3D-DASH: The Widest Near-infrared Hubble Space Telescope Survey

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3D-DASH : The Widest Near-infrared Hubble Space Telescope Survey. / Mowla, Lamiya A.; Cutler, Sam E.; Brammer, Gabriel B.; Momcheva, Ivelina G.; Whitaker, Katherine E.; van Dokkum, Pieter G.; Bezanson, Rachel S.; Schreiber, Natascha M. Forster; Franx, Marijn; Iyer, Kartheik G.; Marchesini, Danilo; Muzzin, Adam; Nelson, Erica J.; Skelton, Rosalind E.; Snyder, Gregory F.; Wake, David A.; Wuyts, Stijn; van der Wel, Arjen.

I: Astrophysical Journal, Bind 933, Nr. 2, 129, 01.07.2022.

Publikation: Bidrag til tidsskrift › Tidsskriftartikel › Forskning › fagfællebedømt

Harvard

Mowla, LA, Cutler, SE, Brammer, GB, Momcheva, IG, Whitaker, KE, van Dokkum, PG, Bezanson, RS, Schreiber, NMF, Franx, M, Iyer, KG, Marchesini, D, Muzzin, A, Nelson, EJ, Skelton, RE, Snyder, GF, Wake, DA, Wuyts, S & van der Wel, A 2022, '3D-DASH: The Widest Near-infrared Hubble Space Telescope Survey', Astrophysical Journal, bind 933, nr. 2, 129. https://doi.org/10.3847/1538-4357/ac71af

APA

Mowla, L. A., Cutler, S. E., Brammer, G. B., Momcheva, I. G., Whitaker, K. E., van Dokkum, P. G., Bezanson, R. S., Schreiber, N. M. F., Franx, M., Iyer, K. G., Marchesini, D., Muzzin, A., Nelson, E. J., Skelton, R. E., Snyder, G. F., Wake, D. A., Wuyts, S., & van der Wel, A. (2022). 3D-DASH: The Widest Near-infrared Hubble Space Telescope Survey. Astrophysical Journal, 933(2), [129]. https://doi.org/10.3847/1538-4357/ac71af

Vancouver

Mowla LA, Cutler SE, Brammer GB, Momcheva IG, Whitaker KE, van Dokkum PG o.a. 3D-DASH: The Widest Near-infrared Hubble Space Telescope Survey. Astrophysical Journal. 2022 jul. 1;933(2). 129. https://doi.org/10.3847/1538-4357/ac71af

Author

Mowla, Lamiya A. ; Cutler, Sam E. ; Brammer, Gabriel B. ; Momcheva, Ivelina G. ; Whitaker, Katherine E. ; van Dokkum, Pieter G. ; Bezanson, Rachel S. ; Schreiber, Natascha M. Forster ; Franx, Marijn ; Iyer, Kartheik G. ; Marchesini, Danilo ; Muzzin, Adam ; Nelson, Erica J. ; Skelton, Rosalind E. ; Snyder, Gregory F. ; Wake, David A. ; Wuyts, Stijn ; van der Wel, Arjen. / 3D-DASH : The Widest Near-infrared Hubble Space Telescope Survey. I: Astrophysical Journal. 2022 ; Bind 933, Nr. 2.

Bibtex

@article{09b674c18b5e404abe9d4534fb338190,
title = "3D-DASH: The Widest Near-infrared Hubble Space Telescope Survey",
abstract = "The 3D-Drift And SHift (3D-DASH) program is a Hubble Space Telescope (HST) WFC3 F160W imaging and G141 grism survey of the equatorial COSMOS field. 3D-DASH extends the legacy of HST near-infrared imaging and spectroscopy to degree-scale swaths of the sky, enabling the identification and study of distant galaxies (z > 2) that are rare or in short-lived phases of galaxy evolution at rest-frame optical wavelengths. Furthermore, when combined with existing ACS/F814W imaging, the program facilitates spatially resolved studies of the stellar populations and dust content of intermediate redshift (0.5 < z < 2) galaxies. Here we present the reduced F160W imaging mosaic available to the community. Observed with the efficient DASH technique, the mosaic comprises 1256 individual WFC3 pointings, corresponding to an area of 1.35 deg(2) (1.43 deg(2) in 1912 when including archival data). The median 5 sigma point-source limit in H (160) is 24.74 +/- 0.20 mag. We also provide a point-spread function (PSF) generator tool to determine the PSF at any location within the 3D-DASH footprint. 3D-DASH is the widest HST/WFC3 imaging survey in the F160W filter to date, increasing the existing extragalactic survey area in the near-infrared at HST resolution by an order of magnitude.",
keywords = "MASSIVE GALAXIES, NUMBER DENSITY, COSMOS-DASH, EVOLUTION, ASTROPY, CANDELS, MERGERS, CLUMPS, PAIRS, II.",
author = "Mowla, {Lamiya A.} and Cutler, {Sam E.} and Brammer, {Gabriel B.} and Momcheva, {Ivelina G.} and Whitaker, {Katherine E.} and {van Dokkum}, {Pieter G.} and Bezanson, {Rachel S.} and Schreiber, {Natascha M. Forster} and Marijn Franx and Iyer, {Kartheik G.} and Danilo Marchesini and Adam Muzzin and Nelson, {Erica J.} and Skelton, {Rosalind E.} and Snyder, {Gregory F.} and Wake, {David A.} and Stijn Wuyts and {van der Wel}, Arjen",
year = "2022",
month = jul,
day = "1",
doi = "10.3847/1538-4357/ac71af",
language = "English",
volume = "933",
journal = "Astrophysical Journal",
issn = "0004-637X",
publisher = "Institute of Physics Publishing, Inc",
number = "2",

}

RIS

TY - JOUR

T1 - 3D-DASH

T2 - The Widest Near-infrared Hubble Space Telescope Survey

AU - Mowla, Lamiya A.

AU - Cutler, Sam E.

AU - Brammer, Gabriel B.

AU - Momcheva, Ivelina G.

AU - Whitaker, Katherine E.

AU - van Dokkum, Pieter G.

AU - Bezanson, Rachel S.

AU - Schreiber, Natascha M. Forster

AU - Franx, Marijn

AU - Iyer, Kartheik G.

AU - Marchesini, Danilo

AU - Muzzin, Adam

AU - Nelson, Erica J.

AU - Skelton, Rosalind E.

AU - Snyder, Gregory F.

AU - Wake, David A.

AU - Wuyts, Stijn

AU - van der Wel, Arjen

PY - 2022/7/1

Y1 - 2022/7/1

N2 - The 3D-Drift And SHift (3D-DASH) program is a Hubble Space Telescope (HST) WFC3 F160W imaging and G141 grism survey of the equatorial COSMOS field. 3D-DASH extends the legacy of HST near-infrared imaging and spectroscopy to degree-scale swaths of the sky, enabling the identification and study of distant galaxies (z > 2) that are rare or in short-lived phases of galaxy evolution at rest-frame optical wavelengths. Furthermore, when combined with existing ACS/F814W imaging, the program facilitates spatially resolved studies of the stellar populations and dust content of intermediate redshift (0.5 < z < 2) galaxies. Here we present the reduced F160W imaging mosaic available to the community. Observed with the efficient DASH technique, the mosaic comprises 1256 individual WFC3 pointings, corresponding to an area of 1.35 deg(2) (1.43 deg(2) in 1912 when including archival data). The median 5 sigma point-source limit in H (160) is 24.74 +/- 0.20 mag. We also provide a point-spread function (PSF) generator tool to determine the PSF at any location within the 3D-DASH footprint. 3D-DASH is the widest HST/WFC3 imaging survey in the F160W filter to date, increasing the existing extragalactic survey area in the near-infrared at HST resolution by an order of magnitude.

AB - The 3D-Drift And SHift (3D-DASH) program is a Hubble Space Telescope (HST) WFC3 F160W imaging and G141 grism survey of the equatorial COSMOS field. 3D-DASH extends the legacy of HST near-infrared imaging and spectroscopy to degree-scale swaths of the sky, enabling the identification and study of distant galaxies (z > 2) that are rare or in short-lived phases of galaxy evolution at rest-frame optical wavelengths. Furthermore, when combined with existing ACS/F814W imaging, the program facilitates spatially resolved studies of the stellar populations and dust content of intermediate redshift (0.5 < z < 2) galaxies. Here we present the reduced F160W imaging mosaic available to the community. Observed with the efficient DASH technique, the mosaic comprises 1256 individual WFC3 pointings, corresponding to an area of 1.35 deg(2) (1.43 deg(2) in 1912 when including archival data). The median 5 sigma point-source limit in H (160) is 24.74 +/- 0.20 mag. We also provide a point-spread function (PSF) generator tool to determine the PSF at any location within the 3D-DASH footprint. 3D-DASH is the widest HST/WFC3 imaging survey in the F160W filter to date, increasing the existing extragalactic survey area in the near-infrared at HST resolution by an order of magnitude.

KW - MASSIVE GALAXIES

KW - NUMBER DENSITY

KW - COSMOS-DASH

KW - EVOLUTION

KW - ASTROPY

KW - CANDELS

KW - MERGERS

KW - CLUMPS

KW - PAIRS

KW - II.

U2 - 10.3847/1538-4357/ac71af

DO - 10.3847/1538-4357/ac71af

M3 - Journal article

VL - 933

JO - Astrophysical Journal

JF - Astrophysical Journal

SN - 0004-637X

IS - 2

M1 - 129

ER -

ID: 315391182