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researcher

P. Ranalli

72 papers hereh-index 338.8k citations122 works total

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

author position
  • sole author4
  • first author8
  • middle author36
  • last author4

Across the 52 of 72 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA22
  • astro-ph.CO17
  • astro-ph15
  • astro-ph.HE14
  • astro-ph.EP1
  • astro-ph.IM1
same name
  • P. Ranalli — 3 papers

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
20022020
most citedThe 2-10 keV luminosity as a Star Formation Rate indicator

589 citations · 6.1k across the 72 of their papers we have counts for

collaborators
Showing 2004 · astro-phShow all

4 papers · 2 filters

astro-ph2004★ 1 cited

High energy emission from starburst galaxies

Piero Ranalli

The star formation (SF) can be regarded as an engine powering the light emission of spiral galaxies at several wavelengths. SF activity also plays a significant role in the evoluti…

astro-ph2004★ 1 cited

X-ray number counts of star forming galaxies

Piero Ranalli, Andrea Comastri, Giancarlo Setti

The behaviour of the X-ray number counts of normal galaxies at faint (-18<Log F<-15 cgs in the 0.5-2.0 keV band) fluxes is investigated. The joint use of information from radio, fa…

astro-ph2004★ 97 cited

The X-Ray Derived Cosmological Star Formation History and the Galaxy X-Ray Luminosity Functions in the Chandra Deep Fields North and South

Colin Norman, Andrew Ptak, Ann Hornschemeier +15

The cosmological star formation rate in the combined Chandra Deep Fields North and South is derived from our X-Ray Luminosity Function for Galaxies in these Deep Fields. Mild evolu…

astro-ph2004★ 68 cited

Stellar and gaseous abundances in M82

L. Origlia, P. Ranalli, A. Comastri +1

The near infrared (IR) absorption spectra of starburst galaxies show several atomic and molecular lines from red supergiants which can be used to infer reliable stellar abundances.…

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