activity
20102026
most citedTracing the formation history of giant planets in protoplanetary disks with Carbon, Oxygen, Nitrogen and Sulphur

193 citations · 319 across the 15 of their papers we have counts for

collaborators

16 papers

astro-ph.IM2026

Planet formation on solar system scales

Francesco Zagaria, Andrés F. Izquierdo, Jaehan Bae +32

Giant planets are often regarded as primordial protoplanetary "architects". Their formation and interactions with planetesimals and other planets during and after the protoplanetar…

astro-ph.EP2026

The refractory fraction of phosphorus in planet-forming discs

Sandipan P. D. Borthakur, Mihkel Kama, Luca Fossati +3

Context. Phosphorus (P) is an essential element for life on Earth and a potential tracer of planet formation history. However, there has been no detection of P-bearing molecules in…

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 T…

astro-ph.SR2026

Detectability of deuterium in spectra of early-type stars

Veronika Mitrokhina, Colin P. Folsom, Mihkel Kama +1

Context: Deuterium is easily destroyed in stellar interiors through nuclear fusion. It is therefore usually not expected to be present in stellar photospheres. Early-type stars, wi…

astro-ph.EP2026

sponchpop: Population synthesis to investigate volatile sulfur as a fingerprint of gas giant formation histories

Anna Sommerville-Thomas, Mihkel Kama, Oliver Shottle +1

Planet population synthesis is an integral tool for linking exoplanets to their formation environments. Most planet population synthesis studies have focused on the carbon-to-oxyge…

astro-ph.EP2025

Planet-induced Gas and Dust Substructure Feedbacks on Disk Thermal Structure

Kan Chen, Paola Pinilla, Mihkel Kama

Protoplanets can interact with their natal disks and generate gas and dust substructures such as gaps and rings. However, how these planet-induced substructures affect the disk tem…