activity
20112026
most citedSn 2008in - bridging the gap between normal and faint supernovae of type IIP

85 citations · 227 across the 50 of their papers we have counts for

collaborators

53 papers

astro-ph.HE2026

Optical observations of supernova candidates with the ILMT

Monalisa Dubey, Bhavya Ailawadhi, Talat Akhunov +10

The International Liquid Mirror Telescope (ILMT) is a 4-m optical ({\em gri} spectral bands) zenithal survey telescope with a field of view of 22.322.3 arcmin, suitable for…

astro-ph.IM2026

Unveiling photometric transients with the ILMT and their follow-up using DOT

Priyanshi Kumari, Bhavya Ailawadhi, Talat Akhunov +10

The two 4-m class telescopes at the Devasthal site in India are complementary: the 4-m International Liquid Mirror Telescope (ILMT) is dedicated to the discovery of new transient p…

astro-ph.IM2026

From Sky to Science: Time Domain Astronomy with the ILMT Survey

Kuntal Misra, Bhavya Ailawadhi, Talat Akhunov +10

The PyLMT transient detection pipeline has been operational since November 2023 and has detected 10,000 transients and variable objects in ILMT images in near real time. The…

astro-ph.IM2026

Modelling the Point Spread Function of ILMT images

Naveen Dukiya, Bhavya Ailawadhi, Talat Akhunov +11

We have devised an approach to model the empirical Point Spread Function (PSF) of the images taken with the 4-meter International Liquid Mirror Telescope (ILMT). The characteristic…

astro-ph.HE2026

Tomography analysis of the intermediate-luminosity Type Iax SN 2024pxl

Barnabás Barna, Mridweeka Singh, Lindsey A. Kwok +90

We present an abundance tomography analysis of SN 2024pxl, an intermediate luminosity Type Iax supernova ( mag), with the most-detailed follow-up in the Type…

astro-ph.HE2026

Early NIR echo and the time variable mass loss history of Type IIn SN 2024kgi

Naveen Dukiya, Kuntal Misra, Andrea Pastorello +30

We present a comprehensive analysis of the long-term photometric and spectroscopic monitoring campaign of the Type IIn Supernova (SN) 2024kgi. The SN reaches at peak an -band ab…