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researcher

P. Chakraborty

4 papers hereh-index 455 citations7 works total

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

author position
  • first author4

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE3
  • astro-ph.CO1
same name
  • P. Chakraborty — 117 papers
  • P. Chakraborty — 27 papers, h 11
  • P. Chakraborty — 27 papers, h 14
  • P. Chakraborty — 21 papers, h 7
  • P. Chakraborty — 15 papers, h 13
  • P. Chakraborty — 15 papers, h 28

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
20192021
most citedX-ray spectroscopy in the microcalorimeter era I: Effects of Fe XXIV Resonance Auger Destruction on Fe XXV Kα spectra

21 citations · 64 across the 4 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

3 papers · 1 filter

astro-ph.HE2021★ 21 cited

X-ray spectroscopy in the microcalorimeter era III: line formation under Case A, Case B, Case C, and Case D in H- and He-like iron for a photoionized cloud

Priyanka Chakraborty, Gary Ferland, Marios Chatzikos +2

Future microcalorimeter X-ray observations will resolve spectral features in unmatched detail. Understanding the line formation processes in the X-rays deserves much attention. The…

astro-ph.HE2020★ 16 cited

X-ray spectroscopy in the microcalorimeter era II: A new Diagnostic on Column Density from the Case A to B Transition in H- and He-like Iron

P. Chakraborty, M. Chatzikos, F. Guzmán +2

The Soft X-ray Spectrometer (SXS) on board \textit{Hitomi}, with the unprecedented resolving power of R∼1250, allowed the detection of members of the Fe XXV \ka\ complex emiss…

astro-ph.HE2020★ 21 cited

X-ray spectroscopy in the microcalorimeter era I: Effects of Fe XXIV Resonance Auger Destruction on Fe XXV Kα spectra

P. Chakraborty, G. J. Ferland, M. Chatzikos +2

We discuss the importance of Fe23+ in determining the line intensities of the Fe XXV Kα complex in an optically thick cloud, and investigate the prediction of Liedahl (2005)…

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