COSMOS-Web: an overview of the JWST Cosmic Origins Survey

Caitlin M. Casey; Jeyhan S. Kartaltepe; Nicole E. Drakos; Maximilien Franco; Santosh Harish; Louise Paquereau; Olivier Ilbert; Caitlin Rose; Isabella G. Cox; James W. Nightingale; Brant E. Robertson; John D. Silverman; Anton M. Koekemoer; Richard Massey; Henry Joy McCracken; Jason Rhodes; Hollis B. Akins; Aristeidis Amvrosiadis; Rafael C. Arango-Toro; Micaela B. Bagley; Angela Bongiorno; Peter L. Capak; Jaclyn B. Champagne; Nima Chartab; Oscar A. Chavez Ortiz; Katherine Chworowsky; Kevin C. Cooke; Olivia R. Cooper; Behnam Darvish; Xuheng Ding; Andreas L. Faisst; Steven L. Finkelstein; Seiji Fujimoto; Fabrizio Gentile; Steven Gillman; Katriona M. L. Gould; Ghassem Gozaliasl; Christopher C. Hayward; Qiuhan He; Shoubaneh Hemmati; Michaela Hirschmann; Knud Jahnke; Shuowen Jin; Ali Ahmad Khostovan; Vasily Kokorev; Erini Lambrides; Clotilde Laigle; Rebecca L. Larson; Gene C. K. Leung; Daizhong Liu; Tobias Liaudat; Arianna S. Long; Georgios Magdis; Guillaume Mahler; Vincenzo Mainieri; Sinclaire M. Manning; Claudia Maraston; Crystal L. Martin; Jacqueline E. McCleary; Jed McKinney; Conor J. R. McPartland; Bahram Mobasher; Rohan Pattnaik; Alvio Renzini; R. Michael Rich; Zahra Sattari; Diana Scognamiglio; Nick Scoville; Kartik Sheth; Marko Shuntov; Martin Sparre; Tomoko L. Suzuki; Margherita Talia; Sune Toft; Benny Trakhtenbrot; C. Megan Urry; Francesco Valentino; Brittany N. Vanderhoof; Eleni Vardoulaki; John R. Weaver; Katherine E. Whitaker; Stephen M. Wilkins; Lilan Yang; Jorge A. Zavala

COSMOS-Web: an overview of the JWST Cosmic Origins Survey

Caitlin M. Casey, Jeyhan S. Kartaltepe, Nicole E. Drakos, Maximilien Franco, Santosh Harish, Louise Paquereau, Olivier Ilbert, Caitlin Rose, Isabella G. Cox, James W. Nightingale, Brant E. Robertson, John D. Silverman, Anton M. Koekemoer, Richard Massey, Henry Joy McCracken, Jason Rhodes, Hollis B. Akins, Aristeidis Amvrosiadis, Rafael C. Arango-Toro, Micaela B. BagleyAngela Bongiorno, Peter L. Capak, Jaclyn B. Champagne, Nima Chartab, Oscar A. Chavez Ortiz, Katherine Chworowsky, Kevin C. Cooke, Olivia R. Cooper, Behnam Darvish, Xuheng Ding, Andreas L. Faisst, Steven L. Finkelstein, Seiji Fujimoto, Fabrizio Gentile, Steven Gillman, Katriona M. L. Gould, Ghassem Gozaliasl, Christopher C. Hayward, Qiuhan He, Shoubaneh Hemmati, Michaela Hirschmann, Knud Jahnke, Shuowen Jin, Ali Ahmad Khostovan, Vasily Kokorev, Erini Lambrides, Clotilde Laigle, Rebecca L. Larson, Gene C. K. Leung, Daizhong Liu, Tobias Liaudat, Arianna S. Long, Georgios Magdis, Guillaume Mahler, Vincenzo Mainieri, Sinclaire M. Manning, Claudia Maraston, Crystal L. Martin, Jacqueline E. McCleary, Jed McKinney, Conor J. R. McPartland, Bahram Mobasher, Rohan Pattnaik, Alvio Renzini, R. Michael Rich, Zahra Sattari, Diana Scognamiglio, Nick Scoville, Kartik Sheth, Marko Shuntov, Martin Sparre, Tomoko L. Suzuki, Margherita Talia, Sune Toft, Benny Trakhtenbrot, C. Megan Urry, Francesco Valentino, Brittany N. Vanderhoof, Eleni Vardoulaki, John R. Weaver, Katherine E. Whitaker, Stephen M. Wilkins, Lilan Yang, Jorge A. Zavala

Institute of Cosmology & Gravitation

Research output: Contribution to journal › Article › peer-review

Abstract

We present the survey design, implementation, and outlook for COSMOS-Web, a 255 hour treasury program conducted by the James Webb Space Telescope in its first cycle of observations. COSMOS Web is a contiguous 0.54 deg² NIR Camimaging survey in four filters (F115W, F150W, F277W, and F444W) that will reach 5σ point source depths ranging ∼27.5–28.2 magnitudes. In parallel, we will obtain 0.19 deg² of MIRI imaging in one filter (F770W) reaching 5σ point source depths of ∼25.326.0 magnitudes. COSMOS-Web will build on the rich heritage of multiwavelength observations and data products available in the COSMOS field. The design of COSMOS-Web is motivated by three primary science goals: (1) to discover thousands of galaxies in the Epoch of Reionization (6<∼z<∼11) and map reionization’s spatial distribution, environments, and drivers on scales sufficiently large to mitigate cosmic variance, (2) to identify hundreds of rare quiescent galaxies at z > 4 and place constraints on the formation of the Universe’s most massive galaxies (M_*> 10¹⁰M_⊙), and (3) directly measure the evolution of the stellar mass to halo mass relation using weak gravitational lensing out to z∼2.5 and measure its variance with galaxies’ star formation histories and morphologies. In addition, we anticipate COSMOS-Web’s legacy value to reach far beyond these scientific goals, touching many other areas of astrophysics, such as the identification of the first direct collapse black hole candidates, ultracool sub-dwarf stars in the Galactic halo, and possibly the identification of z > 10 pair-instability supernovae. In this paper we provide an overview of the survey’s key measurements, specifications, goals, and prospects for new discovery.

Original language	English
Journal	The Astrophysical Journal
Publication status	Accepted for publication - 8 Mar 2023

Embargoed Document

2211.07865v2
Accepted author manuscript (Post-print), 49 MB
Licence: CC BY-NC-ND
Due to publisher’s copyright restrictions, this document is not freely available to download from this website until: 1/01/50

Cite this

Casey, C. M., Kartaltepe, J. S., Drakos, N. E., Franco, M., Harish, S., Paquereau, L., Ilbert, O., Rose, C., Cox, I. G., Nightingale, J. W., Robertson, B. E., Silverman, J. D., Koekemoer, A. M., Massey, R., McCracken, H. J., Rhodes, J., Akins, H. B., Amvrosiadis, A., Arango-Toro, R. C., ... Zavala, J. A. (Accepted/In press). COSMOS-Web: an overview of the JWST Cosmic Origins Survey. The Astrophysical Journal.

@article{33e0c432647b44799503863171114b0e,

title = "COSMOS-Web: an overview of the JWST Cosmic Origins Survey",

abstract = "We present the survey design, implementation, and outlook for COSMOS-Web, a 255 hour treasury program conducted by the James Webb Space Telescope in its first cycle of observations. COSMOS Web is a contiguous 0.54 deg2 NIR Camimaging survey in four filters (F115W, F150W, F277W, and F444W) that will reach 5σ point source depths ranging ∼27.5–28.2 magnitudes. In parallel, we will obtain 0.19 deg2 of MIRI imaging in one filter (F770W) reaching 5σ point source depths of ∼25.326.0 magnitudes. COSMOS-Web will build on the rich heritage of multiwavelength observations and data products available in the COSMOS field. The design of COSMOS-Web is motivated by three primary science goals: (1) to discover thousands of galaxies in the Epoch of Reionization (6<∼z<∼11) and map reionization{\textquoteright}s spatial distribution, environments, and drivers on scales sufficiently large to mitigate cosmic variance, (2) to identify hundreds of rare quiescent galaxies at z > 4 and place constraints on the formation of the Universe{\textquoteright}s most massive galaxies (M* > 1010 M⊙), and (3) directly measure the evolution of the stellar mass to halo mass relation using weak gravitational lensing out to z∼2.5 and measure its variance with galaxies{\textquoteright} star formation histories and morphologies. In addition, we anticipate COSMOS-Web{\textquoteright}s legacy value to reach far beyond these scientific goals, touching many other areas of astrophysics, such as the identification of the first direct collapse black hole candidates, ultracool sub-dwarf stars in the Galactic halo, and possibly the identification of z > 10 pair-instability supernovae. In this paper we provide an overview of the survey{\textquoteright}s key measurements, specifications, goals, and prospects for new discovery.",

author = "Casey, {Caitlin M.} and Kartaltepe, {Jeyhan S.} and Drakos, {Nicole E.} and Maximilien Franco and Santosh Harish and Louise Paquereau and Olivier Ilbert and Caitlin Rose and Cox, {Isabella G.} and Nightingale, {James W.} and Robertson, {Brant E.} and Silverman, {John D.} and Koekemoer, {Anton M.} and Richard Massey and McCracken, {Henry Joy} and Jason Rhodes and Akins, {Hollis B.} and Aristeidis Amvrosiadis and Arango-Toro, {Rafael C.} and Bagley, {Micaela B.} and Angela Bongiorno and Capak, {Peter L.} and Champagne, {Jaclyn B.} and Nima Chartab and Ortiz, {Oscar A. Chavez} and Katherine Chworowsky and Cooke, {Kevin C.} and Cooper, {Olivia R.} and Behnam Darvish and Xuheng Ding and Faisst, {Andreas L.} and Finkelstein, {Steven L.} and Seiji Fujimoto and Fabrizio Gentile and Steven Gillman and Gould, {Katriona M. L.} and Ghassem Gozaliasl and Hayward, {Christopher C.} and Qiuhan He and Shoubaneh Hemmati and Michaela Hirschmann and Knud Jahnke and Shuowen Jin and Khostovan, {Ali Ahmad} and Vasily Kokorev and Erini Lambrides and Clotilde Laigle and Larson, {Rebecca L.} and Leung, {Gene C. K.} and Daizhong Liu and Tobias Liaudat and Long, {Arianna S.} and Georgios Magdis and Guillaume Mahler and Vincenzo Mainieri and Manning, {Sinclaire M.} and Claudia Maraston and Martin, {Crystal L.} and McCleary, {Jacqueline E.} and Jed McKinney and McPartland, {Conor J. R.} and Bahram Mobasher and Rohan Pattnaik and Alvio Renzini and Rich, {R. Michael} and Zahra Sattari and Diana Scognamiglio and Nick Scoville and Kartik Sheth and Marko Shuntov and Martin Sparre and Suzuki, {Tomoko L.} and Margherita Talia and Sune Toft and Benny Trakhtenbrot and Urry, {C. Megan} and Francesco Valentino and Vanderhoof, {Brittany N.} and Eleni Vardoulaki and Weaver, {John R.} and Whitaker, {Katherine E.} and Wilkins, {Stephen M.} and Lilan Yang and Zavala, {Jorge A.}",

note = "46 pages, 16 figures, ApJ accepted. IOP. 12 month embargo. This Accepted Manuscript is available for reuse under a CC BY-NC-ND licence after the 12 month embargo period provided that all the terms and conditions of the licence are adhered to",

year = "2023",

month = mar,

day = "8",

language = "English",

journal = "The Astrophysical Journal",

issn = "0004-637X",

publisher = "IOP Publishing",

}

Casey, CM, Kartaltepe, JS, Drakos, NE, Franco, M, Harish, S, Paquereau, L, Ilbert, O, Rose, C, Cox, IG, Nightingale, JW, Robertson, BE, Silverman, JD, Koekemoer, AM, Massey, R, McCracken, HJ, Rhodes, J, Akins, HB, Amvrosiadis, A, Arango-Toro, RC, Bagley, MB, Bongiorno, A, Capak, PL, Champagne, JB, Chartab, N, Ortiz, OAC, Chworowsky, K, Cooke, KC, Cooper, OR, Darvish, B, Ding, X, Faisst, AL, Finkelstein, SL, Fujimoto, S, Gentile, F, Gillman, S, Gould, KML, Gozaliasl, G, Hayward, CC, He, Q, Hemmati, S, Hirschmann, M, Jahnke, K, Jin, S, Khostovan, AA, Kokorev, V, Lambrides, E, Laigle, C, Larson, RL, Leung, GCK, Liu, D, Liaudat, T, Long, AS, Magdis, G, Mahler, G, Mainieri, V, Manning, SM, Maraston, C, Martin, CL, McCleary, JE, McKinney, J, McPartland, CJR, Mobasher, B, Pattnaik, R, Renzini, A, Rich, RM, Sattari, Z, Scognamiglio, D, Scoville, N, Sheth, K, Shuntov, M, Sparre, M, Suzuki, TL, Talia, M, Toft, S, Trakhtenbrot, B, Urry, CM, Valentino, F, Vanderhoof, BN, Vardoulaki, E, Weaver, JR, Whitaker, KE, Wilkins, SM, Yang, L & Zavala, JA 2023, 'COSMOS-Web: an overview of the JWST Cosmic Origins Survey', The Astrophysical Journal.

TY - JOUR

T1 - COSMOS-Web

T2 - an overview of the JWST Cosmic Origins Survey

AU - Casey, Caitlin M.

AU - Kartaltepe, Jeyhan S.

AU - Drakos, Nicole E.

AU - Franco, Maximilien

AU - Harish, Santosh

AU - Paquereau, Louise

AU - Ilbert, Olivier

AU - Rose, Caitlin

AU - Cox, Isabella G.

AU - Nightingale, James W.

AU - Robertson, Brant E.

AU - Silverman, John D.

AU - Koekemoer, Anton M.

AU - Massey, Richard

AU - McCracken, Henry Joy

AU - Rhodes, Jason

AU - Akins, Hollis B.

AU - Amvrosiadis, Aristeidis

AU - Arango-Toro, Rafael C.

AU - Bagley, Micaela B.

AU - Bongiorno, Angela

AU - Capak, Peter L.

AU - Champagne, Jaclyn B.

AU - Chartab, Nima

AU - Ortiz, Oscar A. Chavez

AU - Chworowsky, Katherine

AU - Cooke, Kevin C.

AU - Cooper, Olivia R.

AU - Darvish, Behnam

AU - Ding, Xuheng

AU - Faisst, Andreas L.

AU - Finkelstein, Steven L.

AU - Fujimoto, Seiji

AU - Gentile, Fabrizio

AU - Gillman, Steven

AU - Gould, Katriona M. L.

AU - Gozaliasl, Ghassem

AU - Hayward, Christopher C.

AU - He, Qiuhan

AU - Hemmati, Shoubaneh

AU - Hirschmann, Michaela

AU - Jahnke, Knud

AU - Jin, Shuowen

AU - Khostovan, Ali Ahmad

AU - Kokorev, Vasily

AU - Lambrides, Erini

AU - Laigle, Clotilde

AU - Larson, Rebecca L.

AU - Leung, Gene C. K.

AU - Liu, Daizhong

AU - Liaudat, Tobias

AU - Long, Arianna S.

AU - Magdis, Georgios

AU - Mahler, Guillaume

AU - Mainieri, Vincenzo

AU - Manning, Sinclaire M.

AU - Maraston, Claudia

AU - Martin, Crystal L.

AU - McCleary, Jacqueline E.

AU - McKinney, Jed

AU - McPartland, Conor J. R.

AU - Mobasher, Bahram

AU - Pattnaik, Rohan

AU - Renzini, Alvio

AU - Rich, R. Michael

AU - Sattari, Zahra

AU - Scognamiglio, Diana

AU - Scoville, Nick

AU - Sheth, Kartik

AU - Shuntov, Marko

AU - Sparre, Martin

AU - Suzuki, Tomoko L.

AU - Talia, Margherita

AU - Toft, Sune

AU - Trakhtenbrot, Benny

AU - Urry, C. Megan

AU - Valentino, Francesco

AU - Vanderhoof, Brittany N.

AU - Vardoulaki, Eleni

AU - Weaver, John R.

AU - Whitaker, Katherine E.

AU - Wilkins, Stephen M.

AU - Yang, Lilan

AU - Zavala, Jorge A.

N1 - 46 pages, 16 figures, ApJ accepted. IOP. 12 month embargo. This Accepted Manuscript is available for reuse under a CC BY-NC-ND licence after the 12 month embargo period provided that all the terms and conditions of the licence are adhered to

PY - 2023/3/8

Y1 - 2023/3/8

N2 - We present the survey design, implementation, and outlook for COSMOS-Web, a 255 hour treasury program conducted by the James Webb Space Telescope in its first cycle of observations. COSMOS Web is a contiguous 0.54 deg2 NIR Camimaging survey in four filters (F115W, F150W, F277W, and F444W) that will reach 5σ point source depths ranging ∼27.5–28.2 magnitudes. In parallel, we will obtain 0.19 deg2 of MIRI imaging in one filter (F770W) reaching 5σ point source depths of ∼25.326.0 magnitudes. COSMOS-Web will build on the rich heritage of multiwavelength observations and data products available in the COSMOS field. The design of COSMOS-Web is motivated by three primary science goals: (1) to discover thousands of galaxies in the Epoch of Reionization (6<∼z<∼11) and map reionization’s spatial distribution, environments, and drivers on scales sufficiently large to mitigate cosmic variance, (2) to identify hundreds of rare quiescent galaxies at z > 4 and place constraints on the formation of the Universe’s most massive galaxies (M* > 1010 M⊙), and (3) directly measure the evolution of the stellar mass to halo mass relation using weak gravitational lensing out to z∼2.5 and measure its variance with galaxies’ star formation histories and morphologies. In addition, we anticipate COSMOS-Web’s legacy value to reach far beyond these scientific goals, touching many other areas of astrophysics, such as the identification of the first direct collapse black hole candidates, ultracool sub-dwarf stars in the Galactic halo, and possibly the identification of z > 10 pair-instability supernovae. In this paper we provide an overview of the survey’s key measurements, specifications, goals, and prospects for new discovery.

AB - We present the survey design, implementation, and outlook for COSMOS-Web, a 255 hour treasury program conducted by the James Webb Space Telescope in its first cycle of observations. COSMOS Web is a contiguous 0.54 deg2 NIR Camimaging survey in four filters (F115W, F150W, F277W, and F444W) that will reach 5σ point source depths ranging ∼27.5–28.2 magnitudes. In parallel, we will obtain 0.19 deg2 of MIRI imaging in one filter (F770W) reaching 5σ point source depths of ∼25.326.0 magnitudes. COSMOS-Web will build on the rich heritage of multiwavelength observations and data products available in the COSMOS field. The design of COSMOS-Web is motivated by three primary science goals: (1) to discover thousands of galaxies in the Epoch of Reionization (6<∼z<∼11) and map reionization’s spatial distribution, environments, and drivers on scales sufficiently large to mitigate cosmic variance, (2) to identify hundreds of rare quiescent galaxies at z > 4 and place constraints on the formation of the Universe’s most massive galaxies (M* > 1010 M⊙), and (3) directly measure the evolution of the stellar mass to halo mass relation using weak gravitational lensing out to z∼2.5 and measure its variance with galaxies’ star formation histories and morphologies. In addition, we anticipate COSMOS-Web’s legacy value to reach far beyond these scientific goals, touching many other areas of astrophysics, such as the identification of the first direct collapse black hole candidates, ultracool sub-dwarf stars in the Galactic halo, and possibly the identification of z > 10 pair-instability supernovae. In this paper we provide an overview of the survey’s key measurements, specifications, goals, and prospects for new discovery.

M3 - Article

SN - 0004-637X

JO - The Astrophysical Journal

JF - The Astrophysical Journal

ER -