CoChat
Sign Up
Cited by 143Galaxies: Formation, Evolution, PhenomenaStellar, planetary, and galactic studiesAstrophysics and Star Formation Studies

The DOI matches its Crossref record; 173 of the 173 references it cites were found in a registry or an index.

ZFOURGE/CANDELS: ON THE EVOLUTION OF M* GALAXY PROGENITORS FROM z= 3 TO 0.5

Open access
Papovich, C., Labbé, I., Quadri, R., Tilvi, V., Behroozi, P., Bell, E. F., Glazebrook, K., Spitler, L., Straatman, C. M. S., Tran, K.-V., Cowley, M., Davé, R., Dekel, A., Dickinson, M., Ferguson, H. C., Finkelstein, S. L., Gawiser, E., Inami, H., Faber, S. M., Kacprzak, G. G., Kawinwanichakij, L., Kocevski, D., Koekemoer, A., Koo, D. C., Kurczynski, P., Lotz, J. M., Lu, Y., Lucas, R. A., McIntosh, D., Mehrtens, N., Mobasher, B., Monson, A., Morrison, G., Nanayakkara, T., Persson, S. E., Salmon, B., Simons, R., Tomczak, A., van Dokkum, P., Weiner, B., Willner, S. P.·2015·The Astrophysical Journal
DOI 10.1088/0004-637x/803/1/26
Open this paper in CoChat — free accountOpen PDF

Abstract

Galaxies with stellar masses near M * contain the majority of stellar mass in the universe, and are therefore of special interest in the study of galaxy evolution. The Milky Way (MW) and Andromeda (M31) have present-day stellar masses near M *, at 5 × 10 10 M ☉ (defined here to be MW-mass) and 10 11 M ☉ (defined to be M31-mass). We study the typical progenitors of these galaxies using the FourStar Galaxy Evolution Survey (ZFOURGE). ZFOURGE is a deep medium-band near-IR imaging survey, which is sensitive to the progenitors of these galaxies out to z ∼ 3. We use abundance-matching techniques to identify the main progenitors of these galaxies at higher redshifts. We measure the evolution in the stellar mass, rest-frame colors, morphologies, far-IR luminosities, and star formation rates, combining our deep multiwavelength imaging with near-IR Hubble Space Telescope imaging from Cosmic Near-IR Deep Extragalactic Legacy Survey (CANDELS), and Spitzer and Herschel far-IR imaging from Great Observatories Origins Deep Survey-Herschel and CANDELS-Herschel. The typical MW-mass and M31-mass progenitors passed through the same evolution stages, evolving from blue, star-forming disk galaxies at the earliest stages to redder dust-obscured IR-luminous galaxies in intermediate stages and to red, more quiescent galaxies at their latest stages. The progenitors of the MW-mass galaxies reached each evolutionary stage at later times (lower redshifts) and with stellar masses that are a factor of two to three lower than the progenitors of the M31-mass galaxies. The process driving this evolution, including the suppression of star formation in present-day M * galaxies, requires an evolving stellar-mass/halo-mass ratio and/or evolving halo-mass threshold for quiescent galaxies. The effective size and SFRs imply that the baryonic cold-gas fractions drop as galaxies evolve from high redshift to z ∼ 0 and are strongly anticorrelated with an increase in the Sérsic index. Therefore, the growth of galaxy bulges in M * galaxies corresponds to a rapid decline in the galaxy gas fractions and/or a decrease in the star formation efficiency.

Overview

The claims and statistics of this paper haven’t been checked yet.

Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.

A few free checks a day · papers already verified open instantly · results are public

Integrity signals

Registry

Crossref · 10.1088/0004-637x/803/1/26

Cites

173 of 173 references verified0 citation errors · 0 not checkable

Statistics

Verification

Claims the paper makes

The claims and statistics of this paper haven’t been checked yet.

Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.

A few free checks a day · papers already verified open instantly · results are public

Self-check

Percentages, sums and reported differences re-computed from the paper’s own numbers.

The self-check needs the paper’s full text.

Citations

Cites

Show all 172 references

Research works printed but not linked: 4

  1. Baldry, 2008, MNRAS, 388, 945
  2. Licquia, 2014, ApJ
  3. Popesso, 2012, A&A
  4. Schreiber, 2014, A&A

Cited by

Sorted by citations

See all 143

Related

Metadata

Authors
Papovich, C., Labbé, I., Quadri, R., Tilvi, V., Behroozi, P., Bell, E. F., Glazebrook, K., Spitler, L., Straatman, C. M. S., Tran, K.-V., Cowley, M., Davé, R., Dekel, A., Dickinson, M., Ferguson, H. C., Finkelstein, S. L., Gawiser, E., Inami, H., Faber, S. M., Kacprzak, G. G., Kawinwanichakij, L., Kocevski, D., Koekemoer, A., Koo, D. C., Kurczynski, P., Lotz, J. M., Lu, Y., Lucas, R. A., McIntosh, D., Mehrtens, N., Mobasher, B., Monson, A., Morrison, G., Nanayakkara, T., Persson, S. E., Salmon, B., Simons, R., Tomczak, A., van Dokkum, P., Weiner, B., & Willner, S. P.
Affiliations
  • Texas A&M University (US)
  • Leiden University (NL)
  • Space Telescope Science Institute (US)
  • University of Michigan (US)
  • Swinburne University of Technology (AU)
  • Australian Astronomical Observatory (AU)
  • Macquarie University (AU)
  • African Institute for Mathematical Sciences (ZA)
  • Hebrew University of Jerusalem (IL)
  • The University of Texas at Austin (US)
  • Rutgers, The State University of New Jersey (US)
  • University of California, Santa Cruz (US)
  • University of Kentucky (US)
  • Kavli Institute for Particle Astrophysics and Cosmology (US)
  • University of Missouri–Kansas City (US)
  • University of California, Riverside (US)
  • Carnegie Observatories (US)
  • University of Hawaiʻi at Mānoa (US)
  • Johns Hopkins University (US)
  • University of Arizona (US)
  • Center for Astrophysics Harvard & Smithsonian (US)
Corresponding author
Papovich, C.
ORCID
Venue
The Astrophysical Journal
Publisher
American Astronomical Society
Published
2015-04-09
Volume
803
Issue
1
Pages
26
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
DOI
10.1088/0004-637x/803/1/26
OpenAlex
W2092240391
Cited by
143
References
172
Citations by year
2026: 2 · 2025: 9 · 2024: 12 · 2023: 5 · 2022: 7 · 2021: 4 · 2020: 9 · 2019: 18 · 2018: 18 · 2017: 23 · 2016: 25 · 2015: 11
FWCI
14.61
Type
journal article
Language
he
Open access
Licence
Locations
  • The Astrophysical Journal (publishedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • QUT ePrints (Queensland University of Technology) (submittedVersion)
  • UKnowledge (University of Kentucky) (submittedVersion)
  • Leiden Repository (Leiden University) (submittedVersion)
  • Data Archiving and Networked Services (DANS) (submittedVersion, other-oa)
  • Ghent University Academic Bibliography (Ghent University) (submittedVersion)
  • OakTrust (Texas A&M University Libraries) (submittedVersion)
  • Swinburne figshare (Swinburne University of Technology) (submittedVersion)
  • arXiv (Cornell University)
Funders
  • National Science Foundation (1009707, 0808133)
  • National Aeronautics and Space Administration (NASA contract NAS5-26555, GO-12060, NAS 526555)
  • California Institute of Technology
  • Space Telescope Science Institute (NAS5- 26555, 26555)
  • Australian Government
  • Nederlandse Organisatie voor Wetenschappelijk Onderzoek
  • Jet Propulsion Laboratory
  • FP7 Ideas: European Research Council (227749)
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysics and Star Formation Studies
Keywords
galaxy progenitors, galaxy evolution, abundance matching, Milky Way progenitors, far-infrared luminosity, star formation rate, dust-obscured galaxies, quiescent galaxies, cold gas fraction, bulge growth, Sérsic index, CANDELS

About these checks

Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.

Statistics and arithmetic are recomputed, not judged.

Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.

What counts as a claim ›How we measure confidence ›How we check this ›

Are you an author, or do you see a problem with this page? Request a review