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M. Ward

32 papers hereh-index 9720 citations14 works total

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

author position
  • middle author15
  • last author13

Across the 28 of 32 papers where every author was matched, so the position is known.

fields
  • astro-ph32
same name
  • M. Ward — 118 papers, h 58
  • M. Ward — 33 papers, h 15
  • M. Ward — 26 papers, h 18
  • M. Ward — 21 papers, h 38
  • M. Ward — 16 papers, h 5
  • M. Ward — 14 papers, h 21

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
19972004
most citedUltraluminous X-Ray Sources in External Galaxies

736 citations · 2.7k across the 32 of their papers we have counts for

collaborators
Showing 1998Show all

4 papers · 1 filter

astro-ph1998

ISOCAM Photometry of Narrow-Line X-ray Galaxies

J. D. Law-Green, A. Zezas, M. J. Ward +1

Mid-infrared photometry of the hosts of Narrow-Line X-ray Galaxies at 6 microns and 12 microns has been attempted with ISOCAM. No conclusive detections have been made. This implies…

astro-ph1998★ 97 cited

ROSAT and ASCA Observations of X-ray Luminous starburst Galaxies : NGC3310 and NGC3690

A. L. Zezas, I. Georgantopoulos, M. J. Ward

We present ROSAT (HRI and PSPC) and ASCA observations of the two luminous (L_x ~10^{41-42} erg s^{-1}) star-forming galaxies NGC3310 and NGC3690. The HRI shows clearly that the sou…

astro-ph1998

Near and Mid Infrared Imaging Polarimetry of NGC1068

S. L. Lumsden, T. J. T. Moore, C. Smith +3

We present the results of a series of observations of the near- and mid-infrared polarisation properties of the Seyfert 2 galaxy NGC1068. Our data agree well with previously publis…

astro-ph1998★ 14 cited

Stellar population in Active Galactic Nuclei. I. The Observations

M. Serote Roos, C. Boisson, M. Joly +1

Recent observations supported by theoretical models have lead to the view that giant and supergiant stars are over abundant, and/or a high metallicity component may be present, in…

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