papers

Publications (10)

astro-ph.GA2016

ALMA observations of atomic carbon in z~4 dusty star-forming galaxies

M. S. Bothwell, J. E. Aguirre, M. Aravena +15

We present ALMA [CI]() (rest frequency 492 GHz) observations for a sample of 13 strongly-lensed dusty star-forming galaxies originally discovered at 1.4mm in a blank-field sur…

astro-ph.GA2015

Stellar masses and star formation rates of lensed dusty star-forming galaxies from the SPT survey

Jingzhe Ma, Anthony H. Gonzalez, J. S. Spilker +18

To understand cosmic mass assembly in the Universe at early epochs, we primarily rely on measurements of stellar mass and star formation rate of distant galaxies. In this paper, we…

astro-ph.GA2014

The Rest-Frame Submillimeter Spectrum of High-Redshift, Dusty, Star-Forming Galaxies

J. S. Spilker, D. P. Marrone, J. E. Aguirre +28

We present the average rest-frame spectrum of high-redshift dusty, star-forming galaxies from 250-770GHz. This spectrum was constructed by stacking ALMA 3mm spectra of 22 such sour…

astro-ph.GA2016

A survey of the cold molecular gas in gravitationally lensed star-forming galaxies at z>2

M. Aravena, J. S. Spilker, M. Bethermin +18

Using the Australia Telescope Compact Array (ATCA), we conducted a survey of CO J=1-0 and J=2-1 line emission towards strongly lensed high-redshift dusty star forming galaxies (DSF…

astro-ph.GA2015

Probing star formation in the dense environments of z~1 lensing halos aligned with dusty star-forming galaxies detected with the South Pole Telescope

N. Welikala, M. Béthermin, D. Guery +46

We probe star formation in the environments of massive dark matter halos at redshifts of . This star formation is linked to a sub-millimetre cl…

astro-ph.GA2020

The [CII]/[NII] ratio in 3 < z < 6 sub-millimetre galaxies from the South Pole Telescope survey

D. J. M. Cunningham, S. C. Chapman, M. Aravena +19

We present Atacama Compact Array and Atacama Pathfinder Experiment observations of the [N II] 205 m fine-structure line in 40 sub-millimetre galaxies lying at redshifts z = 3 t…