The Frontier Fields: Survey Design and Initial Results-Reference-Cited by-同舟云学术

The Frontier Fields: Survey Design and Initial Results

Published:2017-03-07 Issue:1 Volume:837 Page:97
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Lotz J. M.^ORCID,Koekemoer A.^ORCID,Coe D.^ORCID,Grogin N.,Capak P.,Mack J.,Anderson J.,Avila R.,Barker E. A.,Borncamp D.,Brammer G.^ORCID,Durbin M.,Gunning H.,Hilbert B.^ORCID,Jenkner H.,Khandrika H.,Levay Z.,Lucas R. A.,MacKenty J.,Ogaz S.,Porterfield B.,Reid N.,Robberto M.^ORCID,Royle P.,Smith L. J.^ORCID,Storrie-Lombardi L. J.^ORCID,Sunnquist B.,Surace J.^ORCID,Taylor D. C.,Williams R.,Bullock J.,Dickinson M.,Finkelstein S.^ORCID,Natarajan P.^ORCID,Richard J.^ORCID,Robertson B.^ORCID,Tumlinson J.^ORCID,Zitrin A.^ORCID,Flanagan K.,Sembach K.,Soifer B. T.,Mountain M.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/837/i=1/a=97/pdf

Reference230 articles.

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3. Galaxy morphology to I=25 mag in the Hubble Deep Field

4. ULTRA-FAINT ULTRAVIOLET GALAXIES ATz∼ 2 BEHIND THE LENSING CLUSTER A1689: THE LUMINOSITY FUNCTION, DUST EXTINCTION, AND STAR FORMATION RATE DENSITY

5. THE EVOLUTION OF THE FAINT END OF THE UV LUMINOSITY FUNCTION DURING THE PEAK EPOCH OF STAR FORMATION $(1\lt z\lt 3)$

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