FIREWORKS U38-to-24 micron photometry of the GOODS-CDFS: multi-wavelength catalog and total IR properties of distant Ks-selected galaxies
FIREWORKS U38-to-24 micron photometry of the GOODS-CDFS: multi-wavelength catalog and total IR properties of distant Ks-selected galaxies
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GOODS-CDFS 的 FIREWORKS U38 至 24 微米光度测定：遥远 Ks 选择星系的多波长目录和总红外特性
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发表时间：
2008
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通讯作者：
P. V. Dokkum
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作者：
S. Wuyts;I. Labbé;N. F. Schreiber;M. Franx;G. Rudnick;G. Brammer;P. V. Dokkum
我们给出了K S选择的钱德拉深场南方(CDFS)的目录，称为焰火，包含U 38，B 435，B，V，V606，R，I 775，I，z850，J，H，K S，[3.6微米]，[4.5微米]，[5.8微米]，[8.0微米]和MIPS[24微米]频段。该成像具有典型的K tot S，AB极限为24.3mag(5σ)，覆盖范围在所有波段均超过113arcmin2，在除H以外的所有波段均为138arcmin2。我们将我们的星表与Giacconi等人的1ms X射线星表进行了交叉关联。(2002)和迄今为止所有可用的光谱红移。我们fi和解释系统的差异，通过与‘z850+K S’精选商品-音乐目录，涵盖了∼的90%的fi领域的比较。我们利用U38到24微米的光度法来确定哪个K S选择的星系为1。2.5具有最亮的总红外光度，以及哪些星系对综合总红外辐射的贡献最大。这两个问题的答案都是红色星系在红外区占主导地位。无论颜色在静止帧中是DefiNed，还是从UV、光学或光学到NIR，都是如此。然而，我们做了fi，然而，在其余框架光学中最红的星系中，有一群源只有很少的中红外发射，这表明它是静止的。
We present a K s -selected catalog, dubbed FIREWORKS, for the Chandra Deep Field South (CDFS) containing photometry in U 38 , B 435 , B , V , V 606 , R , i 775 , I , z 850 , J , H , K s , [3 . 6 µ m], [4 . 5 µ m], [5 . 8 µ m], [8 . 0 µ m], and the MIPS [24 µ m] band. The imaging has a typical K tot s, AB limit of 24.3 mag (5 σ ) and coverage over 113 arcmin 2 in all bands and 138 arcmin 2 in all bands but H . We cross-correlate our catalog with the 1 Ms X-ray catalog by Giacconi et al. (2002) and with all available spectroscopic redshifts to date. We find and explain systematic differences in a comparison with the ’ z 850 + K s ’-selected GOODS-MUSIC catalog that covers ∼ 90% of the field. We exploit the U 38 -to-24 µ m photometry to determine which K s -selected galaxies at 1 . 5 < z < 2 . 5 have the brightest total IR luminosities and which galaxies contribute most to the integrated total IR emission. The answer to both questions is that red galaxies are dominating in the IR. This is true no matter whether color is defined in the rest-frame UV, optical, or optical-to-NIR. We do find however that among the reddest galaxies in the rest-frame optical, there is a population of sources with only little mid-IR emission, suggesting a quiescent nature.