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M. Mclaughlin

34 papers hereh-index 6623k citations393 works total

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

author position
  • first author6
  • middle author20
  • last author2

Across the 28 of 34 papers where every author was matched, so the position is known.

fields
  • astro-ph29
  • astro-ph.HE3
  • astro-ph.GA1
  • astro-ph.SR1
same name
  • M. Mclaughlin — 21 papers, h 34
  • M. McLaughlin — 9 papers, h 31
  • M. McLaughlin — 1 paper, h 4
  • M. McLaughlin — 1 paper, h 13

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
20022011
most citedA Radio Pulsar/X-ray Binary Link

591 citations · 1.1k across the 23 of their papers we have counts for

collaborators
Showing 2005 · astro-phShow all

4 papers · 2 filters

astro-ph2005

Arecibo Pulsar Survey Using ALFA. I. Survey Strategy and First Discoveries

J. M. Cordes, P. C. C. Freire, D. R. Lorimer +21

We report results from the initial stage of a long-term pulsar survey of the Galactic plane using the Arecibo L-band Feed Array (ALFA), a seven-beam receiver operating at 1.4 GHz w…

astro-ph2005

Arecibo timing and single-pulse observations of 17 pulsars

D. J. Champion, D. R. Lorimer, M. A. McLaughlin +6

We report on timing and single-pulse observations of 17 pulsars discovered at the Arecibo observatory. The highlights of our sample are the recycled pulsars J1829+2456, J1944+0907…

astro-ph2005

Discovery of 10 pulsars in an Arecibo drift-scan survey

D. R. Lorimer, K. M. Xilouris, A. S. Fruchter +8

We present the results of a 430-MHz survey for pulsars conducted during the upgrade to the 305-m Arecibo radio telescope. Our survey covered a total of 1147 square degrees of sky u…

astro-ph2005

A Search for Radio Emission from the Young 16-ms X-ray Pulsar PSR J0537-6910

F. Crawford, M. McLaughlin, S. Johnston +2

PSR J0537-6910 is a young, energetic, rotation-powered X-ray pulsar with a spin period of 16 ms located in the Large Magellanic Cloud. We have searched for previously undetected ra…

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