most citedPossibilities of Identifying Members from Milky Way Satellite Galaxies using Unsupervised Machine Learning Algorithms

1 citations · 1 across the 5 of their papers we have counts for

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7 papers

astro-ph.IM2025

A new broadband atmospheric dispersion corrector for HROS-TMT

Manjunath Bestha, Thirupathi Sivarani, Bachar Wehbe +7

Atmospheric dispersion causes light from celestial objects with different wavelengths to refract at varying angles as it passes through Earth's atmosphere. This effect results in a…

astro-ph.EP2025

High-Resolution Echelle Spectroscopy for Solar System Planets: A Planet-as-Point-Source Analogy

Parvathy Menon, Sivarani T, Sriram S +4

Transmission spectroscopy has proven to be an effective technique for characterizing exoplanet atmospheres. However, transmission spectroscopy requires planetary transits, which oc…

astro-ph.IM2025

Atmospheric Dispersion Measurement at Hanle Site

Manjunath Bestha, Sivarani Thirupathi, Athira Unni +2

Atmospheric dispersion introduces wavelength-dependent effects that significantly impact ground-based observations, particularly in slit- and fibre-fed spectroscopic studies. These…

astro-ph.EP2025

A multi-object approach for studying exoplanet atmospheres using high-resolution spectrographs

Manjunath Bestha, Athira Unni, T. Sivarani +5

Atmospheric characterization of exoplanets has traditionally relied on Low-Resolution Transmission Spectroscopy (LRTS), obtained from both space- and ground-based facilities, as we…

astro-ph.IM2025

Design overview of the fiber feed for the Hobby-Eberly telescope's HRS

Devika K Divakar, Phillip MacQueen, Joseph Strubhar

We present the redesign of the fiber feed for the High Resolution Spectrograph (HRS) at the Hobby Eberly Telescope (HET). The upgrade incorporates a static atmospheric dispersion c…

astro-ph.EP2025

An Initial Assessment of the Hanle Echelle Spectrograph for Exoplanet Atmosphere Studies

Manjunath Bestha, Athira Unni, T. Sivarani +6

Transmission spectroscopy is an effective technique for probing exoplanetary atmospheres. While most observations have relied on space facilities such as HST and JWST, ground-based…