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researcher

M. Orlandini

117 papers hereh-index 294.2k citations224 works total

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

author position
  • sole author1
  • first author7
  • middle author70
  • last author10

Across the 88 of 117 papers where every author was matched, so the position is known.

fields
  • astro-ph73
  • astro-ph.HE30
  • astro-ph.IM12
  • astro-ph.CO1
  • hep-ph1
same name
  • M. Orlandini — 14 papers, h 13
  • M. Orlandini — 10 papers
  • M. Orlandini — 2 papers, h 0
  • M. Orlandini — 1 paper, h 1

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
19972025
most citedDiscovery of the X-Ray Afterglow of the Gamma-Ray Burst of February 28 1997

998 citations · 4.4k across the 116 of their papers we have counts for

collaborators
Showing 2005Show all

4 papers · 1 filter

astro-ph2005★ 12 cited

Broad-band Spectral Properties of Accreting X-ray Binary Pulsars

Mauro Orlandini

Broad-band spectra of accreting X-ray binary pulsars can be fit by a phenomenological model composed by a power law with a high energy rollover above 10 keV, plus a blackbody compo…

astro-ph2005★ 24 cited

A Compton reflection dominated spectrum in a peculiar accreting neutron star

Nanda Rea, Luigi Stella, Gian Luca Israel +5

We report on a puzzling event occurred during a long BeppoSAX observation of the slow-rotating binary pulsar GX 1+4. During this event, lasting about 1 day, the source X-ray flux w…

astro-ph2005

The BeppoSAX view on the galactic high-mass X-ray binary 4U 0114+65

N. Masetti, M. Orlandini, D. Dal Fiume +5

A pointed observation on the galactic high-mass X-ray binary 4U 0114+65 was carried out with BeppoSAX in order to compare the X-ray spectral and timing characteristics observed by…

astro-ph2005★ 3 cited

Exploring the Hard X-/soft gamma-ray Continuum Spectra with Laue Lenses

F. Frontera, A. Pisa, P. De Chiara +17

The history of X-ray astronomy has shown that any advancement in our knowledge of the X-ray sky is strictly related to an increase in instrument sensitivity. At energies above 60 k…

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