Physical Properties of Sub-galactic Clumps at 0.5 ≤Z≤ 1.5 in the UVUDF-Reference-Cited by-同舟云学术

Physical Properties of Sub-galactic Clumps at 0.5 ≤Z≤ 1.5 in the UVUDF

Published:2017-02-27 Issue:1 Volume:837 Page:6
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Soto Emmaris^ORCID,Mello Duilia F. de^ORCID,Rafelski Marc^ORCID,Gardner Jonathan P.,Teplitz Harry I.^ORCID,Koekemoer Anton M.^ORCID,Ravindranath Swara,Grogin Norman A.^ORCID,Scarlata Claudia^ORCID,Kurczynski Peter^ORCID,Gawiser Eric^ORCID

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/837/i=1/a=6/pdf

Reference90 articles.

1. The Morphologies of Distant Galaxies. II. Classifications from the Hubble Space Telescope Medium Deep Survey

2. HIGH-RESOLUTION STUDY OF THE CLUSTER COMPLEXES IN A LENSED SPIRAL AT REDSHIFT 1.5: CONSTRAINTS ON THE BULGE FORMATION AND DISK EVOLUTION

3. Disc formation and the origin of clumpy galaxies at high redshift

4. The Hubble Ultra Deep Field

5. SExtractor: Software for source extraction

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