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Search for variable stars in the open cluster Gulliver 35

descriptionPublicationkeyboard_double_arrow_right Conference object , Other literature type , Article 30 Dec 2022 English Publisher:Zenodo
Authors: Karimov, R.; Hojaev, A.;

doi: 10.5281/zenodo.7494184 , 10.5281/zenodo.7494183 , 10.5281/zenodo.7494214 , 10.5281/zenodo.7494213 , 10.5281/zenodo.7502994

Search for variable stars in the open cluster Gulliver 35

Abstract

We present preliminary results of the analysis of TESS light curves and GAIA DR3 data in the region of the open cluster Gulliver 35 with the aim of searching for variable stars and a more comprehensive study of the open cluster.

{"references": ["Cantat-Gaudin, T., Jordi, C., et al. 2018, A&A, 618, 16."]}

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Keywords

open cluster, variable stars

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This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
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