The Hubble Legacy Field GOODS-S Photometric Catalog

被引:92
|
作者
Whitaker, Katherine E. [1 ,2 ,3 ]
Ashas, Mohammad [2 ]
Illingworth, Garth [4 ]
Magee, Daniel [4 ]
Leja, Joel [5 ]
Oesch, Pascal [3 ,6 ]
van Dokkum, Pieter [7 ]
Mowla, Lamiya [7 ]
Bouwens, Rychard [8 ]
Franx, Marijn [8 ]
Holden, Bradford [4 ]
Labbe, Ivo [9 ]
Rafelski, Marc [10 ,11 ]
Teplitz, Harry [12 ]
Gonzalez, Valentino [13 ]
机构
[1] Univ Massachusetts, Dept Astron, Amherst, MA 01003 USA
[2] Univ Connecticut, Dept Phys, Storrs, CT 06269 USA
[3] Cosm Dawn Ctr DAWN, Copenhagen, Denmark
[4] Univ Calif Santa Cruz, Lick Observ, UCO, Santa Cruz, CA 95064 USA
[5] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
[6] Univ Geneva, Dept Astron, Ch Maillettes 51, CH-1290 Versoix, Switzerland
[7] Yale Univ, Dept Astron, New Haven, CT 06511 USA
[8] Leiden Univ, Leiden Observ, NL-2300 RA Leiden, Netherlands
[9] Swinburne Univ Technol, Hawthorn, Vic 3122, Australia
[10] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA
[11] Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA
[12] CALTECH, Infrared Proc & Anal Ctr, MS 100-22, Pasadena, CA 91125 USA
[13] Univ Chile, Dept Astron, Casilla 36-D, Santiago 7591245, Chile
来源
基金
新加坡国家研究基金会;
关键词
catalogs; galaxies: evolution; galaxies: general; methods: data analysis; techniques: photometric; GALAXIES; EVOLUTION;
D O I
10.3847/1538-4365/ab3853
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
This manuscript describes the public release of the Hubble Legacy Fields (HLF) project photometric catalog for the extended GOODS-South region from the Hubble Space Telescope (HST) archival program AR-13252. The analysis is based on the version 2.0 HLF data release that now includes all ultraviolet (UV) imaging, combining three major UV surveys. The HLF data combines over a decade worth of 7475 exposures taken in 2635 orbits totaling 6.3 Ms with the HST Advanced Camera for Surveys Wide Field Channel (ACS/WFC) and the Wide Field Camera 3 (WFC3) UVIS/IR Channels in the greater GOODS-S extragalactic field, covering all major observational efforts (e.g., GOODS, GEMS, CANDELS, ERS, UVUDF, and many other programs; see Illingworth et al.). The HLF GOODS-S catalogs include photometry in 13 bandpasses from the UV (WFC3/UVIS F225W, F275W, and F336W filters), optical (ACS/WFC F435W, F606W, F775W, F814W and F850LP filters), to near-infrared (WFC3/IR F098M, F105W, F125W, F140W and F160W filters). Such a data set makes it possible to construct the spectral energy distributions (SEDs) of objects over a wide wavelength range from high-resolution mosaics that are largely contiguous. Here, we describe a photometric analysis of 186,474 objects in the HST imaging at wavelengths 0.2-1.6 mu m. We detect objects from an ultra-deep image combining the PSF-homogenized and noise-equalized F850LP, F125W, F140W, and F160W images, including Gaia astrometric corrections. SEDs were determined by carefully taking the effects of the point-spread function in each observation into account. All of the data presented herein are available through the HLF website (https://archive.stsci.edu/prepds/hlf/).
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收藏
页数:19
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