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researcher

E. Sissa

40 papers hereh-index 302.8k citations95 works total

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

author position
  • first author2
  • middle author21

Across the 23 of 40 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP30
  • astro-ph.SR7
  • astro-ph.IM3
same name
  • E. Sissa — 3 papers
  • E. Sissa — 2 papers, h 3
  • E. Sissa — 2 papers

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
20152021
most citedDiscovery of a warm, dusty giant planet around HIP65426

205 citations · 937 across the 21 of their papers we have counts for

collaborators
Showing 2017Show all

4 papers · 1 filter

astro-ph.EP2017★ 45 cited

The HIP 79977 debris disk in polarized light

N. Engler, H. M. Schmid, Ch. Thalmann +40

We present observations of the known edge-on debris disk around HIP 79977 (HD 146897, F star in Upper Sco, 123 pc), taken with the ZIMPOL differential polarimeter of the SPHERE ins…

astro-ph.EP2017★ 76 cited

Investigation of the inner structures around HD169142 with VLT/SPHERE

R. Ligi, A. Vigan, R. Gratton +47

We present observations of the Herbig Ae star HD169142 with VLT/SPHERE instruments InfraRed Dual-band Imager and Spectrograph (IRDIS) (K1K2 and H2H3 bands) and the Integral Fie…

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.EP2017★ 41 cited

New constraints on the disk characteristics and companion candidates around T Cha with VLT/SPHERE

A. Pohl, E. Sissa, M. Langlois +34

The transition disk around the T Tauri star T Cha possesses a large gap, making it a prime target for high-resolution imaging in the context of planet formation. We aim to find sig…

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