About: The spectral energy distributions of z ~ 8 galaxies from the IRAC ultra deep fields: emission lines, stellar masses, and specific star formation rates at 650 myr

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About: The spectral energy distributions of z ~ 8 galaxies from the IRAC ultra deep fields: emission lines, stellar masses, and specific star formation rates at 650 myr Goto Sponge NotDistinct Permalink

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scholarly article

Attributes	Values
rdf:type	Item
description	artículu científicu (ast) wetenschappelijk artikel (nl) scholarly article (en) наукова стаття, опублікована в жовтні 2013 (uk) article scientifique publié en 2013 (fr) im Oktober 2013 veröffentlichter wissenschaftlicher Artikel (de)
publication date	wds:Q58922855-B24AA06E-9447-434D-B3BA-EDA89EB70EA0
publication date	2013-10-22 00:00:00Z (xsd:dateTime)
language of work or name	wds:Q58922855-E46BF697-68ED-476C-899E-9E69D63F873E
language of work or name	English
author name string	wds:Q58922855-748FA170-F3DC-4297-B59F-B51DDE392D22
author name string	D. Magee
rdfs:label	THE SPECTRAL ENERGY DISTRIBUTIONS OFz∼ 8 GALAXIES FROM THE IRAC ULTRA DEEP FIELDS: EMISSION LINES, STELLAR MASSES, AND SPECIFIC STAR FORMATION RATES AT 650 MYR (nl) The spectral energy distributions of z ~ 8 galaxies from the IRAC ultra deep fields: emission lines, stellar masses, and specific star formation rates at 650 myr (en)
skos:prefLabel	THE SPECTRAL ENERGY DISTRIBUTIONS OFz∼ 8 GALAXIES FROM THE IRAC ULTRA DEEP FIELDS: EMISSION LINES, STELLAR MASSES, AND SPECIFIC STAR FORMATION RATES AT 650 MYR (nl) The spectral energy distributions of z ~ 8 galaxies from the IRAC ultra deep fields: emission lines, stellar masses, and specific star formation rates at 650 myr (en)
name	THE SPECTRAL ENERGY DISTRIBUTIONS OFz∼ 8 GALAXIES FROM THE IRAC ULTRA DEEP FIELDS: EMISSION LINES, STELLAR MASSES, AND SPECIFIC STAR FORMATION RATES AT 650 MYR (nl) The spectral energy distributions of z ~ 8 galaxies from the IRAC ultra deep fields: emission lines, stellar masses, and specific star formation rates at 650 myr (en)
author	wds:Q58922855-0F25C6E2-03FA-449C-B957-E3BA0191BD3A wds:Q58922855-23D2A274-F88D-48D0-B67D-B74E75530995 wds:Q58922855-310B14F8-AFFE-4C47-947E-4F8FEA518580 wds:Q58922855-352BC6F1-89AB-486A-A704-D9432C8BB722 wds:Q58922855-6A74D1F7-E125-4A20-BF39-0AB53F1DF71F wds:Q58922855-762645AA-4B5A-486A-B3A0-707320C92626 wds:Q58922855-83A38B76-64E2-4AC9-90FA-2954B9B0EF11 wds:Q58922855-9F252172-297D-4DF5-8575-125EB05240BF wds:Q58922855-A5251F3E-56C2-4675-B82D-47FC4DAFA3CB wds:Q58922855-D1CC1451-8F70-42D0-81D9-968B9C8A9196
author	Marijn Franx Rychard Bouwens Marcella Carollo Garth D. Illingworth Massimo Stiavelli Michele Trenti Pieter van Dokkum Ivo Labbé Pascal Oesch Valentino Gonzalez
title	wds:Q58922855-89E68F4B-6C67-4566-B415-21091C53AA41
title	The spectral energy distributions of z ~ 8 galaxies from the IRAC ultra deep fields: emission lines, stellar masses, and specific star formation rates at 650 myr (en)
page(s)	wds:Q58922855-ABA32B7C-2ED0-4B77-8735-2D841AFDB317
page(s)	19
instance of	wds:Q58922855-A5091EEB-0C3A-44C2-B852-50EBA5E3C102
instance of	scholarly article
published in	wds:Q58922855-79498F2B-2B43-4202-ADC0-E1A5F5724190
full work available at URL	wds:Q58922855-1A579AEB-BD3F-451C-A44C-1DD2F432329F
published in	Letters of the Astrophysical Journal
full work available at URL	https://iopscience.iop.org/article/10.1088/2041-8205/777/2/L19/pdf
issue	wds:Q58922855-23C2C40A-0262-4066-8001-9C9D9657A81D
volume	wds:Q58922855-49E683CC-A581-4D69-B1FE-A5BEEA8F0DA1
issue	2
volume	777
DOI	wds:Q58922855-3C9436CF-A735-4BA7-86B6-A48A123F9135
DOI	http://dx.doi.org/10.1088/2041-8205/777/2/L19
DOI	10.1088/2041-8205/777/2/L19
arXiv ID	wds:Q58922855-9E3450FE-E18B-46DC-B163-57BD2B216C79
arXiv ID	1209.3037
ADS bibcode	wds:Q58922855-4460E9D9-1C28-4A51-9C3F-42B26A64CC0A
ADS bibcode	2013ApJ...777L..19L
is about of	https://www.wikidata.org/wiki/Special:EntityData/Q58922855
is cites work of	Ly α EMISSION FROM A LUMINOUS z = 8.68 GALAXY: IMPLICATIONS FOR GALAXIES AS TRACERS OF COSMIC REIONIZATION The galaxy stellar mass function at 3.5 ≤ z ≤ 7.5 in the CANDELS/UDS, GOODS-South, and HUDF fields The first Frontier Fields cluster: 4.5μm excess in az~ 8 galaxy candidate in Abell 2744 Frontier Fields: Combining HST, VLT, andSpitzerdata to explore thez~ 8 Universe behind the lensing cluster MACSJ0416.1−2403 A spectroscopic redshift measurement for a luminous Lyman break galaxy at z = 7.730 using Keck/MOSFIRE Spectroscopic detections of C iii] λ1909 Å at z ≃ 6–7: a new probe of early star-forming galaxies and cosmic reionization Detecting direct collapse black holes: making the case for CR7 A 52 hours VLT/FORS2 spectrum of a bright z ~ 7 HUDF galaxy: no Ly-α emission Discovery of a Dark, Massive, ALMA-only Galaxy at z ~ 5–6 in a Tiny 3 mm Survey An extreme [O III] emitter atz= 3.2: a low metallicity Lyman continuum source Ultraviolet emission lines in young low-mass galaxies at z ≃ 2: physical properties and implications for studies at z > 7 ALMA Measures Molecular Gas Reservoirs Comparable to Field Galaxies in a Low-mass Galaxy Cluster at z = 1.3 ZFIRE: using Hα equivalent widths to investigate the in situ initial mass function at z ∼ 2 Ultraviolet spectra of extreme nearby star-forming regions – approaching a local reference sample for JWST Spectroscopic confirmation of an ultra-faint galaxy at the epoch of reionization
is cites work of	wds:Q58907773-D59BDE95-1CCA-4D7D-B5DD-C01DBFBC1A0E wds:Q58489695-64AA90A8-560F-4616-AFB3-305FBC70EE2C wds:Q58908305-FD2FA32D-48EC-4F32-98C8-B0430E477911 wds:Q21710613-5770840E-8082-4D2B-BAAE-2B04E218D7EB wds:Q21710624-F8AB0386-C062-4734-9DF7-A4C2908501A3 wds:Q58910624-6112634F-5771-4F73-8B13-5D66F4BF416B wds:Q72015559-56DFAF6D-BA18-4334-9968-6913BEDCBC0A wds:Q58909401-2AB80246-E6F1-4C75-AF4E-05590E677363 wds:Q59268268-E222ED07-C521-4172-AA53-6DDF134A9058 wds:Q59943121-0C3B1BC6-EC66-4E12-97DB-561EC9B4ED62 wds:Q59111058-6D5C59D7-1FA5-4B7C-9947-CBED221E3289 wds:Q59111081-DA6CD99B-21BE-4340-B6DC-2615708F3CD3 wds:Q59111074-D82A9463-814F-4043-AE7B-1D0590B65452 wds:Q58213184-853F2846-B758-483A-A583-32FA5A7885D9 wds:Q114816033-08E39490-9E6B-4E5A-9066-BCD189804722

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