most citedKinematics of galaxies from [CII] line emission

110 citations · 187 across the 3 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2019

A contribution of star-forming clumps and accreting satellites to the mass assembly of z ~ 2 galaxies

A. Zanella, E. Le Floc'h, C. M. Harrison +14

We investigate the contribution of clumps and satellites to the galaxy mass assembly. We analyzed spatially-resolved Hubble Space Telescope observations (imaging and slitless spect…

astro-ph.GA20197 cited

Inquiring into the nature of the Abell 2667 Brightest Cluster Galaxy: physical properties from MUSE

E. Iani, G. Rodighiero, J. Fritz +21

Based on HST and MUSE data, we probe the stellar and gas properties (i.e. kinematics, stellar mass, star formation rate) of the radio-loud brightest cluster galaxy (BCG) located at…

astro-ph.GA2019110 cited

Kinematics of galaxies from [CII] line emission

M. Kohandel, A. Pallottini, A. Ferrara +5

We study the kinematical properties of galaxies in the Epoch of Reionization via the [CII] 158m line emission. The line profile provides information on the kinematics as well as…

astro-ph.GA201991 cited

The ultra-diffuse galaxy NGC 1052-DF2 with MUSE: II. The population of DF2: stars, clusters and planetary nebulae

Jeremy Fensch, Remco F. J. van der Burg, Tereza Jerabkova +13

NGC 1052-DF2, an ultra diffuse galaxy (UDG), has been the subject of intense debate. Its alleged absence of dark matter, and the brightness and number excess of its globular cluste…

astro-ph.GA201925 cited

Deciphering an evolutionary sequence of merger stages in infrared-luminous starburst galaxies at z ~ 0.7

Antonello Calabrò, Emanuele Daddi, Annagrazia Puglisi +18

Based on optical/near-IR Magellan FIRE spectra of 25 starburst galaxies at 0.5 < z < 0.9, Calabrò et al.(2018) showed that their attenuation properties can be explained by a single…

astro-ph.GA2018

The ultra-diffuse galaxy NGC 1052-DF2 with MUSE: I. Kinematics of the stellar body

Eric Emsellem, Remco F. J. van der Burg, Jeremy Fensch +14

The so-called ultra-diffuse galaxy NGC~1052-DF2 was announced to be a galaxy lacking dark matter based on a spectroscopic study of its constituent globular clusters. Here we presen…