Dictionary of Nomenclature of Celestial Objects

 vey. The K-band follow-up in the 0226-04 field.
oCatalogue: <VVDS 02NNNNNNN> N=253588.
 Auth.:TEMPORIN S.+
   Ref:=2009A&A...495...53L
     byLAMAREILLE F.
, BRINCHMANN J., CONTINI T., WALCHER C.J., CHARLOT S., PEREZ-MONTERO E., ZAMORANI G., POZZETTI L., BOLZONELLA M., GARILLI B., PALTANI S., BONGIORNO A., LE FEVRE O., BOTTINI D., LE BRUN V., MACCAGNI D., SCARAMELLA R., SCODEGGIO M., TRESSE L., VETTOLANI G., ZANICHELLI A., ADAMI C., ARNOUTS S., BARDELLI S., CAPPI A., CILIEGI P., FOUCAUD S., FRANZETTI P., GAVIGNAUD I., GUZZO L., ILBERT O., IOVINO A., McCRACKEN H.J., MARANO B., MARINONI C., MAZURE A., MENEUX B., MERIGHI R., PELLO R., POLLO A., RADOVICH M., VERGANI D., ZUCCA E., ROMANO A., GRADO A., LIMATOLA L.
 Astron. Astrophys., 495, 53-72 (2009)

    Physical properties of galaxies and their evolution in the VIMOS VLT deep
    survey. I. The evolution of the mass-metallicity relation up to z ~ 0.9.
=E=Catalogue in electronic form as J/A+A/439/845
=E=Catalogue in electronic form as II/286
=E=Catalogue in electronic form as J/A+A/495/53

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