activity
20042025
most citedOn the incidence of eclipsing Am binary systems in the SuperWASP survey

66 citations · 253 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.GA2025

Ultraviolet Photometry and Reddening Estimation of 105 Galactic Open Clusters

Tahereh Ramezani, Ernst Paunzen, Artem Gorodilov +1

This paper focuses on observing unstudied Galactic open clusters in the Ultraviolet (UV) wavelength range and analyzing their photometric data. The Gaia Data Release 3 (DR3) enable…

astro-ph.SR2020★ 5 cited

Rotational modulation and single g-mode pulsation in the B9pSi star HD174356?

Z. Mikulasek, E. Paunzen, S. Huemmerich +19

Chemically peculiar (CP) stars of the upper main sequence are characterised by specific anomalies in the photospheric abundances of some chemical elements. The group of CP2 stars,…

astro-ph.SR2018★ 9 cited

Orbital parameters and evolutionary status of the highly peculiar binary system HD 66051

E. Paunzen, M. Fedurco, K. G. Helminiak +8

The spectroscopic binary system HD 66051 (V414 Pup) consists of a highly peculiar CP3 (HgMn) star and an A-type component. It also shows out-of-eclipse variability that is due to c…

astro-ph.SR2017★ 3 cited

A search for peculiar stars in the open cluster Hogg 16

Stefano Cariddi, Naira M. Azatyan, Petr Kurfürst +5

The study of chemically peculiar (CP) stars in open clusters provides valuable information about their evolutionary status. Their detection can be performed using the photomet…

astro-ph.SR2014★ 10 cited

A probable pre-main sequence chemically peculiar star in the open cluster Stock 16

M. Netopil, L. Fossati, E. Paunzen +3

We used the Ultraviolet and Visual Echelle Spectrograph of the ESO-Very Large Telescope to obtain a high resolution and high signal-to-noise ratio spectrum of Stock 16-12, an early…

astro-ph.SR2014★ 66 cited

On the incidence of eclipsing Am binary systems in the SuperWASP survey

B. Smalley, J. Southworth, O. I. Pintado +18

The results of a search for eclipsing Am star binaries using photometry from the SuperWASP survey are presented. The light curves of 1742 Am stars fainter than V = 8.0 were analyse…