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 …
The Chandra COSMOS Legacy survey: overview and point source catalog
F Civano, S Marchesi, A Comastri… - The Astrophysical …, 2016 - iopscience.iop.org
The COSMOS-Legacy survey is a 4.6 Ms Chandra program that has imaged 2.2 deg 2 of the
COSMOS field with an effective exposure of $\simeq 160$ ks over the central 1.5 deg 2 and …
COSMOS field with an effective exposure of $\simeq 160$ ks over the central 1.5 deg 2 and …
The near-infrared spectrograph (nirspec) on the james webb space telescope-i. overview of the instrument and its capabilities
P Jakobsen, P Ferruit, CA de Oliveira, S Arribas… - Astronomy & …, 2022 - aanda.org
We provide an overview of the design and capabilities of the near-infrared spectrograph
(NIRSpec) onboard the James Webb Space Telescope. NIRSpec is designed to be capable …
(NIRSpec) onboard the James Webb Space Telescope. NIRSpec is designed to be capable …
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 …
Bubbles and outflows: The novel JWST/NIRSpec view of the z= 1.59 obscured quasar XID2028
Quasar feedback in the form of powerful outflows is invoked as a key mechanism to quench
star formation in galaxies, although direct observational evidence is still scarce and debated …
star formation in galaxies, although direct observational evidence is still scarce and debated …
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 ALPINE-ALMA [CII] survey-The nature, luminosity function, and star formation history of dusty galaxies up to z≃ 6
C Gruppioni, M Béthermin, F Loiacono… - Astronomy & …, 2020 - aanda.org
Aims. We present the detailed characterisation of a sample of 56 sources serendipitously
detected in ALMA band 7 as part of the ALMA Large Program to INvestigate CII at Early …
detected in ALMA band 7 as part of the ALMA Large Program to INvestigate CII at Early …
The VLA-COSMOS 3 GHz Large Project: Continuum data and source catalog release
We present the VLA-COSMOS 3 GHz Large Project based on 384 h of observations with the
Karl G. Jansky Very Large Array (VLA) at 3 GHz (10 cm) toward the two square degree …
Karl G. Jansky Very Large Array (VLA) at 3 GHz (10 cm) toward the two square degree …
The ALPINE-ALMA [CII] survey-Survey strategy, observations, and sample properties of 118 star-forming galaxies at 4< z< 6
The ALMA-ALPINE [CII] survey is aimed at characterizing the properties of a sample of
normal star-forming galaxies (SFGs). The ALMA Large Program to INvestigate (ALPINE) …
normal star-forming galaxies (SFGs). The ALMA Large Program to INvestigate (ALPINE) …
Galaxies at redshifts 5 to 6 with systematically low dust content and high [C ii] emission
The rest-frame ultraviolet properties of galaxies during the first three billion years of cosmic
time (redshift z> 4) indicate a rapid evolution in the dust obscuration of such galaxies,,. This …
time (redshift z> 4) indicate a rapid evolution in the dust obscuration of such galaxies,,. This …