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From the 1 of 16 linked papers with an AI index.

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16 papers

astro-ph.HE2026

Determination of neutron star radius from pulse profile modeling using profile likelihood

Vyaas Ramakrishnan, Shantanu Desai

The paper demonstrates a frequentist profile‑likelihood method for extracting neutron star radii from NICER pulse‑profile data, showing comparable precision to Bayesian approaches…

astro-ph.IM2026

Comparison of symbolic regression algorithms in Star/galaxy/quasar separation

Rachit Deshpande, Shantanu Desai

This work investigates symbolic regression (SR) as an interpretable alternative to black-box machine learning for the classification of stars, galaxies, and quasars in the Sloan Di…

astro-ph.HE2026

Limit on high energy neutrino emission from Abell 119 using IceCube 10-year muon track data

Sri Devaki Meduri, Shantanu Desai

We carry out a search for high energy muon neutrino emission from the galaxy cluster Abell 119, motivated by a recent detection of GeV gamma rays from this cluster using the Fermi-…

astro-ph.CO2026

Probing cosmic anisotropy with galaxy clusters and supernovae

Shubham Barua, Sujit K. Dalui, Shantanu Desai

Using CDM and Padé-(2,1) cosmography, we study directional variations in the Hubble constant, , using galaxy cluster and Type Ia Supernovae (from Pantheon Plus) by the he…

astro-ph.CO2026

Bayesian Model Comparison of versus CDM using HII galaxy Hubble diagram

Yuva Himanshu Pallam, Shantanu Desai

We complement a recent analysis comparing with CDM/CDM using HII galaxies and giant extragalactic HII regions, by carrying out Bayesian model comparison. F…

astro-ph.HE2026

Search for Gamma-ray emission from Abell 119 galaxy cluster using INTEGRAL/ISGRI, COMPTEL, and DAMPE data

Siddhant Manna, Shantanu Desai

We present a comprehensive search for non-thermal high-energy -ray emission from the nearby merging galaxy cluster Abell~119 () using archival observations spanning ov…