activity
20132021
most citedAsteroids' physical models from combined dense and sparse photometry and scaling of the YORP effect by the observed obliquity distribution

85 citations · 201 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.EP202116 cited

Properties of slowly rotating asteroids from the Convex Inversion Thermophysical Model

A. Marciniak, J. Ďurech, V. Alí-Lagoa +73

Results from the TESS mission showed that previous studies strngly underestimated the number of slow rotators, revealing the importance of studying those asteroids. For most slowly…

astro-ph.HE20212 cited

GN-z11-flash was a signal from a man-made satellite not a gamma-ray burst at redshift 11

Michał J. Michałowski, Krzysztof Kamiński, Monika K. Kamińska +1

Long gamma-ray bursts (GRB), explosions of very massive stars, provide crucial information on stellar and galaxy evolution, even at redshifts z ~ 8 - 9.5, when the Universe was onl…

astro-ph.EP201929 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.SR2017

Photometric and spectroscopic variability of 53 Per

E. Niemczura, A. Pigulski, H. Lehmann +4

A new investigation of the variability of the SPB-type star 53 Per is presented. The analysis of the BRITE photometry allowed us to determine eight independent frequencies and the…

astro-ph.EP201732 cited

Against the biases in spins and shapes of asteroids

A. Marciniak, F. Pilcher, D. Oszkiewicz +21

Physical studies of asteroids depend on an availability of lightcurve data. Targets that are easy to observe and analyse naturally have more data available, so their synodic period…

astro-ph.EP201732 cited

Photometric survey, modelling, and scaling of long-period and low-amplitude asteroids

A. Marciniak, P. Bartczak, T. Müller +40

The available set of spin and shape modelled asteroids is strongly biased against slowly rotating targets and those with low lightcurve amplitudes. As a consequence of these select…