about
Rotation in [C ii]-emitting gas in two galaxies at a redshift of 6.8.The evolving far-IR galaxy luminosity function and dust-obscured star formation rate density out to ≃Tracing the Evolution of Dust Obscured Star Formation and Accretion Back to the Reionisation Epoch with SPICAThe MUSE Hubble Ultra Deep Field Survey I. Survey description, data reduction, and source detectionThe ALMA Frontier Fields SurveyThe ALMA Frontier Fields SurveyThe ALMA Redshift 4 Survey (AR4S)
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description
im November 2016 veröffentlichter wissenschaftlicher Artikel
@de
wetenschappelijk artikel
@nl
наукова стаття, опублікована в листопаді 2016
@uk
name
A deep ALMA image of theHubble Ultra Deep Field
@en
A deep ALMA image of theHubble Ultra Deep Field
@nl
type
label
A deep ALMA image of theHubble Ultra Deep Field
@en
A deep ALMA image of theHubble Ultra Deep Field
@nl
prefLabel
A deep ALMA image of theHubble Ultra Deep Field
@en
A deep ALMA image of theHubble Ultra Deep Field
@nl
P2093
P50
P356
P1476
A deep ALMA image of theHubble Ultra Deep Field
@en
P2093
A. D. Biggs
A. Kirkpatrick
B. Robertson
C. C. Hayward
C. Papovich
D. H. Hughes
E. L. Chapin
E. van Kampen
P304
P356
10.1093/MNRAS/STW3088
P407
P50
P577
2016-11-30T00:00:00Z
P818
1606.00227
P819
2017MNRAS.466..861D