Structural and Star-forming Relations since z similar to 3: Connecting Compact Star-forming and Quiescent Galaxies
Guillermo Barro,Guillermo Barro,S. M. Faber,David C. Koo,Avishai Dekel,Jerome J. Fang,Jonathan R. Trump,Pablo G. Pérez-González,Camilla Pacifici,Joel R. Primack,Rachel S. Somerville,Haojing Yan,Yicheng Guo,F. S. Liu,Daniel Ceverino,Dale D. Kocevski,Elizabeth J. McGrath +16 more
TLDR
In this article, the authors study the evolution of scaling relations that compare the effective density (Sigma(e), r 9.6 -9.3M(circle dot) kpc(-2), allowing the most efficient identification of compact SFGs and quiescent galaxies at every redshift.Abstract:
We study the evolution of the scaling relations that compare the effective density (Sigma(e), r 9.6 -9.3M(circle dot) kpc(-2), allowing the most efficient identification of compact SFGs and quiescent galaxies at every redshift.read more
Citations
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The intrinsic characteristics of galaxies on the SFR-stellar mass plane at 1.2<z<4: I. the correlation between stellar age, central density and position relative to the main sequence
Bomee Lee,Mauro Giavalisco,Katherine E. Whitaker,Christina C. Williams,Henry C. Ferguson,Viviana Acquaviva,Anton M. Koekemoer,Amber Straughn,Yicheng Guo,Jeyhan S. Kartaltepe,Jennifer M. Lotz,Camilla Pacifici,Darren J. Croton,Rachel S. Somerville,Yu Lu +14 more
TL;DR: In this paper, the authors used the deep CANDELS observations in the GOODS North and South fields to revisit the correlations between stellar mass, star-formation rate (SFR), and morphology, and to introduce a fourth dimension, the mass-weighted stellar age, in galaxies at 1.2
Journal ArticleDOI
Spatially Resolved Kinematics in the Central 1 kpc of a Compact Star-forming Galaxy at z ∼ 2.3 from ALMA CO Observations
Guillermo Barro,Guillermo Barro,Mariska Kriek,Pablo G. Pérez-González,Tanio Díaz-Santos,Sedona H. Price,Wiphu Rujopakarn,Wiphu Rujopakarn,Wiphu Rujopakarn,Viraj Pandya,David C. Koo,S. M. Faber,Avishai Dekel,Joel R. Primack,Dale D. Kocevski +14 more
TL;DR: In this paper, high spatial resolution (FWHM) observations of the CO(8-7) line in GDS-14876, a compact star-forming galaxy at z = 2.3 with a total stellar mass of log(M-*/M-circle dot) = 10.5.
Journal ArticleDOI
The Intrinsic Characteristics of Galaxies on the SFR–M ∗ Plane at 1.2 < z < 4: I. The Correlation between Stellar Age, Central Density, and Position Relative to the Main Sequence
Bomee Lee,Bomee Lee,Mauro Giavalisco,Katherine E. Whitaker,Katherine E. Whitaker,Christina C. Williams,Henry C. Ferguson,Viviana Acquaviva,Anton M. Koekemoer,Amber N. Straughn,Yicheng Guo,Yicheng Guo,Jeyhan S. Kartaltepe,Jennifer M. Lotz,Camilla Pacifici,Darren J. Croton,Rachel S. Somerville,Rachel S. Somerville,Yu Lu +18 more
TL;DR: In this article, the Downsbrough family presented a method for using the Hubble Space Telescope Science Institute (HF2-51368) grant for the development of the Huygulu Telescope.
Journal ArticleDOI
The Role of Black Hole Feedback on Size and Structural Evolution in Massive Galaxies
Ena Choi,Ena Choi,Rachel S. Somerville,Jeremiah P. Ostriker,Jeremiah P. Ostriker,Thorsten Naab,Michaela Hirschmann +6 more
TL;DR: In this paper, the role of feedback from accreting black holes on the evolution of sizes, compactness, stellar core density and specific star-formation of massive galaxies with stellar masses of $ M{star} > 10^{10.9} M_{\odot} was investigated.
Journal ArticleDOI
Stochastic modelling of star-formation histories I: the scatter of the star-forming main sequence
Neven Caplar,Sandro Tacchella +1 more
TL;DR: In this paper, a framework for modelling the star-formation histories of galaxies as a stochastic process is presented, based on a power spectrum density with a functional form of a broken power-law.
References
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Gustavo Bruzual,Stephane Charlot +1 more
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