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S. Zhang

86 papers hereh-index 7231 citations18 works total

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

author position
  • first author5
  • middle author38
  • last author21

Across the 64 of 86 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE51
  • astro-ph23
  • astro-ph.IM6
  • physics.ins-det3
  • astro-ph.CO1
  • astro-ph.GA1
same name
  • S. Zhang — 276 papers
  • S. Zhang — 196 papers
  • S. Zhang — 146 papers, h 31
  • S. Zhang — 135 papers, h 66
  • S. Zhang — 98 papers, h 52
  • S. Zhang — 93 papers

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
19962026
most citedBlack Hole Spin in X-Ray Binaries: Observational Consequences

526 citations · 2.8k across the 86 of their papers we have counts for

collaborators
Showing 1999Show all

4 papers · 1 filter

astro-ph1999★ 46 cited

The Timing Evolution of 4U 1630-47 During its 1998 Outburst

S. W. Dieters, T. Belloni, E. Kuulkers +8

We report on the evolution of the timing of 4U1630-47 during its 1998 outburst using data obtained with the Rossi X-ray Timing Explorer (RXTE). The count rate and position in hardn…

astro-ph1999★ 12 cited

Hard X-ray detection of the high redshift quasar 4C 71.07

A. Malizia, L. Bassani, A. J. Dean +3

BATSE/OSSE observations of the high redshift quasar 4C 71.07 indicate that this is the brightest and furthest AGN so far detected above 20 keV. BATSE Earth occultation data have be…

astro-ph1999★ 34 cited

BATSE Observations of the Piccinotti Sample of AGN

A. Malizia, L. Bassani, S. N. Zhang +3

BATSE Earth occultation data have been used to search for emission in the 20-100 keV band from all sources in the Piccinotti sample, which represents to date the only complete 2-10…

astro-ph1999★ 7 cited

Hard X-ray lags in GRO J1719-24

F. van der Hooft, C. Kouveliotou, J. van Paradijs +7

We have used the Fourier cross spectra of GRO J1719-24, as obtained with BATSE, to estimate the phase lags between the X-ray flux variations in the 20--50 and 50--100 keV energy ba…

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