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researcher

K. Chan

4 papers hereh-index 222.5k citations110 works total

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

author position
  • middle author4

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

fields
  • astro-ph2
  • astro-ph.IM2
same name
  • K. Chan — 164 papers, h 87
  • K. Chan — 37 papers, h 17
  • K. Chan — 27 papers, h 18
  • K. Chan — 18 papers
  • K. Chan — 17 papers, h 13
  • K. Chan — 14 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

activity
20062023
most citedOverview of the Advanced X-ray Imaging Satellite (AXIS)

77 citations · 216 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.IM2023★ 77 cited

Overview of the Advanced X-ray Imaging Satellite (AXIS)

Christopher S. Reynolds, Erin A. Kara, Richard F. Mushotzky +40

The Advanced X-ray Imaging Satellite (AXIS) is a Probe-class concept that will build on the legacy of the Chandra X-ray Observatory by providing low-background, arcsecond-resolutio…

astro-ph.IM2013★ 53 cited

First results from a next-generation off-plane X-ray diffraction grating

Randall McEntaffer, Casey DeRoo, Ted Schultz +13

Future NASA X-ray spectroscopy missions will require high throughput, high resolution grating spectrometers. Off-plane reflection gratings are capable of meeting the performance re…

astro-ph2006★ 54 cited

Discoveries of Diffuse Iron Line Sources from the Sgr B Region

Katsuji Koyama, Tatsuya Inui, Yoshiaki Hyodo +8

The radio complex Sgr B region is observed with the X-Ray Imaging Spectrometers (XIS) on board Suzaku. This region exhibits diffuse iron lines at 6.4, 6.7 and 6.9 keV, which are K$…

astro-ph2006★ 32 cited

An Apparent Hard X-ray Decline of CH Cygni

Koji Mukai, Manabu Ishida, Caroline Kilbourne +4

CH Cygni is a symbiotic star consisting of an M giant and an accreting white dwarf, which is known to be a highly variable X-ray source with a complex, two-component, spectra. Here…

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