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researcher

K. Iwasawa

4 papers here

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

author position
  • first author2
  • middle author1
  • last author1

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

fields
  • astro-ph2
  • astro-ph.CO1
  • astro-ph.GA1
ORCID 0000-0002-4923-3281
same name
  • K. Iwasawa — 7 papers, h 60
  • K. Iwasawa — 1 paper, h 17

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
20062009
most citedHigh-ionization Fe K emission from luminous infrared galaxies

63 citations · 107 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.CO2009★ 2 cited

The gravitationally lensed, luminous infrared galaxy IRAS F10214+4724 observed with XMM-Newton

K. Iwasawa, C. Vignali, A. S. Evans +2

We report on a short XMM-Newton observation of the gravitationally-lensed, luminous infrared galaxy IRAS F10214+4724 at z=2.3. A faint X-ray source is detected at 4 sigma. The obse…

astro-ph.GA2009★ 63 cited

High-ionization Fe K emission from luminous infrared galaxies

K. Iwasawa, D. B. Sanders, A. S. Evans +3

The Chandra component of the Great Observatories All-Sky LIRG Survey (GOALS) presently contains 44 luminous and ultraluminous infrared galaxies with log (Lir/Lsun) = 11.73-12.57. O…

astro-ph2007★ 14 cited

Compton thick AGN in the Suzaku era

A. Comastri, R. Gilli, C. Vignali +3

Suzaku observations of two hard X-ray (> 10 keV) selected nearby Seyfert 2 galaxies are presented. Both sources were clearly detected with the PIN Hard X-ray Detector up to several…

astro-ph2006★ 28 cited

A longer XMM-Newton look at I Zwicky 1: Variability of the X-ray continuum, absorption, and iron Kalpha line

L. C. Gallo, W. N. Brandt, E. Costantini +3

We present the second XMM-Newton observation (85 ks) of the narrow-line Seyfert 1 galaxy (NLS1) I Zw 1 and describe its mean spectral and timing characteristics. On average, I Zw 1…

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