2012A&A...546A..58R


C.D.S. - SIMBAD4 rel 1.7 - 2021.03.02CET03:24:12

2012A&A...546A..58R - Astronomy and Astrophysics, volume 546A, 58-58 (2012/10-1)

GOODS-Herschel: ultra-deep XMM-Newton observations reveal AGN/star-formation connection.

ROVILOS E., COMASTRI A., GILLI R., GEORGANTOPOULOS I., RANALLI P., VIGNALI C., LUSSO E., CAPPELLUTI N., ZAMORANI G., ELBAZ D., DICKINSON M., HWANG H.S., CHARMANDARIS V., IVISON R.J., MERLONI A., DADDI E., CARRERA F.J., BRANDT W.N., MULLANEY J.R., SCOTT D., ALEXANDER D.M., DEL MORO A., MORRISON G., MURPHY E.J., ALTIERI B., AUSSEL H., DANNERBAUER H., KARTALTEPE J., LEITON R., MAGDIS G., MAGNELLI B., POPESSO P. and VALTCHANOV I.

Abstract (from CDS):

Models of galaxy evolution assume some connection between the AGN and star formation activity in galaxies. We use the multi-wavelength information of the CDFS to assess this issue. We select the AGNs from the 3Ms XMM-Newton survey and measure the star-formation rates of their hosts using data that probe rest-frame wavelengths longward of 20µm, predominantly from deep 100µm and 160µm Herschel observations, but also from Spitzer-MIPS-70µm. Star-formation rates are obtained from spectral energy distribution fits, identifying and subtracting an AGN component. Our sample consists of sources in the z≃0.5-4 redshift range, with star-formation rates SFR≃101-103M/yr and stellar masses M*≃1010-1011.5M. We divide the star-formation rates by the stellar masses of the hosts to derive specific star-formation rates (sSFR) and find evidence for a positive correlation between the AGN activity (proxied by the X-ray luminosity) and the sSFR for the most active systems with X-ray luminosities exceeding Lx≃1043erg/s and redshifts z>1. We do not find evidence for such a correlation for lower luminosity systems or those at lower redshifts, consistent with previous studies. We do not find any correlation between the SFR (or the sSFR) and the X-ray absorption derived from high-quality XMM-Newton spectra either, showing that the absorption is likely to be linked to the nuclear region rather than the host, while the star-formation is not nuclear. Comparing the sSFR of the hosts to the characteristic sSFR of star-forming galaxies at the same redshift (the so-called ``main sequence'') we find that the AGNs reside mostly in main-sequence and starburst hosts, reflecting the AGN-sSFR connection; however the infrared selection might bias this result. Limiting our analysis to the highest X-ray luminosity AGNs (X-ray QSOs with Lx>1044erg/s), we find that the highest-redshift QSOs (with z>2) reside predominantly in starburst hosts, with an average sSFR more than double that of the ``main sequence'', and we find a few cases of QSOs at z≃1.5 with specific star-formation rates compatible with the main-sequence, or even in the ``quiescent'' region. Finally, we test the reliability of the colour-magnitude diagram (plotting the rest-frame optical colours against the stellar mass) in assessing host properties, and find a significant correlation between rest-frame colour (without any correction for AGN contribution or dust extinction) and sSFR excess relative to the ``main sequence'' at a given redshift. This means that the most ``starbursty'' objects have the bluest rest-frame colours.

Abstract Copyright:

Journal keyword(s): galaxies: active - galaxies: Seyfert - galaxies: statistics - galaxies: star formation - X-rays: galaxies - infrared: galaxies

Simbad objects: 4

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Number of rows : 4

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2021
#notes
1 NAME Chandra Deep Field-South reg 03 32 28.0 -27 48 30           ~ 1857 1
2 NAME GOODS Southern Field reg 03 32 28.0 -27 48 30           ~ 1107 1
3 2MASX J04523006-2953353 Sy1 04 52 30.0811 -29 53 35.226 15.07 17.39 15.35 16.06   ~ 119 0
4 NAME Chandra Deep Field-North reg 12 36.8 +62 13           ~ 621 0

    Equat.    Gal    SGal    Ecl

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