activity
19962023
most citedHAT-P-1b: A Large-Radius, Low-Density Exoplanet Transiting one Member of a Stellar Binary

266 citations · 1.8k across the 48 of their papers we have counts for

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Showing astro-ph.SRShow all

15 papers · 1 filter

astro-ph.SR2023★ 3 cited

Toward more accurate RR Lyrae metallicities

Geza Kovacs, Johanna Jurcsik

By using a large sample of published spectroscopic iron abundances, we point out the importance of gravity correction in deriving more accurate metal abundances for RR Lyrae stars.…

astro-ph.SR2023★ 14 cited

A Study of Stellar Spins in 15 Open Clusters

Brian F. Healy, P. R. McCullough, Kevin C. Schlaufman +1

We analyze spectroscopic and photometric data to determine the projected inclinations of stars in 11 open clusters, placing constraints on the spin-axis distributions of six cluste…

astro-ph.SR2021★ 3 cited

Bright single-mode RR Lyrae stars: matching Gaia EDR3 with pulsation and evolutionary models

Geza Kovacs, Behrooz Karamiqucham

We combine observed metallicity, optical and infrared magnitudes with evolutionary and pulsation models to derive average luminosities for 156 single-mode RR Lyrae stars. These lum…

astro-ph.SR2021★ 9 cited

Probing galactic double-mode RR Lyrae stars against Gaia EDR3

Geza Kovacs, Behrooz Karamiqucham

Classical double-mode pulsators (RR Lyrae stars and delta Cepheids) are important for their simultaneous pulsation in low-order radial modes. This enables us to put stringent const…

astro-ph.SR2020★ 1 cited

On the Incidence Rate of Blazhko Stars

Geza Kovacs

In a recent paper (Kovacs 2018) we examined the incidence rate of the modulated RR Lyrae stars by using the data from Campaigns 01 - 04 of the Kepler K2 mission. We found an observ…

astro-ph.SR2019★ 10 cited

On the hierarchical triple nature of the former red nova precursor candidate KIC 9832227

Geza Kovacs, Joel D. Hartman, Gaspar A. Bakos

We revisit the issue of period variation of the recently claimed red nova precursor candidate KIC 9832227. By using the data gathered during the main mission of the Kepler satellit…

astro-ph.SR2018★ 18 cited

Are all RR Lyrae stars modulated?

Geza Kovacs

We analyzed 151 variables previously classified as fundamental mode RR Lyrae stars from Campaigns 01-04 of the Kepler two wheel (K2) archive. By employing a method based on the app…

astro-ph.SR2018★ 1 cited

Big Signals, Small Signals, Systematics

Geza Kovacs

We examine the role of instrumental systematics in the search for small amplitude signal components in the presence of large amplitude signals. Current analyses of variable stars d…

astro-ph.SR2018★ 17 cited

Signature of non-isotropic distribution of stellar rotation inclination angles in the Praesepe cluster

Geza Kovacs

The distribution of the stellar rotation axes of 113 main sequence stars in the open cluster Praesepe are examined by using current photometric rotation periods, spectroscopic rota…

astro-ph.SR2017★ 2 cited

Synergies between Exoplanet Surveys and Variable Star Research

Geza Kovacs

With the discovery of the first transiting extrasolar planetary system back to 1999, a great number of projects started to hunt for other similar systems. Because of the incidence…

astro-ph.SR2015★ 1 cited

The Blazhko phenomenon

Geza Kovacs

In spite of the accumulating high quality data on RR Lyrae stars, the underlying cause of the (quasi)periodic light curve modulation (the so-called Blazhko effect) of these objects…

astro-ph.SR2015★ 12 cited

Are the gyro-ages of field stars underestimated?

Geza Kovacs

By using the current photometric rotational data on eight galactic open clusters, we show that the evolutionary stellar model (isochrone) ages of these clusters are tightly correla…

astro-ph.SR2014★ 39 cited

Stellar rotational periods in the planet hosting open cluster Praesepe

Geza Kovacs, Joel D. Hartman, Gaspar A. Bakos +6

By using the dense coverage of the extrasolar planet survey project HATNet, we Fourier analyze 381 high-probability members of the nearby open cluster Praesepe (Beehive/M44/NGC 263…

astro-ph.SR2014

The rich frequency spectrum of the triple-mode variable AC And

G. Kovacs, G. A. Bakos, J. D Hartman

Fourier analysis of the light curve of AC And from the HATNet database reveals the rich frequency structure of this object. Above 30 components are found down to the amplitude of 3…

astro-ph.SR2009★ 26 cited

Study of Globular Cluster M53: new variables, distance, metallicity

Istvan Dekany, Geza Kovacs

We study the variable star content of the globular cluster M53 to compute the physical parameters of the constituting stars and the distance of the cluster. Covering two adjacent s…