activity
20172020
most citedThe properties of the interstellar medium of galaxies across time as traced by the neutral atomic carbon [CI]

91 citations · 249 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.GA202024 cited

Extinction in the 11.2 micron PAH band and the low L_11.2/L_IR in ULIRGs

Antonio Hernan-Caballero, Henrik W. W. Spoon, Almudena Alonso-Herrero +9

We present a method for recovering the intrinsic (extinction-corrected) luminosity of the 11.2 micron PAH band in galaxy spectra. Using 105 high S/N Spitzer/IRS spectra of star-for…

astro-ph.GA202064 cited

CO emission in distant galaxies on and above the main sequence

Francesco Valentino, Emanuele Daddi, Annagrazia Puglisi +17

We present the detection of multiple CO line transitions with ALMA in a few tens of infrared-selected galaxies on and above the main sequence at z=1.1-1.7. We reliably detected the…

astro-ph.GA2020

Deceptively cold dust in the massive starburst galaxy GN20 at

Isabella Cortzen, Georgios E. Magdis, Francesco Valentino +13

We present new observations, carried out with IRAM NOEMA, of the atomic neutral carbon transitions [CI](1-0) at 492 GHz and [CI](2-1) at 809 GHz of GN20, a well-studied star-bursti…

astro-ph.GA202091 cited

The properties of the interstellar medium of galaxies across time as traced by the neutral atomic carbon [CI]

Francesco Valentino, Georgios E. Magdis, Emanuele Daddi +14

We report ALMA observations of the neutral atomic carbon transitions [CI] and multiple CO lines in a sample of main sequence galaxies at , including novel informat…

astro-ph.GA201944 cited

X-shooter Spectroscopy and HST Imaging of 15 Ultra Massive Quiescent Galaxies at

Mikkel Stockmann, Sune Toft, Anna Gallazzi +23

We present a detailed analysis of a large sample of spectroscopically confirmed ultra-massive quiescent galaxies () at . This sam…

astro-ph.GA201726 cited

The Fine Line Between Normal and Starburst Galaxies

Nicholas Lee, Kartik Sheth, Kimberly S. Scott +10

Recent literature suggests that there are two modes through which galaxies grow their stellar mass - a normal mode characterized by quasi-steady star formation, and a highly effici…