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COSMOS-Web: an overview of the JWST Cosmic Origins Survey
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 …
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 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 Pantheon+ analysis: the full data set and light-curve release
Here we present 1701 light curves of 1550 unique, spectroscopically confirmed Type Ia
supernovae (SNe Ia) that will be used to infer cosmological parameters as part of the …
supernovae (SNe Ia) that will be used to infer cosmological parameters as part of the …
The art of measuring physical parameters in galaxies: a critical assessment of spectral energy distribution fitting techniques
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 …
Life beyond 30: probing the− 20< M UV<− 17 luminosity function at 8< z< 13 with the NIRCam parallel field of the MIRI Deep Survey
We present the ultraviolet luminosity function and an estimate of the cosmic star formation
rate density at 8< z< 13 derived from deep NIRCam observations taken in parallel with the …
rate density at 8< z< 13 derived from deep NIRCam observations taken in parallel with the …
COSMOS2020: The galaxy stellar mass function-The assembly and star formation cessation of galaxies at 0.2< z≤ 7.5
Context. How galaxies form, assemble, and cease their star formation is a central question
within the modern landscape of galaxy evolution studies. These processes are indelibly …
within the modern landscape of galaxy evolution studies. These processes are indelibly …
EPOCHS. II. The ultraviolet luminosity function from 7.5< z< 13.5 using 180 arcmin2 of deep, blank fields from the PEARLS survey and public JWST data
We present an analysis of the ultraviolet luminosity function (UV LF) and star formation rate
density of distant galaxies (7.5< z< 13.5) in the" blank" fields of the Prime Extragalactic Areas …
density of distant galaxies (7.5< z< 13.5) in the" blank" fields of the Prime Extragalactic Areas …
The galaxy UV luminosity function at z ≃ 11 from a suite of public JWST ERS, ERO, and Cycle-1 programs
DJ McLeod, CT Donnan, RJ McLure… - Monthly Notices of …, 2024 - academic.oup.com
We present a new determination of the evolving galaxy ultraviolet (UV) luminosity function
(LF) over the redshift range 9.5< z< 12.5 based on a wide-area (> 250 arcmin2) data set of …
(LF) over the redshift range 9.5< z< 12.5 based on a wide-area (> 250 arcmin2) data set of …