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

C. J.R. Mcpartland; L. Zalesky; J. R. Weaver; S. Toft; D. B. Sanders; B. Mobasher; N. Suzuki; I. Szapudi; I. Valdes; G. Murphree; N. Chartab; N. Allen; S. Taamoli; P. R.M. Eisenhardt; S. Arnouts; H. Atek; J. Brinchmann; M. Castellano; R. Chary; O. Chávez Ortiz; J. G. Cuby; S. L. Finkelstein; T. Goto; S. Gwyn; Y. Harikane; A. K. Inoue; H. J. Mccracken; J. J. Mohr; P. A. Oesch; M. Ouchi; M. Oguri; J. Rhodes; H. J.A. Rottgering; M. Sawicki; R. Scaramella; C. Scarlata; J. D. Silverman; D. Stern; H. I. Teplitz; M. Shuntov; B. Altieri; A. Amara; S. Andreon; S. M. Niemi; A. G. Sánchez; P. Schneider; Y. Wang; G. Gozaliasl; A. Hall; J. Hjorth; Euclid Collaboration

doi:10.1051/0004-6361/202451849

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

C. J.R. Mcpartland^*, L. Zalesky, J. R. Weaver, S. Toft, D. B. Sanders, B. Mobasher, N. Suzuki, I. Szapudi, I. Valdes, G. Murphree, N. Chartab, N. Allen, S. Taamoli, P. R.M. Eisenhardt, S. Arnouts, H. Atek, J. Brinchmann, M. Castellano, R. Chary, O. Chávez OrtizJ. G. Cuby, S. L. Finkelstein, T. Goto, S. Gwyn, Y. Harikane, A. K. Inoue, H. J. Mccracken, J. J. Mohr, P. A. Oesch, M. Ouchi, M. Oguri, J. Rhodes, H. J.A. Rottgering, M. Sawicki, R. Scaramella, C. Scarlata, J. D. Silverman, D. Stern, H. I. Teplitz, M. Shuntov, B. Altieri, A. Amara, S. Andreon, S. M. Niemi, A. G. Sánchez, P. Schneider, Y. Wang, G. Gozaliasl, A. Hall, J. Hjorth, Euclid Collaboration

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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.

Alkuperäiskieli	Englanti
Artikkeli	A259
Sivut	1-15
Sivumäärä	15
Julkaisu	Astronomy and Astrophysics
Vuosikerta	695
DOI - pysyväislinkit	https://doi.org/10.1051/0004-6361/202451849
Tila	Julkaistu - maalisk. 2025
OKM-julkaisutyyppi	A1 Alkuperäisartikkeli tieteellisessä aikakauslehdessä

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10.1051/0004-6361/202451849

Euclid_preparation._LXIV._The_Cosmic_Dawn_Survey_(DAWN)_of_the_Euclid_Deep_and_Auxiliary_FieldsFinal published version, 6,66 MBLisenssi: CC BY

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Mcpartland, C. J. R., Zalesky, L., Weaver, J. R., Toft, S., Sanders, D. B., Mobasher, B., Suzuki, N., Szapudi, I., Valdes, I., Murphree, G., Chartab, N., Allen, N., Taamoli, S., Eisenhardt, P. R. M., Arnouts, S., Atek, H., Brinchmann, J., Castellano, M., Chary, R., ... Euclid Collaboration (2025). Euclid preparation. LXIV. The Cosmic Dawn Survey (DAWN) of the Euclid Deep and Auxiliary Fields. Astronomy and Astrophysics, 695, 1-15. Artikkeli A259. https://doi.org/10.1051/0004-6361/202451849

@article{1702c06520984444b8b87f8d677c6b41,

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.",

keywords = "Catalogs, Galaxies: evolution, Galaxies: high-redshift, Galaxies: luminosity function, Mass function, Surveys",

author = "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 Cuby, {J. G.} 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 S. Andreon and Niemi, {S. M.} and S{\'a}nchez, {A. G.} and P. Schneider and Y. Wang and G. Gozaliasl and A. Hall and J. Hjorth and {Euclid Collaboration}",

note = "Publisher Copyright: {\textcopyright} 2025 The Authors.",

year = "2025",

month = mar,

doi = "10.1051/0004-6361/202451849",

language = "English",

volume = "695",

pages = "1--15",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

}

Mcpartland, CJR, Zalesky, L, Weaver, JR, Toft, S, Sanders, DB, Mobasher, B, Suzuki, N, Szapudi, I, Valdes, I, Murphree, G, Chartab, N, Allen, N, Taamoli, S, Eisenhardt, PRM, Arnouts, S, Atek, H, Brinchmann, J, Castellano, M, Chary, R, Chávez Ortiz, O, Cuby, JG, Finkelstein, SL, Goto, T, Gwyn, S, Harikane, Y, Inoue, AK, Mccracken, HJ, Mohr, JJ, Oesch, PA, Ouchi, M, Oguri, M, Rhodes, J, Rottgering, HJA, Sawicki, M, Scaramella, R, Scarlata, C, Silverman, JD, Stern, D, Teplitz, HI, Shuntov, M, Altieri, B, Amara, A, Andreon, S, Niemi, SM, Sánchez, AG, Schneider, P, Wang, Y, Gozaliasl, G, Hall, A, Hjorth, J & Euclid Collaboration 2025, 'Euclid preparation. LXIV. The Cosmic Dawn Survey (DAWN) of the Euclid Deep and Auxiliary Fields', Astronomy and Astrophysics, Vuosikerta 695, A259, Sivut 1-15. https://doi.org/10.1051/0004-6361/202451849

TY - JOUR

T1 - Euclid preparation. LXIV. The Cosmic Dawn Survey (DAWN) of the Euclid Deep and Auxiliary Fields

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 - Andreon, S.

AU - Niemi, S. M.

AU - Sánchez, A. G.

AU - Schneider, P.

AU - Wang, Y.

AU - Gozaliasl, G.

AU - Hall, A.

AU - Hjorth, J.

AU - Euclid Collaboration

PY - 2025/3

Y1 - 2025/3

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.

KW - Catalogs

KW - Galaxies: evolution

KW - Galaxies: high-redshift

KW - Galaxies: luminosity function

KW - Mass function

KW - Surveys

UR - http://www.scopus.com/inward/record.url?scp=105001863237&partnerID=8YFLogxK

U2 - 10.1051/0004-6361/202451849

DO - 10.1051/0004-6361/202451849

M3 - Article

AN - SCOPUS:105001863237

SN - 0004-6361

VL - 695

SP - 1

EP - 15

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

M1 - A259

ER -

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

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