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A. Marino

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.HE4
ORCID 0000-0001-5674-4664
same name
  • A. Marino — 48 papers, h 36
  • A. Marino — 42 papers, h 46
  • A. Marino — 20 papers, h 35
  • A. Marino — 17 papers, h 10
  • A. Marino — 10 papers, h 11
  • A. Marino — 9 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

most citedOutflows and spectral evolution in the eclipsing AMXP SWIFT J1749.4-2807 with NICER, XMM-Newton and NuSTAR

20 citations · 47 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.HE2023★ 10 cited

An ultrafast outflow in the black hole candidate MAXI J1810-222?

M. Del Santo, C. Pinto, A. Marino +9

The transient X-ray source MAXI J1810-222 was discovered in 2018 and has been active ever since. A long combined radio and X-ray monitoring campaign was performed with ATCA and Swi…

astro-ph.HE2022★ 11 cited

Unveiling the disc structure in ultraluminous X-ray source NGC 55 ULX-1

F. Barra, C. Pinto, D. J. Walton +11

Despite two decades of studies, it is still not clear whether ULX spectral transitions are due to stochastic variability in the wind or variations in the accretion rate or in the s…

astro-ph.HE2022★ 6 cited

A transient ultraluminous X-ray source in NGC 55

A. Robba, C. Pinto, F. Pintore +14

Ultraluminous X-ray sources (ULXs) are a class of accreting compact objects with X-ray luminosities above 1039 erg s−1. The average number of ULXs per galaxy is still not…

astro-ph.HE2022★ 20 cited

Outflows and spectral evolution in the eclipsing AMXP SWIFT J1749.4-2807 with NICER, XMM-Newton and NuSTAR

A. Marino, A. Anitra, S. M. Mazzola +18

The neutron star low-mass X-ray binary SWIFT J1749.4-2807 is the only known eclipsing accreting millisecond X-ray pulsar. In this manuscript we perform a spectral characterization…

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