CLEAR: Boosted Lyα Transmission of the Intergalactic Medium in UV-bright Galaxies, Jung, Intae,Papovich, Casey,Finkelstein, Steven L., The Astrophysical Journal, 933, 2022-07-01 00:00:00, 2022ApJ...933...87J||CLEAR: Emission-line Ratios at Cosmic High Noon, Backhaus, Bren E.,Trump, Jonathan R.,Cleri, Nikko J., The Astrophysical Journal, 926, 2022-02-01 00:00:00, 2022ApJ...926..161B||CLEAR. I. Ages and Metallicities of Quiescent Galaxies at 1.0 < z < 1.8 Derived from Deep Hubble Space Telescope Grism Data, Estrada-Carpenter, Vicente,Papovich, Casey,Momcheva, Ivelina, The Astrophysical Journal, 870, 2019-01-01 00:00:00, 2019ApJ...870..133E||CLEAR. II. Evidence for Early Formation of the Most Compact Quiescent Galaxies at High Redshift, Estrada-Carpenter, Vicente,Papovich, Casey,Momcheva, Ivelina, The Astrophysical Journal, 898, 2020-08-01 00:00:00, 2020ApJ...898..171E||CLEAR: Paschen-β Star Formation Rates and Dust Attenuation of Low-redshift Galaxies, Cleri, Nikko J.,Trump, Jonathan R.,Backhaus, Bren E., The Astrophysical Journal, 929, 2022-04-01 00:00:00, 2022ApJ...929....3C||CLEAR: The Evolution of Spatially Resolved Star Formation in Galaxies between 0.5 ≲ z ≲ 1.7 Using Hα Emission Line Maps, Matharu, Jasleen,Papovich, Casey,Simons, Raymond C., The Astrophysical Journal, 937, 2022-09-01 00:00:00, 2022ApJ...937...16M||CLEAR: The Gas-phase Metallicity Gradients of Star-forming Galaxies at 0.6 < z < 2.6, Simons, Raymond C.,Papovich, Casey,Momcheva, Ivelina, The Astrophysical Journal, 923, 2021-12-01 00:00:00, 2021ApJ...923..203S||CLEAR: The Ionization and Chemical-enrichment Properties of Galaxies at 1.1 < z < 2.3, Papovich, Casey,Simons, Raymond C.,Estrada-Carpenter, Vicente, The Astrophysical Journal, 937, 2022-09-01 00:00:00, 2022ApJ...937...22P||Do Current X-Ray Observations Capture Most of the Black-hole Accretion at High Redshifts?, Yang, Guang,Estrada-Carpenter, Vicente,Papovich, Casey, The As...trophysical Journal, 921, 2021-11-01 00:00:00, 2021ApJ...921..170Y||Extremely Low Molecular Gas Content in the Vicinity of a Red Nugget Galaxy at z = 1.91, Morishita, Takahiro,D'Amato, Q.,Abramson, L., The Astrophysical Journal, 908, 2021-02-01 00:00:00, 2021ApJ...908..163M||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||Spatially Extended Low-ionization Emission Regions (LIERs) at z ∼ 0.9, Hviding, Raphael E.,Brammer, Gabriel B.,Momcheva, Ivelina, The Astrophysical Journal, 868, 2018-11-01 00:00:00, 2018ApJ...868...16H||The missing light of the Hubble Ultra Deep Field, Borlaff, Alejandro,Trujillo, Ignacio,Román, Javier, Astronomy and Astrophysics, 621, 2019-01-01 00:00:00, 2019A&A...621A.133B||The VANDELS survey: a measurement of the average Lyman-continuum escape fraction of star-forming galaxies at z = 3.5, Begley, R.,Cullen, Fergus,McLure, R. J., Monthly Notices of the Royal Astronomical Society, 513, 2022-07-01 00:00:00, 2022MNRAS.513.3510B||Using Multiple Emission Line Ratios to Constrain the Slope of the Dust Attenuation Law, Prescott, Moire K. M.,Finlator, Kristian,Cleri, Nikko J., The Astrophysical Journal, 928, 2022-03-01 00:00:00, 2022ApJ...928...71P
Instrument
WFC3, WFC3/IR
Temporal Coverage
2015-11-14T18:40:27Z/2017-02-19T21:16:19Z
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, 2017, The Candels Lyman-Alpha Emission At Reionization (Clear) Experiment, 1.0, European Space Agency, https://doi.org/10.5270/esa-8kepdy1
