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 …

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 …

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 …

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 …

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 …

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 …

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 …

Dust absorption and the ultraviolet luminosity density at z≈ 3 as calibrated by local starburst galaxies

GR Meurer, TM Heckman, D Calzetti - The Astrophysical Journal, 1999 - iopscience.iop.org
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 …

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 …

Detection of an oxygen emission line from a high-redshift galaxy in the reionization epoch

AK Inoue, Y Tamura, H Matsuo, K Mawatari, I Shimizu… - Science, 2016 - science.org
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 …