A redshift-independent efficiency model: star formation and stellar masses in dark matter halos at z≳ 4
We explore the connection between the UV luminosity functions (LFs) of high-z galaxies and
the distribution of stellar masses and star formation histories (SFHs) in their host dark matter …
the distribution of stellar masses and star formation histories (SFHs) in their host dark matter …
GOODS-ALMA: 1.1 mm galaxy survey-I. Source catalog and optically dark galaxies
Aims. We present a 69 arcmin 2 ALMA survey at 1.1 mm, GOODS-ALMA, matching the
deepest HST-WFC3 H-band part of the GOODS-South field. Methods. We tapered the 0 ″24 …
deepest HST-WFC3 H-band part of the GOODS-South field. Methods. We tapered the 0 ″24 …
The time-scales probed by star formation rate indicators for realistic, bursty star formation histories from the FIRE simulations
JA Flores Velázquez, AB Gurvich… - Monthly Notices of …, 2021 - academic.oup.com
Understanding the rate at which stars form is central to studies of galaxy formation.
Observationally, the star formation rates (SFRs) of galaxies are measured using the …
Observationally, the star formation rates (SFRs) of galaxies are measured using the …
Spectroscopic Confirmation of a Protocluster at z= 3.37 with a High Fraction of Quiescent Galaxies
Spectroscopic Confirmation of a Protocluster at z = 3.37 with a High Fraction of Quiescent
Galaxies - IOPscience This site uses cookies. By continuing to use this site you agree to our …
Galaxies - IOPscience This site uses cookies. By continuing to use this site you agree to our …
The MOSDEF Survey: significant evolution in the rest-frame optical emission line equivalent widths of star-forming galaxies at z= 1.4–3.8
We use extensive spectroscopy from the MOSFIRE Deep Evolution Field survey to
investigate the relationships between rest-frame optical emission line equivalent widths (W) …
investigate the relationships between rest-frame optical emission line equivalent widths (W) …
No strong dependence of Lyman continuum leakage on physical properties of star-forming galaxies at≲ z≲ 3.5
ABSTRACT We present Lyman continuum (LyC) radiation escape fraction (f esc)
measurements for 183 spectroscopically confirmed star-forming galaxies in the redshift …
measurements for 183 spectroscopically confirmed star-forming galaxies in the redshift …
Slicing COSMOS with SC4K: the evolution of typical Ly α emitters and the Ly α escape fraction from z ∼ 2 to 6
We present and explore deep narrow-and medium-band data obtained with the Subaru and
the Isaac Newton Telescopes in the∼ 2 deg2 COSMOS field. We use these data as an …
the Isaac Newton Telescopes in the∼ 2 deg2 COSMOS field. We use these data as an …
Lyman-alpha spectroscopy of extreme [O iii] emitting galaxies at z ≃ 2-3: implications for Lyα visibility and LyC leakage at z > 6
M Tang, DP Stark, J Chevallard… - Monthly Notices of …, 2021 - academic.oup.com
Spectroscopic observations of massive z> 7 galaxies selected to have extremely large [O
iii]+ H β equivalent width (EW∼ 1500 Å) have recently revealed large Ly α detection rates, in …
iii]+ H β equivalent width (EW∼ 1500 Å) have recently revealed large Ly α detection rates, in …
A model for the origin of bursty star formation in galaxies
CA Faucher-Giguère - Monthly Notices of the Royal …, 2018 - academic.oup.com
We propose a simple analytic model to understand when star formation is time steady
versus bursty in galaxies. Recent models explain the observed Kennicutt–Schmidt relation …
versus bursty in galaxies. Recent models explain the observed Kennicutt–Schmidt relation …
MAGAZ3NE: High Stellar Velocity Dispersions for Ultramassive Quiescent Galaxies at z≳ 3
MAGAZ3NE: High Stellar Velocity Dispersions for Ultramassive Quiescent Galaxies at z ≳ 3 -
IOPscience This site uses cookies. By continuing to use this site you agree to our use of cookies …
IOPscience This site uses cookies. By continuing to use this site you agree to our use of cookies …