Pith. sign in

REVIEW 1 cited by

A small survey of the magnetic fields of planet-host stars

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1307.6091 v2 pith:5RVLU3KG submitted 2013-07-23 astro-ph.SR

A small survey of the magnetic fields of planet-host stars

Rim Fares , Claire Moutou , Jean-Fran\c{c}ois Donati , Claude Catala , Evgenya Shkolnik , Moira Jardine , Andrew Cameron , Magali Deleuil This is my paper
classification astro-ph.SR
keywords magneticstarsfieldsurveybeendaysdetectedobservations
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
0 comments
read the original abstract

Using spectropolarimetry, we investigate the large-scale magnetic topologies of stars hosting close-in exoplanets. A small survey of ten stars has been done with the twin instruments TBL/NARVAL and CFHT/ESPaDOnS between 2006 and 2011. Each target consists of circular-polarization observations covering 7 to 22 days. For each of the 7 targets in which a magnetic field was detected, we reconstructed the magnetic field topology using Zeeman-Doppler imaging. Otherwise, a detection limit has been estimated. Three new epochs of observations of Tau Boo are presented, which confirm magnetic polarity reversal. We estimate that the cycle period is 2 years, but recall that a shorter period of 240 days can not still be ruled out. The result of our survey is compared to the global picture of stellar magnetic field properties in the mass-rotation diagram. The comparison shows that these giant planet-host stars tend to have similar magnetic field topologies to stars without detected hot-Jupiters. This needs to be confirmed with a larger sample of stars.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Tentative detection of circularly polarized bursty radio emissions from the HD 189733 exoplanetary system using NenuFAR beamformed observations

    astro-ph.EP 2026-07 conditional novelty 5.5

    NenuFAR beamformed Stokes-V data tentatively show a ~10σ left-hand circularly polarized burst from HD 189733 at 27–40 MHz lasting ~16 min, offset by ~1 h from the imaging burst of Zhang et al. (2025).