Journal
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
Volume 235, Issue 1, Pages -Publisher
IOP PUBLISHING LTD
DOI: 10.3847/1538-4365/aaacce
Keywords
galaxies: evolution; galaxies: high-redshift; infrared: galaxies
Categories
Funding
- National Science Foundation [1513473]
- NASA through Space Telescope Science Institute [HST-AR-14302, HST-AR-14553]
- NASA [NAS5-26555, NAS 5-26555]
- Tufts University
- NASA Keck PI Data Awards
- STScI Director's Discretionary Research Fund
- NWO [614.001.302]
- W.M. Keck Foundation
- HST Frontier Fields program
- Direct For Mathematical & Physical Scien
- Division Of Astronomical Sciences [1513473] Funding Source: National Science Foundation
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We present Hubble multi-wavelength photometric catalogs, including (up to) 17 filters with the Advanced Camera for Surveys and Wide Field Camera 3 from the ultra-violet to near-infrared for the Hubble Frontier Fields and associated parallels. We have constructed homogeneous photometric catalogs for all six clusters and their parallels. To further expand these data catalogs, we have added ultra-deep KS-band imaging at 2.2. mu m from the Very Large Telescope HAWK-I and Keck-I MOSFIRE instruments. We also add post-cryogenic Spitzer imaging at 3.6 and 4.5. mu m with the Infrared Array Camera (IRAC), as well as archival IRAC 5.8 and 8.0. mu m imaging when available. We introduce the public release of the multi-wavelength (0.2-8 mu m) photometric catalogs, and we describe the unique steps applied for the construction of these catalogs. Particular emphasis is given to the source detection band, the contamination of light from the bright cluster galaxies (bCGs), and intra-cluster light (ICL). In addition to the photometric catalogs, we provide catalogs of photometric redshifts and stellar population properties. Furthermore, this includes all the images used in the construction of the catalogs, including the combined models of bCGs and ICL, the residual images, segmentation maps, and more. These catalogs are a robust data set of the Hubble Frontier Fields and will be an important aid in designing future surveys, as well as planning follow-up programs with current and future observatories to answer key questions remaining about first light, reionization, the assembly of galaxies, and many more topics, most notably by identifying high-redshift sources to target.
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