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Muhammad Zeshan Ashraf

Publications and source records attributed to Muhammad Zeshan Ashraf.

3 recordsLinked to original sources

Vetting Ambiguous Planetary Candidates (APC) in TESS Data: Insights from LATTE Package and Detection of Nine Potential Exoplanet Candidates

We present the results of our study of Ambiguous Planetary Candidates (APCs) in data from the Transiting Exoplanet Survey Satellite (TESS) using the open-source LATTE package. LATTE provides an effective framework for distinguishing transit-like signals, including planetary candidates and eclipsing binaries, from stellar variability and instrumental noise. We performed a comprehensive analysis of TESS APCs by applying the LATTE diagnostic tools and visually inspecting the resulting light curves and diagnostic plots to identify false alarms and false positives. Our analysis confirms nine potential exoplanet candidates that warrant follow-up observations with ground-based facilities. These findings demonstrate the effectiveness of the LATTE package for the identification and vetting of exoplanet candidates in TESS data. Future analyses incorporating observations from additional TESS sectors will further improve candidate validation and may lead to the discovery of additional exoplanet candidates.

astro-ph.EP

The Origins of Neutron-capture Elements In Globular Cluster M22

The chemical abundances of metal-poor stars in globular clusters provide important constraints on their evolutionary scenarios. Using both main r-process and weak r-process patterns, we fit the abundances of s-poor stars in the globular cluster M22. The coefficients of the main and weak r-process components are nearly constant for the sample stars, including s-rich stars. By accounting for the contribution of the s-process from low-mass asymptotic giant branch stars, the abundances of s-rich stars in M22 can also be fitted effectively. In addition, the increasing trend in the s-process component coefficients with rising [Fe/H] indicates a gradual increase in the contribution from low-mass asymptotic giant branch stars.

astro-ph.SR

The Abundance Origin Of A Highly r-process-Enhanced r-II Star: LAMOST J020623.21+494127.9

Object LAMOST J020623.21+494127.9 (program star) in the thin disk of the Milky Way (MW) is reported as a highly r-process-enhanced (RPE) r-II star with[Eu/Fe]= +1.32 and [Fe/H]= -0.54. The chemical profile of the star reflects the intrinsic composition of the gas cloud present at its birth. Using an abundance decomposition method, we fit 25 elements from the abundance dataset, including 10 heavy neutron capture elements. We explore the astrophysical origin of the elements in this star through its abundance ratios and component ratios. We find that the contributions from the massive stars played a significant role in the production of light elements in the program star. Our analysis reveals that the heavy neutron-capture elements are produced purely by the main r-process. However, the adopted main r-process model does not adequately fit the observed data, suggesting another main r-process pattern may exist.

astro-ph.SR