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10 papers · 2 filters
Next Generation Very Large Array Memo No. 8 Science Working Group 3: Galaxy Assembly through Cosmic Time
Caitlin M. Casey, Jacqueline A. Hodge, Mark Lacy +14
The Next-Generation Very Large Array (ngVLA) will be critical for understanding how galaxies are built and evolve at the earliest epochs. The sensitivity and frequency coverage wil…
Quantifying the UV continuum slopes of galaxies to z~10 using deep Hubble and Spitzer/IRAC observations
Stephen M. Wilkins, Rychard J. Bouwens, Pascal A. Oesch +5
Measurements of the UV-continuum slopes provide valuable information on the physical properties of galaxies forming in the early universe, probing the dust reddening, age, metal co…
(Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxies - II. The spatial extent of the radio-emitting regions
Oskari Miettinen, Mladen Novak, Vernesa Smolčić +9
Radio emission at cm wavelengths from highly star-forming galaxies, such as SMGs, is dominated by synchrotron radiation arising from supernova activity. Using deep, high-resolution…
ALMA and Herschel reveal that X-ray selected AGN and main-sequence galaxies have different star formation rate distributions
J. R. Mullaney, D. M. Alexander, J. Aird +15
Using deep Herschel and ALMA observations, we investigate the star formation rate (SFR) distributions of X-ray selected AGN host galaxies at 0.5<z<1.5 and 1.5<z<4, comparing them t…
Satellite content and quenching of star formation in galaxy groups at z~1.8
R. Gobat, E. Daddi, M. Béthermin +13
We study the properties of satellites in the environment of massive star-forming galaxies at z~1.8 in the COSMOS field, using a sample of 215 galaxies on the main sequence of star…
A higher efficiency of converting gas to stars push galaxies at z ~ 1.6 well above the star-forming main sequence
J. D. Silverman, E. Daddi, G. Rodighiero +18
Local starbursts have a higher efficiency of converting gas into stars, as compared to typical star-forming galaxies at a given stellar mass, possibly indicative of different modes…
Evidence for feedback in action from the molecular gas content in the z~1.6 outflowing QSO XID2028
M. Brusa, C. Feruglio, G. Cresci +16
Gas outflows are believed to play a pivotal role in shaping galaxies, as they regulate both star formation and black hole growth. Despite their ubiquitous presence, the origin and…
The influence of wavelength, flux, and lensing selection effects on the redshift distribution of dusty, star-forming galaxies
Matthieu Béthermin, Carlos De Breuck, Mark Sargent +1
We interpret the large variety of redshift distributions of galaxies found by far-infrared and (sub-)millimeter deep surveys depending on their depth and wavelength using the Béthe…
A direct constraint on the gas content of a massive, passively evolving elliptical galaxy at z = 1.43
Mark T. Sargent, E. Daddi, F. Bournaud +6
Gas and dust in star-forming galaxies at the peak epoch of galaxy assembly are presently the topic of intense study, but little is known about the interstellar medium (ISM) of dist…
Physical properties of z>4 submillimeter galaxies in the COSMOS field
V. Smolcic, A. Karim, O. Miettinen +30
We study the physical properties of a sample of 6 SMGs in the COSMOS field, spectroscopically confirmed to lie at z>4. We use new GMRT 325 MHz and 3 GHz JVLA data to probe the rest…