activity
20152026
most citedRefining the 2022 OJ 287 impact flare arrival epoch

22 citations · 66 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.HE2026

The October 2022 flare in OJ 287 and the mass of its primary black hole

Mauri J. Valtonen, Staszek Zola, Manpreet Singh +21

The bright blazar OJ~287 has demonstrated a sequence of flares, which are well explained by a quasi-Keplerian orbit model. The flares are associated with the impact of the secondar…

astro-ph.HE2026

Early Optical Follow-up of Gamma-Ray Bursts: The Critical Role of Robotic Telescopes

Rahul Gupta, Judith Racusin, Gor Oganesyan +26

Gamma-ray bursts (GRBs) are the most luminous electromagnetic explosions in the Universe, and offer unique laboratories for studying relativistic jets, compact-object formation, pa…

astro-ph.HE2023★ 7 cited

On the need of an ultramassive black hole in OJ 287

Mauri J. Valtonen, Staszek Zola, Achamveedu Gopakumar +25

The highly variable blazar OJ~287 is commonly discussed as an example of a binary black hole system. The 130 year long optical light curve is well explained by a model where the ce…

astro-ph.HE2023★ 7 cited

Observational Implications of OJ 287's Predicted 2022 Disk Impact in the Black Hole Binary Model

Mauri J. Valtonen, Lankeswar Dey, Achamveedu Gopakumar +24

We present a summary of the results of the OJ 287 observational campaign, which was carried out during the 2021/2022 observational season. This season is special in the binary mode…

astro-ph.IM2023

Mono and stereo performance of the two SST-1M telescope prototypes

J. Jurysek, T. Tavernier, V. Novotný +51

The Single-Mirror Small-Sized Telescope, or SST-1M, was originally developed as a prototype of a small-sized telescope for CTA, designed to form an array for observations of gamma-…

astro-ph.HE2023★ 22 cited

Refining the 2022 OJ 287 impact flare arrival epoch

Mauri J. Valtonen, Staszek Zola, Gopakumar +24

The bright blazar OJ~287 routinely parades high brightness bremsstrahlung flares, which are explained as being a result of a secondary supermassive black hole (SMBH) impacting the…

astro-ph.HE2022★ 17 cited

Prompt emission and early optical afterglow of VHE detected GRB 201015A and GRB 201216C: onset of the external forward shock

Amit Kumar Ror, Rahul Gupta, Martin Jelínek +19

We present a detailed prompt emission and early optical afterglow analysis of the two very high energy (VHE) detected bursts GRB 201015A and GRB 201216C, and their comparison with…

astro-ph.HE2022★ 3 cited

Refining the prediction for OJ 287 next impact flare arrival epoch

Mauri J. Valtonen, Staszek Zola, A. Gopakumar +23

The bright blazar OJ~287 routinely parades high brightness bremsstrahlung flares which are explained as being a result of a secondary supermassive black hole (SMBH) impacting the a…

astro-ph.HE2019★ 4 cited

Looking for fast optical bursts from FRB121102: case study for a small telescopes with sub-second temporal resolution

S. Karpov, M. Jelinek, J. Strobl

To assess the potential of a small telescopes for a high temporal resolution astrophysics, we observed the field of FRB~121102 repeating source of fast radio bursts on a 50-cm D50…

astro-ph.GA2018★ 6 cited

The search for roAp stars: null results and new candidates from Stroemgren-Crawford photometry

E. Paunzen, G. Handler, K. Honkova +10

The rapidly oscillating Ap (roAp) stars exhibit pulsational photometric and/or radial velocity variations on time scales of several minutes, which are essential to test current pul…

astro-ph.HE2015

Astrophysics of "extreme" solar-like stars

M. D. Caballero-Garcia, A. J. Castro-Tirado, A. Claret +8

Only a few red dwarf flaring stars in the solar neighbourhood have undergone exceptional events called superflares. They have been detected with high-energy satellites (i.e. Swift)…