[HTML][HTML] The art of measuring physical parameters in galaxies: a critical assessment of spectral energy distribution fitting techniques
C Pacifici, KG Iyer, B Mobasher… - The Astrophysical …, 2023 - iopscience.iop.org
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 …
An ALMA survey of the SCUBA-2 CLS UDS field: physical properties of 707 sub-millimetre galaxies
U Dudzevičiūtė, I Smail, AM Swinbank… - Monthly Notices of …, 2020 - academic.oup.com
We analyse the physical properties of a large, homogeneously selected sample of ALMA-
located sub-millimetre galaxies (SMGs). This survey, AS2UDS, identified 707 SMGs across …
located sub-millimetre galaxies (SMGs). This survey, AS2UDS, identified 707 SMGs across …
[HTML][HTML] Hidden Giants in JWST's PEARLS: An Ultramassive z= 4.26 Submillimeter Galaxy that Is Invisible to HST
I Smail, U Dudzevičiūtė, M Gurwell… - The Astrophysical …, 2023 - iopscience.iop.org
We present a multiwavelength analysis using the Submillimeter Array (SMA), James Clerk
Maxwell Telescope, NOEMA, JWST, the Hubble Space Telescope (HST), and the Spitzer …
Maxwell Telescope, NOEMA, JWST, the Hubble Space Telescope (HST), and the Spitzer …
[HTML][HTML] Mapping Obscuration to Reionization with ALMA (MORA): 2 mm Efficiently Selects the Highest-redshift Obscured Galaxies
CM Casey, JA Zavala, SM Manning… - The Astrophysical …, 2021 - iopscience.iop.org
We present the characteristics of 2 mm selected sources from the largest Atacama Large
Millimeter/submillimeter Array (ALMA) blank-field contiguous survey conducted to date, the …
Millimeter/submillimeter Array (ALMA) blank-field contiguous survey conducted to date, the …
Automated Mining of the ALMA Archive in the COSMOS Field (A3COSMOS). II. Cold Molecular Gas Evolution out to Redshift 6
D Liu, E Schinnerer, B Groves, B Magnelli… - The Astrophysical …, 2019 - iopscience.iop.org
We present new measurements of the cosmic cold molecular gas evolution out to redshift 6
based on systematic mining of the Atacama Large Millimeter/submillimeter Array (ALMA) …
based on systematic mining of the Atacama Large Millimeter/submillimeter Array (ALMA) …
An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: high-resolution dust continuum morphologies and the link between sub-millimetre …
B Gullberg, I Smail, AM Swinbank… - Monthly Notices of …, 2019 - academic.oup.com
We present an analysis of the morphology and profiles of the dust continuum emission in
153 bright sub-millimetre galaxies (SMGs) detected with ALMA at signal-to-noise ratios of> 8 …
153 bright sub-millimetre galaxies (SMGs) detected with ALMA at signal-to-noise ratios of> 8 …
An ALMA/NOEMA survey of the molecular gas properties of high-redshift star-forming galaxies
JE Birkin, A Weiss, JL Wardlow, I Smail… - Monthly Notices of …, 2021 - academic.oup.com
We have used ALMA and NOEMA to study the molecular gas reservoirs in 61 ALMA-
identified submillimetre galaxies (SMGs) in the COSMOS, UDS, and ECDFS fields. We …
identified submillimetre galaxies (SMGs) in the COSMOS, UDS, and ECDFS fields. We …
Characterization of Two 2 mm detected Optically Obscured Dusty Star-forming Galaxies
SM Manning, CM Casey, JA Zavala… - The Astrophysical …, 2022 - iopscience.iop.org
Abstract The 2 mm Mapping Obscuration to Reionization with ALMA (MORA) Survey was
designed to detect high-redshift (z≳ 4), massive, dusty star-forming galaxies (DSFGs). Here …
designed to detect high-redshift (z≳ 4), massive, dusty star-forming galaxies (DSFGs). Here …
An ALMA survey of the S2CLS UDS field: optically invisible submillimetre galaxies
I Smail, U Dudzevičiūtė, SM Stach… - Monthly Notices of …, 2021 - academic.oup.com
We analyse a robust sample of 30 near-infrared-faint (K AB> 25.3, 5σ) submillimetre
galaxies (SMGs) selected from a 0.96 deg2 field to investigate their properties and the cause …
galaxies (SMGs) selected from a 0.96 deg2 field to investigate their properties and the cause …
Illuminating the dark side of cosmic star formation two billion years after the Big Bang
M Talia, A Cimatti, M Giulietti, G Zamorani… - The Astrophysical …, 2021 - iopscience.iop.org
How and when did galaxies form and assemble their stars and stellar mass? The answer to
these questions, so crucial to astrophysics and cosmology, requires the full reconstruction of …
these questions, so crucial to astrophysics and cosmology, requires the full reconstruction of …