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T. Verdugo

31 papers hereh-index 161.3k citations44 works total

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

author position
  • first author5
  • middle author16
  • last author8

Across the 29 of 31 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO20
  • astro-ph.GA5
  • astro-ph4
  • astro-ph.IM1
  • cs.CV1
same name
  • T. Verdugo — 3 papers
  • T. Verdugo — 2 papers, h 2

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
20032026
most citedA Bayesian approach to strong lensing modelling of galaxy clusters

636 citations · 1.2k across the 30 of their papers we have counts for

collaborators
Showing 2014Show all

4 papers · 1 filter

astro-ph.CO2014★ 29 cited

SARCS strong-lensing galaxy groups: II - mass-concentration relation and strong-lensing bias

G. Foëx, V. Motta, E. Jullo +2

Our work is based on the stacked weak-lensing analysis of a sample of 80 strong-lensing galaxy groups. Our main results are the following: (i) the lensing signal does not allow us…

astro-ph.CO2014★ 9 cited

Characterizing SL2S galaxy groups using the Einstein radius

T. Verdugo, V. Motta, G. Foëx +11

We analyzed the Einstein radius, θE​, in our sample of SL2S galaxy groups, and compared it with RA​ (the distance from the arcs to the center of the lens), using three differen…

astro-ph.CO2014★ 8 cited

The abundance of Bullet-groups in LCDM

J. G. Fernandez-Trincado, J. E. Forero-Romero, G. Foex +2

We estimate the expected distribution of displacements between the two dominant dark matter (DM) peaks (DM-DM displacements) and between DM and gaseous baryon peak (DM-gas displace…

astro-ph.CO2014★ 23 cited

Dark matter-baryons separation at the lowest mass scale: the Bullet Group

F. Gastaldello, M. Limousin, G. Foëx +13

We report on the X-ray observation of a strong lensing selected group, SL2S J08544-0121, with a total mass of 2.4±0.6×1014 M⊙​ which revealed a separatio…

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