activity
20222025
most citedNICER monitoring of supersoft X-ray sources

23 citations · 46 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.HE2025

X-ray Observations of Nova Scorpii 2023 (V1716 Sco) in Outburst

John Worley, Marina Orio, Andrej Dobrotka +5

Nova Scorpii 2023 was first detected as a luminous supersoft X-ray source (SSS) 93 days after outburst and continued emitting soft X-rays for over two months, until it was too clos…

astro-ph.HE2025

Hunt for the mHz variability in the TESS and XMM-Newton observations of nova-like cataclysmic variables

Andrej Dobrotka, Jozef Magdolen, Martin Melicherčík

We analysed the flickering of selected nova-like cataclysmic variables observed by the TESS satellite and XMM-Newton. We searched for break frequencies () in the corresp…

astro-ph.SR2024

Searching for the mHz variability in the TESS observations of nova-like cataclysmic variables

A. Dobrotka, J. Magdolen, D. Janikova

AIMS: We investigated fast optical variability of selected nova-like cataclysmic variables observed by TESS satellite. We searched for break frequencies (f_b) in the corresponding…

astro-ph.HE2023

The RS Oph outburst of 2021 monitored in X-rays with NICER

Marina Orio, Keith Gendreau, Morgan Giese +19

The 2021 outburst of the symbiotic recurrent nova RS Oph was monitored with the Neutron Star Interior Composition Explorer Mission (NICER) in the 0.2-12 keV range from day one afte…

astro-ph.SR2023★ 7 cited

Recurrent mini-outbursts and a magnetic white dwarf in the symbiotic system FN Sgr

J. Magdolen, A. Dobrotka, M. Orio +5

AIMS: We investigated the optical variability of the symbiotic binary FN Sgr, with photometric monitoring during 55 years and with a high-cadence Kepler light curve lasting…

astro-ph.HE2022★ 16 cited

High Resolution X-ray Spectra of RS Ophiuchi (2006 and 2021): Revealing the cause of SSS variability

J. -U. Ness, A. P. Beardmore, M. F. Bode +9

Swift observed the SSS phase in RS Oph much fainter in 2021 than in 2006, and we compare an XMM-Newton grating spectrum on day 55.6 in 2021 (2021d55.6) to SSS Chandra and XMM-Newto…

astro-ph.HE2022★ 23 cited

NICER monitoring of supersoft X-ray sources

M. Orio, K. Gendreau, M. Giese +9

We monitored four supersoft sources - two persistent ones, CAL 83 and MR Vel, and the recent novae YZ Ret (Nova Ret 2020) and V1674 Her (Nova Her 2021) - with NICER. The two persis…