collaborators

6 papers

astro-ph.IM2026

The Tartu Observatory Fiber-fed Echelle Spectrograph (TOFES) Data Reduction Pipeline

Sandipan P. D. Borthakur, Tõnis Eenmäe, Nikolai Piskunov +9

We introduce the data reduction pipeline for the Tartu Observatory Fiber-fed Echelle Spectrograph (TOFES). TOFES is installed in the Coudé room and will be connected to the 1.5 m…

astro-ph.SR2026

Ariel stellar characterisation IV. Fundamental parameters of 18 hot stars in the Ariel mission candidate sample

H. Ramler, S. P. D. Borthakur, C. P. Folsom +16

The characterisation of exoplanetary systems depends on the accurate determination of host star parameters. The Ariel mission will probe the atmospheres of a statistically signific…

astro-ph.EP2025

NLTE atmospheric modelling of the ultra-hot Jupiter WASP-178b and comparison with UV and optical observations

L. Fossati, A. G. Sreejith, T. Koskinen +6

We model the atmosphere of the ultra-hot Jupiter (UHJ) WASP-178b accounting for NLTE effects and compare synthetic transmission spectra with NUV and optical observations. We use th…

astro-ph.EP2025

Refractory phosphorus in the HD 100546 protoplanetary disk

Mihkel Kama, Oliver Shorttle, Sandipan P. D. Borthakur +5

The phosphorus budget of planets is intertwined with their formation history and is thought to influence their habitability. The chemical reservoirs and volatile \emph{vs} refracto…

astro-ph.SR2025

Abundance analysis of stars hosting gas-rich debris disks

Sandipan P. D. Borthakur, Mihkel Kama, Luca Fossati +4

Accretion from protoplanetary or debris disks can contaminate the stellar photosphere, which is detectable in stars with radiative envelopes due to relatively slower photospheric m…

astro-ph.SR2025

Atmospheric dynamics of the hypergiant RW Cep during the Great Dimming

A. Kasikov, I. Kolka, A. Aret +5

The hypergiant RW Cep is one of the largest stars in our galaxy. The evolution and mass loss of such stars has profound effects on their surrounding regions and the galaxy as a who…