A Census of the Bright z = 8.5-11 Universe with the Hubble and Spitzer Space Telescopes in the CANDELS Fields, Finkelstein, Steven L.,Bagley, Micaela B.,Song, Mimi, The Astrophysical Journal, 928, 2022-03-01 00:00:00, 2022ApJ...928...52F||A quantitative assessment of completeness correction methods and public release of a versatile simulation code, Leethochawalit, Nicha,Trenti, Michele,Morishita, Takahiro, Monthly Notices of the Royal Astronomical Society, 509, 2022-02-01 00:00:00, 2022MNRAS.509.5836L||Candidate z ∼ 2.5 Lyman Continuum Sources in the GOODS Fields, Jones, L. H.,Barger, A. J.,Cowie, L. L., The Astrophysical Journal, 908, 2021-02-01 00:00:00, 2021ApJ...908..222J||Early- and late-stage mergers among main sequence and starburst galaxies at 0.2 ≤ z ≤ 2, Cibinel, A.,Daddi, E.,Sargent, M. T., Monthly Notices of the Royal Astronomical Society, 485, 2019-06-01 00:00:00, 2019MNRAS.485.5631C||Extremely Small Sizes for Faint z ∼ 2-8 Galaxies in the Hubble Frontier Fields: A Key Input for Establishing Their Volume Density and UV Emissivity, Bouwens, R. J.,Illingworth, G. D.,Oesch, P. A., The Astrophysical Journal, 843, 2017-07-01 00:00:00, 2017ApJ...843...41B||FUV and NIR size of the HI selected low surface brightness galaxies, Cheng, Cheng,Du, Wei,Xu, Cong Kevin, Research in Astronomy and Astrophysics, 21, 2021-04-01 00:00:00, 2021RAA....21...76C||Galaxy luminosity function pipeline for cosmology and astrophysics, Sabti, Nashwan,Muñoz, Julian B.,Blas, Diego, Physical Review D, 105, 2022-02-01 00:00:00, 2022PhRvD.105d3518S||HDUV: The Hubble Deep UV Legacy Survey, Oesch, P. A.,Montes, M.,Reddy, N., The Astrophysical Journal Supplement Series, 237, 2018-07-01 00:00:00, 2018ApJS..237...12O||Lyman continuum escape fraction in Ly α emitters at z ≃ 3.1, Bian, Fuyan,Fan, Xiaohui, Monthly Notices of the Royal Astronomical Society, 493, 2020-03-01 00:00:00, 2020MNRAS.493L..65B||Massive Dead Galaxies at z ∼ 2 with HST Grism... Spectroscopy. I. Star Formation Histories and Metallicity Enrichment, Morishita, Takahiro,Abramson, L.,Treu, T., The Astrophysical Journal, 877, 2019-06-01 00:00:00, 2019ApJ...877..141M||Millimeter Mapping at z ∼ 1: Dust-obscured Bulge Building and Disk Growth, Nelson, Erica J.,Tadaki, Ken-ichi,Tacconi, L. 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J., Monthly Notices of the Royal Astronomical Society, 513, 2022-07-01 00:00:00, 2022MNRAS.513.3510B||Ultra-deep Large Binocular Camera U-band Imaging of the GOODS-North Field: Depth Versus Resolution, Ashcraft, Teresa A.,Windhorst, Rogier A.,Jansen, Rolf A., Publications of the Astronomical Society of the Pacific, 130, 2018-06-01 00:00:00, 2018PASP..130f4102A||UV and NIR size of the low-mass field galaxies: the UV compact galaxies, Cheng, Cheng,Xu, Cong Kevin,Xie, Lizhi, Astronomy and Astrophysics, 633, 2020-01-01 00:00:00, 2020A&A...633A.105C
Instrument
ACS, ACS/WFC, WFC3, WFC3/UVIS
Temporal Coverage
2014-11-25T08:35:43Z/2015-11-16T17:28:38Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
European Space Agency, 2015, The Goods Uv Legacy Fields: A Full Census Of Faint Star-Forming Galaxies At Z~0.5-2, 1.0, European Space Agency, https://doi.org/10.5270/esa-l58iizo
