activity
20162020
most citedThe size, shape, density and ring of the dwarf planet Haumea from a stellar occultation

258 citations · 377 across the 9 of their papers we have counts for

collaborators

9 papers

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.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.EP2019★ 29 cited

Thermal properties of slowly rotating asteroids: Results from a targeted survey

A. Marciniak, V. Alí-Lagoa, T. G. Müller +51

Context. Earlier work suggests that slowly rotating asteroids should have higher thermal inertias than faster rotators because the heat wave penetrates deeper into the sub-surface.…

astro-ph.EP2017★ 26 cited

Small Bodies Near and Far (SBNAF): a benchmark study on physical and thermal properties of small bodies in the Solar System

T. G. Müller, A. Marciniak, C. Kiss +15

The combination of visible and thermal data from the ground and astrophysics space missions is key to improving the scientific understanding of near-Earth, main-belt, trojans, cent…

astro-ph.EP2017★ 4 cited

Statistical analysis of the ambiguities in the asteroid period determinations

M. Butkiewicz-Bąk, T. Kwiatkowski, P. Bartczak +2

Among asteroids there exist ambiguities in their rotation period determinations. They are due to incomplete coverage of the rotation, noise and/or aliases resulting from gaps betwe…

astro-ph.SR2017★ 4 cited

MN Draconis - peculiar, active dwarf nova in the period gap

K. Bakowska, A. Olech, R. Pospieszynski +7

Context: We present results of an extensive world-wide observing campaign of MN Draconis. Aims: MN Draconis is a poorly known active dwarf nova in the period gap and is one of the…

astro-ph.EP2016★ 5 cited

Large Halloween Asteroid at Lunar Distance

T. G. Müller, A. Marciniak, M. Butkiewicz-Bąk +7

The near-Earth asteroid (NEA) 2015 TB145 had a very close encounter with Earth at 1.3 lunar distances on October 31, 2015. We obtained 3-band mid-infrared observations with the ESO…