activity
20032022
most citedSignatures of a jet cocoon in early spectra of a supernova associated with a -ray burst

151 citations · 405 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.EP2022★ 12 cited

Asteroid phase curves using sparse Gaia DR2 data and differential dense light curves

E. Wilawer, D. Oszkiewicz, A. Kryszczyńska +10

The amount of sparse asteroid photometry being gathered by both space- and ground-based surveys is growing exponentially. This large volume of data poses a computational challenge…

astro-ph.EP2021★ 9 cited

Photometry and model of near-Earth asteroid 2021 DW1 from one apparition

T. Kwiatkowski, P. Koleńczuk, A. Kryszczyńska +17

On 4 March 2021 at 9 UTC a 30-m in diameter near-Earth asteroid 2021 DW1 passed the Earth at a distance of 570000 km, reaching the maximum brightness of V=14.6 mag. We observed it…

astro-ph.EP2021★ 9 cited

Photometry of selected outer main belt asteroids

V. Shevchenko, O. Mikhalchenko, I. Belskaya +17

We present new photometric observations for twelve asteroids ((122) Gerda, (152) Atala, (260) Huberta, (665) Sabine, (692) Hippodamia, (723) Hammonia, (745) Mauritia, (768) Struvea…

astro-ph.HE2019★ 151 cited

Signatures of a jet cocoon in early spectra of a supernova associated with a -ray burst

L. Izzo, A. de Ugarte Postigo, K. Maeda +39

Long gamma-ray bursts mark the death of massive stars, as revealed by their association with energetic broad-lined stripped-envelope supernovae. The scarcity of nearby events and t…

astro-ph.EP2017★ 5 cited

Shape and spin determination of Barbarian asteroids

M. Devogèle, P. Tanga, P. Bendjoya +51

Context. The so-called Barbarian asteroids share peculiar, but common polarimetric properties, probably related to both their shape and composition. They are named after (234) Barb…

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…