activity
20132026
most citedMultiwavelength Study of Quiescent States of Mrk 421 with Unprecedented Hard X-Ray Coverage Provided by NuSTAR in 2013

143 citations · 896 across the 61 of their papers we have counts for

collaborators

63 papers

astro-ph.HE2026

Multi-band optical photometric variability of the blazar OJ 287 from 2015 to 2025

Alok C. Gupta, Karan Dogra, Mark Kidger +101

We present the most densely sampled multi-band optical photometric observations of the peculiar BL Lacertae object OJ 287 from 2015 to 2025 with a focus on its optical activity on…

astro-ph.HE2024

Multi-wavelength picture of the misaligned BL Lac object 3C 371

J. Otero-Santos, C. M. Raiteri, A. Tramacere +52

The BL Lac object 3C 371 is one of the targets that are regularly monitored by the Whole Earth Blazar Telescope (WEBT) Collaboration to study blazar variability on both short and l…

astro-ph.HE2024★ 13 cited

Optical variability of the blazar 3C 371: from minute to year timescales

J. Otero-Santos, C. M. Raiteri, J. A. Acosta-Pulido +41

The BL Lac object 3C 371 has been observed by the Transiting Exoplanet Survey Satellite (\textit{TESS}) for approximately a year, between July 2019 and July 2020, with an unmatched…

astro-ph.HE2024★ 9 cited

The variability patterns of the TeV blazar PG 1553+113 from a decade of MAGIC and multi-band observations

MAGIC Collaboration, H. Abe, S. Abe +264

PG 1553+113 is one of the few blazars with a convincing quasi-periodic emission in the gamma-ray band. The source is also a very high-energy (VHE; >100 GeV) gamma-ray emitter. To b…

astro-ph.SR2023

Photometric monitoring of PMS stars with the telescopes at Rozhen Observatory

Evgeni Semkov, Sunay Ibryamov, Stoyanka Peneva +1

For several decades we have been performing photometric monitoring of some of the star formation regions. Significant place in our program take observations of objects of the type…

astro-ph.HE2023

Extreme photometric and polarimetric variability of blazar S4 0954+65 at its maximum optical and -ray brightness levels

C. M. Raiteri, M. Villata, M. I. Carnerero +64

In 2022 the BL Lac object S4 0954+65 underwent a major variability phase, reaching its historical maximum brightness in the optical and -ray bands. We present optical photometri…

astro-ph.HE2023★ 12 cited

Multi-year characterisation of the broad-band emission from the intermittent extreme BL Lac 1ES~2344+514

H. Abe, S. Abe, V. A. Acciari +232

The BL Lac 1ES 2344+514 is known for temporary extreme properties (e.g., a shift of the synchrotron SED peak energy above 1keV). While those extreme states were so fa…

astro-ph.SR2023★ 1 cited

Study of the long-term photometric variability of eight PMS stars in the young open cluster Trumpler 37

Sunay Ibryamov, Gabriela Zidarova, Evgeni Semkov +1

This paper reports results from our long-term photometric CCD observations of eight pre-main-sequence stars collected from June 2008 to October 2022. These stars are l…

astro-ph.HE2023★ 24 cited

The optical behaviour of BL Lacertae at its maximum brightness levels: a blend of geometry and energetics

C. M. Raiteri, M. Villata, S. G. Jorstad +13

In 2021 BL Lacertae underwent an extraordinary activity phase, which was intensively followed by the Whole Earth Blazar Telescope (WEBT) Collaboration. We present the WEBT optical…

astro-ph.HE2022★ 7 cited

Multi-band Optical Variability of the TeV Blazar PG 1553+113 in 2019

Vinit Dhiman, Alok C. Gupta, Sofia O. Kurtanidze +20

We report the flux and spectral variability of PG 1553+113 on intra-night (IDV) to short-term timescales using BVRI data collected over 91 nights from 28 February to 8 November 201…

astro-ph.SR2022★ 1 cited

Long-term Photometric Study of the Pre-main Sequence Star V1180 Cas

Asen Mutafov, Evgeni Semkov, Stoyanka Peneva +1

In this paper results from the optical photometric observations of the pre-main-sequence star V1180 Cas are reported. The star is a young variable associated with the dark cloud Ly…

astro-ph.SR2022

Long-term optical photometry of the PMS stars V2764 Ori and LkH 301 in the field of the McNeil's Nebula

G. Zidarova, S. Ibryamov, E. Semkov +1

In this paper, we present results from long-term photometric observations of the pre-main-sequence stars V2764 Ori and LkH 301, located in the field of the McNeil's…

astro-ph.SR2021★ 6 cited

The FUor star V2493 Cyg (HBC 722) -- eleven years at maximum brightness

Evgeni Semkov, Sunay Ibryamov, Stoyanka Peneva

At the time of stellar evolution, young stellar objects go through processes of increased activity and instability. Star formation takes place in several stages during which the st…

astro-ph.HE2021★ 49 cited

Investigation of the correlation patterns and the Compton dominance variability of Mrk 421 in 2017

MAGIC Collaboration, V. A. Acciari, S. Ansoldi +284

We present a detailed characterisation and theoretical interpretation of the broadband emission of the paradigmatic TeV blazar Mrk 421, with special focus on the multi-band flux co…

astro-ph.SR2021

Long-term optical photometric monitoring of the FUor star V900 Mon

Evgeni Semkov, Stoyanka Peneva, Sunay Ibryamov

We present results from photometric monitoring of V900 Mon, one of the newly discovered and still under-studied object from FU Orionis type. FUor phenomenon is very rarely observed…

astro-ph.SR2021

New Results from Long-time Photometric Study of UX Orionis Star GM Cephei

Asen Mutafov, Evgeni Semkov, Stoyanka Peneva +1

New results from long-term optical photometric observations of the pre-main sequence star GM Cep from UX Orionis type are reported. During ongoing photometric monitoring of the GM…

astro-ph.SR2021

Long-term CCD photometry of pre-main-sequence stars in the association Cepheus OB3

Sunay Ibryamov, Gabriela Zidarova, Evgeni Semkov +1

Results from optical CCD photometric observations of 13 pre-main-sequence stars collected during the period from February 2007 to November 2020 are presented. These stars are locat…

astro-ph.SR2020★ 2 cited

A new prolonged decrease event in the brightness of the young stellar object V2492 Cygni

Sunay Ibryamov, Evgeni Semkov

Results from the BV(RI)c photometric observations of the young stellar object V2492 Cyg collected in the period from April 2018 to September 2020 are presented. These observations…

astro-ph.GA2020★ 1 cited

Multi-Wavelength Variability of BL Lacertae Measured with High Time Resolution

Zachary R. Weaver, K. E. Williamson, S. G. Jorstad +54

In an effort to locate the sites of emission at different frequencies and physical processes causing variability in blazar jets, we have obtained high time-resolution observations…

astro-ph.SR2020★ 2 cited

BV(RI)c photometric study of three variable PMS stars in the field of V733 Cephei

Sunay Ibryamov, Evgeni Semkov, Stoyanka Peneva +1

This paper report results from the first long-term BV(RI)c photometric CCD observations of three variable pre-main-sequence stars collected during the period from February 2007 to…

astro-ph.SR2020

Intra-night flickering of RS Ophiuchi: III. Modes of quasi-periods in the minute scale and their evolution

Ts. B. Georgiev, R. K. Zamanov, S. Boeva +7

We study the photometric behavior of the recurrent nova RS Oph by 58 monitoring light curves (LCs), taken by 5 telescopes. All LCs show repeating time structures with some quasi-pe…

astro-ph.HE2020★ 50 cited

Unravelling the complex behavior of Mrk 421 with simultaneous X-ray and VHE observations during an extreme flaring activity in April 2013

MAGIC collaboration, V. A. Acciari, S. Ansoldi +237

We report on a multi-band variability and correlation study of the TeV blazar Mrk 421 during an exceptional flaring activity observed from 2013 April 11 to 2013 April 19. The study…

astro-ph.HE2020★ 51 cited

Multiwavelength behaviour of the blazar 3C279: decade-long study from -ray to radio

V. M. Larionov, S. G. Jorstad, A. P. Marscher +84

We report the results of decade-long (2008-2018) -ray to 1 GHz radio monitoring of the blazar 3C 279, including GASP/WEBT, and data, as well as polarim…

astro-ph.SR2020★ 3 cited

International observational campaign of the 2014 eclipse of EE Cep

D. Pieńkowski, C. Gałan, T. Tomov +64

Context. EE Cep is one of few eclipsing binary systems with a dark, dusty disk around an invisible object similar to ε Aur. The system is characterized by grey and asymmetric eclip…