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I. Prandoni

28 papers hereh-index 7510 citations34 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author26

Across the 26 of 28 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA27
  • astro-ph.HE1
same name
  • I. Prandoni — 144 papers, h 31
  • I. Prandoni — 14 papers
  • I. Prandoni — 14 papers, h 8
  • I. Prandoni — 10 papers, h 3
  • I. Prandoni — 9 papers, h 7
  • I. Prandoni — 6 papers, h 4

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20182026
most citedThe infrared-radio correlation of star-forming galaxies is strongly M⋆​-dependent but nearly redshift-invariant since z∼4

130 citations · 476 across the 27 of their papers we have counts for

collaborators
Showing 2023Show all

3 papers · 1 filter

astro-ph.HE2023★ 20 cited

X-ray properties and obscured fraction of AGN in the J1030 Chandra field

Matilde Signorini, Stefano Marchesi, Roberto Gilli +13

The 500ks Chandra ACIS-I observation of the field around the z=6.31 quasar SDSS J1030+0524 is currently the 5th deepest extragalactic X-ray survey. The rich multi-band coverage o…

astro-ph.GA2023★ 3 cited

LBT-MODS spectroscopy of high-redshift candidates in the Chandra J1030 field. A newly discovered z∼2.8 large scale structure

Stefano Marchesi, Marco Mignoli, Roberto Gilli +13

We present the results of a spectroscopic campaign with the Multi-Object Double Spectrograph (MODS) instrument mounted on the Large Binocular Telescope (LBT), aimed at obtaining a…

astro-ph.GA2023★ 7 cited

AGN feedback in an infant galaxy cluster: the LOFAR-Chandra view of the giant FRII radio galaxy J103025+052430 at z=1.7

M. Brienza, R. Gilli, I. Prandoni +19

In the nearby universe jets from AGN are observed to have a dramatic impact on their surrounding extragalactic environment. Their effect at the `cosmic noon' (z>1.5), the epoch whe…

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