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researcher

R. Sánchez-Janssen

4 papers hereh-index 12 citations4 works total

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

author position
  • middle author4

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

fields
  • astro-ph.GA4
same name
  • R. Sánchez-Janssen — 4 papers, h 4
  • R. Sánchez-Janssen — 4 papers, h 31
  • R. Sánchez-Janssen — 4 papers, h 5

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.GA2026

The Pristine Dwarf Galaxy Survey -- VII. The metallicity distributions of 12 Milky Way faint satellites

S. Taibi, P. Jablonka, N. Longeard +10

Spectroscopic studies of ultra-faint dwarf galaxies are typically limited to small samples of stars due to the scarcity of sufficiently bright targets. The small number statistics…

astro-ph.GA2025

Dwarf galaxies in the MATLAS Survey: Hubble Space Telescope observations of nuclear star clusters

Mélina Poulain, Francine R. Marleau, Pierre-Alain Duc +8

In dwarf galaxies, nuclear star clusters (NSCs) are believed to primarily form from the migration and merger of globular clusters (GCs), with a possible contribution from in-situ s…

astro-ph.GA2025

The Next Generation Virgo Cluster Survey (NGVS). XL. The Morphological Classification of Virgo Cluster Galaxies

Max M. Kurzner, Patrick Côté, Laura Ferrarese +19

We present a study of morphologies, based on deep u∗g′i′z′ imaging of the Virgo Cluster from the Next Generation Virgo Cluster Survey (NGVS), for 3689…

astro-ph.GA2025

AVID: Formation and evolution of a coalesced major merger of late-type dwarf galaxies (VCC 479) on the outskirts of the Virgo cluster

Weibin Sun, Hong-Xin Zhang, Rory Smith +24

Dwarf-dwarf galaxy mergers are among the least explored aspects of dwarf galaxy pre-processing as they fall into clusters. We present the first case study of a coalesced late-type…

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