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20132026
most citedHydrogen reionisation ends by : Lyman- optical depth measured by the XQR-30 sample

302 citations · 6.5k across the 129 of their papers we have counts for

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Showing 2017Show all

11 papers · 1 filter

astro-ph.GA2017★ 157 cited

Kiloparsec-scale gaseous clumps and star formation at

S. Carniani, R. Maiolino, R. Amorin +13

We investigate the morphology of the [CII] emission in a sample of "normal" star-forming galaxies at in relation to their UV (rest-frame) counterpart. We use new ALMA obs…

astro-ph.GA2017★ 41 cited

Galaxy evolution studies with the SPace IR telescope for Cosmology and Astrophysics (SPICA): the power of IR spectroscopy

L. Spinoglio, A. Alonso-Herrero, L. Armus +65

IR spectroscopy in the range 12-230 micron with the SPace IR telescope for Cosmology and Astrophysics (SPICA) will reveal the physical processes that govern the formation and evolu…

astro-ph.GA2017★ 79 cited

CO line emission from galaxies in the Epoch of Reionization

L. Vallini, A. Pallottini, A. Ferrara +3

We study the CO line luminosity (), the shape of the CO Spectral Line Energy Distribution (SLED), and the value of the CO-to- conversion factor in galaxies in…

astro-ph.GA2017★ 104 cited

ALMA reveals metals yet no dust within multiple components in CR7

J. Matthee, D. Sobral, F. Boone +8

We present spectroscopic follow-up observations of CR7 with ALMA, targeted at constraining the infrared (IR) continuum and [CII] line-emission at high spatial resolu…

astro-ph.GA2017★ 22 cited

Molecular clumps photoevaporation in ionized regions

Davide Decataldo, Andrea Ferrara, Andrea Pallottini +2

We study the photoevaporation of molecular clumps exposed to a UV radiation field including hydrogen-ionizing photons ( eV) produced by massive stars or quasars. We follo…

astro-ph.GA2017★ 131 cited

The impact of chemistry on the structure of high-z galaxies

A. Pallottini, A. Ferrara, S. Bovino +4

To improve our understanding of high-z galaxies we study the impact of H chemistry on their evolution, morphology and observed properties. We compare two zoom-in high-resolut…

astro-ph.GA2017★ 66 cited

Quasar outflows at : the impact on the host galaxies

Paramita Barai, Simona Gallerani, Andrea Pallottini +5

We investigate quasar outflows at by performing zoom-in cosmological hydrodynamical simulations. By employing the SPH code GADGET-3, we zoom in the region ar…

astro-ph.GA2017★ 26 cited

X-ray spectroscopy of the z=6.4 quasar J1148+5251

Simona Gallerani, Luca Zappacosta, Maria Carmela Orofino +9

We present the 78-ks Chandra observations of the quasar SDSS J1148+5251. The source is clearly detected in the energy range 0.3-7 keV with 42 counts (with a significance $\…

astro-ph.GA2017★ 39 cited

The nature of the Lyman Alpha Emitter CR7: a persisting puzzle

Fabio Pacucci, Andrea Pallottini, Andrea Ferrara +1

The peculiar emission properties of the Ly emitter CR7 have been initially interpreted with the presence of either a direct collapse black hole (DCBH) or a substant…

astro-ph.CO2017★ 91 cited

High Mass X-ray Binaries and the Cosmic 21-cm Signal: Impact of Host Galaxy Absorption

Arpan Das, Andrei Mesinger, Andrea Pallottini +2

By heating the intergalactic medium (IGM) before reionization, X-rays are expected to play a prominent role in the early Universe. The cosmic 21-cm signal from this "Epoch of Heati…

astro-ph.GA2017★ 151 cited

Extended ionised and clumpy gas in a normal galaxy at z=7.1 revealed by ALMA

S. Carniani, R. Maiolino, A. Pallottini +10

We present new ALMA observations of the [OIII]88m line and high angular resolution observations of the [CII]158m line in a normal star forming galaxy at z7.1. Previous [CI…