2. That so few stars are present in UCAC2 is a first suggestion that the Roslund et al red magnitudes are much too bright compared to the standard system (either Johnson or Cousins R). I matched the corrected positions again in VizieR with GSC-2.2, USNO-B1.0, and the DENIS catalogue to obtain at least a "representative" V (or 'mv') magnitude, sometimes inferred from adjacent colors. Most of these come from the short-V plate data provided in GSC-2.2, where my experience with the same sorts of stars suggests the zero-point and scale are under good control. It was also easy to compare at the same time the Roslund R(max) magnitudes with the photo-red and I-band data listed in the three surveys just mentioned. This indicates the Roslund 'R' is at least one and more likely _two_ full magnitudes too bright even accounting for the large amplitudes of the variables---the zero-point is nearly that of the USNO-B1.0 or DENIS I-band magnitudes, rather than R. Finally, I matched the stars with the MSX6C and IRAS catalogues and also GCVS v4.2. Most stars have an MSX link, but probably the bright IR background close to the galactic center precluded many IRAS detections. I also searched each position in SIMBAD (3' search radius): the stars with Terzan links are shown, but the rest of the stars are not present in the database. Please note the following: where no reasonably bright red star appeared near the Roslund position on 2MASS J-band images, I used the identifications with the Terzan survey of the same region to obtain improved positions. This allowed all but one star to be recovered unambiguously.
CDS
2007-09-12T20:01:14
ivo://CDS.VizieR/J/other/IBVS/5633
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/ChJAA/6.435
2019-06-21T18:30:00Z
J.other
ivo_managed
Proper motions in NGC 6530 (Zhao+, 2006)
Zhao J.-L., Chen L., Wen W.
The six photographic plates used for proper motion reduction of the open cluster NGC 6530 were all taken by the 40cm double astrograph with focal length of 6.9m at Sheshan (Zo Se) Station of Shanghai Astronomical Observatory, Chinese Academy of Sciences, with two first epoch plates and four second epoch ones taken in 1912 and 1999 respectively, with a time baseline extending over 87 years.
CDS
2007-09-19T15:32:14
ivo://CDS.VizieR/J/other/ChJAA/6.435
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/Ap/46.475
2019-06-21T18:30:00Z
J.other
ivo_managed
FBS 14th list of late M and carbon stars (Gigoyan+, 2003)
Gigoyan K.S., Abrahamyan H.V., Azzopardi M., Mauron N., Russeil D., Sinamyan P.
We present the fourteenth list of faint late M and carbon type stars detected on the plates of the First Byurakan Spectral Sky Survey in the zone +13{deg}<=DE<=+33{deg} covering about 4736deg^2^. From 260 stars, 118 are newly detected objects: they are 19 carbon stars, 5 carbon star candidates, and 94 M-type stars. Among 118 detected objects 73 (57 PSC + 16 FSC) are unclassified IRAS sources. Accurate positions, spectral classes, red magnitudes, color indices, and near-infrared J, H and K photometry are given, using several astronomical databases. Finding charts from DSS are given for the most interesting objects.
CDS
2007-10-01T13:54:33
ivo://CDS.VizieR/J/other/Ap/46.475
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/APh/26.367
2019-06-21T18:30:00Z
J.other
ivo_managed
GRB from RICE data (Besson+, 2007)
Besson D., Razzaque S., Adams J., Harris P.
We present limits on ultra-high energy (UHE; E_{nu}_>10^15^eV) neutrino fluxes from gamma-ray bursts (GRBs), based on recently presented data, limits, and simulations from the RICE experiment. We use data from five recorded transients with sufficient photon spectral shape and redshift information to derive an expected neutrino flux, assuming that the observed photons are linked to neutrino production through pion decay via the well-known Waxman-Bahcall prescription. Knowing the declination of the observed burst, as well as the RICE sensitivity as a function of polar angle and the previously published non-observation of any neutrino events allows an estimate of the sensitivity to a given neutrino flux. Although several orders of magnitude weaker than the expected fluxes, our GRB neutrino flux limits are nevertheless the first in the PeVEeV energy regime. For completeness, we also provide a listing of other bursts, recorded at times when the RICE experiment was active, but requiring some assumptions regarding luminosity and redshift to permit estimates of the neutrino flux.
CDS
2007-10-25T10:25:04
ivo://CDS.VizieR/J/other/APh/26.367
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/NewA/12.461
2019-06-21T18:30:00Z
J.other
ivo_managed
CCD UBVIc photometry of Ruprecht 58 (Giorgi+, 2007)
Giorgi E., Vazquez R.A., Solivella G.R., Orellana R.B., Nunez J.
CCD observations in the UBVI system were carried out in the field of Ruprecht 58 on the nights of December 24 and 25, 2003, at the Complejo Astronomico El Leoncito, CASLEO, Argentina.
CDS
2007-12-05T15:03:55
ivo://CDS.VizieR/J/other/NewA/12.461
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/KFNT/22.231
2019-06-21T18:30:00Z
J.other
ivo_managed
UBVR photometry in NGC 6913 (Andruk+, 2006)
Andruk V.N., Butenko G.Z.
The CCD observations of a sky area in the NGC 6913 cluster were performed with the 2-meter telescope of the Terskol Peak Observatory (Northern Caucasus, Russian Federation). The magnitudes and coordinates of stars down to V=20mag were determined for a 7'x5' field. The equatorial coordinates of stars were obtained in the reference system of the USNO A2.0 catalog (Cat. <I/252>) with an accuracy of 0.35". The relationship between the instrumental photometric system and the Johnson UBVR system was derived.
CDS
2008-12-20T08:42:03
ivo://CDS.VizieR/J/other/KFNT/22.231
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/JAVSO/34.222
2019-06-21T18:30:00Z
J.other
ivo_managed
New Northern Hemisphere Variables (Davies+, 2006)
Davies D.
A survey looking for previously unknown variable stars has been carried out in the declination range 30-39 degrees and in the R.A. range 0-24 hours. The survey was done in I-band, and was carried out from October 2003 to December of 2004. Seventy-five new and previously suspected variable stars were detected. This paper presents a brief description of the survey and identifies the new variables.
CDS
2009-03-09T13:01:58
ivo://CDS.VizieR/J/other/JAVSO/34.222
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/Ap/50.426
2019-06-21T18:30:00Z
J.other
ivo_managed
HII regions in NGC 6384 (Hakobyan+, 2007)
Hakobyan A.A., Petrosian A.R., Yeghazaryan A.A., Boulesteix J.
The observations have been made with the CIGAL equipment which mainly consists of a mainly focal reducer with IPCS and scanning Fabry-Perot interferometer attached to the F/3.8 prime focus of the 2.6-m telescope of Byurakan Observatory (Armenia) on September 7, 1985.
CDS
2009-04-26T16:01:15
ivo://CDS.VizieR/J/other/Ap/50.426
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/AstBu/64.123
2019-06-21T18:30:00Z
J.other
ivo_managed
Catalog of radio galaxies with z>0.3 (Khabibullina+, 2009)
Khabibullina M.L., Verkhodanov O.V.
This catalog groups the 2442 galaxies making up the sample of distant galaxies prepared by the authors published as 3 papers in 2009: radio data (paper I, table1), photometric data (paper II, table2), and angular sizes (paper III, table 3). The sample of distant (z>0.3) radio galaxies is aimed at application in cosmological tests. It was created using NED, SDSS, and CATS databases, and is assumed to be cleaned from objects with quasar properties.
CDS
2009-10-12T10:07:21
ivo://CDS.VizieR/J/other/AstBu/64.123
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/AstBu/64.276
2019-06-21T18:30:00Z
J.other
ivo_managed
Catalog of radio galaxies with z>0.3 (Khabibullina+, 2009)
Khabibullina M.L., Verkhodanov O.V.
This catalog groups the 2442 galaxies making up the sample of distant galaxies prepared by the authors published as 3 papers in 2009: radio data (paper I, table1), photometric data (paper II, table2), and angular sizes (paper III, table 3). The sample of distant (z>0.3) radio galaxies is aimed at application in cosmological tests. It was created using NED, SDSS, and CATS databases, and is assumed to be cleaned from objects with quasar properties.
CDS
2009-10-28T14:34:07
ivo://CDS.VizieR/J/other/AstBu/64.276
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/JAVSO/37.169
2019-06-21T18:30:00Z
J.other
ivo_managed
Red variable stars in NSVS (Nicholson, 2009)
Nicholson M.
Astrometric and photometric data are presented for 1233 previously unreported variable stars extracted from the Northern Sky Variability Survey. Cross referenced identifiers to Two Micron All Sky Survey (2MASS), Guide Star Catalog (GSC) and Tycho numbers are also included.
CDS
2010-02-07T11:12:22
ivo://CDS.VizieR/J/other/JAVSO/37.169
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/Nat/463.513
2019-06-21T18:30:00Z
J.other
ivo_managed
Radio observations of SN 2009bb (Soderberg+, 2010)
Soderberg A.M., Chakraborti S., Pignata G., et al.
Long duration gamma-ray bursts (GRBs) mark the explosive death of some massive stars and are a rare sub-class of type Ibc supernovae. They are distinguished by the production of an energetic and collimated relativistic outflow powered by a central engine (an accreting black hole or neutron star). Observationally, this outflow is manifested in the pulse of gamma-rays and a long-lived radio afterglow. Until now, central-engine-driven supernovae have been discovered exclusively through their gamma-ray emission, yet it is expected that a larger population goes undetected because of limited satellite sensitivity or beaming of the collimated emission away from our line of sight. In this framework, the recovery of undetected GRBs may be possible through radio searches for type Ibc supernovae with relativistic outflows. Here we report the discovery of luminous radio emission from the seemingly ordinary type Ibc SN 2009bb, which requires a substantial relativistic outflow powered by a central engine. A comparison with our radio survey of type Ibc supernovae reveals that the fraction harbouring central engines is low, about one per cent, measured independently from, but consistent with, the inferred rate of nearby GRBs. Independently, a second mildly relativistic supernova has been reported.
CDS
2010-05-16T03:25:24
ivo://CDS.VizieR/J/other/Nat/463.513
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/AstBu/65.42
2019-06-21T18:30:00Z
J.other
ivo_managed
RCR (RATAN COLD REFINED) catalogue (Soboleva+, 2010)
Soboleva N.S., Majorova E.K., Zhelenkova O.P., Temirova A.V., Bursov N.N.
From 1980 till 1999 7 surveys of 40' width sky strip, centred on SS433 declination have been carried out on the radio telescope RATAN-600. Observations were spent on 7.6cm wavelength in the range of right ascensions 4h<RA<22h and on 31cm in an interval 4h<RA<13h. On a basis of the given observations 1980-1981 on 7.6cm wavelength (experiment "Cold") has been obtained the RC catalogue of radio sources. Re-processing of the surveys data in the range of 7h<RA<17h is conducted for improvement of coordinates and flux densities of the RC catalogue sources The results of data processing by two methods described in the paper are included in the RCR catalogue. The NVSS catalogue was used as reference one. The RCR table includes NVSS coordinates of sources, differences between NVSS right ascension and right ascension obtained by the first and second method of scan data processing, and also errors, flux density on 7.6cm or 3.9GHz (also defined by two methods) and errors. We fitted available flux density data by curves and obtained 3.94GHz and 0.5GHz spectral indexes for the whole source list. At construction of spectra in addition to the available data of known catalogues we used estimated values of flux density obtained on the VLSS and GB6 images. Estimated values of 4.85GHz flux density have allowed to confirm reliability of weak objects allocation on the scans. In total in a strip of right ascensions 7h<RA<17h was evolved 550 objects, from them are 18 blinds and 15 double sources. All of them are identified with objects of the NVSS catalogue.
CDS
2010-06-02T11:19:01
ivo://CDS.VizieR/J/other/AstBu/65.42
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/AstBu/65.150
2019-06-21T18:30:00Z
J.other
ivo_managed
Spectral line identification in 3 Pup (Chentsov+, 2010)
Chentsov E.L., Klochkova V.G., Miroshnichenko A.S.
Catalogue of residual intensities r and radial velocities RV presented is based on spectral observations of the peculiar supergiant 3 Pup made with the echelle spectrograph NES of the 6m telescope of Special Astrophysical Observatory of Russian Academy of Sciences. Original results of spectroscopy of 3Pup published by Chentsov, Klochkova and Miroshnichenko in Astrophysical Bulletin, 65, No.1, 2010. The Catalogue is presented as a table. The columns of the table contain the r and RV for individual lines in the high-resolution spectra of 3 Pup, for 5 observing dates. The work is supported by the Russian Fondation for Basic Research (project 08-02-00072).
CDS
2010-08-07T14:03:25
ivo://CDS.VizieR/J/other/AstBu/65.150
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/PZP/9.5
2019-06-21T18:30:00Z
J.other
ivo_managed
I light curves of RR Lyrae from OGLE II (Bernhard+, 2009)
Bernhard K., Wils P.
We present the discovery of ten RR Lyrae variables. They were found in a search for new variables in the OGLE II Photometric Database (Szymanski 2005AcA....55...43S, Udalski et al. 1997AcA....47..319U). Suitable parameters (e.g. Isig>0.1, e_Imed<Isig) were used in the OGLE Photometry Database Query Page (http://ogledb.astrouw.edu.pl/~ogle/photdb/) for stars in the Galactic Disk. Period analysis was made with the software AVE (GEA).
CDS
2010-11-02T14:49:00
ivo://CDS.VizieR/J/other/PZP/9.5
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/PASA/24.118
2019-06-21T18:30:00Z
J.other
ivo_managed
Wide southern double stars (Bauer+, 2007)
Bauer C., White G.L., Blank D., Jones P.A.
Observations were made during three periods, 6-10 October 1992, 4-25 November 1992 and 8-12 December 1993, with the last session being primarily concerned with calibration. The mean epoch of the observations is 1992.9. We used an SBIG ST6 CCD camera mounted on the f/18 focus of the 24 inch (0.6m) telescope of Mount Stromlo and Siding Spring Observatory (MSSSO) at Siding Spring Observatory (SSO), Australia. Images were obtained of each star through uncalibrated Cousins R and I filters. The stars were sufficiently bright that exposure times could be kept short, typically 180s or less.
CDS
2010-11-07T13:08:22
ivo://CDS.VizieR/J/other/PASA/24.118
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/Ser/179.87
2019-06-21T18:30:00Z
J.other
ivo_managed
H{alpha} in HII regions of Holmberg IX (Arbutina+, 2009)
Arbutina B., Ilic D., Stavrev K., Urosevic D., Vukotic B., Onic D.
We present observations of the nearby tidal dwarf galaxy Holmberg IX in M81 galaxy group in narrow band [SII] and H{alpha} filters, carried out in March and November 2008 with the 2m RCC telescope at NAO Rozhen, Bulgaria. Our search for resident supernova remnants (identified as sources with enhanced [SII] emission relative to their H{alpha} emission) in this galaxy yielded no sources of this kind, besides M&H 10-11 or HoIX X-1. Nevertheless, we found a number of objects with significant H{alpha} emission that probably represent uncatalogued HII regions.
CDS
2011-04-26T15:56:59
ivo://CDS.VizieR/J/other/Ser/179.87
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/Ser/166.13
2019-06-21T18:30:00Z
J.other
ivo_managed
Multi-frequency study of the Pavo field (Filipovic+, 2003)
Filipovic M.D., Anderson M., Ekers R.D., Danziger I.J., Zimmermann H.-U., White G.L., Jones P.A., Borun B.C.P., Payne J.L., Dionne M., Ganis M., Ognjanovic M.
We test the prediction of Hamilton and Helfand (1993ApJ...418...55H) that faint radio selected galaxies are a new class contributing to the diffuse X-ray background (XRB) radiation. The test is based on the correlation of X-ray, optical and radio positions for sources detected in ROSAT (S_0.08-2.4keV_>6x10^-15^erg/s/cm^2^, 69 sources) and ATCA (S_1.42GHz_>250uJy, 93 sources) observations of the Einstein Pavo field. A total of six ATCA radio sources inside the inner ring of the ROSAT image are located within 10" of the ROSAT X-ray positions, with one associated by random chance.
CDS
2011-04-26T15:59:18
ivo://CDS.VizieR/J/other/Ser/166.13
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/Ap/54.81
2019-06-21T18:30:00Z
J.other
ivo_managed
Spectroscopy of {theta}1 Ori C system (Vitrichenko+, 2011)
Vitrichenko E.A., Tsymbal V., Bychkova L, Bychkov V.
High quality spectra of the triple star theta1 Ori C in the Orion Trapezium show that one more star in this system is a spectral binary. Its components are young main-sequence A-stars with masses of 1.3 and 1.4 solar mass. Radial velocities of stellar lines indicate that this binary runs away from the system in the direction to an observer with a large negative velocity. For the primary star (C3p) and the secondary (C3s) a list of lines, wavelength and equivalent width are given.
CDS
2011-07-10T22:39:04
ivo://CDS.VizieR/J/other/Ap/54.81
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/RAA/11.924
2019-06-21T18:30:00Z
J.other
ivo_managed
Atmospheric parameters for 771 stars (Wu+, 2011)
Wu Y., Luo A.L., Li H.N., Shi J.R., Prugniel P., Liang Y.C., Zhao Y.H., Zhang J.N., Bai Z.R., Wei P., Dong W.X., Zhang H.T., Chen J.J.
A number of spectroscopic surveys have been carried out or are planned to study the origin of the Milky Way. Their exploitation requires reliable automated methods and softwares to measure the fundamental parameters of the stars. Adopting the ULySS package, we have tested the effect of different resolutions and signal-to-noise ratios (SNR) on the measurement of the stellar atmospheric parameters (effective temperature Teff, surface gravity logg, and metallicity [Fe/H]). We show that ULySS is reliable to determine these parameters with medium-resolution spectra (R~2000). Then, we applied the method to measure the parameters of 771 stars selected in the commissioning database of the Guoshoujing Telescope (GSJT). The results were compared with the SDSS/SEGUE Stellar Parameter Pipeline (SSPP), and we derived precisions of 167K, 0.34dex, and 0.16dex for Teff, logg and [Fe/H] respectively. Furthermore, 120 of these stars are selected to construct the primary stellar spectra template library (Version 1.0) of GSJT, and will be deployed as basic ingredients for the GSJT automated parametrization pipeline.
CDS
2011-08-09T21:49:02
ivo://CDS.VizieR/J/other/RAA/11.924
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/Ser/178.65
2019-06-21T18:30:00Z
J.other
ivo_managed
Strongest radio point sources in LMC field (Payne+, 2009)
Payne J.L., Tauber L.A., Filipovic M.D., Crawford E.J., De Horta A.Y
During October 1994 and February 1995, the LMC was surveyed in mosaic mode, centred at 1.4GHz (bandwidth 128MHz), using the Australia Telescope Compact Array (ATCA). This survey divided the LMC into 12 regions, each containing 112 pointing centres. Each pointing centre was observed approximately 115 times (ranging from 95 to 140) for 15s.
CDS
2011-10-16T15:44:01
ivo://CDS.VizieR/J/other/Ser/178.65
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/JAD/16.2
2019-06-21T18:30:00Z
J.other
ivo_managed
New times of maximum of CY Aqr (Tuvikene+, 2010)
Tuvikene T., Sterken C., Brogt E., Cont D., Henden A., Papadaki C., Volkov I., Wiedemair C.
We present a collection of 102 new times of maximum of the SX Phoenicis star CY Aquarii. These times, together with 20 times of maximum taken from the literature, lead to a new local linear ephemeris for 2003-2009 with a formally slightly shorter period than the one for 1996-2002. It will require at least another half decade of additional monitoring before any significant update to any model can be considered. Such monitoring should preferably occur at regular intervals, be done in a consistent photometric band, and at high time resolution. A set of 114 new times of maximum obtained since 2002 leads to a new local linear ephemeris for 2003-2009: Tmax=2426159.512(+/-0.001)+0.061038349E(+/-0.000000002).
CDS
2012-01-29T13:00:09
ivo://CDS.VizieR/J/other/JAD/16.2
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/BASI/38.103
2019-06-21T18:30:00Z
J.other
ivo_managed
610-MHz survey of Lockman Hole with GMRT. II. (Garn+, 2010)
Garn T.S., Green D.A., Riley J.M., Alexander P.
An earlier survey (Garn et al., 2008, Cat. J/MNRAS/387/1037) had 12 pointings covering ~5 square degrees in the centre of the Lockman Hole, and here a further 26 pointings in the outer parts of the Lockman Hole are added, to cover a total of ~14 square degrees. To match the earlier survey, images were made with a resolution of 6"x5", position angle +45{deg]. The majority of the pointings have an rms noise of ~80uJy before primary beam correction, but the noise in the west - particularly near the very bright source 3C244.1 - is worse.
CDS
2012-02-14T16:02:26
ivo://CDS.VizieR/J/other/BASI/38.103
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/RAA/11.245
2019-06-21T18:30:00Z
J.other
ivo_managed
Galaxies in the field of RX J0054.0-2823 (Giraud+, 2011)
Giraud E., Gu Q.-S., Melnick J., Quintana H., Selman F., Toledo I., Zelaya P.
The observations (ESO program 078A-0456(A)) were obtained with the FORS2 instrument at the Cassegrain focus of the VLT UT1 telescope in multi-object spectroscopy mode with the exchangeable mask unit (MXU). They were acquired in service observing and were spread over the two periods, 78 and 80, to satisfy our observing requirements.
CDS
2012-02-18T22:10:36
ivo://CDS.VizieR/J/other/RAA/11.245
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/JAD/14.3
2019-06-21T18:30:00Z
J.other
ivo_managed
Emission lines in 32 Cygni (Eaton, 2008)
Eaton J.A.
The observations analyzed consist of a pair of deeply exposed IUE spectra of 32 Cyg taken in total eclipse on 31 March 1981 by R.E. Stencel.
CDS
2012-03-06T11:28:53
ivo://CDS.VizieR/J/other/JAD/14.3
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/Ser/183.103
2019-06-21T18:30:00Z
J.other
ivo_managed
SMC observations at 13, 20 and 36cm (Wong+, 2011)
Wong G.F., Filipovic M.D., Crawford E.J., Tothill F.H., de Horta A.Y., Draskovic D., Galvin T.J., Collier J.D., Payne J.L.
The 13cm radio-continuum catalogue was produced from a SMC mosaic radio survey of 20 square degrees (Filipovic et al., 2002, Cat. J/MNRAS/335/1085). These observations have a beam size of ~40" and r.m.s. noise of 0.4mJy/beam.
CDS
2012-03-12T23:37:22
ivo://CDS.VizieR/J/other/Ser/183.103
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/RAA/11.309
2019-06-21T18:30:00Z
J.other
ivo_managed
Nearby early-type galaxies in Stripe 82 (Jiang+, 2011)
Jiang F.-Z., Huang S., Gu Q.-S.
We make use of the images from the Sloan Digital Sky Survey Stripe 82 (Stripe 82) to present an analysis of r band surface brightness profiles and radial color gradients (g-r, u-r) in our sample of 111 nearby early-type galaxies (ETGs). Thanks to the Stripe 82 images, each of which is co-added from about 50 single frames, we are able to pay special attention to the low-surface-brightness areas (LSB areas) of the galaxies.
CDS
2012-03-16T05:51:10
ivo://CDS.VizieR/J/other/RAA/11.309
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/JAD/18.3
2019-06-21T18:30:00Z
J.other
ivo_managed
Infrared extinction spectra of aerosols (Sterken+, 2012)
Knox K.J., Lang E.K., Signorell R.
Mid-infrared extinction spectra (500-6000cm^-1^) of a series of single-component aerosol particle ensembles representative of those found in a range of planetary and lunar atmospheres are presented. The aerosols were generated in the laboratory via condensation from the gas phase in a bath gas cooling cell, and the spectra recorded using a Fourier transform infrared spectrometer. This paper is the first in a series aimed towards building a spectral database for use in remote sensing of aerosols. The aerosol substances included here are methane, ethane, propane, butane, pentane, ethylene, acetylene, carbon dioxide, ammonia and sulfur dioxide.
CDS
2012-04-22T22:53:05
ivo://CDS.VizieR/J/other/JAD/18.3
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/NewA/17.160
2019-06-21T18:30:00Z
J.other
ivo_managed
UBVRI photometry of Stock 18 (Bhatt+, 2012)
Bhatt H., Sagar R., Pandey J.-C.
The CCD UBVRI photometric data were acquired using 104-cm Sampurnanand Telescope (ST) of ARIES, Nainital, on 08/10/2007 and 19/12/2006.
CDS
2012-05-20T17:14:08
ivo://CDS.VizieR/J/other/NewA/17.160
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/NewA/17.347
2019-06-21T18:30:00Z
J.other
ivo_managed
Eclipsing times of BE Cep (Dai+, 2012)
Dai H.-F., Yang Y.-G., Hu S.-M., Guo D.-F.
New CCD observations of BE Cep were carried out from 2008 to 2011, using the 1.0m Cassegrain telescope at the Weihai Astronomical Observatory (WHAO) of Shandong University, the 85cm telescope and the 60cm telescope at the Xinglong station (XLs) of National Astronomical Observatories of China (NAOC), and the 1.56m telescope at the Sheshan Station of Shanghai Astronomical Observatory (SHAO).
CDS
2012-05-20T17:31:58
ivo://CDS.VizieR/J/other/NewA/17.347
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/JApA/32.567
2019-06-21T18:30:00Z
J.other
ivo_managed
Rotation measures in A2255 at 18, 21, 25, 85cm (Pizzo+ 2011)
Pizzo R.F.
After calibration, we produced Q and U channel images for each dataset and we inspected them to remove those affected by residual RFI (radio interferences) and/or problems related to specific telescopes. The final images were carried through for further processing in RM synthesis. To improve the resolution in RM space, as well as the sensitivity, we combined the 18, 21 and 25cm datasets, producing a single high-frequency RM cube. In addition, we made RM cubes at 85 and 200cm.
CDS
2012-05-22T15:49:47
ivo://CDS.VizieR/J/other/JApA/32.567
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/PASA/17.92
2019-06-21T18:30:00Z
J.other
ivo_managed
CO emission towards Southern dark clouds (Otrupcek+ 2000)
Otrupcek R.E., Hartley M., Wang J.-S.
Using the 22-m 'Mopra' antenna (near Coonabarabran, NSW) of the Australia Telescope National Facility (ATNF), we have observed emission from the 115-GHz J=1-0 transition of CO towards the centre of each of the 1101 clouds listed in the Hartley et al. Catalogue of Southern Dark Clouds (SDC, Cat. <VII/191>). The velocity range covered was -96 to +70km/s, with a velocity resolution of 0.120km/s. CO was detected at 1049 of the positions, with 367 spectra showing emission at more than one radial velocity. Here we present the most comprehensive general survey of the SDC catalogue, with the intensity, velocity and half-width of the CO detection and a code describing the profile shape. The presence of blue- or red-shifted wings in many observations can provide a starting point in searches for star-forming regions.
CDS
2012-09-24T07:35:31
ivo://CDS.VizieR/J/other/PASA/17.92
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/CoSka/33.159
2019-06-21T18:30:00Z
J.other
ivo_managed
Asteroid positions in 2002 (Neslusan+, 2003)
Neslusan L.
The paper presents the results of position determinations of minor planets carried out at the Skalnate Pleso Observatory in the year 2002. 109 CCD observations of 21 minor planets are given together with the list of reference stars.
CDS
2012-09-24T08:14:54
ivo://CDS.VizieR/J/other/CoSka/33.159
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/RoAJ/10.51
2019-06-21T18:30:00Z
J.other
ivo_managed
Standard errors for PPM and Tycho stars (Bocsa, 2000)
Bocsa G.
The connection between the optical reference frame and the radio one constitutes one of the main purposes of the astrometry. The paper is pointing out the contribution of the Bucharest Observatory in this direction. The statistic analysis of the standard errors for the astrometric PPM and TYCHO stars is presented.
CDS
2012-09-24T08:53:31
ivo://CDS.VizieR/J/other/RoAJ/10.51
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/PNAOJ/7.37
2019-06-21T18:30:00Z
J.other
ivo_managed
KUG survey, second series. IV. (Miyauchi-isobe+, 2003)
Miyauchi-Isobe N., Maehara H.
The catalogue list and the identification chart of ultraviolet (UV)-excess galaxies which have been detected on two-color Kiso Schmidt plates are presented for 10 Schmidt fields. Catalogued are 189 objects, down to the photographic magnitude ~18.0 in the sky area of some 300 square degrees. The total number of KUGs newly detected in the second survey reaches 1829.
CDS
2012-09-24T08:53:59
ivo://CDS.VizieR/J/other/PNAOJ/7.37
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/PNAOJ/6.107
2019-06-21T18:30:00Z
J.other
ivo_managed
KUG survey, second series. III (Miyauchi-Isobe+, 2002)
Miyauchi-Isobe N., Maehara H.
The catalogue list and the identification chart of ultraviolet (UV)-excess galaxies which have been detected on two-color Kiso Schmidt plates are presented for 10 Schmidt fields. Catalogued are 710 objects, down to the photographic magnitude ~17.5 in the sky area of some 300 square degrees. The total number of KUGs newly detected in the second survey reaches 1642.
CDS
2012-09-24T09:05:27
ivo://CDS.VizieR/J/other/PNAOJ/6.107
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/BSAO/45.136
2019-06-21T18:30:00Z
J.other
ivo_managed
Zelenchuk survey 9h<=RA<=12h, 0<=DE<=8{deg} (Ugolkova, 1998)
Ugolkova L.S.
Optical identification of Zelenchuk Survey radio sources at 3.9GHz from 9h to 12h in right ascension and between 0{deg} and 8{deg} in declination is reported in this paper. Some optical characteristics of identified radio sources are presented in the table.
CDS
2012-09-28T08:18:58
ivo://CDS.VizieR/J/other/BSAO/45.136
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/BSAO/46.28
2019-06-21T18:30:00Z
J.other
ivo_managed
Complete sample of PMN survey spectra (Mingaliev+, 1998)
Mingaliev M.G., Botashev A.M., Stolyarov V.A.
In this report we present the results of observations of a complete sample of sources from the PMN Survey. The adopted selection criteria were: flux density >200mJy at the PMN Survey frequency 4.8GHz; 0h<RA<24h; -21{deg}<=Dec<=-17{deg}; |b|>=10(deg} to exclude the galactic plane. Five runs of observations were accomplished in 1995-1996. The observations were made at 0.96, 2.3, 3.9, 7.7 and 11.2GHz at the RATAN-600 radio telescope. For all sources of the sample, flux densities at five frequencies and their simultaneous spectra were determined, accuracies in RA were improved 5-10 times. Identifications with data from the Texas Survey were performed.
CDS
2012-10-23T12:23:49
ivo://CDS.VizieR/J/other/BSAO/46.28
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/PZ/23.141
2019-06-21T18:30:00Z
J.other
ivo_managed
Flare stars in the Pleiades (Kazarovets 1993)
Kazarovets E.V.
A brief account is given of the problems in identifying newly discovered variable stars with already known ones. These problems are most acute in dense stellar fields, for instance, in the Pleiades. To arrive to a homogeneous coordinates system for variable stars in the Pleiades, the author has measured the coordinates for nearly 550 stars in the region centered on Alcyone. This has made it possible to obtain for the first time accurate coordinates for 165 flare stars; then, for 46 stars we have round significant errors in the published coordinates. A cross-identification table between the GCVS (Cat. <II/139>) and the catalogue of Haro et al. (1982, Cat. <II/131>) has been compiled.
CDS
2012-11-13T14:17:27
ivo://CDS.VizieR/J/other/PZ/23.141
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/Ap/31.714
2019-06-21T18:30:00Z
J.other
ivo_managed
Faint carbon stars in 90<l<115, |b|<5 (Kurtanidze+, 1989)
Kurtanidze O.M., Nikolashvili M.G.
A low dispersion spectral survey (1250{AA}/mm near H{gamma}) made with the 70-cm meniscus telescope in the region 90{deg}<=l<=115{deg}, -5{deg}<=b<=+5{deg} has led to the discovery of 267 carbon stars, 146 of which have been found for the first time. The distribution of the carbon stars in the investigated region with respect to latitude and longitude is uniform, and they have a Poisson surface distribution. The "nearest-neighbor" method shows that there is no excess of pairs of carbon stars or possible members of star clusters above their mathematical expectation.
CDS
2012-11-13T14:17:34
ivo://CDS.VizieR/J/other/Ap/31.714
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/PASA/16.113
2019-06-21T18:30:00Z
J.other
ivo_managed
New structure in Shapley supercluster (Drinkwater+, 1999)
Drinkwater M.J., Proust D., Parker Q.A., Quintana H., Slezak E.
We present new radial velocities for 306 bright (R<16) galaxies in a 77{deg}^2^ region of the Shapley supercluster, measured with the FLAIR-II spectrograph on the UK Schmidt Telescope. The galaxies we measured were uniformly distributed over the survey area, in contrast to previous samples which were concentrated in several rich Abell clusters. Most of the galaxies (230) were members of the Shapley supercluster: they trace out two previously unknown sheets of galaxies linking the Abell clusters of the supercluster. In a 44{deg}^2^ area of the supercluster excluding the Abell clusters, these sheets alone represent an overdensity of a factor of 2.0+/-0.2 compared to a uniform galaxy distribution. The supercluster is not flattened in the Declination direction as has been suggested in previous papers. Within our survey area the new galaxies contribute an additional 50% to the known contents of the Shapley supercluster, with a corresponding increase in its contribution to the motion of the Local Group.
CDS
2012-11-13T14:17:54
ivo://CDS.VizieR/J/other/PASA/16.113
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/ChJAA/3.49
2019-06-21T18:30:00Z
J.other
ivo_managed
Velocity and distance of methanol maser sources (Xu+, 2003)
Xu Y., Zheng X.-W., Jiang D.-R.
We have searched the literature for all known 6.7GHz methanol maser sources and found a total of 482 objects. Among these, 361 have IRAS identifications.
CDS
2012-11-13T14:18:13
ivo://CDS.VizieR/J/other/ChJAA/3.49
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/BSAO/40.128
2019-06-21T18:30:00Z
J.other
ivo_managed
RATAN-600 radio sources spectra (Bursov 1996)
Bursov N.N
In accordance with the program "Cold" in 1987-1988 and in 1996 deep surveys of the sky strip at the declination of the source SS 433 ({delta}~5{deg}+/-20') were made at the radio telescope RATAN-600. For the first time spectral characteristics of 400 sources from the RC catalog have been determined using only the data obtained with the RATAN-600. The maximum of the flux density distributions at the central wavelength {lambda}7.6cm is ~30mJy. The lower flux limit in the sample of the sources at the wavelengths 3.9, 7.6, 13.0, 31.0cm is 16, 9, 37, 61mJy, respectively. Spectra of 112 sources (28%) have been obtained for the first time, spectra of 90 (23%) sources have been made more accurate. For the first time the fluxes at the wavelengths 2.7, 3.9, 13.0 and 31.0cm (90% of data) have been measured. The maximum of the distribution of spectral indices for the entire sample of sources in the interval {lambda}{lambda}7.6-31.0cm falls at {alpha}=-0.86+/-0.04 (S_{nu}_{prop.to}{nu}^alpha^). About 20 (5%) sources of the sample have a maximum of radiation at a frequency of about 1GHz (GHz-Peaked-Spectrum radio sources), about 40 (10%) have a low-frequency cut off of the spectrum. About 70 (19%) sources have flat spectra ({alpha}>-0.5), 64 (18%) very steep ({alpha}<-1.1) spectra.
CDS
2013-02-08T15:47:20
ivo://CDS.VizieR/J/other/BSAO/40.128
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/AuJPA/14.77
2019-06-21T18:30:00Z
J.other
ivo_managed
408MHz galactic radio sources (Shaver+ 1970)
Shaver P.A., Goss W.M.
Contour maps of 58 regions are presented showing 408 MHz radioisophotes for over 200 galactic radio sources. Positions and integrated flux densities are listed for all the sources.
CDS
2013-02-11T12:42:39
ivo://CDS.VizieR/J/other/AuJPA/14.77
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/Sci/338.355
2019-06-21T18:30:00Z
J.other
ivo_managed
1.3mm VLBI detections of M87 (Doeleman+, 2012)
Doeleman S.S., Fish V.L., Schenck D.E., et al.
We observed M87 over 3 consecutive days with a 1.3-mm wavelength VLBI array consisting of four telescopes at three geographical locations: the James Clerk Maxwell Telescope (JCMT) on Mauna Kea in Hawaii, the Arizona Radio Observatory's Submillimeter Telescope (SMT) in Arizona, and two telescopes of the Combined Array for Research in Millimeter-wave Astronomy (CARMA, located ~60m apart) in California.
CDS
2013-02-14T06:49:00
ivo://CDS.VizieR/J/other/Sci/338.355
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/RAA/12.1381
2019-06-21T18:30:00Z
J.other
ivo_managed
BATC photometry on A119 (Tian+, 2012)
Tian J.-T., Yuan Q.-R., Zhou X., Jiang Z.-J., Ma J., Wu J.-H., Wu Z.-Y., Fan Z., Zhang T.-M., Zou H.
This paper presents multicolor optical photometry of the nearby galaxy cluster Abell 119 (z=0.0442) with the Beijing-Arizona-Taiwan-Connecticut system of 15 intermediate bands. Within the BATC field of view of 58'x58', there are 368 galaxies with known spectroscopic redshifts, including 238 member galaxies (called sample I). Based on the spectral energy distributions of 1376 galaxies brighter than i_BATC_=19.5, the photometric redshift technique and the color-magnitude relation of early-type galaxies are applied to select faint member galaxies. As a result, 117 faint galaxies were selected as new member galaxies. Combined with sample I, an enlarged sample (called sample II) of 355 member galaxies is obtained. Spatial distribution and localized velocity structure for two samples demonstrate that A119 is a dynamically complex cluster with at least three prominent substructures in the central region within 1Mpc. A large velocity dispersion for the central clump indicates a merging along the line of sight. No significant evidence for morphology or luminosity segregations is found in either sample. With the PEGASE evolutionary synthesis model, the environmental effect on the properties of star formation is confirmed. Faint galaxies in the low-density region tend to have longer time scales of star formation, smaller mean stellar ages, and lower metallicities in their interstellar medium, which is in agreement with the context of the hierarchical cosmological scenario.
CDS
2013-02-17T21:53:33
ivo://CDS.VizieR/J/other/RAA/12.1381
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/PASAu/6.471
2019-06-21T18:30:00Z
J.other
ivo_managed
Magellanic Clouds bridge region HI profiles (McGee+ 1986)
McGee R.X., Newton L.M.
Two hundred and seventeen HI profiles at positions approximately 1degree apart in the bridge region between the Small and Large Magellanic Clouds have been observed with a 15' arc beam. Diagrams of all the profiles, lists of column densities and average radial velocities are given, together with details of the extensive Gaussian analysis needed to account for the components. It is shown that the bridge region is most complex. (a) Two radial velocity (1) groups, +214 and +238km/s, represent the actual HI bridge between the two galaxies. (b) Three other components, at mean radial velocities of +155, +177 and +195km/s are seen to be integral parts of the SMC, stretching east to RA~04h. (c) A further three components in groups at mean radial Velocities +253, +272 and +293km/s appear to be extensions of HI from the main body of the LMC. Nine sets of five closely spaced observations in the lower Magellanic Stream and in the bridge region at high sensitivity supply further information about the region.
CDS
2013-02-26T11:57:01
ivo://CDS.VizieR/J/other/PASAu/6.471
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/ApL/30.1
2019-06-21T18:30:00Z
J.other
ivo_managed
Southern catalogue of isolated pairs extension (Reduzzi+ 1995)
Reduzzi L., Rampazzo R.
The paper presents a sample of double galaxies selected from The Surface Photometry Catalog of the ESO-Uppsala Galaxies (Cat. <VII/115>) using the Karachentsev (1972: K72, Cat. <VII/77>) criteria. Considering the large and growing number of observing facilities in that hemisphere, the sample aims to supply investigators with targets as homogeneous as possible to those in the Northern Catalog of Isolated Pairs of Galaxies (K72) which have been studied in a large frequency range. The paper discusses the sample degree of completeness, separation and velocity distributions. First inferences are sketched from the morphological association of pair members and from the study of the Holmberg effect. Being the primary purpose of the paper to provide a tool to investigators, an Atlas of images for the 301 best candidate pairs obtained using the Digitized Sky Survey (The Digitized Sky Survey was produced at the Space Telescope Science Institute (ST ScI) under U.S. Government grant NAG W-2166) is given. The Atlas reports for each pair member the relevant data as obtained from the current literature.
CDS
2013-03-04T07:53:49
ivo://CDS.VizieR/J/other/ApL/30.1
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/ApSS/344.175
2019-06-21T18:30:00Z
J.other
ivo_managed
Protoclusters and subclusters (Majaess, 2013)
Majaess D.
This file contains a subsample of the embedded clusters identified, with an emphasis on smaller overlooked subclusters, whereby subclusters are offshoot clumps of emerging stars tied to broader star-forming regions (hierarchical clustering). The bulk of the targets deviate from spherical symmetry and are typically associated with larger complexes. Apparent sizes for the (sub)clusters are tabulated, and those entries tagged by an asterisk contain few members. The majority of the targets will dissolve prior to becoming an intermediate-age cluster. Clusters which were serendipitously identified as a result of the analysis are likewise tabulated. Numerous objects are not discernible in optical and even W1 images, which underscores the extreme obscuration endemic to the host environment. Following discussions with Dias et al., the cluster of class I/f YSOs discovered near the classical Cepheid SU Cas (Majaess et al. 2012MNRAS.421.1040M) is included as Majaess 230. New WISE mid-IR data unambiguously revealed a cluster of numerous class I/f YSOs centred at J2000 02:54:31.4 +69:20:32.5, and a nearby YSO and 2MASS overdensity were noted previously (e.g. Straizys & Kazlauskas 2010BaltA..19....1S, Froebrich et al. 2007MNRAS.374..399F). In sum, the results reaffirm the importance of the latest generation of infrared surveys (e.g., WISE) for enabling the detection of YSOs and their nascent environments. However, significant work remains and subsequent refinement to the YSO selection scheme pending the identification of biases is inevitable. Spectroscopic, deep IR photometric, and sub-mm (ALMA) follow-up observations for the cluster targets are desirable, and forthcoming. This publication makes use of data products from WISE, 2MASS, CDS, arXiv, NASA/IPAC ISA, and NASA ADS.
CDS
2013-03-04T11:03:33
ivo://CDS.VizieR/J/other/ApSS/344.175
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/Sci/340.45
2019-06-21T18:30:00Z
J.other
ivo_managed
Fast shocks around SN 1006 (Nikolic+, 2013)
Nikolic S., Van De Ven G., Heng K., Kupko D., Husemann B., Raymond J.C., Hughes J.P., Falcon-Barroso J.
Supernova remnants are among the most spectacular examples of astrophysical pistons in our cosmic neighborhood. The gas expelled by the supernova explosion is launched with velocities ~1000 kilometers per second into the ambient, tenuous interstellar medium, producing shocks that excite hydrogen lines. We have used an optical integral-field spectrograph to obtain high-resolution spatial-spectral maps that allow us to study in detail the shocks in the northwestern rim of supernova 1006. The two-component H{alpha} line is detected at 133 sky locations. Variations in the broad line widths and the broad-to-narrow line intensity ratios across tens of atomic mean free paths suggest the presence of suprathermal protons, the potential seed particles for generating high-energy cosmic rays.
CDS
2013-06-09T12:23:06
ivo://CDS.VizieR/J/other/Sci/340.45
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/Ser/184.93
2019-06-21T18:30:00Z
J.other
ivo_managed
6cm and 3cm sources in SMC (Wong+, 2012)
Wong G.F., Crawford E.J., Filipovic M.D., de Horta A.Y., Tothill N.F.H., Collier J.D., Draskovic D., Galvin T.J., Payne J.L.
We present two new catalogues of radio-continuum sources in the field of the Small Magellanic Cloud (SMC). These catalogues contain sources found at 4800MHz ({lambda}=6cm) and 8640MHz ({lambda}=3cm). Some 457 sources have been detected at 3cm with 601 sources at 6cm created from new high-sensitivity and resolution radio-continuum images of the SMC from Crawford et al. (2011SerAJ.183...95C).
CDS
2013-07-17T12:46:30
ivo://CDS.VizieR/J/other/Ser/184.93
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/BSAO/46.62
2019-06-21T18:30:00Z
J.other
ivo_managed
RATAN observations of Galactic SNRs (Trushkin+, 1998)
Trushkin S.A.
We present radio continuum spectra for 200 Galactic supernova remnants (SNRs) from 220 known and included in Green's (1998, Cat. VII/211) catalog. The spectra can be plotted only for 200 SNRs because about 20 remaining new and weak SNRs (Whiteoak and Green, 1996, Cat. J/A+AS/118/329; Gray, 1994MNRAS.270..847G) have only one-frequency flux density measurements. Spectrum plotting is an "on-line" procedure of the CATS database (Verkhodanov et al., 1997ASPCo.125..322V) created for some other multi-frequency catalogs. These spectra include most of the measurements available in literature, as well as multi-frequency measurements of nearly 120 SNRs with the RATAN-600 radio telescope in 1, 2 and 4 Galactic quadrants and from the Galactic plane survey at 960 and 3900MHz (Trushkin, 1986ATsir1453....4T, 1987AISAO..25...84T, 1989, Ph.D. Thesis. SAO, Nizhnij Arkhyz, 1996BSAO...41...64T, 1998BSAO...46...62T). The measurements have been placed on the same absolute flux density scale of Baars (1977A&A....61...99B) as in the paper by Kassim (1989ApJ...347..915K), using the correcting factor from the compiled catalog (Kuhr et al., 1981, Cat. VIII/5). The presented compilation has given a possibility of plotting quite accurate spectra with the thermal plasma free-free absorption in fitting the spectra accounted for.
CDS
2013-09-11T06:45:13
ivo://CDS.VizieR/J/other/BSAO/46.62
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/Nat/498.198
2019-06-21T18:30:00Z
J.other
ivo_managed
Na abundances in NGC6752 (Campbell+, 2013)
Campbell S.W., D'Orazi V., Yong D., Constantino T.N., Lattanzio J.C., Stancliffe R.J., Angelou G.C., Wylie-de Boer E.C., Grundahl F.
We obtained high-resolution spectra (R~24000) for a sample of 20 AGB stars and 24 red giant branch stars in the Galactic globular cluster NGC 6752.
CDS
2013-10-19T14:40:19
ivo://CDS.VizieR/J/other/Nat/498.198
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/RAA/10.1
2019-06-21T18:30:00Z
J.other
ivo_managed
BATC photometry in A98 cluster (Zhang+, 2010)
Zhang L., Yuan Q.-R., Zhou X., Jiang Z.-J., Yang Y.-B., Ma J., Wu J.-H., Wu Z.-Y.
From 1996 to 2006, we accumulated 37h in only 12 bands, from d to p, with the old CCD camera. In the last two years, exposures in the a, b, and c filters were completed with the new CCD camera.
CDS
2013-12-20T13:28:49
ivo://CDS.VizieR/J/other/RAA/10.1
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/BSAO/40.5
2019-06-21T18:30:00Z
J.other
ivo_managed
RATAN-600 RC radio sources (Parijskij+ 1996)
Parijskij Yu.N., Goss W.M., Kopylov A.I., Soboleva N.S., Temirova A.V., Verkhodanov O.V., Zhelenkova O.P., Naugolnaya M.N.
We use the RATAN-600 radio telescope for picking up the most distant objects in the Universe. As a first step, about 100 steep spectrum FRII radio galaxies (SS FRII RG) from the RATAN-600 RC catalog (Parijskij et al., 1991, Cat. <J/A+AS/87/1>; 1992A&AS...96..583P) were mapped by the VLA and identified with optical objects down to 24-25 R mag. All the VLA images and all the deep CCD images of the RC SS fields, collected up to now, are given. An updated list of calibrators with the known redshifts of the same SS FRII class RGs was compiled to estimate photometric redshifts, redshifts from angular size - redshift relations and by the radio "standard candle" method. The mean redshift of the RC SS FRII RG list happened to be greater than 2. BVRI photometry was made, and by standard model fittings we estimated "color" redshifts and the ages of stellar systems of the parent gE galaxies in 14 cases. Several objects were found in which active star formation began in the first billion years after the Big Bang. We believe that more than 10000 of such old active galaxies are available on the sky and all of them are in the range of present day optical and radio facilities.
CDS
2014-02-19T15:06:36
ivo://CDS.VizieR/J/other/BSAO/40.5
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/AstBu/68.262
2019-06-21T18:30:00Z
J.other
ivo_managed
Sample of 467 GPS candidates (Mingaliev+, 2013)
Mingaliev M.G., Sotnikova Yu.V., Mufakharov T.V., Erkenov A.K., Udovitskiy R.Yu.
We selected objects with convex radio spectra from a flux-density complete sample: S>=200mJy at 4.8 or 5GHz (we define the spectral index alpha such that S{prop.to}nu^alpha^) using multifrequency measurements of the RATAN-600 radio telescope (2012A&A...544A..25M) and data from the CATS astrophysical catalogs support system (1997BaltA...6..275V). As a result, we selected 467 GPS candidates by spectral type, with redshift data available for 249 of these objects. The sample contains 118 galaxies, 187 quasars, and 162 sources without optical counterparts. For each source name in J2000 equatorial coordinates, the optical counterpart, redshift, peak frequency, radio flux density, spectral indexes, FWHM, blazar type, morphological type and variability are presented.
CDS
2014-03-15T16:28:44
ivo://CDS.VizieR/J/other/AstBu/68.262
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/PASA/26.454
2019-06-21T18:30:00Z
J.other
ivo_managed
Precise positions of methanol masers (Caswell, 2009)
Caswell J.L.
The methanol maser observations described here were obtained with the ATCA in many sessions since 1993 February, chiefly in any of the four standard '6-km' configurations (instantaneously yielding 15 baselines ranging from 76 to 6000m).
CDS
2014-11-20T11:13:37
ivo://CDS.VizieR/J/other/PASA/26.454
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/RMxAA/44.111
2019-06-21T18:30:00Z
J.other
ivo_managed
ubvy{beta} photometry of NGC 6882/5 stars (Pena+, 2008)
Pena J.H., Peniche R., Garrido R., Paparo M., Garcia-Cole A.
All the observations were carried out at the Observatorio Astromonico Nacional at San Pedro Martir, Mexico with the 150cm telescope equipped with a spectrometer, in three seasons: July-August 1986 (four nights), Jun 1997 (6 nights) and July 2000 (4 nights).
CDS
2014-12-05T14:52:47
ivo://CDS.VizieR/J/other/RMxAA/44.111
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/AcApS/18.302
2019-06-21T18:30:00Z
J.other
ivo_managed
Molecular clouds in 8<l<38, -1<b<+1 (Sun+, 1998)
Sun Y.-C., Sun J.
A systematic comparison between molecular clouds in different evolutionary stages and processes of star formation is made over the range of 8{deg} to 38{deg} in Galactic longitude and -1{deg} to +1{deg} in Galactic latitude by using the Massachusetts-Stony Brook Survey data of ^12^CO in the Galactic plane (HPFW=47") and the IRAS Infrared Sky Survey image data (1.5' per pixel). This region is divided into thirty subregions. Then, the space distribution of CO(1-0) emission and the corresponding infrared intensity at 60ymis obtained for each subregion, and the contours of infrared color temperatures and optical depths of molecular cloud complexes in the corresponding regions are calculated and derived. Moreover, the catalogs of the IRAS infrared point sources and HII regions are used. Thus, molecular clouds in different evolutionary stages are identified and divided into four groups ranging from young clouds to evolved clouds, and their main characteristics and relations to the processes of star formation are analysed. The Galatic-longitude distributions of ultracompact HII regions and candidate protostars as well as the ratio between HII region-molecular cloud and candidate protostar-molecular cloud associations are analysed statistically. The results indicate that star formation activities are currently still going on in our Galaxy.
CDS
2014-12-05T14:53:22
ivo://CDS.VizieR/J/other/AcApS/18.302
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/SoSyR/45.523
2019-06-21T18:30:00Z
J.other
ivo_managed
CCD observations of saturnian satellites (Grosheva+, 2011)
Grosheva E.A., Izmailov I.S., Kiseleva T.P.
All observations were carried out with 26-inch Zeiss refractor(D=650mm, F=10413mm, scale is 19.80"/mm) at Pulkovo (code is 084). CCD camera FLI Pro Line 09000 (3056x3056pix) was used. Scale per pixel is 0.24" and field observed with this camera is 12'x12'. Time of exposures is 1.5s. All presented positions are topocentric. Ephemerides for comparison are given by web-server "Natural Satellites Ephemeride Server MULTI-SAT" developed by N.V. Emelyanov (http://lnfm1.sai.msu.ru/neb/nss/nssephmr.htm).
CDS
2015-01-19T11:58:05
ivo://CDS.VizieR/J/other/SoSyR/45.523
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
ivo://CDS.VizieR/J/other/BOBeo/155.3
2019-06-21T18:30:00Z
J.other
ivo_managed
Belgrade meridian circle catalog (Sadzakov+, 1997)
Sadzakov S., Dacic M., Cvetkovic Z.
The authors present an observational catalogue containing the positions of 351 stars situated in the vicinity of radio sources (RRS2, Tel'nyuk-Adamchuk & Kumkova, 1991, IAU Colloq. 127, 363) worked out by differential method in the FK5 system. The (O-C) corrections to the positions of 267 fundamental stars used in the determination of the instrument parameters are also presented. The star positions are derived from the observations with the Belgrade Large Meridian Circle during 1991-1993.
CDS
2015-03-03T13:58:13
ivo://CDS.VizieR/J/other/BOBeo/155.3
en
http://cdsweb.u-strasbg.fr
unrestricted
Dataset
J.other!!!oai_dc!100