activity
20112024
most citedNew and updated convex shape models of asteroids based on optical data from a large collaboration network

84 citations · 408 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.EP2024

Comet 81/P Wild 2: changes in the spin axis orientation during the last five apparitions

V. Oldani, F. Manzini, P. Ochner +8

Comet 81P (Wild 2) is characterized by the presence of a prominent-fan shaped dust emission originating from an active source at high latitude on the nucleus, whose axis is assumed…

astro-ph.EP2023★ 11 cited

Scaling slowly rotating asteroids by stellar occultations

A. Marciniak, J. Ďurech, A. Choukroun +176

As evidenced by recent survey results, majority of asteroids are slow rotators (P>12 h), but lack spin and shape models due to selection bias. This bias is skewing our overall unde…

astro-ph.HE2022★ 17 cited

GRANDMA Observations of ZTF/Fink Transients during Summer 2021

V. Aivazyan, M. Almualla, S. Antier +80

We present our follow-up observations with GRANDMA of transient sources revealed by the Zwicky Transient Facility (ZTF). Over a period of six months, all ZTF triggers were examined…

astro-ph.EP2018★ 72 cited

The extraordinary composition of the "blue comet" C/2016 R2 (PanSTARRS)

N. Biver, D. Bockelée-Morvan, G. Paubert +9

We present a multi-wavelength study of comet C/2016 R2 (PanSTARRS). This comet was observed on 23-24 January 2018 with the IRAM 30m telescope, and in January to March 2018 with the…

astro-ph.EP2017★ 46 cited

3D shape of asteroid (6)~Hebe from VLT/SPHERE imaging: Implications for the origin of ordinary H chondrites

M. Marsset, B. Carry, C. Dumas +15

Context. The high-angular-resolution capability of the new-generation ground-based adaptive-optics camera SPHERE at ESO VLT allows us to assess, for the very first time, the crater…

astro-ph.EP2016★ 32 cited

EPIC211089792 b: an aligned and inflated hot jupiter in a young visual binary

A. Santerne, G. Hébrard, J. Lillo-Box +71

In the present paper we report the discovery of a new hot Jupiter, EPIC211089792 b, first detected by the Super-WASP observatory and then by the K2 space mission during its campaig…

astro-ph.EP2015★ 84 cited

New and updated convex shape models of asteroids based on optical data from a large collaboration network

J. Hanuš, J. Ďurech, D. A. Oszkiewicz +165

Asteroid modeling efforts in the last decade resulted in a comprehensive dataset of almost 400 convex shape models and their rotation states. This amount already provided a deep in…

astro-ph.SR2014★ 29 cited

The historical vanishing of the Blazhko effect of RR Lyr from GEOS and Kepler surveys

J. F. Le Borgne, E. Poretti, A. Klotz +20

RR Lyr is one of the most studied variable stars. Its light curve has been regularly monitored since the discovery of the periodic variability in 1899. Analysis of all observed max…

astro-ph.IM2013★ 57 cited

Instrumental Methods for Professional and Amateur Collaborations in Planetary Astronomy

O. Mousis, R. Hueso, J. -P. Beaulieu +57

Amateur contributions to professional publications have increased exponentially over the last decades in the field of Planetary Astronomy. Here we review the different domains of t…

astro-ph.SR2012★ 25 cited

The all-sky GEOS RR Lyr survey with the TAROT telescopes. Analysis of the Blazhko effect

J. -F. Le Borgne, A. Klotz, E. Poretti +9

We used the GEOS database to study the Blazhko effect of galactic RRab stars. The database is continuously enriched by maxima supplied by amateur astronomers and by a dedicated sur…

astro-ph.HE2011★ 35 cited

GRB 110205A: Anatomy of a long gamma-ray burst

B. Gendre, J. L. Atteia, M. Boër +8

The Swift burst GRB 110205A was a very bright burst visible in the Northern hemisphere. GRB 110205A was intrinsically long and very energetic and it occurred in a low-density inter…