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 …
Machine learning for observational cosmology
An array of large observational programs using ground-based and space-borne telescopes
is planned in the next decade. The forthcoming wide-field sky surveys are expected to …
is planned in the next decade. The forthcoming wide-field sky surveys are expected to …
First results from the IllustrisTNG simulations: A tale of two elements–chemical evolution of magnesium and europium
The distribution of elements in galaxies provides a wealth of information about their
production sites and their subsequent mixing into the interstellar medium. Here we …
production sites and their subsequent mixing into the interstellar medium. Here we …
Supernova constraints and systematic uncertainties from the first three years of the supernova legacy survey
We combine high-redshift Type Ia supernovae from the first three years of the Supernova
Legacy Survey (SNLS) with other supernova (SN) samples, primarily at lower redshifts, to …
Legacy Survey (SNLS) with other supernova (SN) samples, primarily at lower redshifts, to …
Correcting type Ia supernova distances for selection biases and contamination in photometrically identified samples
R Kessler, D Scolnic - The Astrophysical Journal, 2017 - iopscience.iop.org
We present a new technique to create a bin-averaged Hubble diagram (HD) from
photometrically identified SN Ia data. The resulting HD is corrected for selection biases and …
photometrically identified SN Ia data. The resulting HD is corrected for selection biases and …
Nearby supernova rates from the Lick Observatory Supernova Search–II. The observed luminosity functions and fractions of supernovae in a complete sample
W Li, J Leaman, R Chornock… - Monthly Notices of …, 2011 - academic.oup.com
This is the second paper of a series in which we present new measurements of the observed
rates of supernovae (SNe) in the local Universe, determined from the Lick Observatory …
rates of supernovae (SNe) in the local Universe, determined from the Lick Observatory …
Nearby supernova rates from the Lick Observatory Supernova Search–III. The rate–size relation, and the rates as a function of galaxy Hubble type and colour
W Li, R Chornock, J Leaman… - Monthly Notices of …, 2011 - academic.oup.com
This is the third paper of a series in which we present new measurements of the observed
rates of supernovae (SNe) in the local Universe, determined from the Lick Observatory …
rates of supernovae (SNe) in the local Universe, determined from the Lick Observatory …
Gravitationally lensed quasars and supernovae in future wide-field optical imaging surveys
Cadenced optical imaging surveys in the next decade will be capable of detecting time-
varying galaxy-scale strong gravitational lenses in large numbers, increasing the size of the …
varying galaxy-scale strong gravitational lenses in large numbers, increasing the size of the …
The optical light curve of GRB 221009A: the afterglow and the emerging supernova
We present extensive optical photometry of the afterglow of GRB 221009A. Our data cover
0.9–59.9 days from the time of Swift and Fermi gamma-ray burst (GRB) detections …
0.9–59.9 days from the time of Swift and Fermi gamma-ray burst (GRB) detections …
The dependence of Type Ia Supernovae luminosities on their host galaxies
Abstract Precision cosmology with Type Ia supernovae (SNe Ia) makes use of the fact that
SN Ia luminosities depend on their light-curve shapes and colours. Using Supernova …
SN Ia luminosities depend on their light-curve shapes and colours. Using Supernova …