activity
20122026
most citedExtensive Spectroscopy and Photometry of the Type IIP Supernova 2013ej

64 citations · 185 across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.SR2026

Stellar Forcing of (exo)Planetary Environments

Julián D. Alvarado-Gómez, Erika Palmerio, Manuel Güdel +13

The environments of exoplanets are fundamentally shaped by the magnetic activity of their host stars through radiative, plasma, and particle-driven processes. This article presents…

astro-ph.HE2026

Long-term optical and near-infrared photometric evolution of SN 2019vxm, an interacting Type IIn supernova

Klára Lelkes, László Molnár, József Vinkó +12

The diversity of Type IIn supernovae is largely driven by the properties of the circumstellar material (CSM) they explode into. We examine the temporal evolution of SN 2019vxm, an…

astro-ph.HE2026

Distance estimate to NGC 6951 from supernova siblings Type IIP SN 2020dpw and Type Ib SN 2021sjt

Réka Könyves-Tóth, Zsófia Bodola, Tamás Szalai +24

{Supernova (SN) siblings are powerful tools used to calibrate and improve distance measurement methods, and to make the systematic uncertainty to distances to their host galaxies c…

astro-ph.SR2025

The Preliminary Mauve Science Programme: Science themes identified for the first year of operations

Mauve Science Collaboration, Marcel Agueros, Don Dixon +22

Mauve is a low-cost small satellite developed and operated by Blue Skies Space Ltd. The payload features a 13 cm telescope connected with a fibre that feeds into a UV-Vis spectrome…

astro-ph.HE2025

SN 2023ixf in M101: physical parameters from bolometric light curve modeling

J. Vinko, Zs. R. Bodola, A. Godeny +25

We present new photometric observations of the core-collapse supernova SN 2023ixf occurred in M101, taken with the RC80 and BRC80 robotic telescopes in Hungary. The initial nickel…

astro-ph.SR2025★ 4 cited

Short- and long-term variations of the high mass accretion rate classical T Tauri star DR Tau

Gabriella Zsidi, Ágnes Kóspál, Péter Ábrahám +20

Classical T Tauri stars are newly formed, low mass stars which may display both periodic and random variations in their brightness. The interaction between the star and its circums…

astro-ph.HE2024

Ejecta masses in Type Ia Supernovae -- Implications for the Progenitor and the Explosion Scenario

Zsófia Bora, Réka Könyves-Tóth, József Vinkó +35

The progenitor system(s) as well as the explosion mechanism(s) of thermonuclear (Type Ia) supernovae are long-standing issues in astrophysics. Here we present ejecta masses and oth…

astro-ph.SR2024★ 1 cited

Stellar flares, superflares and coronal mass ejections -- entering the Big data era

Krisztián Vida, Zsolt Kővári, Martin Leitzinger +6

Flares, sometimes accompanied by coronal mass ejections (CMEs), are the result of sudden changes in the magnetic field of stars with high energy release through magnetic reconnecti…

astro-ph.SR2024

NEOWISE-R Caught the Luminous SN 2023ixf in Messier 101

Schuyler D. Van Dyk, Tamas Szalai, Roc M. Cutri +16

The reactivated Near-Earth Object Wide-field Infrared Survey Explorer (NEOWISE-R) serendipitously caught the Type II supernova SN 2023ixf in Messier 101 on the rise, starting day 3…

astro-ph.SR2024★ 5 cited

The Enigma of Gaia18cjb: a Rare Hybrid of FUor and EXor?

Eleonora Fiorellino, Peter Abraham, Agnes Kospal +28

Context. Gaia18cjb is one of the Gaia-alerted eruptive young star candidates which has been experiencing a slow and strong brightening during the last 13 years, similar to some FU…

astro-ph.EP2024★ 3 cited

Abundant sub-micron grains revealed in newly discovered extreme debris discs

A. Moór, P. Ábrahám, K. Y. L. Su +7

Extreme debris discs (EDDs) are bright and warm circumstellar dusty structures around main sequence stars. They may represent the outcome of giant collisions occuring in the terres…

astro-ph.SR2020★ 2 cited

Flare stars in nearby Galactic open clusters based on {\it TESS} data

O. Maryeva, K. Bicz, C. Xia +3

The study is devoted to search for flare stars among confirmed members of Galactic open clusters using high-cadence photometry from {\it TESS} mission. We analyzed 957 high-cadence…

astro-ph.HE2020★ 18 cited

The Exotic Type Ic Broad-Lined Supernova SN 2018gep: Blurring the Line Between Supernovae and Fast Optical Transients

T. A. Pritchard, Katarzyna Bensch, Maryam Modjaz +28

In the last decade a number of rapidly evolving transients have been discovered that are not easily explained by traditional supernovae models. We present optical and UV data on on…

astro-ph.HE2017★ 54 cited

SN 2016coi/ASASSN-16fp: An example of residual helium in a type Ic supernova?

S. J. Prentice, C. Ashall, P. A. Mazzali +35

The optical observations of Ic-4 supernova (SN) 2016coi/ASASSN-16fp, from to days after explosion, are presented along with analysis of its physical properties.…

astro-ph.SR2015★ 64 cited

Extensive Spectroscopy and Photometry of the Type IIP Supernova 2013ej

G. Dhungana, R. Kehoe, J. Vinko +32

We present extensive optical (, , and open CCD) and near-infrared () photometry for the very nearby Type IIP SN ~2013ej extending from +1 to +461 days after…

astro-ph.SR2013★ 2 cited

The Kep-Cont Mission: Continuing the observation of high-amplitude variable stars in the Kepler field of view

L. Molnár, R. Szabó, K. Kolenberg +7

As a response to the Kepler white paper call, we propose to keep Kepler pointing to its current field of view and continue observing thousands of large amplitude variables (Cepheid…

astro-ph.HE2012★ 30 cited

Identifying the Location in the Host Galaxy of the Short GRB 111117A with the Chandra Sub-arcsecond Position

T. Sakamoto, E. Troja, K. Aoki +31

We present our successful Chandra program designed to identify, with sub-arcsecond accuracy, the X-ray afterglow of the short GRB 111117A, which was discovered by Swift and Fermi.…

astro-ph.SR2012★ 2 cited

First Results of The Konkoly Blazhko Survey II

Á. Sódor, J. Jurcsik, L. Molnár +17

The two parts of the Konkoly Blazhko Survey (KBS I and II) are introduced. The most important preliminary findings of the second part are presented in comparison to the results of…