activity
20182021
most citedA low-luminosity core-collapse supernova very similar to SN 2005cs

14 citations · 30 across the 3 of their papers we have counts for

collaborators

13 papers

astro-ph.SR202111 cited

HD344787: a true Polaris analogue?

V. Ripepi, G. Catanzaro, L. Molnár +10

Classical Cepheids (DCEPs) are the most important primary indicators for the extragalactic distance scale, but they are also important objects per se, allowing us to put constraint…

astro-ph.SR202014 cited

A low-luminosity core-collapse supernova very similar to SN 2005cs

Zoltán Jäger, József Vinkó, Barna I. Bíró +5

We present observations and analysis of PSN J17292918+7542390, a low-luminosity Type II-P supernova (LL SN IIP). The observed sample of such events is still low, and their nature i…

astro-ph.EP2020

Light curves of ten Centaurs from K2 measurements

G. Marton, Cs. Kiss, L. Molnár +12

Here we present the results of visible range light curve observations of ten Centaurs using the Kepler Space Telescope in the framework of the K2 mission. Well defined periodic lig…

astro-ph.EP2020

Rotational properties of Hilda asteroids observed by the K2 mission

Gyula M. Szabó, Csaba Kiss, Róbert Szakáts +7

Hilda asteroids orbit at the outer edge, or just outside of the Main Belt, occupying the 2:3 mean motion resonance with Jupiter. It is known that the group shows a mixed taxonomy t…

astro-ph.EP2020

Solar System objects observed with TESS -- First data release: bright main-belt and Trojan asteroids from the Southern Survey

András Pál, Róbert Szakáts, Csaba Kiss +10

Compared with previous space-borne surveys, the Transiting Exoplanet Survey Satellite (TESS) provides a unique and new approach to observe Solar System objects. While its primary m…

astro-ph.SR20205 cited

X-ray Observations of the Peculiar Cepheid V473 Lyr Identify A Low-Mass Companion

Nancy Remage Evans, Ignazio Pillitteri, Laszlo Molnar +17

V473 Lyr is a classical Cepheid which is unique in having substantial amplitude variations with a period of approximately 3.3 years, thought to be similar to the Blazhko variations…