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researcher

C. Salvaggio

4 papers hereh-index 584 citations15 works total

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

author position
  • middle author3

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE4
same name
  • C. Salvaggio — 5 papers, h 21

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
20182021
most citedThe Ultraluminous X-ray sources population of the galaxy NGC 7456

18 citations · 36 across the 2 of their papers we have counts for

collaborators

4 papers

astro-ph.HE2021★ 18 cited

The rare X-ray flaring activity of the Ultraluminous X-ray source NGC 4559 X7

Fabio Pintore, S. Motta, C. Pinto +9

Ultraluminous X-ray sources are considered amongst the most extremely accreting objects in the local Universe. The recent discoveries of pulsating neutron stars in ULXs strengthene…

astro-ph.HE2020★ 18 cited

The Ultraluminous X-ray sources population of the galaxy NGC 7456

F. Pintore, M. Marelli, R. Salvaterra +28

Ultraluminous X-ray sources (ULXs) are a class of accreting compact objects with X-ray luminosities above 1e39 erg/s. The ULX population counts several hundreds objects but only a…

astro-ph.HE2019

Diffuse X-ray emission around an ultraluminous X-ray pulsar

Andrea Belfiore, Paolo Esposito, Fabio Pintore +17

Ultraluminous X-ray sources (ULXs) are extragalactic X-ray emitters located off-center of their host galaxy and with a luminosity in excess of a few 1039 erg s−1,…

astro-ph.HE2018

A new Ultraluminous X-ray source in the galaxy NGC 5907

F. Pintore, A. Belfiore, G. Novara +14

We report on the serendipitous discovery of a new transient in NGC 5907, at a peak luminosity of 6.4x10^{39} erg/s. The source was undetected in previous 2012 Chandra observations…

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