On the Nature of AGN and Star Formation Enhancement in the z = 3.1 SSA22 Protocluster: The HST WFC3 IR View-Reference-Cited by-同舟云学术

On the Nature of AGN and Star Formation Enhancement in the z = 3.1 SSA22 Protocluster: The HST WFC3 IR View

Published:2021-09-01 Issue:1 Volume:919 Page:51
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Monson Erik B.^ORCID,Lehmer Bret D.^ORCID,Doore Keith^ORCID,Eufrasio Rafael T.^ORCID,Bonine Brett^ORCID,Alexander David M.^ORCID,Harrison Chris M.,Kubo Mariko^ORCID,Mantha Kameswara B.,Saez Cristian,Straughn Amber^ORCID,Umehata Hideki^ORCID

Funder

Space Telescope Science Institute

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/1538-4357/ac0f84/pdf

Reference95 articles.

1. A New Approach to Galaxy Morphology. I. Analysis of the Sloan Digital Sky Survey Early Data Release

2. ALMA observations of az≈ 3.1 protocluster: star formation from active galactic nuclei and Lyman-alpha blobs in an overdense environment

3. The Astropy Project: Building an Open-science Project and Status of the v2.0 Core Package

4. Astropy: A community Python package for astronomy

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