COSMOS-Web: an overview of the JWST Cosmic Origins Survey
CM Casey, JS Kartaltepe, NE Drakos… - The Astrophysical …, 2023 - iopscience.iop.org
We present the survey design, implementation, and outlook for COSMOS-Web, a 255 hr
treasury program conducted by the James Webb Space Telescope in its first cycle of …
treasury program conducted by the James Webb Space Telescope in its first cycle of …
Ram pressure stripping in high-density environments
Galaxies living in rich environments are suffering different perturbations able to drastically
affect their evolution. Among these, ram pressure stripping, ie the pressure exerted by the …
affect their evolution. Among these, ram pressure stripping, ie the pressure exerted by the …
A Comprehensive Study of Galaxies at z∼ 9–16 Found in the Early JWST Data: Ultraviolet Luminosity Functions and Cosmic Star Formation History at the Pre …
We conduct a comprehensive study on dropout galaxy candidates at z∼ 9–16 using the first
90 arcmin 2 James Webb Space Telescope (JWST) Near Infrared Camera images taken by …
90 arcmin 2 James Webb Space Telescope (JWST) Near Infrared Camera images taken by …
CEERS spectroscopic confirmation of NIRCam-selected z≳ 8 galaxy candidates with JWST/NIRSpec: initial characterization of their properties
S Fujimoto, PA Haro, M Dickinson… - The Astrophysical …, 2023 - iopscience.iop.org
We present JWST NIRSpec spectroscopy for 11 galaxy candidates with photometric
redshifts of z≃ 9− 13 and M UV∈[− 21,− 18] newly identified in NIRCam images in the …
redshifts of z≃ 9− 13 and M UV∈[− 21,− 18] newly identified in NIRCam images in the …
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< …
Pure Spectroscopic Constraints on UV Luminosity Functions and Cosmic Star Formation History from 25 Galaxies at z spec= 8.61–13.20 Confirmed with JWST …
Y Harikane, K Nakajima, M Ouchi… - The Astrophysical …, 2023 - iopscience.iop.org
We present pure spectroscopic constraints on the UV luminosity functions and cosmic star
formation rate (SFR) densities from 25 galaxies at z spec= 8.61–13.20. By reducing the …
formation rate (SFR) densities from 25 galaxies at z spec= 8.61–13.20. By reducing the …
Evolution of the UV LF from z ∼ 15 to z ∼ 8 using new JWST NIRCam medium-band observations over the HUDF/XDF
RJ Bouwens, M Stefanon, G Brammer… - Monthly Notices of …, 2023 - academic.oup.com
We present the first constraints on the prevalence of z> 10 galaxies in the Hubble Ultra Deep
Field (HUDF) leveraging new NIRCam observations from JEMS (JWST Extragalactic …
Field (HUDF) leveraging new NIRCam observations from JEMS (JWST Extragalactic …
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 …
Extreme value statistics of the halo and stellar mass distributions at high redshift: are JWST results in tension with ΛCDM?
CC Lovell, I Harrison, Y Harikane… - Monthly Notices of …, 2023 - academic.oup.com
The distribution of dark matter halo masses can be accurately predicted in the lambda cold
dark matter (ΛCDM) cosmology. The presence of a single massive halo or galaxy at a …
dark matter (ΛCDM) cosmology. The presence of a single massive halo or galaxy at a …
From dawn till disc: Milky Way's turbulent youth revealed by the APOGEE+Gaia data
V Belokurov, A Kravtsov - Monthly Notices of the Royal …, 2022 - academic.oup.com
We use accurate estimates of aluminium abundance from the APOGEE Data Release 17
and Gaia Early Data Release 3 astrometry to select a highly pure sample of stars with …
and Gaia Early Data Release 3 astrometry to select a highly pure sample of stars with …