Dictionary of Nomenclature of Celestial Objects
(Last update: 13-Nov-2020)

Result of query: info cati VVDS$

Details on Acronym:   VVDS
   VVDS (VIMOS VLT Deep Survey) Write:<<VVDS HHNNNNNNN>>
<<VVDS JHHMMSS.ss+DDMMSS.s>> N: 8981+253588 Object:?  (SIMBAD class: Unknown = Object of unknown nature) Note:The VVDS is a faint-imaging and I(AB) magnitude-limited VLT VIMOS spectroscopic survey. In 2006A&A...457...79G search for AGNs in the VVDS. See also VCDFS in the CDFS. Ref:=2005A&A...439..845L byLE FEVRE O. , VETTOLANI G., GARILLI B., TRESSE L., BOTTINI D., LE BRUN V., MACCAGNI D., PICAT J.P., SCARAMELLA R., SCODEGGIO M., ZANICHELLI A., ADAMI C., ARNABOLDI M., ARNOUTS S., BARDELLI S., BOLZONELLA M., CAPPI A., CHARLOT S., CILIEGI P., CONTINI T., FOUCAUD S., FRANZETTI P., GAVIGNAUD I., GUZZO L., ILBERT O., IOVINO A., McCRACKEN H.J., MARANO B., MARINONI C., MATHEZ G., MAZURE A., MENEUX B., MERIGHI R., PALTANI S., PELLO R., POLLO A., POZZETTI L., RADOVICH M., ZAMORANI G., ZUCCA E., BONDI M., BONGIORNO A., BUSARELLO G., LAMAREILLE F., MELLIER Y., MERLUZZI P., RIPEPI V., RIZZO D. Astron. Astrophys., 439, 845-862 (2005) The VIMOS VLT deep survey. First epoch VVDS-deep survey: 11564 spectra with 17.5≤I_{AB}≤24, and the redshift distribution over 0≤z≤5. oCatalog, col(1): <VVDS HHNNNNNNN> N=8981 = Catalog, col(2): <VVDS JHHMMSS.ss+DDMMSS.s> N=8981. Ref:=2008A&A...482...81T byTEMPORIN S. , IOVINO A., BOLZONELLA M., McCRACKEN H.J., SCODEGGIO M., GARILLI B., BOTTINI D., LE BRUN V., LE FEVRE O., MACCAGNI D., PICAT J.P., SCARAMELLA R., TRESSE L., VETTOLANI G., ZANICHELLI A., ADAMI C., ARNOUTS S., BARDELLI S., CAPPI A., CHARLOT S., CILIEGI P., CONTINI T., CUCCIATI O., FOUCAUD S., FRANZETTI P., GAVIGNAUD I., GUZZO L., ILBERT O., MARANO B., MARINONI C., MAZURE A., MENEUX B., MERIGHI R., PALTANI S., PELLO R., POLLO A., POZZETTI L., RADOVICH M., VERGANI D., ZAMORANI G., ZUCCA E., BONDI M., BONGIORNO A., BRINCHMANN J., DE LA TORRE S., LAMAREILLE F., MELLIER Y., WALCHER C.J. Astron. Astrophys., 482, 81-95 (2008) The VIMOS VLT deep survey. The K-band follow-up in the 0226-04 field. oCatalogue: <VVDS 02NNNNNNN> N=253588. 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 Originof the Acronym: A = Assigned by the author(s)

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