Age, metallicity, and star formation history of spheroidal galaxies in cluster atz∼ 1.2-Reference-Cited by-同舟云学术

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Age, metallicity, and star formation history of spheroidal galaxies in cluster atz∼ 1.2

Published:2018-12-29 Issue:2 Volume:484 Page:2281-2295
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Saracco P¹^ORCID,La Barbera F²,Gargiulo A³,Mannucci F⁴,Marchesini D⁵,Nonino M⁶,Ciliegi P⁷

Affiliation:

1. INAF – Osservatorio Astronomico di Brera, via Brera 28, I-20121 Milano, Italy

2. INAF – Osservatorio Astronomico di Capodimonte, sal. Moiariello 16, I-80131 Napoli, Italy

3. INAF – Istituto di Astrofisica e Fisica Cosmica, IASF, via E. Bassini 15, I-20133 Milano, Italy

4. INAF – Osservatorio Astrofisico di Arcetri, Largo Enrico Fermi 5, I-50125 Firenze, Italy

5. Physics and Astronomy Department, Tufts University, 574 Boston Ave, Medford, 02155 MA, USA

6. INAF – Osservatorio Astronomico di Trieste, Via G.B. Tiepolo 11, I-34143 Trieste, Italy

7. INAF – Osservatorio Astronomico di Bologna, Via Piero Gobetti, 93/3, 40129 Bologna, Italy

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/484/2/2281/27635740/sty3509.pdf

Reference97 articles.

1. Batch discovery of ninez∼ 1 clusters using X-ray andKorR,z′ images

2. The history of star-forming galaxies in the Sloan Digital Sky Survey

3. Differential Galaxy Evolution in Cluster and Field Galaxies at \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $z\approx 0.3$ \end{document}

4. The KMOS Cluster Survey (KCS). I. The Fundamental Plane and the Formation Ages of Cluster Galaxies at Redshift 1.4

5. On the spectral resolution of the MILES stellar library

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1. The Heavy Metal Survey: Star Formation Constraints and Dynamical Masses of 21 Massive Quiescent Galaxies at z = 1.3–2.3;The Astrophysical Journal;2024-04-24

2. The star formation history and the nature of the mass–metallicity relation of passive galaxies at 1.0 <z< 1.4 from VANDELS;Monthly Notices of the Royal Astronomical Society;2023-01-23

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4. MAGAZ3NE: High Stellar Velocity Dispersions for Ultramassive Quiescent Galaxies at z ≳ 3*;The Astrophysical Journal;2022-10-01

5. Reconstructing the Assembly of Massive Galaxies. I. The Importance of the Progenitor Effect in the Observed Properties of Quiescent Galaxies at z ≈ 2;The Astrophysical Journal;2022-08-01

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