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 dust attenuation law in galaxies
S Salim, D Narayanan - Annual Review of Astronomy and …, 2020 - annualreviews.org
Understanding the properties of dust attenuation curves in galaxies and the physical
mechanisms that shape them are among the fundamental questions of extragalactic …
mechanisms that shape them are among the fundamental questions of extragalactic …
The ALMA Spectroscopic Survey Large Program: The Infrared Excess of z= 1.5–10 UV-selected Galaxies and the Implied High-redshift Star Formation History
R Bouwens, J González-López… - The Astrophysical …, 2020 - iopscience.iop.org
We make use of sensitive (9.3 μJy beam− 1 rms) 1.2 mm continuum observations from the
Atacama Large Millimeter/submillimeter Array (ALMA) Spectroscopic Survey in the Hubble …
Atacama Large Millimeter/submillimeter Array (ALMA) Spectroscopic Survey in the Hubble …
Modeling the panchromatic spectral energy distributions of galaxies
C Conroy - Annual Review of Astronomy and Astrophysics, 2013 - annualreviews.org
The spectral energy distributions (SEDs) of galaxies are shaped by nearly every physical
property of the system, including the star-formation history, metal content, abundance …
property of the system, including the star-formation history, metal content, abundance …
An older, more quiescent universe from panchromatic SED fitting of the 3D-HST survey
J Leja, BD Johnson, C Conroy… - The Astrophysical …, 2019 - iopscience.iop.org
Galaxy observations are influenced by many physical parameters: stellar masses, star
formation rates (SFRs), star formation histories (SFHs), metallicities, dust, black hole activity …
formation rates (SFRs), star formation histories (SFHs), metallicities, dust, black hole activity …
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 …
The relation between Star Formation Rate and Stellar Mass for Galaxies at 3.5⩽ z⩽ 6.5 in CANDELS
B Salmon, C Papovich, SL Finkelstein… - The Astrophysical …, 2015 - iopscience.iop.org
Distant star-forming galaxies show a correlation between their star formation rates (SFRs)
and stellar masses, and this has deep implications for galaxy formation. Here, we present a …
and stellar masses, and this has deep implications for galaxy formation. Here, we present a …
Dust absorption and the ultraviolet luminosity density at z≈ 3 as calibrated by local starburst galaxies
We refine a technique to measure the absorption-corrected ultraviolet (UV) luminosity of
starburst galaxies using rest-frame UV quantities alone and apply it to Lyman-limit U …
starburst galaxies using rest-frame UV quantities alone and apply it to Lyman-limit U …
The dust opacity of star‐forming galaxies
D Calzetti - Publications of the Astronomical Society of the Pacific, 2001 - iopscience.iop.org
The presence of dust in galaxies removes one‐half or more of the stellar energy from the UV‐
optical budget of the universe and has a profound impact on our understanding of how …
optical budget of the universe and has a profound impact on our understanding of how …
Detection of an oxygen emission line from a high-redshift galaxy in the reionization epoch
The physical properties and elemental abundances of the interstellar medium in galaxies
during cosmic reionization are important for understanding the role of galaxies in this …
during cosmic reionization are important for understanding the role of galaxies in this …