◍wovepaper
SearchResearchersInstitutions
Sign in
researcher

A. Sander

43 papers hereh-index 10379 citations55 works total

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

author position
  • first author2
  • middle author35
  • last author2

Across the 39 of 43 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR32
  • astro-ph.GA6
  • astro-ph.HE3
  • astro-ph.IM1
  • physics.gen-ph1
same name
  • A. Sander — 30 papers, h 55
  • A. Sander — 19 papers, h 2
  • A. Sander — 16 papers, h 4
  • A. Sander — 12 papers
  • A. Sander — 11 papers, h 16
  • A. Sander — 3 papers, h 30

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 citedBinarity at LOw Metallicity (BLOeM): a spectroscopic VLT monitoring survey of massive stars in the SMC

37 citations · 340 across the 36 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

3 papers · 1 filter

astro-ph.HE2024

Not just winds: why models find binary black hole formation is metallicity dependent, while binary neutron star formation is not

L. A. C. van Son, S. K. Roy, I. Mandel +6

Both detailed and rapid population studies alike predict that binary black hole (BHBH) formation is orders of magnitude more efficient at low metallicity than high metallicity, whi…

astro-ph.HE2024★ 4 cited

Multi-wavelength spectroscopic analysis of the ULX Holmberg II X-1 and its nebula suggests the presence of a heavy black hole accreting from a B-type donor

S. Reyero Serantes, L. Oskinova, W. -R. Hamann +11

Ultra-luminous X-ray sources (ULXs) are high-mass X-ray binaries with an X-ray luminosity above 1039 erg s−1. These ULXs can be powered by black holes that are more massi…

astro-ph.HE2023

A soft and transient ultraluminous X-ray source with 6-h modulation in the NGC 300 galaxy

A. Sacchi, P. Esposito, D. de Martino +13

We investigate the nature of CXOU J005440.5-374320 (J0054), a peculiar bright (∼4×1039 erg/s) and soft X-ray transient in the spiral galaxy NGC 300 with a 6-hour per…

◍wovepaper

Papers, researchers and institutions, woven together.

Explore
  • Search
  • Researchers
  • Institutions
Account
  • Library
  • Chat
Data
  • arXiv.org
  • Semantic Scholar
  • OpenAlex
  • Latest RSS
AboutContactPrivacyDevelopersllms.txtopenapi.json
Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.