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researcher

C. D. de Vries

53 papers hereh-index 191.4k citations59 works total

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

author position
  • first author3
  • middle author24
  • last author11

Across the 38 of 53 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE17
  • astro-ph.IM13
  • astro-ph8
  • astro-ph.CO6
  • astro-ph.GA6
  • astro-ph.SR2
same name
  • C. D. de Vries — 1 paper, h 6

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
20002022
most citedA fast and long-lived outflow from the supermassive black hole in NGC 5548

247 citations · 2.7k across the 53 of their papers we have counts for

collaborators
Showing 2013Show all

4 papers · 1 filter

astro-ph.IM2013★ 43 cited

A Comprehensive X-ray Absorption Model for Atomic Oxygen

T. W. Gorczyca, M. A. Bautista, M. F. Hasoglu +9

An analytical formula is developed to represent accurately the photoabsorption cross section of O I for all energies of interest in X-ray spectral modeling. In the vicinity of the…

astro-ph.IM2013★ 43 cited

The Hot and Energetic Universe: The X-ray Integral Field Unit (X-IFU) for Athena+

D. Barret, J. W. den Herder, L. Piro +55

The Athena+ mission concept is designed to implement the Hot and Energetic Universe science theme submitted to the European Space Agency in response to the call for White Papers fo…

astro-ph.HE2013★ 24 cited

The X-ray/UV absorber in NGC 4593

J. Ebrero, J. S. Kaastra, G. A. Kriss +2

We present the results of a recent (March 2011) 160 ks Chandra-LETGS observation of the Seyfert galaxy NGC 4593, and the analysis of archival X-ray and UV spectra taken with XMM-Ne…

astro-ph.GA2013★ 110 cited

ISM composition through X-ray spectroscopy of LMXBs

C. Pinto, J. S. Kaastra, E. Costantini +1

The diffuse interstellar medium (ISM) is an integral part of the evolution of the entire Galaxy. Metals are produced by stars and their abundances are the direct testimony of the h…

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