activity
20192023
most citedMultiwavelength Period-Luminosity and Period-Luminosity-Color relations at maximum-light for Mira variables in the Magellanic Clouds

26 citations · 50 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2023★ 2 cited

Zwicky Transient Facility and Globular Clusters: the gr-Band Period-Luminosity Relations for Mira Variables at Maximum Light and Their Applications to Local Galaxies

Chow-Choong Ngeow, Jia-Yu Ou, Anupam Bhardwaj +3

Based on 14 Miras located in 7 globular clusters, we derived the first gr-band period-luminosity (PL) at maximum light for the large-amplitude Mira variables using the multi-year l…

astro-ph.SR2023★ 9 cited

A Distance Measurement to M33 Using Optical Photometry of Mira Variables

Jia-Yu Ou, Chow-Choong Ngeow, Anupam Bhardwaj +4

We present a systematic analysis to determine and improve the pulsation periods of 1637 known long-period Mira variables in M33 using -band light curves spanning ~year…

astro-ph.SR2022★ 6 cited

Difference of photometric properties between regular and non-regular Miras in the Magellanic Clouds

Jia-Yu Ou, Chow-Choong Ngeow

Mira variables are asymptotic giant branch pulsating stars with long pulsation periods and large amplitudes in optical bands. By applying the random forest algorithm to the I-band…

astro-ph.SR2021★ 7 cited

HO Puppis: Not a Be Star but a Newly Confirmed IW And-Type Star

Chien-De Lee, Jia-Yu Ou, Po-Chieh Yu +19

HO Puppis (HO Pup) was considered as a Be-star candidate based on its gamma-Cassiopeiae-type light curve, but lacked spectroscopic confirmation. Using distance measured from Gaia D…

astro-ph.SR2019★ 26 cited

Multiwavelength Period-Luminosity and Period-Luminosity-Color relations at maximum-light for Mira variables in the Magellanic Clouds

Anupam Bhardwaj, Shashi Kanbur, Shiyuan He +8

We present Period-Luminosity and Period-Luminosity-Color relations at maximum-light for Mira variables in the Magellanic Clouds using time-series data from the Optical Gravitationa…