We examined three Cepheid candidates observed by the Kepler space telescope in the K2 mission, and we concluded that their light variations are caused by stellar activity
In the second phase of the NASA Kepler mission (K2), the Kepler spacecraft observed fields along the...
The extended Kepler mission, K2, is now providing photometry of new fields every three months in a s...
The extended Kepler mission, K2, is now providing photometry of new fields every three months in a s...
We present the results of the analysis of Type II and anomalous Cepheids using the data from the Kep...
We have obtained VR photometry of 282 Cepheid variable star candidates from the northern part of the...
High-precision time series photometry with the Kepler satellite has been crucial to our understandin...
We present 741 new photometric observations for 22 Cepheids with periods between 3 and 8 days. Many ...
We have undertaken a project to discover new type II Cepheids in two large-area sky surveys. However...
The Kepler space telescope has revolutionized our knowledge about exoplanets and stars and is contin...
We present a detailed period analysis of the bright Cepheid-type variable star V1154 Cygni (V1154 C...
We present 1256 new photometric observations of 36 Cepheids with periods longer than 8 days. The maj...
Context. The second data release of the Gaia mission (DR2) includes an advance catalogue of variable...
TESS has a significant advantage in variable star classification over all-sky surveys that work with...
Over 2500 eclipsing binaries were identified and characterized from the ultraprecise photometric dat...
The MOST space telescope observed four Cepheid variables so far, all of different subtypes. Here we ...
In the second phase of the NASA Kepler mission (K2), the Kepler spacecraft observed fields along the...
The extended Kepler mission, K2, is now providing photometry of new fields every three months in a s...
The extended Kepler mission, K2, is now providing photometry of new fields every three months in a s...
We present the results of the analysis of Type II and anomalous Cepheids using the data from the Kep...
We have obtained VR photometry of 282 Cepheid variable star candidates from the northern part of the...
High-precision time series photometry with the Kepler satellite has been crucial to our understandin...
We present 741 new photometric observations for 22 Cepheids with periods between 3 and 8 days. Many ...
We have undertaken a project to discover new type II Cepheids in two large-area sky surveys. However...
The Kepler space telescope has revolutionized our knowledge about exoplanets and stars and is contin...
We present a detailed period analysis of the bright Cepheid-type variable star V1154 Cygni (V1154 C...
We present 1256 new photometric observations of 36 Cepheids with periods longer than 8 days. The maj...
Context. The second data release of the Gaia mission (DR2) includes an advance catalogue of variable...
TESS has a significant advantage in variable star classification over all-sky surveys that work with...
Over 2500 eclipsing binaries were identified and characterized from the ultraprecise photometric dat...
The MOST space telescope observed four Cepheid variables so far, all of different subtypes. Here we ...
In the second phase of the NASA Kepler mission (K2), the Kepler spacecraft observed fields along the...
The extended Kepler mission, K2, is now providing photometry of new fields every three months in a s...
The extended Kepler mission, K2, is now providing photometry of new fields every three months in a s...
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