SIMBAD references

2020ApJ...889..189S - Astrophys. J., 889, 189-189 (2020/February-1)

RELICS: the Reionization Lensing Cluster Survey and the brightest high-z galaxies.

SALMON B., COE D., BRADLEY L., BOUWENS R., BRADAC M., HUANG K.-H., OESCH P.A., STARK D., SHARON K., TRENTI M., AVILA R.J., OGAZ S., ANDRADE-SANTOS F., CARRASCO D., CERNY C., DAWSON W., FRYE B.L., HOAG A., JOHNSON T.L., JONES C., LAM D., LOVISARI L., MAINALI R., PAST M., PATERNO-MAHLER R., PETERSON A., RIESS A.G., RODNEY S.A., RYAN R.E., SENDRA-SERVER I., STRAIT V., STROLGER L.-G., UMETSU K., VULCANI B. and ZITRIN A.

Abstract (from CDS):

Massive foreground galaxy clusters magnify and distort the light of objects behind them, permitting a view into both the extremely distant and intrinsically faint galaxy populations. We present here the z∼6–8 candidate high-redshift galaxies from the Reionization Lensing Cluster Survey (RELICS), a Hubble and Spitzer Space Telescope survey of 41 massive galaxy clusters spanning an area of ≃200 arcmin2. These clusters were selected to be excellent lenses, and we find similar high-redshift sample sizes and magnitude distributions as the Cluster Lensing And Supernova survey with Hubble (CLASH). We discover 257, 57, and eight candidate galaxies at z ∼ 6, 7, and 8 respectively, (322 in total). The observed (lensed) magnitudes of the z ∼ 6 candidates are as bright as AB mag ∼23, making them among the brightest known at these redshifts, comparable with discoveries from much wider, blank-field surveys. RELICS demonstrates the efficiency of using strong gravitational lenses to produce high-redshift samples in the epoch of reionization. These brightly observed galaxies are excellent targets for follow-up study with current and future observatories, including the James Webb Space Telescope.

Abstract Copyright: © 2020. The American Astronomical Society. All rights reserved.

Journal keyword(s): Galaxies - galaxies: high-redshift

VizieR on-line data: <Available at CDS (J/ApJ/889/189): table1.dat table234.dat>

Simbad objects: 364

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