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Euclid preparation: LXIV. The Cosmic Dawn Survey (DAWN) of the Euclid Deep and Auxiliary Fields

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Euclid preparation: LXIV. The Cosmic Dawn Survey (DAWN) of the Euclid Deep and Auxiliary Fields. / Euclid Collaboration.
In: Astronomy and Astrophysics, Vol. 695, A259, 31.03.2025.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

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Euclid Collaboration. Euclid preparation: LXIV. The Cosmic Dawn Survey (DAWN) of the Euclid Deep and Auxiliary Fields. Astronomy and Astrophysics. 2025 Mar 31;695:A259. Epub 2025 Mar 28. doi: 10.1051/0004-6361/202451849

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Euclid Collaboration. / Euclid preparation : LXIV. The Cosmic Dawn Survey (DAWN) of the Euclid Deep and Auxiliary Fields. In: Astronomy and Astrophysics. 2025 ; Vol. 695.

Bibtex

@article{2282fa8b02864f0bb54a6d8e8c6ac5ce,
title = "Euclid preparation: LXIV. The Cosmic Dawn Survey (DAWN) of the Euclid Deep and Auxiliary Fields",
abstract = "Euclid will provide deep near-infrared (NIR) imaging to ∼26.5 AB magnitude over ∼59 deg2 in its deep and auxiliary fields. The Cosmic DAWN survey combines dedicated and archival UV–NIR observations to provide matched depth multiwavelength imaging of the Euclid deep and auxiliary fields. The DAWN survey will provide consistently measured Euclid NIR-selected photometric catalogues, accurate photometric redshifts, and measurements of galaxy properties to a redshift of z ∼ 10. The DAWN catalogues include Spitzer IRAC data that are critical for stellar mass measurements at z ≳ 2.5 and high-z science. These catalogues complement the standard Euclid catalogues, which will not include Spitzer IRAC data. In this paper, we present an overview of the survey, including the footprints of the survey fields, the existing and planned observations, and the primary science goals for the combined data set.",
author = "{Euclid Collaboration} and McPartland, {C. J. R.} and L. Zalesky and Weaver, {J. R.} and S. Toft and Sanders, {D. B.} and B. Mobasher and N. Suzuki and I. Szapudi and I. Valdes and G. Murphree and N. Chartab and N. Allen and S. Taamoli and Eisenhardt, {P. R. M.} and S. Arnouts and H. Atek and J. Brinchmann and M. Castellano and R. Chary and {Ch{\'a}vez Ortiz}, O. and J.-G. Cuby and Finkelstein, {S. L.} and T. Goto and S. Gwyn and Y. Harikane and Inoue, {A. K.} and McCracken, {H. J.} and Mohr, {J. J.} and Oesch, {P. A.} and M. Ouchi and M. Oguri and J. Rhodes and Rottgering, {H. J. A.} and M. Sawicki and R. Scaramella and C. Scarlata and Silverman, {J. D.} and D. Stern and Teplitz, {H. I.} and M. Shuntov and B. Altieri and A. Amara and I. Hook and Y. Wang and J. Weller and Ferrari, {A. G.} and A. Hall and Hartley, {W. G.} and D. Potter and C. Tao",
year = "2025",
month = mar,
day = "31",
doi = "10.1051/0004-6361/202451849",
language = "English",
volume = "695",
journal = "Astronomy and Astrophysics",
issn = "0004-6361",
publisher = "EDP Sciences",

}

RIS

TY - JOUR

T1 - Euclid preparation

T2 - LXIV. The Cosmic Dawn Survey (DAWN) of the Euclid Deep and Auxiliary Fields

AU - Euclid Collaboration

AU - McPartland, C. J. R.

AU - Zalesky, L.

AU - Weaver, J. R.

AU - Toft, S.

AU - Sanders, D. B.

AU - Mobasher, B.

AU - Suzuki, N.

AU - Szapudi, I.

AU - Valdes, I.

AU - Murphree, G.

AU - Chartab, N.

AU - Allen, N.

AU - Taamoli, S.

AU - Eisenhardt, P. R. M.

AU - Arnouts, S.

AU - Atek, H.

AU - Brinchmann, J.

AU - Castellano, M.

AU - Chary, R.

AU - Chávez Ortiz, O.

AU - Cuby, J.-G.

AU - Finkelstein, S. L.

AU - Goto, T.

AU - Gwyn, S.

AU - Harikane, Y.

AU - Inoue, A. K.

AU - McCracken, H. J.

AU - Mohr, J. J.

AU - Oesch, P. A.

AU - Ouchi, M.

AU - Oguri, M.

AU - Rhodes, J.

AU - Rottgering, H. J. A.

AU - Sawicki, M.

AU - Scaramella, R.

AU - Scarlata, C.

AU - Silverman, J. D.

AU - Stern, D.

AU - Teplitz, H. I.

AU - Shuntov, M.

AU - Altieri, B.

AU - Amara, A.

AU - Hook, I.

AU - Wang, Y.

AU - Weller, J.

AU - Ferrari, A. G.

AU - Hall, A.

AU - Hartley, W. G.

AU - Potter, D.

AU - Tao, C.

PY - 2025/3/31

Y1 - 2025/3/31

N2 - Euclid will provide deep near-infrared (NIR) imaging to ∼26.5 AB magnitude over ∼59 deg2 in its deep and auxiliary fields. The Cosmic DAWN survey combines dedicated and archival UV–NIR observations to provide matched depth multiwavelength imaging of the Euclid deep and auxiliary fields. The DAWN survey will provide consistently measured Euclid NIR-selected photometric catalogues, accurate photometric redshifts, and measurements of galaxy properties to a redshift of z ∼ 10. The DAWN catalogues include Spitzer IRAC data that are critical for stellar mass measurements at z ≳ 2.5 and high-z science. These catalogues complement the standard Euclid catalogues, which will not include Spitzer IRAC data. In this paper, we present an overview of the survey, including the footprints of the survey fields, the existing and planned observations, and the primary science goals for the combined data set.

AB - Euclid will provide deep near-infrared (NIR) imaging to ∼26.5 AB magnitude over ∼59 deg2 in its deep and auxiliary fields. The Cosmic DAWN survey combines dedicated and archival UV–NIR observations to provide matched depth multiwavelength imaging of the Euclid deep and auxiliary fields. The DAWN survey will provide consistently measured Euclid NIR-selected photometric catalogues, accurate photometric redshifts, and measurements of galaxy properties to a redshift of z ∼ 10. The DAWN catalogues include Spitzer IRAC data that are critical for stellar mass measurements at z ≳ 2.5 and high-z science. These catalogues complement the standard Euclid catalogues, which will not include Spitzer IRAC data. In this paper, we present an overview of the survey, including the footprints of the survey fields, the existing and planned observations, and the primary science goals for the combined data set.

U2 - 10.1051/0004-6361/202451849

DO - 10.1051/0004-6361/202451849

M3 - Journal article

VL - 695

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

SN - 0004-6361

M1 - A259

ER -