Star formation in galaxies along the Hubble sequence
RC Kennicutt Jr - Annual Review of Astronomy and Astrophysics, 1998 - annualreviews.org
▪ Abstract Observations of star formation rates (SFRs) in galaxies provide vital clues to the
physical nature of the Hubble sequence and are key probes of the evolutionary histories of …
physical nature of the Hubble sequence and are key probes of the evolutionary histories of …
Cosmic star-formation history
P Madau, M Dickinson - Annual Review of Astronomy and …, 2014 - annualreviews.org
Over the past two decades, an avalanche of new data from multiwavelength imaging and
spectroscopic surveys has revolutionized our view of galaxy formation and evolution. Here …
spectroscopic surveys has revolutionized our view of galaxy formation and evolution. Here …
Spectroscopic confirmation of four metal-poor galaxies at z = 10.3–13.2
Finding and characterizing the first galaxies that illuminated the early universe at cosmic
dawn is pivotal to understand the physical conditions and the processes that led to the …
dawn is pivotal to understand the physical conditions and the processes that led to the …
CEERS Epoch 1 NIRCam imaging: reduction methods and simulations enabling early JWST science results
MB Bagley, SL Finkelstein… - The Astrophysical …, 2023 - iopscience.iop.org
We present the data release and data reduction process for the Epoch 1 NIRCam
observations for the Cosmic Evolution Early Release Science Survey (CEERS). These data …
observations for the Cosmic Evolution Early Release Science Survey (CEERS). These data …
New Determinations of the UV Luminosity Functions from z∼ 9 to 2 Show a Remarkable Consistency with Halo Growth and a Constant Star Formation Efficiency
RJ Bouwens, PA Oesch, M Stefanon… - The Astronomical …, 2021 - iopscience.iop.org
Here we provide the most comprehensive determinations of the rest-frame UV luminosity
function (LF) available to date with the Hubble Space Telescope (HST) at z∼ 2–9 …
function (LF) available to date with the Hubble Space Telescope (HST) at z∼ 2–9 …
The main sequence of star-forming galaxies across cosmic times
P Popesso, A Concas, G Cresci, S Belli… - Monthly Notices of …, 2023 - academic.oup.com
By compiling a comprehensive census of literature studies, we investigate the evolution of
the main sequence (MS) of star-forming galaxies (SFGs) in the widest range of redshift (0< …
the main sequence (MS) of star-forming galaxies (SFGs) in the widest range of redshift (0< …
The Swift gamma-ray burst mission
N Gehrels, G Chincarini, PE Giommi… - The Astrophysical …, 2004 - iopscience.iop.org
The Swift mission, scheduled for launch in 2004, is a multiwavelength observatory for
gamma-ray burst (GRB) astronomy. It is a first-of-its-kind autonomous rapid-slewing satellite …
gamma-ray burst (GRB) astronomy. It is a first-of-its-kind autonomous rapid-slewing satellite …
CANDELS: the cosmic assembly near-infrared deep extragalactic legacy survey
ABSTRACT The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey
(CANDELS) is designed to document the first third of galactic evolution, over the …
(CANDELS) is designed to document the first third of galactic evolution, over the …
UV luminosity functions at redshifts z∼ 4 to z∼ 10: 10,000 galaxies from HST legacy fields
RJ Bouwens, GD Illingworth, PA Oesch… - The Astrophysical …, 2015 - iopscience.iop.org
ABSTRACT The remarkable Hubble Space Telescope (HST) data sets from the CANDELS,
HUDF09, HUDF12, ERS, and BoRG/HIPPIES programs have allowed us to map the …
HUDF09, HUDF12, ERS, and BoRG/HIPPIES programs have allowed us to map the …
The many lives of active galactic nuclei: cooling flows, black holes and the luminosities and colours of galaxies
We simulate the growth of galaxies and their central supermassive black holes by
implementing a suite of semi-analytic models on the output of the Millennium Run, a very …
implementing a suite of semi-analytic models on the output of the Millennium Run, a very …