The BUFFALO HST Survey

被引：78

作者：

Steinhardt, Charles L. ^{[1
,2
]}

Jauzac, Mathilde ^{[3
,4
,5
]}

Acebron, Ana ^{[6
]}

Atek, Hakim ^{[7
]}

Capak, Peter ^{[1
,8
]}

Davidzon, Iary ^{[1
,2
]}

Eckert, Dominique ^{[9
]}

Harvey, David ^{[10
]}

Koekemoer, Anton M. ^{[11
]}

Lagos, Claudia D. P. ^{[1
,12
,13
]}

Mahler, Guillaume ^{[14
]}

Montes, Mireia ^{[15
]}

Niemiec, Anna ^{[14
]}

Nonino, Mario ^{[16
]}

Oesch, P. A. ^{[17
,18
]}

Richard, Johan ^{[19
]}

Rodney, Steven A. ^{[20
]}

Schaller, Matthieu ^{[21
]}

Sharon, Keren ^{[14
]}

Strolger, Louis-Gregory ^{[11
,22
]}

Allingham, Joseph ^{[23
]}

Amara, Adam ^{[24
]}

Bahe, Yannick ^{[21
]}

Boehm, Celine ^{[25
]}

Bose, Sownak ^{[26
]}

Bouwens, Rychard J. ^{[21
]}

Bradley, Larry D. ^{[11
]}

Brammer, Gabriel ^{[1
,2
]}

Broadhurst, Tom ^{[27
,28
,80
]}

Canas, Rodrigo ^{[12
,13
]}

Cen, Renyue ^{[29
]}

Clement, Benjamin ^{[30
]}

Clowe, Douglas ^{[31
]}

Coe, Dan ^{[11
]}

Connor, Thomas ^{[32
,33
]}

Darvish, Behnam ^{[34
]}

Diego, Jose M. ^{[35
]}

Ebeling, Harald ^{[36
]}

Edge, A. C. ^{[3
]}

Egami, Eiichi ^{[37
]}

Ettori, Stefano ^{[38
,39
]}

Faisst, Andreas L. ^{[8
]}

Frye, Brenda ^{[40
]}

Furtak, Lukas J. ^{[41
]}

Gomez-Guijarro, C. ^{[42
]}

Gonzalez, J. D. Remolina ^{[14
]}

Gonzalez, Anthony ^{[43
]}

Graur, Or ^{[26
,44
]}

Gruen, Daniel ^{[45
,46
]}

Hensley, Hagan ^{[1
,47
]}

机构：

[1] Cosm Dawn Ctr DAWN, Copenhagen, Denmark

[2] Univ Copenhagen, Niels Bohr Inst, Lyngbyvej 2, DK-2100 Copenhagen O, Denmark

[3] Univ Durham, Ctr Extragalact Astron, South Rd, Durham DH1 3LE, England

[4] Univ Durham, Inst Computat Cosmol, South Rd, Durham DH1 3LE, England

[5] Univ KwaZulu Natal, Sch Math Sci, Astrophys & Cosmol Res Unit, ZA-4041 Durban, South Africa

[6] Ben Gurion Univ Negev, Phys Dept, POB 653, IL-8410501 Beer Sheva, Israel

[7] Sorbonne Univ, Inst Astrophys Paris, CNRS UMR7095, 98bis Blvd Arago, F-75014 Paris, France

[8] CALTECH, IPAC, 1200 E Calif Blvd, Pasadena, CA 91125 USA

[9] Univ Geneva, Ch Ecogia 16, CH-1290 Versoix, Switzerland

[10] Leiden Univ, Lorentz Inst, Niels Bohrweg 2, NL-2333 CA Leiden, Netherlands

[11] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA

[12] Univ Western Australia, Int Ctr Radio Astron Res, 35 Stirling Hwy, Crawley, WA 6009, Australia

[13] Arc Ctr Excellence All Sky Astrophys 3 Dimens, ASTRO 3D, Perth, WA, Australia

[14] Univ Michigan, Dept Astron, 1085 S Univ Ave, Ann Arbor, MI 48109 USA

[15] Univ New South Wales, Sch Phys, Sydney, NSW 2052, Australia

[16] INAF Trieste Astron Observ, Trieste, Italy

[17] Univ Geneva, Dept Astron, 51 Ch Maillettes, CH-1290 Versoix, Switzerland

[18] Cosm Dawn Ctr DAWN, Int Associate, Zurich, Switzerland

[19] Univ Lyon, Univ Lyon1, Ctr Rech Astrophys Lyon UMR5574, CNRS, F-69230 St Genis Laval, France

[20] Univ South Carolina, Dept Phys & Astron, Columbia, SC 29208 USA

[21] Leiden Univ, Leiden Observ, POB 9513, NL-2300 RA Leiden, Netherlands

[22] Johns Hopkins Univ, Baltimore, MD 21218 USA

[23] Univ Sydney, Sch Phys, Sydney Inst Astron, A28, Sydney, NSW 2006, Australia

[24] Univ Portsmouth, Inst Cosmol & Gravitat, Dennis Sciama Bldg, Portsmouth PO1 3FX, Hants, England

[25] Univ Sydney, Sch Phys, Sydney, NSW 2006, Australia

[26] Ctr Astrophys Harvard & Smithsonian, 60 Garden St, Cambridge, MA 02138 USA

[27] Univ Basque Country, Dept Phys, Leioa, Spain

[28] Donostia Int Phys Ctr, San Sebastian, Spain

[29] Dept Astrophys Sci, 4 Ivy Lane, Princeton, NJ 08544 USA

[30] EPFL, Observ Sauverny, Lab Astrophys, Inst Phys, CH-1290 Versoix, Switzerland

[31] Ohio Univ, Dept Phys & Astron, Clippinger Labs 251B, Athens, OH 45701 USA

[32] CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA

[33] Observ Carnegie Inst Sci, 813 Santa Barbara St, Pasadena, CA 91101 USA

[34] CALTECH, Cahill Ctr Astrophys, 1216 E Calif Blvd, Pasadena, CA 91125 USA

[35] Inst Fis Cantabria CSIC UC, Edificio Juan Jorda Avda Los Castros S-N, E-39005 Santander, Spain

[36] Univ Hawaii, Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA

[37] Univ Arizona, Steward Observ, 933 N Cherry Ave, Tucson, AZ 85721 USA

[38] Osservatorio Astrofis & Sci Spazio, INAF, Via Pietro Gobetti 93-3, I-40129 Bologna, Italy

[39] INFN, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy

[40] Univ Arizona, Dept Astron, Steward Observ, 933 N Cherry Ave, Tucson, AZ 85721 USA

[41] Sorbonne Univ, Inst Astrophys Paris, CNRS UMR 7095, 98 Bis Bd Arago, F-75014 Paris, France

[42] CEA DSM CNRS Univ Paris Diderot, Irfu Serv Astrophys, Lab AIM Paris Saclay, Orme Merisiers, F-91191 Gif Sur Yvette, France

[43] Univ Florida, Dept Astron, 211 Bryant Space Ctr, Gainesville, FL 32611 USA

[44] Amer Museum Nat Hist, Dept Astrophys, New York, NY 10024 USA

[45] Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, POB 2450, Stanford, CA 94305 USA

[46] Stanford Univ, Dept Phys, 382 Via Pueblo Mall, Stanford, CA 94305 USA

[47] CALTECH, 1200 E Calif Blvd, Pasadena, CA 91125 USA

[48] CALTECH, Div Phys Math & Astron, Pasadena, CA 91125 USA

[49] EPFL, Inst Phys, Lab Astrophys, CH-1290 Observatoire, Versoix, Switzerland

[50] Univ PSL, Observ Paris, CNRS, GEPI, Pl Jules Janssen, F-92190 Meudon, France

来源：

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES | 2020年 / 247卷 / 02期

基金：

英国科学技术设施理事会; 美国国家科学基金会; 新加坡国家研究基金会; 欧盟地平线“2020”;

关键词：

Hubble Space Telescope; Galaxy clusters; Galaxy evolution; Gravitational lensing; Catalogs; Supernovae; High-redshift galaxies; HUBBLE-FRONTIER-FIELDS; SPECTRAL ENERGY-DISTRIBUTIONS; STRONG-LENSING ANALYSIS; MASSIVE GALAXY CLUSTERS; DARK-MATTER; STAR-FORMATION; INTRACLUSTER LIGHT; MULTIPLE IMAGES; COSMOLOGICAL SIMULATIONS; WEAK;

D O I：

10.3847/1538-4365/ab75ed

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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.

引用

页数：20

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