SIMBAD references

2006A&A...457...79G - Astronomy and Astrophysics, volume 457, 79-90 (2006/10-1)

The VIMOS VLT Deep Survey: the faint type-1 AGN sample.

GAVIGNAUD I., BONGIORNO A., PALTANI S., MATHEZ G., ZAMORANI G., MOLLER P., PICAT J.P., LE BRUN V., MARANO B., LE FEVRE O., BOTTINI D., GARILLI B., MACCAGNI D., SCARAMELLA R., SCODEGGIO M., TRESSE L., VETTOLANI G., ZANICHELLI A., ADAMI C., ARNABOLDI M., ARNOUTS S., BARDELLI S., BOLZONELLA M., CAPPI A., CHARLOT S., CILIEGI P., CONTINI T., FOUCAUD S., FRANZETTI P., GUZZO L., ILBERT O., IOVINO A., McCRACKEN H.J., MARINONI C., MAZURE A., MENEUX B., MERIGHI R., PELLO R., POLLO A., POZZETTI L., RADOVICH M., ZUCCA E., BONDI M., BUSARELLO G., CUCCIATI O., DE LA TORRE S., GREGORINI L., LAMAREILLE F., MELLIER Y., MERLUZZI P., RIPEPI V., RIZZO D. and VERGANI D.

Abstract (from CDS):

We present the type-1 active galactic nuclei (AGN) sample extracted from the VIMOS VLT Deep Survey's first observations of 21000 spectra in 1.75deg2. This sample, which is purely magnitude-limited and free of morphological or color-selection biases, contains 130 broad-line AGN (BLAGN) spectra with redshift up to 5. Our data are divided into a wide (IAB≤22.5) and a deep (IAB≤24) subsample containing 56 and 74 objects, respectively. Because of its depth and selection criteria, this sample is uniquely suited for studying the population of faint type-1 AGN. Our measured surface density (∼472±48 BLAGN per square degree with IAB≤24) is significantly higher than that of any other optically selected sample of BLAGN with spectroscopic confirmation. By applying a morphological and color analysis to our AGN sample, we find that (1) ∼23% of the AGN brighter than IAB=22.5 are classified as extended, and this percentage increases to ∼42% for those with z<1.6; (2) a non-negligible fraction of our BLAGN are lying close to the color-space area occupied by stars in the u*-g' versus g'-r' color-color diagram. This leads us to the conclusion that the classical optical-ultraviolet preselection technique, if employed at such deep magnitudes (IAB=22.5) in conjuction with a preselection of point-like sources, can miss up to ∼35% of the AGN population. Finally, we present a composite spectrum of our sample of objects. While the continuum shape is very similar to that of the SDSS composite at short wavelengths, it is much redder than that of the SDSS composite at λ≥3000Å. We interpret this as due to significant contamination from emission of the host galaxies, as expected from the faint absolute magnitudes sampled by our survey.

Abstract Copyright:

Journal keyword(s): catalogs - surveys - galaxies: active - galaxies: Seyfert - quasars: general

VizieR on-line data: <Available at CDS (J/A+A/457/79): tablea1.dat tablea2.dat>

Nomenclature: Tables A3-A4: VVDS HHNNNNNNN N=62+18+38.

CDS comments: Tables A1-A2: In CDFS objects are designated as VCDFS NNNNN in SIMBAD.

Simbad objects: 131

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2021.06.24-01:16:45

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