Dictionary of Nomenclature of Celestial Objects

n and kinematic structure of 10000 nearby galaxies. MaNGA uses integral field unit (IFU) spectroscopy to measure spectra for hundreds of points within each galaxy.

The format NN-NNNNNNNNN is the combination of the catalog ID and the line number ("CatalogID-LineNumber").
The format NNNNN-NNNNN is composed of the plate ID and the IFU design ID ("plate-ifudsgn").

For more information, visit: http://www.sdss.org/surveys/manga/
To search, access, and visualize the MaNGA data, visit: https://dr16.sdss.org/marvin/

In bright time, the MaNGA instrument has been used to observe stars for MaNGA Stellar Library (MaStar), to build a comprehensive optical stellar spectral library with which to calibrate the galaxy observations.
For more information on this stellar library, visit the MaStar survey page (https://www.sdss.org/surveys/mastar/).

Only the first references citing MaNGA sources are listed here.

Ref:=2015ApJ...798....7B
byBUNDY K. , BERSHADY M.A., LAW D.R., YAN R., DRORY N., MacDONALD N., WAKE D.A., CHERINKA B., SANCHEZ-GALLEGO J.R., WEIJMANS A.-M., THOMAS D., TREMONTI C., MASTERS K., COCCATO L., DIAMOND-STANIC A.M., ARAGON-SALAMANCA A., AVILA-REESE V., BADENES C., FALCON-BARROSO J., BELFIORE F., BIZYAEV D., BLANC G.A., BLAND-HAWTHORN J., BLANTON M.R., BROWNSTEIN J.R., BYLER N., CAPPELLARI M., CONROY C., DUTTON A.A., EMSELLEM E., ETHERINGTON J., FRINCHABOY P.M., FU H., GUNN J.E., HARDING P., JOHNSTON E.J., KAUFFMANN G., KINEMUCHI K., KLAENE M.A., KNAPEN J.H., LEAUTHAUD A., LI C., LIN L., MAIOLINO R., MALANUSHENKO V., MALANUSHENKO E., MAO S., MARASTON C., McDERMID R.M., MERRIFIELD M.R., NICHOL R.C., ORAVETZ D., PAN K., PAREJKO J.K., SANCHEZ S.F., SCHLEGEL D., SIMMONS A., STEELE O., STEINMETZ M., THANJAVUR K., THOMPSON B.A., TINKER J.L., VAN DEN BOSCH R.C.E., WESTFALL K.B., WILKINSON D., WRIGHT S., XIAO T., ZHANG K.
 Astrophys. J., 798, 7 (2015)
  Overview of the SDSS-IV MaNGA survey: Mapping Nearby Galaxies at Apache Point Observatory.
oTable 5, col(2): <MaNGA N-NNNNNN> N=18.
Ref:=2015ApJ...804..125L
byLI C. , WANG E., LIN L., BERSHADY M.A., BUNDY K., TREMONTI C.A., XIAO T., YAN R., BIZYAEV D., BLANTON M., CALES S., CHERINKA B., CHEUNG E., DRORY N., EMSELLEM E., FU H., GELFAND J., LAW D.R., LIN L., MacDONALD N., MARASTON C., MASTERS K.L., MERRIFIELD M.R., PAN K., SANCHEZ S.F., SCHNEIDER D.P., THOMAS D., WAKE D., WANG L., WEIJMANS A.-M., WILKINSON D., YOACHIM P., ZHANG K., ZHENG T.
 Astrophys. J., 804, 125 (2015)
  P-MaNGA: gradients in recent star formation histories as diagnostics for galaxy growth and death.
oTable 1, col(3): <MaNGA N-NNNNNN> N=12.
=E=Catalogue in electronic form as <J/ApJ/883/175/>

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