Periods and classifications of RR Lyrae stars in the globular cluster M15

Author:

Hoffman Andrew M12,Murakami Yukei S12ORCID,Zheng WeiKang1,Stahl Benjamin E12ORCID,Filippenko Alexei V13

Affiliation:

1. Department of Astronomy, University of California, Berkeley, CA 94720-3411, USA

2. Department of Physics, University of California, Berkeley, CA 94720-7300, USA

3. Miller Senior Fellow, Miller Institute for Basic Research in Science, University of California, Berkeley, CA 94720, USA

Abstract

ABSTRACT We present measurements of the periods, amplitudes, and types of 74 RR Lyrae stars in the globular cluster M15 derived from Nickel 1 m telescope observations conducted at Lick Observatory in 2019 and 2020. Of these RR Lyrae stars, two were previously reported but without a determination of the period. In addition, we identify five Type II Cepheid variable stars for which we report three novel period determinations, and a further 34 stars with uncertain classifications and periods. We discuss the development and subsequent application to our data of a new python package, Period-determination and Identification Pipeline Suite (pips), based on a new adaptive free-form fitting technique to detect the periods of variable stars with a clear treatment of uncertainties.

Funder

Adolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California Berkeley

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Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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