A Census of Photometrically Selected Little Red Dots at 4 < z < 9 in JWST Blank Fields
A first look at spatially resolved star formation at 4.8 < z < 6.5 with JWST FRESCO NIRCam slitless spectroscopy
CLEAR: Boosted Lya Transmission of the Intergalactic Medium in UV-bright Galaxies
CLEAR: Emission-line Ratios at Cosmic High Noon
CLEAR: High-ionization Ne V l3426 Emission-line Galaxies at 1.4 < z < 2.3
CLEAR. I. Ages and Metallicities of Quiescent Galaxies at 1.0 < z < 1.8 Derived from Deep Hubble Space Telescope Grism Data
CLEAR. II. Evidence for Early Formation of the Most Compact Quiescent Galaxies at High Redshift
CLEAR: Paschen-b Star Formation Rates and Dust Attenuation of Low-redshift Galaxies
CLEAR: Spatially Resolved Emission Lines and Active Galactic Nuclei at 0.6 < z < 1.3
CLEAR: Survey Overview, Data Analysis, and Products
CLEAR: The Evolution of Spatially Resolved Star Formation in Galaxies between 0.5 z 1.7 Using Ha Emission Line Maps
CLEAR: The Gas-phase Metallicity Gradients of Star-forming Galaxies at 0.6 < z < 2.6
CLEAR: The Ionization and Chemical-enrichment Properties of Galaxies at 1.1 < z < 2.3
CLEAR: The Morphological Evolution of Galaxies in the Green Valley
Deciphering Gas Dynamics and Star Formation in a z = 1.1 Main-sequence Spiral Galaxy with ALMA and JWST
Do Current X-Ray Observations Capture Most of the Black-hole Accretion at High Redshifts?
Dust in Little Red Dots
Evaluating the Accuracy of Non-parametric Galaxy Morphological Indicator Measurements in the CSST Imaging Survey
Exploring the Gas-phase Metallicity Gradients of Star-forming Galaxies at Cosmic Noon
Extremely Low Molecular Gas Content in the Vicinity of a Red Nugget Galaxy at z = 1.91
Massive Dead Galaxies at z ~ 2 with HST Grism Spectroscopy. I. Star Formation Histories and Metallicity Enrichment
Not Just a Dot: The Complex UV Morphology and Underlying Properties of Little Red Dots
Spatially Extended Low-ionization Emission Regions (LIERs) at z ~ 0.9
The ALMA-CRISTAL survey: Resolved kinematic studies of main sequence star-forming galaxies at 4 < z < 6
The AstroSat UV Deep Field North: The IRX-b Relation for the UV-selected Galaxies at z ~ 0.5-0.7
The AstroSat UV Deep Field South. II. A Diverse Set of Lyman-continuum Leakers at z ~ 1
The AstroSat UV Deep Field South. V. Constraints on the Average Escape of Ionizing Photons in the Cosmic Dusk
The Leakage of Lyman-continuum Photons from a Major Merger at z ~ 1
The missing light of the Hubble Ultra Deep Field
The VANDELS survey: a measurement of the average Lyman-continuum escape fraction of star-forming galaxies at z = 3.5
Using Multiple Emission Line Ratios to Constrain the Slope of the Dust Attenuation Law
Using Ne V/Ne III to Understand the Nature of Extreme-ionization Galaxies
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, Papovich et al., 2017, 'The CANDELS Lyman-alpha Emission At Reionization (CLEAR) Experiment', 1.0, European Space Agency, https://doi.org/10.5270/esa-8kepdy1