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researcher

C. Brown

4 papers hereh-index 335 citations10 works total

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

author position
  • middle author2
  • last author1

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE4
same name
  • C. Brown — 3 papers, h 2
  • C. Brown — 2 papers, h 3
  • C. Brown — 1 paper, h 24
  • C. Brown — 1 paper, h 14
  • C. Brown — 1 paper, h 5
  • C. Brown — 1 paper, 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

collaborators

4 papers

astro-ph.HE2026

Population synthesis predictions of the Galactic compact binary gravitational wave foreground detectable by LISA

Jake McMillan, Adam Ingram, Cordelia Dashwood Brown +4

We use population synthesis modelling to predict the gravitational wave (GW) signal that the Laser Interferometer Space Antenna (LISA) will detect from the Galactic population of c…

astro-ph.HE2026

A comprehensive search for high-velocity X-ray sources: New compact object binary candidates in the Gaia era

Yue Zhao, Poshak Gandhi, Christian Knigge +6

We perform a comprehensive search for high-velocity X-ray sources with large X-ray/optical flux ratios (FX​/FG​), identifying candidates for interacting black h…

astro-ph.HE2025

Infrared Synchrotron Emission in the Soft State of GX 339-4 and the Mid-Infrared/X-ray Luminosity Plane of Black Hole X-ray Binaries

P. Gandhi, D. M. Russell, M. C. Baglio +33

Progress in understanding the growth of accreting black holes remains hampered by a lack of sensitive coordinated multiwavelength observations. In particular, the mid-infrared (MIR…

astro-ph.HE2025

Further evidence for natal kick segregation by spectral type in high-mass X-ray binaries

Pornisara Nuchvanichakul, Poshak Gandhi, Christian Knigge +4

High-mass X-ray binaries (HMXBs) are systems in which a neutron star or black hole accretes material from a massive companion. HMXBs are expected to have experienced a supernova in…

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