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researcher

P. Stecchini

3 papers here

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

author position
  • first author3

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

fields
  • astro-ph.HE3

identity via Semantic Scholar / OpenAlex

most citedBroadband X-ray analysis of 1E 1740.7-2942: constraints on spin, inclination and a tentative black hole mass

13 citations · 17 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.HE2020

On the behavior of the black hole candidate 1E 1740.7-2942's corona based on long-term INTEGRAL database

Paulo Eduardo Stecchini, Jurandi Leão, Manuel Castro +1

One of the most straightforward ways to explain the hard X-ray spectra observed in X-ray binaries is to assume that comptonization of soft photons from the accretion disk is occurr…

astro-ph.HE2020★ 13 cited

Broadband X-ray analysis of 1E 1740.7-2942: constraints on spin, inclination and a tentative black hole mass

Paulo E. Stecchini, Flavio D'Amico, Francisco Jablonski +2

1E 1740.7-2942 is one of the strongest hard X-ray emitters in the Galactic Centre region, believed to be a black hole in a high-mass X-ray binary system. Although extensively studi…

astro-ph.HE2017★ 4 cited

Tandem Swift and INTEGRAL Data to Revisit the Orbital and Superorbital Periods of 1E 1740.7-2942

Paulo Eduardo Stecchini, Manuel Castro, Francisco Jablonski +2

The black hole candidate 1E 1740.7-2942 is one of the strongest hard X-ray sources in the Galactic Center region. No counterparts in longer wavelengths have been identified for thi…

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