◍wovepaper
SearchResearchersInstitutions
Sign in
researcher

C. Tasse

160 papers hereh-index 519.2k citations257 works total

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

author position
  • sole author1
  • first author2
  • middle author91
  • last author23

Across the 117 of 160 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA70
  • astro-ph.IM33
  • astro-ph.CO24
  • astro-ph.HE17
  • astro-ph.SR11
  • astro-ph.EP4
same name
  • C. Tasse — 14 papers, h 3
  • C. Tasse — 11 papers, h 5
  • C. Tasse — 3 papers
  • C. Tasse — 2 papers, h 3
  • C. Tasse — 1 paper
  • C. Tasse — 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
20072026
most citedLOFAR: The LOw-Frequency ARray

2.7k citations · 12.9k across the 158 of their papers we have counts for

collaborators
Showing astro-ph.EPShow all

4 papers · 1 filter

astro-ph.EP2026

Radio emission from star-planet interactions

H. K. Vedantham, A. Strugarek, C. K. Louis +12

Stars interact with their exoplanets though gravity, radiation, plasma and magnetic fields. Stellar plasma and magnetic fields impose electrodynamic effects on exoplanet atmosphere…

astro-ph.EP2025★ 3 cited

A circularly polarized low-frequency radio burst from the exoplanetary system HD 189733

X. Zhang, P. Zarka, J. N. Girard +17

We aim to detect low-frequency radio emission from exoplanetary systems, which can provide insights into planetary magnetic fields, star-planet interactions, stellar activity, and…

astro-ph.EP2020★ 146 cited

Coherent radio emission from a quiescent red dwarf indicative of star-planet interaction

H. K. Vedantham, J. R. Callingham, T. W. Shimwell +11

Low frequency (ν≲150MHz) stellar radio emission is expected to originate in the outer corona at heights comparable to and larger than the stellar radius. Such emission…

astro-ph.EP2015★ 53 cited

Imaging Jupiter's radiation belts down to 127 MHz with LOFAR

J. N. Girard, P. Zarka, C. Tasse +71

Context. Observing Jupiter's synchrotron emission from the Earth remains today the sole method to scrutinize the distribution and dynamical behavior of the ultra energetic electron…

◍wovepaper

Papers, researchers and institutions, woven together.

Explore
  • Search
  • Researchers
  • Institutions
Account
  • Library
  • Chat
Data
  • arXiv.org
  • Semantic Scholar
  • OpenAlex
  • Latest RSS
AboutContactPrivacyDevelopersllms.txtopenapi.json
Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.