Results 121 to 130 of about 49,160 (208)
We present new Hubble Space Telescope/Wide Field Camera 3 G141 grism observations for COBRA 1411+3415, originally identified as a high-redshift cluster candidate in the Clusters Occupied by Bent Radio AGN (COBRA) survey using radio, infrared, and optical
Courtney B. Watson +6 more
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Galaxy Clusters and Large Scale Structure at High Redshifts
We present a detailed study of a rich galaxy cluster at z=2.38. We demonstrate that this cluster contains large overdensities of damped Ly-alpha absorption lines, of Ly-alpha emitting galaxies and of extremely red objects. The overdensity of extremely red objects in this field demonstrates that many are high z galaxies.
Francis, Paul J. +2 more
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We present a selection of candidates of clusters and protoclusters of galaxies identified in the photometric data of the HSC-SSP Wide Public Data Release 3 (PDR3), spanning the redshift range 0.1 ≤ z ≤ 2. The selection method, detailed in Vicentin et al.,
Marcelo C. Vicentin +4 more
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Is Earendel a Star Cluster?: Metal-poor Globular Cluster Progenitors at z ∼ 6
The strongly lensed z ∼ 6 Sunrise galaxy offers an incredible opportunity to investigate star formation in the early Universe on parsec or smaller scales.
Massimo Pascale +3 more
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Efficient Survey Design for Finding High-redshift Galaxies with JWST
Several large JWST blank field observing programs have not yet discovered the first galaxies expected to form at 15 ≤ z ≤ 20. This has motivated the search for more effective survey strategies that will be able to effectively probe this redshift range ...
Luka Vujeva +11 more
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A Type Ia supernova (SN) at z = 1.78 was discovered in James Webb Space Telescope Near Infrared Camera imaging of the galaxy cluster PLCK G165.7+67.0 (G165; z = 0.35).
Brenda L. Frye +40 more
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Clusters of galaxies host spectacular diffuse radio sources, extending over scales from 100 kpc to several Mpcs. These sources, with extremely faint surface brightness ( μ Jy/arcsec ^2 level), are not tied to individual galaxies but trace synchrotron ...
Julie HLavacek-Larrondo +12 more
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Cluster Candidates with Massive Quiescent Galaxies at z ∼ 2
Galaxy clusters are crucial to understanding the role of the environment in galaxy evolution. However, due to their rarity, only a limited number of clusters have been identified at z ≳ 2. In this paper, we report a discovery of seven cluster candidates
Tomokazu Kiyota +9 more
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The Photometric Analysis of the Environment Around Two Dusty Star-forming Galaxies at z ∼ 2
Studying the environments of dusty star-forming galaxies (DSFGs) provides insight into whether these luminous systems are reliable signposts of large-scale overdensities.
Joe Bhangal +9 more
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High-Redshift Quasars as Probes of Galaxy and Cluster Formation
Invited review, to appear in ``The Hy-Redshift Universe: Galaxy Formation and Evolution at High Redshift'', eds. A.J. Bunker and W.J.M. van Breugel, A.S.P.Conf.Ser. in press (1999).
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