The BUFFALO HST Survey
The Astrophysical Journal Supplement Series, vol. 247, pp. 64
Abstract
Abstract The Beyond Ultra-deep Frontier Fields and Legacy Observations (BUFFALO) is a 101 orbit + 101 parallel Cycle 25 Hubble Space Telescope ( HST ) Treasury program taking data from 2018 to 2020. BUFFALO will expand existing coverage of the Hubble Frontier Fields (HFF) in Wide Field Camera 3/IR F105W, F125W, and F160W and Advanced Camera for Surveys/WFC F606W and F814W around each of the six HFF clusters and flanking fields. This additional area has not been observed by HST but is already covered by deep multiwavelength data sets, including Spitzer and Chandra . As with the original HFF program, BUFFALO is designed to take advantage of gravitational lensing from massive clusters to simultaneously find high-redshift galaxies that would otherwise lie below HST detection limits and model foreground clusters to study the properties of dark matter and galaxy assembly. The expanded area will provide the first opportunity to study both cosmic variance at high redshift and galaxy assembly in the outskirts of the large HFF clusters. Five additional orbits are reserved for transient follow-up. BUFFALO data including mosaics, value-added catalogs, and cluster mass distribution models will be released via MAST on a regular basis as the observations and analysis are completed for the six individual clusters.
Authors 12
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Charles Louis Steinhardt corresponding
Affiliation as printed
Cosmic Dawn Center (DAWN), Denmark; steinhardt@nbi.ku.dk
Niels Bohr Institute, University of Copenhagen, Lyngbyvej 2, Copenhagen Ø DK-2100, Denmark
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Durham University · University of KwaZulu-Natal
Affiliation as printed
Astrophysics and Cosmology Research Unit, School of Mathematical Sciences, University of KwaZulu-Natal, Durban 4041, South Africa
Centre for Extragalactic Astronomy, Durham University, South Road, Durham DH1 3LE, UK
Institute for Computational Cosmology, Durham University, South Road, Durham DH1 3LE, UK
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Centre National de la Recherche Scientifique · Institut d'Astrophysique de Paris · Sorbonne Université
Affiliation as printed
Institut d’astrophysique de Paris, CNRS UMR7095, Sorbonne Université, 98bis Boulevard Arago, F-75014 Paris, France
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California Institute of Technology · Infrared Processing and Analysis Center
Affiliation as printed
Cosmic Dawn Center (DAWN), Denmark; steinhardt@nbi.ku.dk
IPAC, California Institute of Technology, 1200 E. California Blvd., Pasadena, CA 91125, USA
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Space Telescope Science Institute
Affiliation as printed
Space Telescope Science Institute, 3700 San Martin Dr., Baltimore, MD 21218, USA
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Affiliation as printed
Department of Astronomy, University of Michigan, 1085 S. University Ave., Ann Arbor, MI 48109, USA
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Centre National de la Recherche Scientifique · Centre de Recherche Astrophysique de Lyon
Affiliation as printed
Univ Lyon, Univ Lyon1, Ens de Lyon, CNRS, Centre de Recherche Astrophysique de Lyon UMR5574, F-69230, Saint-Genis-Laval, France
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Affiliation as printed
Department of Astronomy, University of Michigan, 1085 S. University Ave., Ann Arbor, MI 48109, USA
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University of the Basque Country · Donostia International Physics Center
Affiliation as printed
Department of Physics, University of the Basque Country, Spain
Donostia International Physics Center, San Sebastian, Spain
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Centre National de la Recherche Scientifique · Institut d'Astrophysique de Paris · Sorbonne Université
Affiliation as printed
Institut d’astrophysique de Paris, Sorbonne Université, CNRS UMR 7095, 98 bis bd Arago, F-75014 Paris, France
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Osservatorio di Astrofisica e Scienza dello Spazio · National Institute for Astrophysics
Affiliation as printed
INAF–Osservatorio di Astrofisica e Scienza dello Spazio, Via Gobetti 93/3, I-40129 Bologna, Italy
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Ikerbasque · University of the Basque Country
Affiliation as printed
Department of Theoretical Physics, University of the Basque Country UPV/EHU, E-48080 Bilbao, Spain
Ikerbasque, Basque Foundation for Science, E-48011 Bilbao, Spain
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