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S. Pike

3 papers hereh-index 213 citations4 works total

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

author position
  • middle author3

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

fields
  • astro-ph.HE3
same name
  • S. Pike — 15 papers, h 9
  • S. Pike — 9 papers, h 2
  • S. Pike — 1 paper, h 4

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 citedThe High Energy X-ray Probe (HEX-P): Probing Accretion onto Stellar Mass Black Holes

1 citations · 2 across the 2 of their papers we have counts for

collaborators

3 papers

astro-ph.HE2025

Double-hump spectrum, pulse profile dip, and pulsed fraction spectra from the low-accretion regime in the X-ray pulsar MAXI J0655-013

C. Malacaria, S. N. Pike, A. D'Aì +18

Accreting X-ray pulsars (XRPs) undergo different physical regimes depending on the mass accretion rate. Recent observations have shown a dramatic change in the emission properties…

astro-ph.HE2023★ 1 cited

The High Energy X-ray Probe (HEX-P): Probing Accretion onto Stellar Mass Black Holes

Riley Connors, John Tomsick, Paul Draghis +20

Accretion is a universal astrophysical process that plays a key role in cosmic history, from the epoch of reionization to galaxy and stellar formation and evolution. Accreting stel…

astro-ph.HE2023★ 1 cited

The High Energy X-ray Probe (HEX-P): A New Window into Neutron Star Accretion

R. M. Ludlam, C. Malacaria, E. Sokolova-Lapa +15

Accreting neutron stars (NSs) represent a unique laboratory for probing the physics of accretion in the presence of strong magnetic fields (B≳108 G). Additionally, the ma…

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