ALMA Lensing Cluster Survey: Hubble Space Telescope and Spitzer Photometry of 33 Lensed Fields Built with CHArGE
Artikel i vetenskaplig tidskrift, 2022
We present a set of multiwavelength mosaics and photometric catalogs in the Atacama Large Millimeter/ submillimeter Array (ALMA) lensing cluster survey fields. The catalogs were built by the reprocessing of archival data from the Complete Hubble Archive for Galaxy Evolution compilation, taken by the Hubble Space Telescope (HST) in the Reionization Lensing Cluster Survey, Cluster Lensing And Supernova survey with Hubble, and Hubble Frontier Fields. Additionally, we have reconstructed the Spitzer Infrared Array Camera 3.6 and 4.5 μm mosaics, by utilizing all the available archival IPAC Infrared Science Archive/Spitzer Heritage Archive exposures. To alleviate the effect of blending in such a crowded region, we have modeled the Spitzer photometry by convolving the HST detection image with the Spitzer point-spread function using the novel GOLFIR software. The final catalogs contain 218,000 sources, covering a combined area of 690 arcmin2, a factor of ∼2 improvement over the currently existing photometry. A large number of detected sources is a result of reprocessing of all available and sometimes deeper exposures, in conjunction with a combined optical–near-IR detection strategy. These data will serve as an important tool in aiding the search of the submillimeter galaxies in future ALMA surveys, as well as follow-ups of the HST dark and high-z sources with JWST. Coupled with the available HST photometry, the addition of the 3.6 and 4.5 μm bands will allow us to place a better constraint on the photometric redshifts and stellar masses of these objects, thus giving us an opportunity to identify high-redshift candidates for spectroscopic follow-ups and to answer the important questions regarding the Epoch of Reionization and formation of the first galaxies. The mosaics, photometric catalogs, and the best-fit physical properties are publicly available at https:// github.com/dawn-cph/alcs-clusters.
Författare
V. Kokorev
Cosmic Dawn Center (DAWN)
Niels Bohr Institute
G. Brammer
Niels Bohr Institute
Cosmic Dawn Center (DAWN)
S. Fujimoto
Cosmic Dawn Center (DAWN)
Niels Bohr Institute
K. Kohno
Research Center for the Early Universe
University of Tokyo
Georgios E. Magdis
Cosmic Dawn Center (DAWN)
Niels Bohr Institute
Danmarks Tekniske Universitet (DTU)
F. Valentino
Niels Bohr Institute
Cosmic Dawn Center (DAWN)
Sune Toft
Danmarks Tekniske Universitet (DTU)
Cosmic Dawn Center (DAWN)
Niels Bohr Institute
Pascal A. Oesch
Cosmic Dawn Center (DAWN)
Université de Genève
I. Davidzon
Cosmic Dawn Center (DAWN)
Niels Bohr Institute
F. E. Bauer
Instituto Milenio de Astrofísica
Pontificia Universidad Catolica de Chile
D. Coe
Space Telescope Science Institute (STScI)
E. Egami
University of Arizona
M. Oguri
Research Center for the Early Universe
University of Tokyo
Chiba University
Masami Ouchi
National Astronomical Observatory of Japan
University of Tokyo
M. Postman
Space Telescope Science Institute (STScI)
J. Richard
CRAL Le Centre de Recherche Astronomique de Lyon
Jean Baptiste Jolly
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
Max-Planck-Gesellschaft
Kirsten Knudsen
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
Fengwu Sun
University of Arizona
J. R. Weaver
University of Massachusetts
Cosmic Dawn Center (DAWN)
Y. Ao
University of Science and Technology of China
Chinese Academy of Sciences
A. J. Baker
Rutgers University
University of the Western Cape
L. Bradley
Space Telescope Science Institute (STScI)
Karina I. Caputi
Rijksuniversiteit Groningen
M. Dessauges-Zavadsky
Université de Genève
D. Espada
Universidad de Granada
B. Hatsukade
University of Tokyo
Anton M. Koekemoer
Space Telescope Science Institute (STScI)
A. M. Muñoz Arancibia
Instituto Milenio de Astrofísica
Universidad de Chile (UCH)
K. Shimasaku
University of Tokyo
Research Center for the Early Universe
H. Umehata
Nagoya University
T. Wang
Nanjing University
Wei Hao Wang
Academia Sinica
Astrophysical Journal, Supplement Series
0067-0049 (ISSN) 1538-4365 (eISSN)
Vol. 263 2 38Ämneskategorier
Annan data- och informationsvetenskap
Astronomi, astrofysik och kosmologi
Datorseende och robotik (autonoma system)
DOI
10.3847/1538-4365/ac9909