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[CII] line intensity mapping the epoch of reionization with the Prime-Cam on FYST
C. Karoumpis, B. Magnelli, E. Romano-Díaz +2
We predict the three-dimensional intensity power spectrum (PS) of the [CII] 158m line throughout the epoch of (and post) reionization at redshifts from 3.5 to 8. We…
COLDz: Probing Cosmic Star Formation With Radio Free-free Emission
Hiddo S. B. Algera, Jacqueline A. Hodge, Dominik A. Riechers +17
Radio free-free emission is considered to be one of the most reliable tracers of star formation in galaxies. However, as it constitutes the faintest part of the radio spectrum -- b…
CCAT-prime Collaboration: Science Goals and Forecasts with Prime-Cam on the Fred Young Submillimeter Telescope
Prime collaboration, M. Aravena, J. E. Austermann +84
We present a detailed overview of the science goals and predictions for the Prime-Cam direct detection camera/spectrometer being constructed by the CCAT-prime collaboration for ded…
GOODS-ALMA 2.0: Source catalog, number counts, and prevailing compact sizes in 1.1 mm galaxies
C. Gómez-Guijarro, D. Elbaz, M. Xiao +36
Submillimeter/millimeter observations of dusty star-forming galaxies with the Atacama Large Millimeter/submillimeter Array (ALMA) have shown that dust continuum emission generally…
The non-linear infrared-radio correlation of low-z galaxies: implications for redshift evolution, a new radio SFR recipe, and how to minimize selection bias
Daniel Cs. Molnar, Mark T. Sargent, Sarah Leslie +7
The infrared-radio correlation (IRRC) underpins many commonly used radio luminosity-star formation rate (SFR) calibrations. In preparation for the new generation of radio surveys w…