activity
20032022
most citedConsistent dust and gas models for protoplanetary disks. I. Disk shape, dust settling, opacities, and PAHs

379 citations · 5.3k across the 87 of their papers we have counts for

collaborators

84 papers

astro-ph.EP2022★ 39 cited

H2S and SO2 detectability in Hot Jupiters: Sulfur species as indicator of metallicity and C/O ratio

J. Polman, L. B. F. M. Waters, M. Min +2

The high cosmic abundance and the intermediate volatility and chemical properties of sulfur allow the use of sulfur-bearing species as a tracer of the chemical processes in the atm…

astro-ph.EP2022★ 22 cited

A retrieval challenge exercise for the Ariel mission

Joanna K. Barstow, Quentin Changeat, Katy L. Chubb +5

The Ariel mission, due to launch in 2029, will obtain spectroscopic information for 1000 exoplanets, providing an unprecedented opportunity for comparative exoplanetology. Retrieva…

astro-ph.EP2022★ 30 cited

Convolutional neural networks as an alternative to Bayesian retrievals

Francisco Ardevol Martinez, Michiel Min, Inga Kamp +1

Exoplanet observations are currently analysed with Bayesian retrieval techniques. Due to the computational load of the models used, a compromise is needed between model complexity…

astro-ph.EP2022★ 24 cited

Investigating the detectability of hydrocarbons in exoplanet atmospheres with JWST

Danny Gasman, Michiel Min, Katy L. Chubb

We investigate at what abundances various hydrocarbon molecules (e.g. acetylene (CH), ethylene (CH), and methane (CH)) become detectable when observing the atmo…

astro-ph.EP2021★ 20 cited

Self-consistent modelling of the dust component in protoplanetary and circumplanetary disks: the case of PDS 70

B. Portilla-Revelo, I. Kamp, Ch. Rab +4

Direct observations of young stellar objects are important to test established theories of planet formation. PDS 70 is one of the few cases where robust evidence favours the presen…

astro-ph.EP2021★ 31 cited

SimAb: A simple, fast and flexible model to assess the effects of planet formation on the atmospheric composition of gas giants

N. Khorshid, M. Min, J. M. Désert +2

We present a basic, fast, and flexible planet formation model, called SimAb (Simulating Abundances), to form giant planets and study their primary atmospheric composition soon afte…