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researcher

M. Kramer

214 papers hereh-index 7423.8k citations497 works total

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

author position
  • sole author9
  • first author8
  • middle author150
  • last author21

Across the 188 of 214 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE73
  • astro-ph59
  • astro-ph.IM24
  • astro-ph.GA22
  • astro-ph.SR21
  • gr-qc12
same name
  • M. Kramer — 98 papers, h 29
  • M. Kramer — 72 papers, h 39
  • M. Kramer — 72 papers, h 48
  • M. Kramer — 58 papers, h 53
  • M. Kramer — 37 papers, h 17
  • M. Kramer — 33 papers, h 23

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
19982021
most citedA Massive Pulsar in a Compact Relativistic Binary

3.9k citations · 24.6k across the 209 of their papers we have counts for

collaborators
Showing 2018 · astro-ph.IMShow all

3 papers · 2 filters

astro-ph.IM2018

RFI Flagging Implications for Short-Duration Transients

Y. Cendes, P. Prasad, A. Rowlinson +24

With their wide fields of view and often relatively long coverage of any position in the sky in imaging survey mode, modern radio telescopes provide a data stream that is naturally…

astro-ph.IM2018

LOFT-e: Localisation Of Fast Transients with e-MERLIN

C. R. H. Walker, R. P. Breton, P. A. Harrison +8

The majority of fast radio bursts (FRBs) are poorly localised, hindering their potential scientific yield as galactic, intergalactic, and cosmological probes. LOFT-e, a digital bac…

astro-ph.IM2018★ 28 cited

MeerTime - the MeerKAT Key Science Program on Pulsar Timing

M. Bailes, E. Barr, N. D. R. Bhat +28

The MeerKAT telescope represents an outstanding opportunity for radio pulsar timing science with its unique combination of a large collecting area and aperture efficiency (effectiv…

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