CLEAR: Survey Overview, Data Analysis and Products
arXiv:2303.09570 · doi:10.3847/1538-4365/acc517
Abstract
We present an overview of the CANDELS Lyman-a Emission At Reionization (CLEAR) survey. CLEAR is a 130 orbit program of the Hubble Space Telescope using the Wide Field Camera 3 (WFC3) IR G102 grism. CLEAR targets 12 pointings divided between the GOODS-N and GOODS-S fields of the Cosmic Assembly Near-IR Deep Extragalactic Legacy Survey (CANDELS). Combined with existing spectroscopic data from other programs, the full CLEAR dataset includes spectroscopic imaging of these fields over 0.8-1.7 um. In this Paper, we describe the CLEAR survey, the survey strategy, the data acquisition, reduction, processing, and science products and catalogs released alongside this paper. The catalogs include emission line fluxes and redshifts derived from the combination of the photometry and grism spectroscopy for 6048 galaxies, primarily ranging from 0.2 < z < 3. We also provide an overview of CLEAR science goals and results. In conjunction with this Paper we provide links to electronic versions of the data products, including 1D + 2D extracted spectra and emission line maps.
arXiv commentAccepted in ApJS. 29 pages, 14 figures. The data products (1D + 2D spectra, emission line maps) and catalogs (photometric and spectroscopic catalogs of GOODS-N and GOODS-S) are available at https://archive.stsci.edu/hlsp/clear
References in corpus (105)
- Array Programming with NumPy
- Astropy: A Community Python Package for Astronomy
- The chemical composition of the Sun
- Galactic Stellar and Substellar Initial Mass Function
- The Astropy Project: Building an inclusive, open-science project and status of the v2.0 core package
- Cosmic Star Formation History
- CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey
- CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey - The Hubble Space Telescope Observations, Imaging Data Products and Mosaics
- The propagation of uncertainties in stellar population synthesis modeling I: The relevance of uncertain aspects of stellar evolution and the IMF to the derived physical properties of galaxies
- EAZY: A Fast, Public Photometric Redshift Code
- The Great Observatories Origins Deep Survey: Initial Results From Optical and Near-Infrared Imaging
- K-corrections and filter transformations in the ultraviolet, optical, and near infrared
- The propagation of uncertainties in stellar population synthesis modeling III: model calibration, comparison, and evaluation
- The SINS survey: SINFONI Integral Field Spectroscopy of z ~ 2 Star-forming Galaxies
- 3D-HST WFC3-selected Photometric Catalogs in the Five CANDELS/3D-HST Fields: Photometry, Photometric Redshifts and Stellar Masses
- The Hubble Ultra Deep Field
- The 3D-HST Survey: Hubble Space Telescope WFC3/G141 grism spectra, redshifts, and emission line measurements for galaxies
- The Evolution of the Galaxy Rest-Frame Ultraviolet Luminosity Function Over the First Two Billion Years
- 3D-HST: A wide-field grism spectroscopic survey with the Hubble Space Telescope
- Lyman Break Galaxies at Redshift z~3: Survey Description and Full Data Set
- The Frontier Fields: Survey Design
- Strong Nebular Line Ratios in the Spectra of z~2-3 Star-forming Galaxies: First Results from KBSS-MOSFIRE
- The KMOS^3D Survey: design, first results, and the evolution of galaxy kinematics from 0.7<z<2.7
- New Constraints on Cosmic Reionization from the 2012 Hubble Ultra Deep Field Campaign
- SINFONI Integral Field Spectroscopy of z~2 UV-selected Galaxies: Rotation Curves and Dynamical Evolution
- The Stellar Initial Mass Function in Early-Type Galaxies From Absorption Line Spectroscopy. II. Results
- Keck Spectroscopy of Faint 3<z<7 Lyman Break Galaxies: - I. New constraints on cosmic reionisation from the luminosity and redshift-dependent fraction of Lyman-alpha emission
- The MOSFIRE Deep Evolution Field (MOSDEF) Survey: Rest-Frame Optical Spectroscopy for ~1500 H-Selected Galaxies at 1.37 < z < 3.8
- Reconciling the Stellar and Nebular Spectra of High Redshift Galaxies
- Cosmic X-ray Surveys of Distant Active Galaxies: The Demographics, Physics, and Ecology of Growing Supermassive Black Holes
- Photometric Redshifts for Hyper Suprime-Cam Subaru Strategic Program Data Release 1
- A Deep, Wide Field, Optical, and Near Infrared Catalog of a Large Area around the Hubble Deep Field North
- GaBoDS: The Garching-Bonn Deep Survey; IV. Methods for the Image reduction of multi-chip Cameras
- New observations of z~7 galaxies: evidence for a patchy reionization
- The Multiwavelength Survey by Yale-Chile (MUSYC): Deep Medium-Band optical imaging and high quality 32-band photometric redshifts in the ECDF-S
- A Rapidly Star-forming Galaxy 700 Million Years After the Big Bang at z=7.51
- Nebular Emission Line Ratios in z~2-3 Star-Forming Galaxies with KBSS-MOSFIRE: Exploring the Impact of Ionization, Excitation, and Nitrogen-to-Oxygen Ratio
- The MOSDEF Survey: Mass, Metallicity, and Star-formation Rate at z~2.3
- Where stars form: inside-out growth and coherent star formation from HST Halpha maps of 2676 galaxies across the main sequence at z~1
- Studying Reionization with Ly-alpha Emitters
- The Epoch of Disk Settling: z~1 to Now
- A Spectroscopic Redshift Measurement for a Luminous Lyman Break Galaxy at z=7.730 using Keck/MOSFIRE
- The Grism Lens-Amplified Survey from Space (GLASS). I. Survey overview and first data release
- The Stellar Mass Tully-Fisher Relation to z=1.2 from AEGIS
- Physical Properties of Emission-Line Galaxies at z ~ 2 from Near-Infrared Spectroscopy with Magellan FIRE
- A Survey of Galaxy Kinematics to z ~ 1 in the TKRS/GOODS-N Field. I. Rotation and Dispersion Properties
- Constraining the neutral fraction of hydrogen in the IGM at redshift 7.5
- The Evolution and Origin of Ionized Gas Velocity Dispersion from to with KMOS
- Deep U band and R imaging of GOODS-South: Observations,data reduction and first results
- Dust attenuation, bulge formation and inside-out cessation of star-formation in Star-Forming Main Sequence galaxies at z~2
- The KMOS^3D Survey: data release and final survey paper
- The Assembly Histories of Quiescent Galaxies Since z=0.7 from Absorption Line Spectroscopy
- Texas Spectroscopic Search for Ly Emission at the End of Reionization III. the Ly Equivalent-width Distribution and Ionized Structures at
- The WFC3 Infrared Spectroscopic Parallel (WISP) Survey
- The Great Observatories Origins Deep Survey - VLT/ISAAC Near-Infrared Imaging of the GOODS-South Field
- z~2: An Epoch of Disk Assembly
- Measuring the Physical Conditions in High-Redshift Star-Forming Galaxies: Insights from KBSS-MOSFIRE
- A massive, quiescent, population II galaxy at a redshift of 2.1
- CANDELSz7: a large spectroscopic survey of CANDELS galaxies in the reionization epoch
- The Taiwan ECDFS Near-Infrared Survey: Ultra-deep J and Ks Imaging in the Extended Chandra Deep Field-South
- Theoretical ISM pressure and electron density diagnostics for local and high-redshift galaxies
- The THESAN project: Lyman-alpha emission and transmission during the Epoch of Reionization
- The KLEVER Survey: Spatially resolved metallicity maps and gradients in a sample of 1.2 < z < 2.5 lensed galaxies
- GaBoDS: The Garching-Bonn Deep Survey V. Data release of the ESO Deep-Public-Survey
- Inferences on the distribution of Ly-alpha emission of z~7 and z~8 galaxies
- The MOSDEF-LRIS Survey: The Interplay Between Massive Stars and Ionized Gas in High-Redshift Star-Forming Galaxies
- Measuring the properties of reionised bubbles with resolved Lyman alpha spectra
- CLEAR: The Gas-Phase Metallicity Gradients of Star-Forming Galaxies at 0.6 < z < 2.6
- Discovery of Strongly Inverted Metallicity Gradients in Dwarf Galaxies at 2
- The Grism Lens-Amplified Survey from Space (GLASS) X. Sub-kpc resolution gas-phase metallicity maps at cosmic noon behind the Hubble Frontier Fields cluster MACS1149.6+2223
- CLEAR I: Ages and Metallicities of Quiescent Galaxies at Derived from Deep Hubble Space Telescope Grism Data
- The Grism Lens-Amplified Survey from Space (GLASS). III. A census of Lyα Emission at 7 from HST Spectroscopy
- The regulation of galaxy growth along the size-mass relation by star-formation, as traced by H in KMOS galaxies at 0.7 < z < 2.7
- Kinematic Downsizing at z~2
- Stellar Metallicities and Elemental Abundance Ratios of z~1.4 Massive Quiescent Galaxies
- The MOSDEF Survey: Kinematic and Structural Evolution of Star-Forming Galaxies at
- CLEAR II: Evidence for Early Formation of the Most Compact Quiescent Galaxies at High Redshift
- MOIRCS Deep Survey. IX. Deep Near-Infrared Imaging Data and Source Catalog
- Chemical abundance scaling relations for multiple elements in z~2-3 star-forming galaxies
- First results from Faint Infrared Grism Survey (FIGS): first simultaneous detection of Lyman-alpha emission and Lyman break from a galaxy at z=7.51
- A Census of Sub-kiloparsec Resolution Metallicity Gradients in Star-forming Galaxies at Cosmic Noon from HST Slitless Spectroscopy
- FIGS -- Faint Infrared Grism Survey: Description and Data Reduction
- Hubble Space Telescope WFC3 Grism Spectroscopy and Imaging of a Growing Compact Galaxy at z=1.9
- The Late Reionization of Filaments
- A Type Ia Supernova at Redshift 1.55 in Hubble Space Telescope Infrared Observations from CANDELS
- Spectroscopically Confirmed Lyman-Alpha Emitters from Redshift 5 to 7 Behind Ten Galaxy Cluster Lenses
- The mass-metallicity relation at z~1-2 and its dependence on star formation rate
- The mass-metallicity relation at cosmic noon in overdense environments: first results from the MAMMOTH-Grism HST slitless spectroscopic survey
- Crucial Factors for Lyα Transmission in the Reionizing Intergalactic Medium: Infall Motion, HII Bubble Size, and Self-shielded Systems
- Discovery of a z = 7.452 High Equivalent Width Lyman-α Emitter from the Hubble Space Telescope Faint Infrared Grism Survey
- Dark-ages Reionization and Galaxy Formation Simulation XX. The Ly IGM transmission properties and environment of bright galaxies during the Epoch of Reionization
- Hubble Space Telescope WFC3 Early Release Science: Emission-Line Galaxies from Infrared Grism Observations
- Texas Spectroscopic Search for Ly Emission at the End of Reionization I. Constraining the Ly Equivalent Width Distribution at 6.0 < < 7.0
- First Census of Gas-phase Metallicity Gradients of Star-forming Galaxies in Overdense Environments at Cosmic Noon
- Tracing the Sources of Reionization in Cosmological Radiation Hydrodynamics Simulations
- CLEAR: The Evolution of Spatially Resolved Star Formation in Galaxies between using H Emission Line Maps
- Stellar population properties of individual massive early-type galaxies at 1.4 < z < 2
- CLEAR: Paschen- Star Formation Rates and Dust Attenuation of Low Redshift Galaxies
- Texas Spectroscopic Search for Ly Emission at the End of Reionization II. The Deepest Near-Infrared Spectroscopic Observation at
- CLEAR: Boosted Ly Transmission of the Intergalactic Medium in UV bright Galaxies
- A Two-Dimensional Spectroscopic Study of Emission Line Galaxies in the Faint Infrared Grism Survey (FIGS) I: Detection Method and Catalog
- The MUSE Ultra Deep Field (MUDF). III. Hubble Space Telescope WFC3 Grism Spectroscopy and Imaging
- 3D-DASH: The Widest Near-Infrared Hubble Space Telescope Survey
- Do current X-ray observations capture most of the black-hole accretion at high redshifts?
- CLEAR: Spatially Resolved Emission Lines and Active Galactic Nuclei at
Cited by in corpus (6)
- Using [Ne V]/[Ne III] to Understand the Nature of Extreme-Ionization Galaxies
- A First Look at Spatially Resolved Star Formation at with JWST FRESCO NIRCam Slitless Spectroscopy
- CLEAR: The Morphological Evolution of Galaxies in the Green Valley
- Exploring the Gas-Phase Metallicity Gradients of Star-forming Galaxies at Cosmic Noon
- NGDEEP: The Star Formation and Ionization Properties of Galaxies at
- The leakage of Lyman-continuum photons from a major merger at