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About:
Dust attenuation in UV-selected starbursts at high redshift and their local counterparts: implications for the cosmic star formation rate density
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description
wetenschappelijk artikel
(nl)
article scientifique publié en 2010
(fr)
наукова стаття, опублікована в грудні 2010
(uk)
im Dezember 2010 veröffentlichter wissenschaftlicher Artikel
(de)
publication date
wds:Q59714086-0B482DB4-AACD-4C50-821D-9CA10ED8037E
publication date
2010-12-10 00:00:00Z
(
xsd:dateTime
)
language of work or name
wds:Q59714086-90016131-EB80-4615-8030-42E79B6E4C99
language of work or name
English
author name string
wds:Q59714086-26295682-B5B1-4C87-9951-B546D1031619
wds:Q59714086-4265252F-26B4-4741-9CB4-0F3BC1C6EE99
wds:Q59714086-77C1744F-40CC-49F7-9A08-C29918FC5C04
wds:Q59714086-CE841BD1-279E-48AD-B03A-F66303AB411D
author name string
Justin Howell
D. Christopher Martin
James D. Neill
Thiago S. Gonçalves
rdfs:label
Dust attenuation in UV-selected starbursts at high redshift and their local counterparts: implications for the cosmic star formation rate density
(en)
DUST ATTENUATION IN UV-SELECTED STARBURSTS AT HIGH REDSHIFT AND THEIR LOCAL COUNTERPARTS: IMPLICATIONS FOR THE COSMIC STAR FORMATION RATE DENSITY
(nl)
skos:prefLabel
Dust attenuation in UV-selected starbursts at high redshift and their local counterparts: implications for the cosmic star formation rate density
(en)
DUST ATTENUATION IN UV-SELECTED STARBURSTS AT HIGH REDSHIFT AND THEIR LOCAL COUNTERPARTS: IMPLICATIONS FOR THE COSMIC STAR FORMATION RATE DENSITY
(nl)
name
Dust attenuation in UV-selected starbursts at high redshift and their local counterparts: implications for the cosmic star formation rate density
(en)
DUST ATTENUATION IN UV-SELECTED STARBURSTS AT HIGH REDSHIFT AND THEIR LOCAL COUNTERPARTS: IMPLICATIONS FOR THE COSMIC STAR FORMATION RATE DENSITY
(nl)
author
wds:Q59714086-021E3B0F-CA10-4DAF-909A-F199DD1CD5E3
wds:Q59714086-16C2BD4B-07F4-4F09-9BAD-668A93575C74
wds:Q59714086-22357071-F742-4AC0-B2D3-CAA32679C813
wds:Q59714086-2A3AA339-6E20-4EF3-9425-FE38C8BE00E3
wds:Q59714086-2E18C161-11F7-444A-A8B8-6DD1C9DAEB8B
wds:Q59714086-37A0450A-5907-4EA5-9740-F8B479B8A9D0
wds:Q59714086-4110C5F6-FDFD-4EC2-B0EB-2EBC41B2F3DD
wds:Q59714086-412A5AE4-EE11-4020-A38F-61EF94DEDD03
wds:Q59714086-601CCFD9-B98B-447B-9157-487BD322615D
wds:Q59714086-72BEDBE5-9FD6-4702-8F82-8842559F84CF
wds:Q59714086-9DB6B97A-C44E-4BB1-A273-948DA9BD360B
wds:Q59714086-EB7382F6-FD71-409A-BEE5-C6711D778823
wds:Q59714086-F591403E-3E19-4FBF-9F0F-86BFB2070C67
author
Véronique Buat
Jing Wang
Stéphane Charlot
Robert Rich
Gerhardt Meurer
Roderik Overzier
Samir Salim
David Schiminovich
Lee Armus
Timothy Heckman
Mark Seibert
Brian D. Siana
Antara R. Basu-Zych
title
wds:Q59714086-2ACFABED-08EA-43AC-93E1-A9ED805CA936
title
Dust attenuation in UV-selected starbursts at high redshift and their local counterparts: implications for the cosmic star formation rate density
(en)
page(s)
wds:Q59714086-F7E402B0-9F5B-4354-9F85-F9F128C92EA9
page(s)
7
instance of
wds:Q59714086-01CAE87F-3BD6-4C9D-900B-C6DD943D6265
instance of
scholarly article
published in
wds:Q59714086-AD3649D4-AEFD-4E7B-9485-300A952C3751
full work available at URL
wds:Q59714086-992E36C4-DC76-444B-A0EB-F4CBBBD59A6D
published in
Letters of the Astrophysical Journal
full work available at URL
https://iopscience.iop.org/article/10.1088/2041-8205/726/1/L7/pdf
issue
wds:Q59714086-88202556-F06F-4766-8FF3-DFF4B6B8F7E8
volume
wds:Q59714086-033C8FF3-1147-40E4-9B95-BE5900F1EB65
issue
1
volume
726
DOI
wds:Q59714086-698FBB75-3486-4D85-87B5-A09D18057672
DOI
http://dx.doi.org/10.1088/2041-8205/726/1/L7
DOI
10.1088/2041-8205/726/1/L7
skos:altLabel
DUST ATTENUATION IN UV-SELECTED STARBURSTS AT HIGH REDSHIFT AND THEIR LOCAL COUNTERPARTS: IMPLICATIONS FOR THE COSMIC STAR FORMATION RATE DENSITY
(en)
arXiv ID
wds:Q59714086-745E76A8-C61F-42E9-A561-E5CCEC43718B
arXiv ID
1011.6098
ADS bibcode
wds:Q59714086-9A7B0D06-9564-46F2-A004-2B62217603C1
ADS bibcode
2011ApJ...726L...7O
is
about
of
https://www.wikidata.org/wiki/Special:EntityData/Q59714086
is
cites work
of
The far-infrared, UV, and molecular gas relation in galaxies up to z = 2.5
Interstellar medium conditions in z ~ 0.2 Lyman-break analogs
Lyman Break and ultraviolet-selected galaxies at z ∼ 1 – II. PACS 100 μm/160 μm FIR detections
ALPINE: A Large Survey to Understand Teenage Galaxies
is
cites work
of
wds:Q58911902-F467E491-2433-4F7F-BBF6-772AD0051FFB
wds:Q112766966-E82F9B56-DE5D-4679-98CA-09E2F3786E5A
wds:Q69055533-7C5468B3-43BC-4AAA-8A49-14568A0DD8C2
wds:Q60013019-34DE8E8D-EA11-489F-A1D5-4F355B90C852
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