activity
20182025
most citedK2 Observations of SN 2018oh Reveal a Two-Component Rising Light Curve for a Type Ia Supernova

106 citations · 191 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.EP2025★ 2 cited

Asteroid sizes determined with thermophysical model and stellar occultations

A. Choukroun, A. Marciniak, J. Ďurech +165

Context. The sizes of many asteroids, especially slowly rotating, low-amplitude targets, remain poorly constrained due to selection effects. These biases limit the availability of…

astro-ph.EP2023★ 11 cited

Scaling slowly rotating asteroids by stellar occultations

A. Marciniak, J. Ďurech, A. Choukroun +176

As evidenced by recent survey results, majority of asteroids are slow rotators (P>12 h), but lack spin and shape models due to selection bias. This bias is skewing our overall unde…

astro-ph.SR2022★ 6 cited

Mid-infrared time-domain study of recent dust production events in the extreme debris disc of TYC 4209-1322-1

A. Moór, P. Ábrahám, Á. Kóspál +23

Extreme debris discs are characterized by unusually strong mid-infrared excess emission, which often proves to be variable. The warm dust in these discs is of transient nature and…

astro-ph.SR2022★ 18 cited

A multi-epoch, multi-wavelength study of the classical FUor V1515 Cyg approaching quiescence

Zs. M. Szabó, Á. Kóspál, P. Ábrahám +28

Historically, FU Orionis-type stars are low-mass, pre-main sequence stars. The members of this class experience powerful accretion outbursts and remain in an enhanced accretion sta…

astro-ph.SR2021★ 16 cited

V899 Mon: a peculiar eruptive young star close to the end of its outburst

Sunkyung Park, Ágnes Kóspál, Fernando Cruz-Sáenz de Miera +15

V899 Mon is an eruptive young star showing characteristics of both FUors and EXors. It reached a peak brightness in 2010, then briefly faded in 2011, followed by a second outburst.…

astro-ph.SR2019★ 15 cited

SN 2017cfd: A Normal Type Ia Supernova Discovered Very Young

Xuhui Han, WeiKang Zheng, Benjamin E. Stahl +22

The Type~Ia supernova (SN~Ia) 2017cfd in IC~0511 (redshift z = 0.01209+- 0.00016$) was discovered by the Lick Observatory Supernova Search 1.6+-0.7 d after the fitted first-light t…