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相关论文: K2 Photometry of RR Lyrae Stars

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Light curves for RR Lyrae stars can be difficult to obtain properly in the K2 mission due to the similarities between the timescales of the observed physical phenomena and the instrumental signals appearing in the data. We developed a new…

天体物理仪器与方法 · 物理学 2020-09-21 Emese Plachy , Pál Szabó , Attila Bódi , László Molnár , Róbert Szabó

We present the method of the Extended Aperture Photometry (EAP) that we applied to K2 RR Lyrae stars. Our aim is to minimize the instrumental variations of attitude control maneuvers by using apertures that cover the positional changes in…

太阳与恒星天体物理 · 物理学 2017-11-08 E. Plachy , P. Klagyivik , L. Molnár , Á. Sódor , R. Szabó

The \textit{Kepler} space telescope observed thousands of RR Lyrae stars in the K2 mission. In this paper we present our photometric solutions using extended apertures in order to conserve the flux of the stars to the highest possible…

Proper photometric data are challenging to obtain in the K2 mission of the Kepler space telescope due to strong systematics caused by the two-wheel-mode operation. It is especially true for variable stars wherein physical phenomena occur on…

天体物理仪器与方法 · 物理学 2022-02-09 Attila Bódi , Pál Szabó , Emese Plachy , László Molnár , Róbert Szabó

Nearly continuous, densely sampled, space-based photometry allows us to recover the finest details in the light variations of stars. The number of such light curves have been increasing rapidly in the last few years thanks to the extended…

太阳与恒星天体物理 · 物理学 2023-12-18 E. Plachy

The Pan-STARRS 3$\pi$ survey has detected hundreds of thousands of variable stars thanks to its coverage and 4-year time span, even though the sampling of the light curves is relatively sparse. These light curves contain only 10-15…

太阳与恒星天体物理 · 物理学 2024-08-27 Adrienn Forró , László Molnár , Emese Plachy , Áron Juhász , Róbert Szabó

We have started a comprehensive analysis of the Kepler K2 Field 3 data set. Our goals are to assess the statistics of the sample, and to search for peculiar stars. We found a candidate triple-mode RRab star, where the first and ninth…

太阳与恒星天体物理 · 物理学 2016-03-30 Á. Juhász , L. Molnár , E. Plachy

In this paper we report the discovery of 35 new RR Lyrae variables. These stars were found by a special searching technique. We crossmatched the catalog of the PanSTARRS (PS) sky survey with K2 space photometry data to the validate…

太阳与恒星天体物理 · 物理学 2018-03-28 Áron L. Juhász , László Molnár

A detailed analysis is presented of 33 RR Lyrae stars in Pisces observed with the Kepler space telescope over the 8.9-day long K2 Two-Wheel Concept Engineering Test. The sample includes not only fundamental-mode and first overtone (RRab and…

太阳与恒星天体物理 · 物理学 2015-08-19 L. Molnár , R. Szabó , P. A. Moskalik , J. M. Nemec , E. Guggenberger , R. Smolec , R. Poleski , E. Plachy , K. Kolenberg , Z. Kolláth

With the step-and-stare approach of the K2 mission, Kepler will be able to observe a large number of Cepheid an RR Lyrae stars. In this paper we describe the target selection efforts, and the first impressions based on the K2 two-wheel…

太阳与恒星天体物理 · 物理学 2015-07-21 L. Molnár , E. Plachy , R. Szabó

We present multi-epoch infrared photometry in the $K_s$-band for 74 bright RR Lyrae variable stars tied directly to the 2MASS photometric system. We systematize additional $K$-band photometry from the literature to the 2MASS system and…

星系天体物理 · 物理学 2019-08-21 Andrew C. Layden , Glenn P. Tiede , Brian Chaboyer , Curtis Bunner , Michael T. Smitka

High-precision time series photometry with the Kepler satellite has been crucial to our understanding both of exoplanets, and via asteroseismology, of stellar physics. After the failure of two reaction wheels, the Kepler satellite has been…

We present an update to the EVEREST K2 pipeline that addresses various limitations in the previous version and improves the photometric precision of the de-trended light curves. We develop a fast regularization scheme for third order pixel…

天体物理仪器与方法 · 物理学 2018-08-29 Rodrigo Luger , Ethan Kruse , Daniel Foreman-Mackey , Eric Agol , Nicholas Saunders

In this paper we describe a project we initiated to investigate individual pixels in the downloaded Kepler apertures in order to find objects in the background of the main targets with variable brightness. In the first paper of this series…

太阳与恒星天体物理 · 物理学 2022-05-25 Adrienn Forró , Róbert Szabó , Attila Bódi , Kornél Császár

The unprecedented photometric precision along with the quasi-continuous sampling provided by the Kepler space telescope revealed new and unpredicted phenomena that reformed and invigorated RR Lyrae star research. The discovery of period…

太阳与恒星天体物理 · 物理学 2020-11-25 Emese Plachy , Róbert Szabó

The K2 mission is a repurposed use of the Kepler spacecraft to perform high-precision photometry of selected fields in the ecliptic. We have developed an aperture photometry pipeline for K2 data which performs dynamic automated aperture…

天体物理仪器与方法 · 物理学 2015-12-01 Derek L. Buzasi , Lindsey Carboneau , Carly Hessler , Andy Lezcano , Heather Preston

With only two functional reaction wheels, Kepler cannot maintain stable pointing at its original target field and entered a new mode of observation called K2. Our method is based on many years of experience in planet hunting for the CoRoT…

地球与行星天体物理 · 物理学 2016-10-19 S. C. C. Barros , O. Demangeon , M. Deleuil

Context: After the loss of a second reaction wheel the Kepler mission was redesigned as the K2 mission, pointing towards the ecliptic and delivering data for new fields approximately every 80 days. The steady flow of data obtained with a…

太阳与恒星天体物理 · 物理学 2016-12-21 R. Handberg , M. N. Lund

Context. Modern space telescopes are currently providing high-precision light curves for a large fraction of the sky, such that many new variable stars are being discovered. However, some stars have periodic variability with periods of…

太阳与恒星天体物理 · 物理学 2019-08-28 Dominic M. Bowman , Daniel L. Holdsworth

We present results of the analysis of light and radial velocity (RV) curves of eight detached eclipsing binaries observed by the All-Sky Automated Survey, which we have followed up with high-resolution spectroscopy, and were later observed…

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