The BUFFALO HST Survey

Charles L. Steinhardt; Mathilde Jauzac; Ana Acebron; Hakim Atek; Peter Capak; Iary Davidzon; Dominique Eckert; David Harvey; Anton M. Koekemoer; Claudia D.P. Lagos; Guillaume Mahler; Mireia Montes; Anna Niemiec; Mario Nonino; P. A. Oesch; Johan Richard; Steven A. Rodney; Matthieu Schaller; Keren Sharon; Louis Gregory Strolger; Joseph Allingham; Adam Amara; Yannick Bahé; Céline Bœhm; Sownak Bose; Rychard J. Bouwens; Larry D. Bradley; Gabriel Brammer; Tom Broadhurst; Rodrigo Ca&ntilde;as; Renyue Cen; Benjamin Clément; Douglas Clowe; Dan Coe; Thomas Connor; Behnam Darvish; Jose M. Diego; Harald Ebeling; A. C. Edge; Eiichi Egami; Stefano Ettori; Andreas L. Faisst; Brenda Frye; Lukas J. Furtak; C. Gómez-Guijarro; J. D. Remolina González; Anthony Gonzalez; Or Graur; Daniel Gruen; David Harvey; Hagan Hensley; Beryl Hovis-Afflerbach; Pascale Jablonka; Saurabh W. Jha; Eric Jullo; Jean Paul Kneib; Vasily Kokorev; David J. Lagattuta; Marceau Limousin; Anja Von Der Linden; Nora B. Linzer; Adrian Lopez; Georgios E. Magdis; Richard Massey; Daniel C. Masters; Matteo Maturi; Curtis McCully; Sean L. McGee; Massimo Meneghetti; Bahram Mobasher; Leonidas A. Moustakas; Eric J. Murphy; Priyamvada Natarajan; Mark Neyrinck; Kyle O'Connor; Masamune Oguri; Amanda Pagul; Jason Rhodes; R. Michael Rich; Andrew Robertson; Mauro Sereno; Huanyuan Shan; Graham P. Smith; Albert Sneppen; Gordon K. Squires; Sut Ieng Tam; Céline Tchernin; Sune Toft; Keiichi Umetsu; John R. Weaver; R. J. Van Weeren; Liliya L.R. Williams; Tom J. Wilson; Lin Yan; Adi Zitrin

doi:10.3847/1538-4365/ab75ed

The BUFFALO HST Survey

Charles L. Steinhardt, Mathilde Jauzac, Ana Acebron, Hakim Atek, Peter Capak, Iary Davidzon, Dominique Eckert, David Harvey, Anton M. Koekemoer, Claudia D.P. Lagos, Guillaume Mahler, Mireia Montes, Anna Niemiec, Mario Nonino, P. A. Oesch, Johan Richard, Steven A. Rodney, Matthieu Schaller, Keren Sharon, Louis Gregory StrolgerJoseph Allingham, Adam Amara, Yannick Bahé, Céline Bœhm, Sownak Bose, Rychard J. Bouwens, Larry D. Bradley, Gabriel Brammer, Tom Broadhurst, Rodrigo Cañas, Renyue Cen, Benjamin Clément, Douglas Clowe, Dan Coe, Thomas Connor, Behnam Darvish, Jose M. Diego, Harald Ebeling, A. C. Edge, Eiichi Egami, Stefano Ettori, Andreas L. Faisst, Brenda Frye, Lukas J. Furtak, C. Gómez-Guijarro, J. D. Remolina González, Anthony Gonzalez, Or Graur, Daniel Gruen, David Harvey, Hagan Hensley, Beryl Hovis-Afflerbach, Pascale Jablonka, Saurabh W. Jha, Eric Jullo, Jean Paul Kneib, Vasily Kokorev, David J. Lagattuta, Marceau Limousin, Anja Von Der Linden, Nora B. Linzer, Adrian Lopez, Georgios E. Magdis, Richard Massey, Daniel C. Masters, Matteo Maturi, Curtis McCully, Sean L. McGee, Massimo Meneghetti, Bahram Mobasher, Leonidas A. Moustakas, Eric J. Murphy, Priyamvada Natarajan, Mark Neyrinck, Kyle O'Connor, Masamune Oguri, Amanda Pagul, Jason Rhodes, R. Michael Rich, Andrew Robertson, Mauro Sereno, Huanyuan Shan, Graham P. Smith, Albert Sneppen, Gordon K. Squires, Sut Ieng Tam, Céline Tchernin, Sune Toft, Keiichi Umetsu, John R. Weaver, R. J. Van Weeren, Liliya L.R. Williams, Tom J. Wilson, Lin Yan, Adi Zitrin

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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.

Original language	English (US)
Article number	64
Journal	Astrophysical Journal, Supplement Series
Volume	247
Issue number	2
DOIs	https://doi.org/10.3847/1538-4365/ab75ed
State	Published - Apr 2020
Externally published	Yes

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© 2020. The American Astronomical Society. All rights reserved..

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Steinhardt, C. L., Jauzac, M., Acebron, A., Atek, H., Capak, P., Davidzon, I., Eckert, D., Harvey, D., Koekemoer, A. M., Lagos, C. D. P., Mahler, G., Montes, M., Niemiec, A., Nonino, M., Oesch, P. A., Richard, J., Rodney, S. A., Schaller, M., Sharon, K., ... Zitrin, A. (2020). The BUFFALO HST Survey. Astrophysical Journal, Supplement Series, 247(2), Article 64. https://doi.org/10.3847/1538-4365/ab75ed

Steinhardt, CL, Jauzac, M, Acebron, A, Atek, H, Capak, P, Davidzon, I, Eckert, D, Harvey, D, Koekemoer, AM, Lagos, CDP, Mahler, G, Montes, M, Niemiec, A, Nonino, M, Oesch, PA, Richard, J, Rodney, SA, Schaller, M, Sharon, K, Strolger, LG, Allingham, J, Amara, A, Bahé, Y, Bœhm, C, Bose, S, Bouwens, RJ, Bradley, LD, Brammer, G, Broadhurst, T, Cañas, R, Cen, R, Clément, B, Clowe, D, Coe, D, Connor, T, Darvish, B, Diego, JM, Ebeling, H, Edge, AC, Egami, E, Ettori, S, Faisst, AL, Frye, B, Furtak, LJ, Gómez-Guijarro, C, Remolina González, JD, Gonzalez, A, Graur, O, Gruen, D, Harvey, D, Hensley, H, Hovis-Afflerbach, B, Jablonka, P, Jha, SW, Jullo, E, Kneib, JP, Kokorev, V, Lagattuta, DJ, Limousin, M, Von Der Linden, A, Linzer, NB, Lopez, A, Magdis, GE, Massey, R, Masters, DC, Maturi, M, McCully, C, McGee, SL, Meneghetti, M, Mobasher, B, Moustakas, LA, Murphy, EJ, Natarajan, P, Neyrinck, M, O'Connor, K, Oguri, M, Pagul, A, Rhodes, J, Rich, RM, Robertson, A, Sereno, M, Shan, H, Smith, GP, Sneppen, A, Squires, GK, Tam, SI, Tchernin, C, Toft, S, Umetsu, K, Weaver, JR, Van Weeren, RJ, Williams, LLR, Wilson, TJ, Yan, L & Zitrin, A 2020, 'The BUFFALO HST Survey', Astrophysical Journal, Supplement Series, vol. 247, no. 2, 64. https://doi.org/10.3847/1538-4365/ab75ed

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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.",

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doi = "10.3847/1538-4365/ab75ed",

language = "English (US)",

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T1 - The BUFFALO HST Survey

AU - Steinhardt, Charles L.

AU - Jauzac, Mathilde

AU - Acebron, Ana

AU - Atek, Hakim

AU - Capak, Peter

AU - Davidzon, Iary

AU - Eckert, Dominique

AU - Harvey, David

AU - Koekemoer, Anton M.

AU - Lagos, Claudia D.P.

AU - Mahler, Guillaume

AU - Montes, Mireia

AU - Niemiec, Anna

AU - Nonino, Mario

AU - Oesch, P. A.

AU - Richard, Johan

AU - Rodney, Steven A.

AU - Schaller, Matthieu

AU - Sharon, Keren

AU - Strolger, Louis Gregory

AU - Allingham, Joseph

AU - Amara, Adam

AU - Bahé, Yannick

AU - Bœhm, Céline

AU - Bose, Sownak

AU - Bouwens, Rychard J.

AU - Bradley, Larry D.

AU - Brammer, Gabriel

AU - Broadhurst, Tom

AU - Cañas, Rodrigo

AU - Cen, Renyue

AU - Clément, Benjamin

AU - Clowe, Douglas

AU - Coe, Dan

AU - Connor, Thomas

AU - Darvish, Behnam

AU - Diego, Jose M.

AU - Ebeling, Harald

AU - Edge, A. C.

AU - Egami, Eiichi

AU - Ettori, Stefano

AU - Faisst, Andreas L.

AU - Frye, Brenda

AU - Furtak, Lukas J.

AU - Gómez-Guijarro, C.

AU - Remolina González, J. D.

AU - Gonzalez, Anthony

AU - Graur, Or

AU - Gruen, Daniel

AU - Harvey, David

AU - Hensley, Hagan

AU - Hovis-Afflerbach, Beryl

AU - Jablonka, Pascale

AU - Jha, Saurabh W.

AU - Jullo, Eric

AU - Kneib, Jean Paul

AU - Kokorev, Vasily

AU - Lagattuta, David J.

AU - Limousin, Marceau

AU - Von Der Linden, Anja

AU - Linzer, Nora B.

AU - Lopez, Adrian

AU - Magdis, Georgios E.

AU - Massey, Richard

AU - Masters, Daniel C.

AU - Maturi, Matteo

AU - McCully, Curtis

AU - McGee, Sean L.

AU - Meneghetti, Massimo

AU - Mobasher, Bahram

AU - Moustakas, Leonidas A.

AU - Murphy, Eric J.

AU - Natarajan, Priyamvada

AU - Neyrinck, Mark

AU - O'Connor, Kyle

AU - Oguri, Masamune

AU - Pagul, Amanda

AU - Rhodes, Jason

AU - Rich, R. Michael

AU - Robertson, Andrew

AU - Sereno, Mauro

AU - Shan, Huanyuan

AU - Smith, Graham P.

AU - Sneppen, Albert

AU - Squires, Gordon K.

AU - Tam, Sut Ieng

AU - Tchernin, Céline

AU - Toft, Sune

AU - Umetsu, Keiichi

AU - Weaver, John R.

AU - Van Weeren, R. J.

AU - Williams, Liliya L.R.

AU - Wilson, Tom J.

AU - Yan, Lin

AU - Zitrin, Adi

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N2 - 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.

AB - 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.

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The BUFFALO HST Survey

Abstract

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