papers

Publications (7)

astro-ph.EP2010

Physical properties of ESA Rosetta target asteroid (21) Lutetia: Shape and flyby geometry

B. Carry, M. Kaasalainen, C. Leyrat +22

Aims. We determine the physical properties (spin state and shape) of asteroid (21) Lutetia, target of the ESA Rosetta mission, to help in preparing for observations during the flyb…

astro-ph2008

New determination of the size and bulk density of the binary asteroid 22 Kalliope from observations of mutual eclipses

P. Descamps, F. Marchis, J. Pollock +16

In 2007, the M-type binary asteroid 22 Kalliope reached one of its annual equinoxes. As a consequence, the orbit plane of its small moon, Linus, was aligned closely to the Sun's li…

astro-ph.EP2015

The non-convex shape of (234) Barbara, the first Barbarian

P. Tanga, B. Carry, F. Colas +37

Asteroid (234) Barbara is the prototype of a category of asteroids that has been shown to be extremely rich in refractory inclusions, the oldest material ever found in the Solar Sy…

astro-ph.EP2010

Triplicity and Physical Characteristics of Asteroid (216) Kleopatra

Pascal Descamps, F. Marchis, J. Berthier +16

To take full advantage of the September 2008 opposition passage of the M-type asteroid (216) Kleopatra, we have used near-infrared adaptive optics (AO) imaging with the W.M. Keck I…

astro-ph.SR2016

The multi-faceted Type II-L supernova 2014G from pre-maximum to nebular phase

G. Terreran, A. Jerkstrand, S. Benetti +18

We present multi-band ultraviolet, optical, and near-infrared photometry, along with visual-wavelength spectroscopy, of supernova (SN) 2014G in the nearby galaxy NGC 3448 (25 Mpc).…

astro-ph.HE2021

How low can you go? SN 2018zd as a low-mass Fe core-collapse supernova

E. Callis, M. Fraser, A. Pastorello +38

We present spectroscopy and photometry of SN 2018zd, a Type IIP core-collapse supernova with signatures of interaction with circumstantial material in its earliest spectra. High io…

astro-ph.EP2009

A Giant Crater on 90 Antiope?

P. Descamps, F. Marchis, T. Michalowski +11

Mutual event observations between the two components of 90 Antiope were carried out in 2007-2008. The pole position was refined to lambda0 = 199.5+/-0.5 eg and beta0 = 39.8+/-5 deg…