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20212026
most citedPhotometric and spectroscopic analysis of the Type II SN 2020jfo with a short plateau

15 citations · 46 across the 35 of their papers we have counts for

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12 papers · 1 filter

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.EP2026

Post-perihelion Photometric and Spectroscopic Monitoring of the Interstellar Comet 3I/ATLAS

Goldy Ahuja, Shashikiran Ganesh, K. Aravind +12

The third interstellar object, comet 3I/ATLAS, was observed using various Indian telescopes during its post-perihelion evolution. We carried out imaging and spectroscopic observati…

astro-ph.IM2026

Demonstrating the Time-Domain Capabilities of the 4-m International Liquid Mirror Telescope: An Early Census of Transient and Variable Detections

Kumar Pranshu, Kuntal Misra, Bhavya Ailawadhi +11

The PyLMT transient detection pipeline has been operational since November 2023, detecting transient and variable objects in the ILMT images in almost real time. Using the image su…

astro-ph.HE2026

Wild behaviour near the finish line: the Type Ibn SN 2020able and its stratified environment

L. Tartaglia, E. Cappellaro, G. Valerin +29

We present spectrophotometric observations of the Type Ibn supernova SN~2020able, along with a comprehensive analysis and modelling of its evolution. The transient occurred in SDSS…

astro-ph.EP2026

Detection and identification of asteroids with the 4-m ILMT

Sara Filali, Bhavya Ailawadhi, Talat Akhunov +11

The International Liquid Mirror Telescope (ILMT) covers a 22.3' wide strip of sky in declination (δ), centred at δ = +29° 21' 41.4'' and right ascension (α) in the range 0 h <= α <…

astro-ph.IM2026

Astrometric Calibration of the 4-m International Liquid Mirror Telescope Observations

Vibhore Negi, Naveen Dukiya, Gokul Singh Mehra +12

The 4-m International Liquid Mirror Telescope (ILMT) is a dedicated time domain survey telescope that continuously scans the zenithal sky over the Indian Himalayas in the g', r' an…

astro-ph.HE2026

SN 2024dy: Dust formation in a long-lived Type IIn supernova and constraints on the dust mass

Sota Goto, Masayuki Yamanaka, Koji S. Kawabata +10

Type~IIn supernovae (SNe) are a subclass of core-collapse SNe powered by interaction between the ejecta and the dense circumstellar material. Among them, long-lived Type~IIn events…

astro-ph.EP2026

Performance of the 4-m International Liquid Mirror Telescope tested in two fields at high and low ecliptic and galactic latitudes

Sara Filali, Kumar Pranshu, Jean Surdej +10

The 4-m International Liquid Mirror Telescope (ILMT) offers a unique opportunity to detect transients in a narrow strip of sky. We explore ILMT's potential to detect astrometric an…

astro-ph.HE2026

Early interaction signatures and an extended plateau phase in Type II SN 2020aze

B. Ailawadhi, R. Dastidar, K. Misra +27

We present a photometric and spectroscopic analysis of the fast-declining Type II SN 2020aze, observed in optical bands from 2.2 to 137.4 days after explosion. The V-band light cur…