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20082026
most citedThe size, shape, density and ring of the dwarf planet Haumea from a stellar occultation

258 citations · 1.3k across the 47 of their papers we have counts for

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Showing 2020Show all

9 papers · 1 filter

astro-ph.HE2020★ 70 cited

SN 2019ehk: A Double-Peaked Ca-rich Transient with Luminous X-ray Emission and Shock-Ionized Spectral Features

Wynn V. Jacobson-Galán, Raffaella Margutti, Charles D. Kilpatrick +64

We present panchromatic observations and modeling of the Calcium-rich supernova 2019ehk in the star-forming galaxy M100 (d16.2 Mpc) starting 10 hours after explosion and c…

astro-ph.SR2020★ 48 cited

Gaia 18dvy: a new FUor in the Cygnus OB3 association

E. Szegedi-Elek, P. Ábrahám, L. Wyrzykowski +59

We present optical-infrared photometric and spectroscopic observations of Gaia18dvy, located in the Cygnus OB3 association at a distance of 1.88 kpc. The object was noted by the Ga…

astro-ph.EP2020★ 258 cited

The size, shape, density and ring of the dwarf planet Haumea from a stellar occultation

J. L. Ortiz, P. Santos-Sanz, B. Sicardy +90

Among the four known transneptunian dwarf planets, Haumea is an exotic, very elongated, and fast rotating body. In contrast to the other dwarf planets, its size, shape, albedo, and…

astro-ph.EP2020★ 23 cited

The large Trans-Neptunian Object 2002 TC from combined stellar occultation, photometry and astrometry data

J. L. Ortiz, P. Santos-Sanz, B. Sicardy +78

On 28th January 2018, the large Trans-Neptunian Object (TNO) 2002TC302 occulted a m15.3 star with ID 130957813463146112 in the Gaia DR2 stellar catalog. 12 positive occultati…

astro-ph.EP2020★ 20 cited

Thermal properties of large main-belt asteroids observed by Herschel PACS

V. Alí-Lagoa, T. G. Müller, C. Kiss +11

Non-resolved thermal infrared observations enable studies of thermal and physical properties of asteroid surfaces provided the shape and rotational properties of the target are wel…

astro-ph.IM2020★ 20 cited

Small Bodies: Near and Far Database for thermal infrared observations of small bodies in the Solar System

Róbert Szakáts, Thomas Müller, Víctor Alí-Lagoa +4

In this paper we present the "Small Bodies: Near and Far" Infrared Database, an easy-to-use tool intended to facilitate the modeling of thermal emission of small Solar System bodie…

astro-ph.EP2020★ 8 cited

Physical parameters of selected Gaia mass asteroids

E. Podlewska-Gaca, A. Marciniak, V. Alí-Lagoa +36

Thanks to the Gaia mission, it will be possible to determine the masses of approximately hundreds of large main belt asteroids with very good precision. We currently have diameter…

astro-ph.EP2020★ 18 cited

Rotational properties of Hilda asteroids observed by the K2 mission

Gyula M. Szabó, Csaba Kiss, Róbert Szakáts +7

Hilda asteroids orbit at the outer edge, or just outside of the Main Belt, occupying the 2:3 mean motion resonance with Jupiter. It is known that the group shows a mixed taxonomy t…

astro-ph.EP2020★ 91 cited

Solar System objects observed with TESS -- First data release: bright main-belt and Trojan asteroids from the Southern Survey

András Pál, Róbert Szakáts, Csaba Kiss +10

Compared with previous space-borne surveys, the Transiting Exoplanet Survey Satellite (TESS) provides a unique and new approach to observe Solar System objects. While its primary m…