837 citations · 11.1k across the 165 of their papers we have counts for
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Deep MUSE observations in the HDFS. Morpho-kinematics of distant star-forming galaxies down to M
T. Contini, B. Epinat, N. Bouché +20
(Abridged) We make use of the deepest VLT/MUSE observations performed so far on the Hubble Deep Field South (HDFS) to characterize the low-mass (< M) galaxy popula…
The SFR-M* Relation and Empirical Star-Formation Histories from ZFOURGE at 0.5 < z < 4
Adam R. Tomczak, Ryan F. Quadri, Kim-Vy H. Tran +19
We explore star-formation histories (SFHs) of galaxies based on the evolution of the star-formation rate stellar mass relation (SFR-M*). Using data from the FourStar Galaxy Evoluti…
Excitation Mechanisms for HCN (1-0) and HCO+ (1-0) in Galaxies from the Great Observatories All-sky LIRG Survey
G. C. Privon, R. Herrero-Illana, A. S. Evans +18
We present new IRAM 30m spectroscopic observations of the GHz band, including emission from the CCH (n=1-0) multiplet, HCN (1-0), HCO+ (1-0), and HNC (1-0), for a sample o…
Dusty galaxies and the degeneracy between their dust distributions and the attenuation formula
Kyle Penner, Mark Dickinson, Benjamin Weiner +7
Do spatial distributions of dust grains in galaxies have typical forms, as do spatial distributions of stars? We investigate whether or not the distributions resemble uniform foreg…
Hyper-luminous Dust Obscured Galaxies discovered by the Hyper Suprime-Cam on Subaru and WISE
Yoshiki Toba, Tohru Nagao, Michael A. Strauss +31
We present the photometric properties of a sample of infrared (IR) bright dust obscured galaxies (DOGs). Combining wide and deep optical images obtained with the Hyper Suprime-Cam…
Thirty Meter Telescope International Observatory Detailed Science Case 2024
Warren Skidmore, Bob Kirshner, David Andersen +168
The Thirty Meter Telescope (TMT) International Observatory (TIO) will be a revolutionary leap forward in astronomical observing capabilities, enabling us to address some of the mos…
Measuring Star-formation Rate and Far-Infrared Color in High-redshift Galaxies Using the CO (7-6) and [NII] 205 micron Lines
Nanyao Lu, Yinghe Zhao, C. Kevin Xu +13
To better characterize the global star formation (SF) activity in a galaxy, one needs to know not only the star formation rate (SFR) but also the rest-frame, far-infrared (FIR) col…