activity
20022026
most citedGRB 080913 at redshift 6.7

220 citations · 3.8k across the 111 of their papers we have counts for

collaborators
Showing 2019 · astro-ph.EPShow all

5 papers · 2 filters

astro-ph.EP2019★ 9 cited

The first observed stellar occultations by the irregular satellite (Saturn IX) Phoebe and improved rotational period

A. R. Gomes-Júnior, M. Assafin, F. Braga-Ribas +24

We report six stellar occultations by (Saturn IX) Phoebe, an irregular satellite of Saturn, obtained between mid-2017 and mid-2019. The 2017 July 06 event is the first stellar occu…

astro-ph.EP2019★ 20 cited

Ground-based follow-up observations of TRAPPIST-1 transits in the near-infrared

A. Y. Burdanov, S. M. Lederer, M. Gillon +10

The TRAPPIST-1 planetary system is a favorable target for the atmospheric characterization of temperate earth-sized exoplanets by means of transmission spectroscopy with the forthc…

astro-ph.EP2019★ 24 cited

WASP-180Ab: Doppler tomography of an hot Jupiter orbiting the primary star in a visual binary

L. Y. Temple, C. Hellier, D. R. Anderson +26

We report the discovery and characterisation of WASP-180Ab, a hot Jupiter confirmed by the detection of its Doppler shadow and by measuring its mass using radial velocities. We fin…

astro-ph.EP2019★ 17 cited

The shape of (7) Iris as evidence of an ancient large impact?

J. Hanuš, M. Marsset, P. Vernazza +35

Asteroid (7) Iris is an ideal target for disk-resolved imaging owing to its brightness (V7-8) and large angular size of 0.33 arcsec during its apparitions. Iris is believed t…

astro-ph.EP2019★ 32 cited

The homogeneous internal structure of CM-like asteroid (41) Daphne

B. Carry, F. Vachier, J. Berthier +48

Context. CM-like asteroids (Ch and Cgh classes) are a major population within the broader C-complex, encompassing about 10% of the mass of the main asteroid belt. Their internal st…