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researcher

M. Ng

54 papers hereh-index 121.1k citations59 works total

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

author position
  • first author5
  • middle author44
  • last author1

Across the 50 of 54 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE52
  • astro-ph.SR2
same name
  • M. Ng — 28 papers, h 80
  • M. Ng — 19 papers, h 21
  • M. Ng — 13 papers, h 2
  • M. Ng — 7 papers, h 8
  • M. Ng — 4 papers, h 3
  • M. Ng — 2 papers, h 3

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
20172026
most citedBinary Population and Spectral Synthesis Version 2.1: construction, observational verification and new results

953 citations · 1.7k across the 52 of their papers we have counts for

collaborators
Showing 2026Show all

3 papers · 1 filter

astro-ph.HE2026

Discovery of the Infrared Counterpart of the Rapid Burster with JWST

Malina M. Desai, Kevin B. Burdge, Cristina Pallanca +8

The Rapid Burster (MXB 1730−335) is the only known neutron star to produce both Type I and Type II X-ray bursts, making it a key system for understanding accretion physics onto n…

astro-ph.HE2026

Evidence for Millihertz Oscillations in the bright atoll source GX 3+1

Malu Sudha, Renee M. Ludlam, Diego Altamirano +2

We report evidence for millihertz (mHz) QPOs in the bright atoll neutron star low-mass X-ray binary (NS LMXB) source GX 3+1 using NICER in the 0.5--10 keV energy band. Across 7 obs…

astro-ph.HE2026

Pulse profile modelling of the 2024 outburst of the accreting millisecond pulsar SRGA J144459.2-604207

Bas Dorsman, Tuomo Salmi, Anna L. Watts +14

Pulse profile modelling via relativistic ray-tracing can constrain the system parameters of neutron stars, notably their mass and radius. Among these objects, accreting millisecond…

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