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researcher

M. Serylak

103 papers hereh-index 335.4k citations159 works total

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

author position
  • first author5
  • middle author59
  • last author11

Across the 75 of 103 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE61
  • astro-ph.GA15
  • astro-ph.IM15
  • astro-ph.SR8
  • astro-ph3
  • astro-ph.EP1
same name
  • M. Serylak — 2 papers

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
20082026
most citedLOFAR: The LOw-Frequency ARray

2.7k citations · 7.1k across the 101 of their papers we have counts for

collaborators
Showing 2014 · astro-ph.GAShow all

3 papers · 2 filters

astro-ph.GA2014★ 34 cited

LOFAR low-band antenna observations of the 3C295 and Bootes fields: source counts and ultra-steep spectrum sources

R. J. van Weeren, W. L. Williams, C. Tasse +98

We present LOFAR Low Band observations of the Bootes and 3C295 fields. Our images made at 34, 46, and 62 MHz reach noise levels of 12, 8, and 5 mJy beam−1, making them the dee…

astro-ph.GA2014★ 30 cited

LOFAR observations of PSR B0943+10: profile evolution and discovery of a systematically changing profile delay in Bright mode

A. Bilous, J. Hessels, V. Kondratiev +10

We present broadband, low-frequency (25-80 MHz and 110-190 MHz) LOFAR observations of PSR B0943+10, with the goal of better illuminating the nature of its enigmatic mode-switching…

astro-ph.GA2014★ 82 cited

Initial LOFAR observations of Epoch of Reionization windows: II. Diffuse polarized emission in the ELAIS-N1 field

V. Jelic, A. G. de Bruyn, M. Mevius +106

This study aims to characterise the polarized foreground emission in the ELAIS-N1 field and to address its possible implications for the extraction of the cosmological 21-cm signal…

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