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researcher

P. Maxted

251 papers hereh-index 5710.7k citations370 works total

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

author position
  • sole author6
  • first author21
  • middle author173
  • last author8

Across the 208 of 251 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP120
  • astro-ph.SR92
  • astro-ph34
  • astro-ph.IM5
same name
  • P. Maxted — 120 papers, h 33
  • P. Maxted — 2 papers, h 1
  • P. Maxted — 2 papers, h 2
  • P. Maxted — 1 paper, h 1

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
19992026
most citedThe WASP Project and the SuperWASP Cameras

1.2k citations · 17.1k across the 247 of their papers we have counts for

collaborators
Showing 2000 · astro-phShow all

4 papers · 2 filters

astro-ph2000★ 93 cited

Radial velocity measurements of white dwarfs

P. F. L. Maxted, T. R. Marsh, C. K. J. Moran

We present 594 radial velocity measurements for 71 white dwarfs obtained during our search for binary white dwarfs and not reported elsewhere. We identify three excellent candidate…

astro-ph2000★ 57 cited

WD1953-011 - a magnetic white dwarf with peculiar field structure

P. F. L. Maxted, L. Ferrario, T. R. Marsh +1

We present H-alpha spectra of the magnetic white dwarf star WD1953-011 which confirm the presence of the broad Zeeman components corresponding to a field strength of about 500kG fo…

astro-ph2000★ 49 cited

Discovery of the optical counterpart and early optical observations of GRB990712

Kailash C. Sahu

We present the discovery observations of the optical counterpart of the gamma-ray burster GRB990712 taken 4.16 hours after the outburst and discuss its light curve observed in the…

astro-ph2000★ 61 cited

The triple degenerate star WD1704+481

P. F. L. Maxted, T. R. Marsh, C. K. J. Moran +1

WD1704+481 is a visual binary in which both components are white dwarfs. We present spectra of the H-alpha line of both stars which show that one component (WD1704+481.2 = Sandulea…

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