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F. Paerels

3 papers here

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

author position
  • middle author2
  • last author1

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

fields
  • astro-ph3
same name
  • F. Paerels — 117 papers, h 46
  • F. Paerels — 7 papers, h 5
  • F. Paerels — 6 papers
  • F. Paerels — 6 papers, h 5
  • F. Paerels — 5 papers, h 2
  • F. Paerels — 5 papers, h 7

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 citedNon-Detection of Gravitationally Redshifted Absorption Lines in the X-ray Burst Spectra of GS 1826-24

22 citations · 24 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph2007★ 22 cited

Non-Detection of Gravitationally Redshifted Absorption Lines in the X-ray Burst Spectra of GS 1826-24

Albert K. H. Kong, Jon M. Miller, Mariano Mendez +6

During a 200 ks observation with the XMM-Newton Reflection Grating Spectrometer, we detected 16 type-I X-ray bursts from GS 1826-24. We combined the burst spectra in an attempt to…

astro-ph2002★ 1 cited

High Resolution X-Ray Spectroscopic Constraints on Cooling Flow Models of Clusters of Galaxies and Gaseous Haloes Around Elliptical Galaxies

S. M. Kahn, J. R. Peterson, F. B. S. Paerels +6

In many clusters of galaxies, the cooling time at the core of the intracluster medium is much less than the age of the system, suggesting that the the gas should continually lose e…

astro-ph2002★ 1 cited

Spectral and Timing Properties of the Low-mass X-ray Binary 4U 0614+09 with XMM-Newton

M. Mendez, Jean Cottam, F. Paerels

4U 0614+09 is a low-mass X-ray binary with a weakly magnetized neutron star primary. It shows variability on time scales that range from years down to ~0.8 milliseconds. Before the…

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