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researcher

S. Balman

40 papers hereh-index 141k citations114 works total

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

author position
  • sole author8
  • first author9
  • middle author9
  • last author11

Across the 37 of 40 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE26
  • astro-ph8
  • astro-ph.GA2
  • astro-ph.IM2
  • astro-ph.SR2
same name
  • S. Balman — 4 papers, h 3
  • S. Balman — 3 papers, h 3

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
20032026
most citedScience with e-ASTROGAM (A space mission for MeV-GeV gamma-ray astrophysics)

253 citations · 996 across the 40 of their papers we have counts for

collaborators
Showing 2020 · astro-ph.HEShow all

3 papers · 2 filters

astro-ph.HE2020★ 6 cited

The ULX Source X-3 in NGC 4258: A Search for Its X-ray and Optical Properties

A. Akyuz, S. Avdan, S. Allak +3

We present the results of a search for the nature of ultraluminous X-ray source (ULX) X-3 in the nearby galaxy NGC 4258. We use archival data from {\it XMM-Newton}, {\it Chandra},…

astro-ph.HE2020★ 28 cited

Accretion Flows in Nonmagnetic White Dwarf Binaries as Observed in X-rays

Solen Balman

Cataclysmic Variables (CVs) are compact binaries with white dwarf (WD) primaries. CVs and other accreting WD binaries (AWBs) are useful laboratories for studying accretion flows, g…

astro-ph.HE2020★ 5 cited

X-ray properties of dwarf nova EY Cyg and the companion star using an XMM-Newton observation

Armin Nabizadeh, Solen Balman

We present the X-ray analysis of dwarf nova EY Cyg using the 45 ks \textit{XMM-Newton} observatory archival data obtained in quiescence. We find orbital modulations in X-rays. We s…

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