About: Reversal of fortune: confirmation of an increasing star formation-density relation in a cluster at z = 1.62

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About: Reversal of fortune: confirmation of an increasing star formation-density relation in a cluster at z = 1.62 Goto Sponge NotDistinct Permalink

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rdf:type	Item
description	wetenschappelijk artikel (nl) article scientifique publié en 2010 (fr) наукова стаття, опублікована в липні 2010 (uk) im Juli 2010 veröffentlichter wissenschaftlicher Artikel (de)
publication date	wds:Q59716020-51102AE6-147B-4B8B-BF1F-B14D4135F261
publication date	2010-07-27 00:00:00Z (xsd:dateTime)
language of work or name	wds:Q59716020-FA6808FE-D94B-414E-A3AA-A44ACD060FA8
language of work or name	English
author name string	wds:Q59716020-10A7365F-4DC2-488D-8BB4-7C7D36649C32 wds:Q59716020-2D781DEB-82F0-4FB1-8084-081EF34E8DA6 wds:Q59716020-45744392-DCE3-424A-ADD1-899BFDA3911B wds:Q59716020-A8BF6E1E-3522-47DE-90D6-BF354A67D327 wds:Q59716020-CF77FB9A-0CF5-4ADE-B964-2F59A8B8B432 wds:Q59716020-FE0F355D-E7A8-4BEE-92F6-40C193A55631
author name string	Mark Brodwin Kim-Vy H. Tran Duncan Farrah Christopher N. A. Willmer Ross J. McLure Keely D. Finkelstein
rdfs:label	Reversal of fortune: confirmation of an increasing star formation-density relation in a cluster at z = 1.62 (en) REVERSAL OF FORTUNE: CONFIRMATION OF AN INCREASING STAR FORMATION–DENSITY RELATION IN A CLUSTER AT z = 1.62 (nl)
skos:prefLabel	Reversal of fortune: confirmation of an increasing star formation-density relation in a cluster at z = 1.62 (en) REVERSAL OF FORTUNE: CONFIRMATION OF AN INCREASING STAR FORMATION–DENSITY RELATION IN A CLUSTER AT z = 1.62 (nl)
name	Reversal of fortune: confirmation of an increasing star formation-density relation in a cluster at z = 1.62 (en) REVERSAL OF FORTUNE: CONFIRMATION OF AN INCREASING STAR FORMATION–DENSITY RELATION IN A CLUSTER AT z = 1.62 (nl)
author	wds:Q59716020-047F3E97-747F-45D1-9FE4-801FC986B1DB wds:Q59716020-319703D8-EDDA-4A76-890B-C4A961BBAAB3 wds:Q59716020-81EFE0E6-AFEB-4601-815A-BD71D7F04C33 wds:Q59716020-B7C843F7-D30E-4245-80EC-9A9AC9BEBFF4 wds:Q59716020-DD9755E4-715C-4FB2-9591-3856D3B574F2 wds:Q59716020-FE67D9D5-FA60-49CA-A7A3-0B8D7349C93B
author	James Scott Dunlop Jennifer Lotz Steven Finkelstein Casey Papovich Ivelina Momcheva Amélie Saintonge
title	wds:Q59716020-3EFD0074-E683-4252-902A-8A70049E66FC
title	Reversal of fortune: confirmation of an increasing star formation-density relation in a cluster at z = 1.62 (en)
page(s)	wds:Q59716020-F3A7FA30-B30E-4A93-A4F2-E3653834480A
page(s)	126–129
instance of	wds:Q59716020-F7EE1CCC-671E-4CEA-A5AC-0DE9745C60F0
instance of	scholarly article
published in	wds:Q59716020-EF9EDC3E-B97A-413A-944A-C179DAA6264F
full work available at URL	wds:Q59716020-AE1D4428-DFEE-4B9F-BA24-F7DFE8481F9A
published in	Letters of the Astrophysical Journal
full work available at URL	https://iopscience.iop.org/article/10.1088/2041-8205/719/2/L126/pdf
issue	wds:Q59716020-B120A135-F6A0-44D1-A1EC-4012F0788BF8
volume	wds:Q59716020-7891AD2F-7C29-4064-A18F-573D4BE44A5B
issue	2
volume	719
DOI	wds:Q59716020-D6A12676-73B2-4805-B683-0E57DCBEBC0E
DOI	http://dx.doi.org/10.1088/2041-8205/719/2/L126
DOI	10.1088/2041-8205/719/2/L126
arXiv ID	wds:Q59716020-6263BDC2-662C-46DC-AA8E-922890F85499
arXiv ID	1005.5126
ADS bibcode	wds:Q59716020-CF7738BE-7864-42AB-B539-C530F02BA24D
ADS bibcode	2010ApJ...719L.126T
is about of	https://www.wikidata.org/wiki/Special:EntityData/Q59716020
is cites work of	The effect of environment on star forming galaxies at redshift Reversal or no reversal: the evolution of the star formation rate–density relation up to z ∼ 1.6 Discovery of a strong lensing galaxy embedded in a cluster at z = 1.62 ALMA Observations of Gas-rich Galaxies in z ∼ 1.6 Galaxy Clusters: Evidence for Higher Gas Fractions in High-density Environments The lack of star formation gradients in galaxy groups up to z ∼ 1.6 The Massive and Distant Clusters of WISE Survey. I. Survey Overview and a Catalog of >2000 Galaxy Clusters at z ≃ 1 ALMA Measures Molecular Gas Reservoirs Comparable to Field Galaxies in a Low-mass Galaxy Cluster at z = 1.3 On the Gas Content, Star Formation Efficiency, and Environmental Quenching of Massive Galaxies in Protoclusters at <i>z</i> ≈ 2.0–2.5 Galaxy Merger Candidates in High-redshift Cluster Environments
is cites work of	wds:Q59740605-7F5A0B72-BCE5-4CB2-B868-C259EEFA9A50 wds:Q62624325-482C8EC4-4CAD-438C-A243-79E68F1D7F40 wds:Q58911976-5718980A-1FBC-4C50-BA95-75720DBD4C58 wds:Q21710631-AA73090D-ED3C-440B-9417-01918BD30987 wds:Q59740600-91FB0EF4-710C-4C91-A3FA-248B7CEFD460 wds:Q58909486-DC6E889F-39BA-4CAC-B836-B5E4BE6E2319 wds:Q58909544-34888053-2625-439D-9D59-1C811302C735 wds:Q114816038-EB937DC6-E2C4-4344-A9B3-C81B5E200BC3 wds:Q114816033-F301D8F4-A97B-49D3-BADB-AE751D15A5B0

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