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Fabio Di Mascia

4 papers here

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

author position
  • first author1
  • middle author3

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA4
ORCID 0000-0002-9263-7900

identity via Semantic Scholar / OpenAlex

most citedEnhanced star formation in z∼6 quasar companions

21 citations · 60 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.GA2023★ 5 cited

Probing z≳6 massive black holes with gravitational waves

Srija Chakraborty, Simona Gallerani, Tommaso Zana +6

We investigate the coalescence of massive black hole (MBH​≳106 M⊙​) binaries (MBHBs) at 6<z<10 by adopting a suite of cosmological hydrodynamical simu…

astro-ph.GA2023★ 20 cited

Accurate dust temperature and star formation rate in the most luminous z>6 quasar in the HYPerluminous quasars at the Epoch of ReionizatION (HYPERION) sample

Roberta Tripodi, Chiara Feruglio, Francisca Kemper +14

We present ALMA Band 9 continuum observation of the ultraluminous quasi-stellar object (QSO) SDSS J0100+2802, providing a ∼10σ detection at ∼670 GHz. SDSS J0100+2802 is…

astro-ph.GA2022★ 14 cited

Is the star formation rate in z∼6 quasars overestimated?

Fabio Di Mascia, Stefano Carniani, Simona Gallerani +4

The large total infrared (TIR) luminosities (LTIR​≳1012 L⊙​) observed in z∼6 quasars are generally converted into high star formation rates ($SFR \gtr…

astro-ph.GA2022★ 21 cited

Enhanced star formation in z∼6 quasar companions

Tommaso Zana, Simona Gallerani, Stefano Carniani +5

Quasars powered by supermassive black holes (MBH, >108 M⊙​) at z∼6 are predicted to reside in cosmic over-dense regions. However, observations so far could not confi…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.