Showing 41–60 of 81 results
/ Date/ Name
Mar 27, 2023Predicting light curves of RR Lyrae variables using artificial neural network based interpolation of a grid of pulsation modelsJan 22, 2024A theoretical framework for BL Her stars -- II. New period-luminosity relations in the Gaia passbandsFeb 8, 2024Classical Cepheid Pulsation properties in the Rubin-LSST filtersMar 8, 2024The Hertzsprung progression of Classical Cepheids in the Gaia eraJan 4, 2025The Lack of RR Lyrae Variables in Ultrafaint Dwarf Galaxy Sextans IIFeb 6, 2025Candidate RR Lyrae Associated with the Ultrafaint Dwarf Galaxy Aquarius IIISep 21, 2017Young and Intermediate-age Distance IndicatorsJul 2, 2025Extraction of Physical Parameters of RRab Variables using Neural Network based InterpolatorJun 18, 2025Multiwavelength study of observed and predicted pulsation properties of First overtone Cepheids in the Magellanic CloudsApr 29, 2026SRGA J115215.0$-$510656: an unusual long-period eclipsing dwarf nova with disc wind signaturesSep 8, 2023A multiphase study of classical Cepheids in the Magellanic Clouds- Models and ObservationsDec 5, 2023Geometry of the LMC based on multi-phase analysis of multi-wavelength Cepheid light curves using OGLE-IV and Gaia DR3 dataMar 15, 2023A multiphase study of theoretical and observed light curves of classical Cepheids in the Magellanic CloudsAug 30, 2022Zwicky Transient Facility and Globular Clusters: The Period-Luminosity and Period-Wesenheit Relations for Anomalous Cepheids Supplemented with Large Magellanic Cloud SampleAug 26, 2022Period-Colour and Amplitude-Colour relations for OGLE-$δ$ Scuti stars in the Galactic Bulge and LMCFeb 6, 2023A Distance Measurement to M33 Using Optical Photometry of Mira VariablesJul 13, 2023Zwicky Transient Facility and Globular Clusters: the gr-Band Period-Luminosity Relations for Mira Variables at Maximum Light and Their Applications to Local GalaxiesApr 17, 2019Light Curve Parameters of Cepheid and RR Lyrae Variables at Multiple Wavelengths $-$ Models vs. ObservationsNov 23, 2020A theoretical framework of BL Her stars. I. Effect of metallicity and convection parameters on period-luminosity and period-radius relationsDec 28, 2020Detecting shock waves in non-fundamental mode RR Lyrae using large sample of spectra in SDSS and LAMOST