The MOSDEF Survey: Broad Emission Lines at z = 1.4–3.8

The MOSDEF Survey: Broad Emission Lines at z = 1.4–3.8

We present results from the MOSFIRE Deep Evolution Field survey on broad flux from the nebular emission lines H α , [N ii ], [O iii ], H β , and [S ii ]. The sample consists of 127 star-forming galaxies at 1.37 

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Veröffentlicht in:The Astrophysical journal 2019-03, Vol.873 (2), p.102
Hauptverfasser: Freeman, William R., Siana, Brian, Kriek, Mariska, Shapley, Alice E., Reddy, Naveen, Coil, Alison L., Mobasher, Bahram, Muratov, Alexander L., Azadi, Mojegan, Leung, Gene, Sanders, Ryan, Shivaei, Irene, Price, Sedona H., DeGroot, Laura, Kereš, Dušan
Format: Artikel
Sprache:eng
Schlagworte:
Active galactic nuclei
Astrophysics
Diagnostic systems
Emission
Emission lines
Fluctuations
Flux
Galaxies
H alpha line
Outflow
Physical properties
Polls & surveys
Stacks
Star & galaxy formation
Star formation
Star formation rate
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Zusammenfassung:We present results from the MOSFIRE Deep Evolution Field survey on broad flux from the nebular emission lines H α , [N ii ], [O iii ], H β , and [S ii ]. The sample consists of 127 star-forming galaxies at 1.37 
ISSN:0004-637X
1538-4357
DOI:10.3847/1538-4357/ab0655