activity
19952026
most citedMass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function

2k citations · 36.1k across the 358 of their papers we have counts for

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Showing 2017 · astro-ph.GAShow all

12 papers · 2 filters

astro-ph.GA2017★ 12 cited

Unveiling the inner morphology and gas kinematics of NGC 5135 with ALMA

G. Sabatini, C. Gruppioni, M. Massardi +5

The local Seyfert 2 galaxy NGC5135, thanks to its almost face-on appearance, a bulge overdensity of stars, the presence of a large-scale bar, an AGN and a Supernova Remnant, is an…

astro-ph.GA2017★ 35 cited

Discovery of a z = 7.452 High Equivalent Width Lyman-α Emitter from the Hubble Space Telescope Faint Infrared Grism Survey

Rebecca L. Larson, Steven L. Finkelstein, Norbert Pirzkal +18

We present the results of an unbiased search for Lyα emission from continuum-selected 6 < z < 8 galaxies. Our dataset consists of 160 orbits of G102 slitless grism spectroscopy obt…

astro-ph.GA2017★ 44 cited

The VANDELS survey: Dust attenuation in star-forming galaxies at

F. Cullen, R. J. McLure, S. Khochfar +15

We present the results of a new study of dust attenuation at redshifts based on a sample of star-forming galaxies from the VANDELS spectroscopic survey. Motivated…

astro-ph.GA2017★ 20 cited

The MUSE 3D view of feedback in a high-metallicity radio galaxy at z = 2.9

M. Silva, A. Humphrey, P. Lagos +8

We present a detailed study of the kinematic, chemical and excitation properties of the giant Ly emitting nebula and the giant \ion{H}{I} absorber associated with the …

astro-ph.GA2017★ 34 cited

CO excitation in the Seyfert galaxy NGC 34: stars, shock or AGN driven?

M. Mingozzi, L. Vallini, F. Pozzi +7

We present a detailed analysis of the X-ray and molecular gas emission in the nearby galaxy NGC 34, to constrain the properties of molecular gas, and assess whether, and to what ex…

astro-ph.GA2017★ 11 cited

The Green Bank Ammonia Survey: Unveiling the Dynamics of the Barnard 59 star-forming Clump

E. Redaelli, F. O. Alves, P. Caselli +17

Understanding the early stages of star formation is a research field of ongoing development, both theoretically and observationally. In this context, molecular data have been conti…

astro-ph.GA2017★ 66 cited

The VIMOS Ultra-Deep Survey: evidence for AGN feedback in galaxies with CIII]-1908Å~emission 10.8 to 12.5 Gyr ago

O. Le Fèvre, B. C. Lemaux, K. Nakajima +19

We analyze the CIII]-1908Åemission properties in a sample of 3899 star-forming galaxies (SFGs) at 2<z<3.8 from the VIMOS Ultra-Deep Survey (VUDS). We find a median EW(CIII])=2.0$\p…

astro-ph.GA2017★ 22 cited

Predicting emission line fluxes and number counts of distant galaxies for cosmological surveys

F. Valentino, E. Daddi, J. D. Silverman +9

We estimate the number counts of line emitters at high redshift and their evolution with cosmic time based on a combination of photometry and spectroscopy. We predict the H, H$β…

astro-ph.GA2017★ 52 cited

FIGS -- Faint Infrared Grism Survey: Description and Data Reduction

Norbert Pirzkal, Sangeeta Malhotra, Russell E. Ryan +26

The Faint Infrared Grism Survey (FIGS) is a deep Hubble Space Telescope (HST) WFC3/IR (Wide Field Camera 3 Infrared) slitless spectroscopic survey of four deep fields. Two fields a…

astro-ph.GA2017★ 14 cited

Reconstructing the galaxy density field with photometric redshifts: II. Environment-dependent galaxy evolution since

Nicola Malavasi, Lucia Pozzetti, Olga Cucciati +3

Although extensively investigated, the role of the environment in galaxy formation is still not well understood. In this context, the Galaxy Stellar Mass Function (GSMF) is a power…

astro-ph.GA2017★ 14 cited

A methodology to select galaxies just after the quenching of star formation

Annalisa Citro, Lucia Pozzetti, Salvatore Quai +3

We propose a new methodology aimed at finding star-forming galaxies in the phase which immediately follows the star-formation (SF) quenching, based on the use of high- to low-ioniz…

astro-ph.GA2017★ 3 cited

Analogs of primeval galaxies two billion years after the Big Bang

Ricardo Amorín, A. Fontana, E. Pérez-Montero +30

Deep observations are revealing a growing number of young galaxies in the first billion year of cosmic time. Compared to typical galaxies at later times, they show more extreme emi…