Photometric redshifts for next-generation surveys
Photometric redshifts are essential in studies of both galaxy evolution and cosmology, as
they enable analyses of objects too numerous or faint for spectroscopy. The Rubin …
they enable analyses of objects too numerous or faint for spectroscopy. The Rubin …
The galaxy cluster mass scale and its impact on cosmological constraints from the cluster population
The total mass of a galaxy cluster is one of its most fundamental properties. Together with
the redshift, the mass links observation and theory, allowing us to use the cluster population …
the redshift, the mass links observation and theory, allowing us to use the cluster population …
The evolution of the galaxy UV luminosity function at redshifts z ≃ 8 – 15 from deep JWST and ground-based near-infrared imaging
CT Donnan, DJ McLeod, JS Dunlop… - Monthly Notices of …, 2023 - academic.oup.com
We reduce and analyse the available JWST ERO and ERS NIRCam imaging (SMACS0723,
GLASS, CEERS) in combination with the latest deep ground-based near-infrared imaging in …
GLASS, CEERS) in combination with the latest deep ground-based near-infrared imaging in …
Discovery and properties of ultra-high redshift galaxies (9 < z < 12) in the JWST ERO SMACS 0723 Field
We present a reduction and analysis of the James Webb Space Telescope (JWST) SMACS
0723 field using new post-launch calibrations to conduct a search for ultra-high-redshift …
0723 field using new post-launch calibrations to conduct a search for ultra-high-redshift …
The art of measuring physical parameters in galaxies: a critical assessment of spectral energy distribution fitting techniques
C Pacifici, KG Iyer, B Mobasher… - The Astrophysical …, 2023 - iopscience.iop.org
The study of galaxy evolution hinges on our ability to interpret multiwavelength galaxy
observations in terms of their physical properties. To do this, we rely on spectral energy …
observations in terms of their physical properties. To do this, we rely on spectral energy …
Reionization era bright emission line survey: selection and characterization of luminous interstellar medium reservoirs in the z> 6.5 Universe
RJ Bouwens, R Smit, S Schouws… - The Astrophysical …, 2022 - iopscience.iop.org
Abstract The Reionization Era Bright Emission Line Survey (REBELS) is a cycle-7 ALMA
Large Program (LP) that is identifying and performing a first characterization of many of the …
Large Program (LP) that is identifying and performing a first characterization of many of the …
A surprising abundance of massive quiescent galaxies at 3 < z < 5 in the first data from JWST CEERS
AC Carnall, DJ McLeod, RJ McLure… - Monthly Notices of …, 2023 - academic.oup.com
We report a robust sample of 10 massive quiescent galaxies at redshift, z> 3, selected using
the first data from the JWST Cosmic Evolution Early Release Science programme. Three of …
the first data from the JWST Cosmic Evolution Early Release Science programme. Three of …
First batch of z≈ 11–20 candidate objects revealed by the James Webb Space Telescope early release observations on SMACS 0723-73
H Yan, Z Ma, C Ling, C Cheng… - The Astrophysical …, 2022 - iopscience.iop.org
On 2022 July 13, NASA released to the whole world the data obtained by the James Webb
Space Telescope (JWST) Early Release Observations (ERO). These are the first set of …
Space Telescope (JWST) Early Release Observations (ERO). These are the first set of …
The fourteenth data release of the Sloan digital sky survey: First spectroscopic data from the extended baryon oscillation spectroscopic survey and from the second …
B Abolfathi, DS Aguado, G Aguilar… - The Astrophysical …, 2018 - iopscience.iop.org
It is now 16 years since the first data release from the Sloan Digital Sky Survey (SDSS; York
et al. 2000). This Early Data Release, or EDR, occurred in 2001 June (Stoughton et al …
et al. 2000). This Early Data Release, or EDR, occurred in 2001 June (Stoughton et al …
Panic! at the Disks: First Rest-frame Optical Observations of Galaxy Structure at z> 3 with JWST in the SMACS 0723 Field
We present early results regarding the morphological and structural properties of galaxies
seen with the James Webb Space Telescope (JWST) at z> 3 in the Early Release …
seen with the James Webb Space Telescope (JWST) at z> 3 in the Early Release …