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P. Blanchard

2 papers hereh-index 151.3k citations41 works total

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

author position
  • middle author1

Across the 1 of 2 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP2
same name
  • P. Blanchard — 33 papers, h 30
  • P. Blanchard — 12 papers
  • P. Blanchard — 3 papers, h 42
  • P. Blanchard — 1 paper, h 2
  • P. Blanchard — 1 paper
  • P. Blanchard — 1 paper, h 31

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

most citedDiscovery of a warm, dusty giant planet around HIP65426

205 citations · 205 across the 1 of their papers we have counts for

collaborators

4 papers

astro-ph.SR2020★ 11 cited

The circumstellar environment of EX Lup: the SPHERE and SINFONI views

E. Rigliaco, R. Gratton, A. Kospal +15

EX Lup is a well-studied T Tauri star that represents the prototype of young eruptive stars EXors. In this paper we analyze new adaptive optics imaging and spectroscopic observatio…

astro-ph.EP2019

Shadowing and multiple rings in the protoplanetary disk of HD 139614

G. A. Muro-Arena, M. Benisty, C. Ginski +20

Shadows in scattered light images of protoplanetary disks are a common feature and support the presence of warps or misalignments between disk regions. These warps are possibly due…

astro-ph.EP2017★ 205 cited

Discovery of a warm, dusty giant planet around HIP65426

G. Chauvin, S. Desidera, A. -M. Lagrange +120

The SHINE program is a large high-contrast near-infrared survey of 600 young, nearby stars. It is aimed at searching for and characterizing new planetary systems using VLT/SPHERE's…

astro-ph.EP2016

Discovery of concentric broken rings at sub-arcsec separations in the HD 141569A gas-rich, debris disk with VLT/SPHERE

C. Perrot, A. Boccaletti, E. Pantin +45

Transition disks correspond to a short stage between the young protoplanetary phase and older debris phase. Along this evolutionary sequence, the gas component disappears leaving r…

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