Stellar Kinematics and Environment at z ∼ 0.8 in the LEGA-C Survey: Massive Slow Rotators Are Built First in Overdense Environments-Reference-Cited by-同舟云学术

Stellar Kinematics and Environment at z ∼ 0.8 in the LEGA-C Survey: Massive Slow Rotators Are Built First in Overdense Environments

Published:2020-02-20 Issue:2 Volume:890 Page:L25
ISSN:2041-8213
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Cole Justin^ORCID,Bezanson Rachel^ORCID,van der Wel Arjen^ORCID,Bell Eric^ORCID,D’Eugenio Francesco^ORCID,Franx Marijn^ORCID,Gallazzi Anna^ORCID,van Houdt Josha,Muzzin Adam^ORCID,Pacifici Camilla^ORCID,van de Sande Jesse^ORCID,Sobral David^ORCID,Straatman Caroline^ORCID,Wu Po-Feng^ORCID

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/2041-8213/ab7241/pdf

Reference67 articles.

1. Astropy: A community Python package for astronomy

2. USING CUMULATIVE NUMBER DENSITIES TO COMPARE GALAXIES ACROSS COSMIC TIME

3. MOSFIRE SPECTROSCOPY OF QUIESCENT GALAXIES AT 1.5

4. Spatially Resolved Stellar Kinematics from LEGA-C: Increased Rotational Support in z ∼ 0.8 Quiscent Galaxies

Cited by 12 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Lyman-α at Cosmic Noon II: The relationship between kinematics and Lyman-α in z ∼ 2–3 Lyman break galaxies;Publications of the Astronomical Society of Australia;2023-11-30

2. Full spectrum fitting with photometry in ppxf: stellar population versus dynamical masses, non-parametric star formation history and metallicity for 3200 LEGA-C galaxies at redshift z ≈ 0.8;Monthly Notices of the Royal Astronomical Society;2023-08-31

3. Evolution in the orbital structure of quiescent galaxies from MAGPI, LEGA-C, and SAMI surveys: direct evidence for merger-driven growth over the last 7 Gyr;Monthly Notices of the Royal Astronomical Society;2023-08-21

4. Origin of the differences in rotational support among early-type galaxies: The case of galaxies outside clusters;Astronomy & Astrophysics;2023-03-27

5. 3D intrinsic shapes of quiescent galaxies in observations and simulations;Monthly Notices of the Royal Astronomical Society;2022-05-23