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O. Perdereau

25 papers here

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

author position
  • middle author1

Across the 1 of 25 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO16
  • astro-ph4
  • astro-ph.IM3
  • astro-ph.GA1
  • hep-ex1
same name
  • O. Perdereau — 157 papers, h 87
  • O. Perdereau — 2 papers, h 6
  • O. Perdereau — 1 paper

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
19942016
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations · 15.9k across the 25 of their papers we have counts for

collaborators
Showing astro-phShow all

4 papers · 1 filter

astro-ph2004★ 31 cited

EROS 2 photometry of probable R Coronae Borealis stars in the Small Magellanic Cloud

P. Tisserand, J. B. Marquette, J. P. Beaulieu +1

EROS 2 (Experience de Recherche d'Objets Sombres) conducted a survey of the SMC between July 1996 and February 2003 in two EROS broad-band colours, V_E and R_E. The photometric dat…

astro-ph2001★ 25 cited

Photometric Constraints on Microlens Spectroscopy of EROS-BLG-2000-5

C. Afonso

We apply EROS photometric data to interpret previously published Keck and VLT spectra of the binary-microlens caustic-crossing event EROS-BLG-2000-5. We show that the VLT data impl…

astro-ph2000★ 51 cited

Observation of Microlensing towards the Galactic Spiral Arms. EROS II 3 year survey

EROS Collaboration

We present an analysis of the light curves of 9.1 million stars observed during three seasons by EROS (Experience de Recherche d'Objets Sombres), in the Galactic plane away from th…

astro-ph1997

AGAPEROS: Searches for microlensing in the LMC with the Pixel Method. I. Data treatment and pixel light curves production

A. -L. Melchior

Recent surveys monitoring millions of light curves of resolved stars in the LMC have discovered several microlensing events. Unresolved stars could however significantly contribute…

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