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researcher

A. Zdziarski

366 papers hereh-index 6821k citations593 works total

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

author position
  • sole author9
  • first author61
  • middle author106
  • last author57

Across the 233 of 366 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE230
  • astro-ph101
  • astro-ph.IM15
  • astro-ph.CO8
  • astro-ph.GA7
  • astro-ph.SR4
same name
  • A. Zdziarski — 48 papers, h 23
  • A. Zdziarski — 4 papers, h 6
  • A. Zdziarski — 1 paper, h 0

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
19952026
most citedAn Exceptional VHE Gamma-Ray Flare of PKS 2155-304

816 citations · 22.2k across the 358 of their papers we have counts for

collaborators
Showing 1997Show all

4 papers · 1 filter

astro-ph1997★ 1 cited

Thermal/non-thermal model of Cyg X-1 in the soft state

Marek Gierlinski, Andrzej A. Zdziarski, Paolo S. Coppi +3

We analyze X-ray/gamma-ray observations of Cyg X-1 in the soft state. We find the hybrid thermal/non-thermal model fits the data very well. The significant contribution from the no…

astro-ph1997★ 1 cited

X-ray and gamma-ray spectra of Cyg X-1 in the soft state

Marek Gierlinski, Andrzej A. Zdziarski, Tadayasu Dotani +3

We present X-ray/gamma-ray observations of Cyg X-1 in the soft state during 1996 May-June. We analyze ASCA, RXTE and OSSE data. The spectrum consists of soft X-ray blackbody emissi…

astro-ph1997

Broad-band continuum and variability of NGC 5548

P. Magdziarz, O. M. Blaes, A. A. Zdziarski +2

We analyze a composite broad-band optical/UV/Xgamma-ray spectrum of the Seyfert 1 galaxy NGC 5548. The spectrum consists of an average of simultaneous optical/IUE/Ginga observation…

astro-ph1997★ 11 cited

Thermal conduction in accretion disk coronae

Andrzej Maciolek-Niedzwiecki, Julian H. Krolik, Andrzej A. Zdziarski

We study the effects of thermal conduction in a hot, active corona above an accretion disk. We assume that all of the dissipative heating takes place in the corona. We find that th…

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