most citedMolecular Cross Sections for High Resolution Spectroscopy of Super Earths, Warm Neptunes and Hot Jupiters

74 citations · 179 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.EP2022★ 14 cited

Water observed in the atmosphere of τ Bootis Ab with CARMENES/CAHA

Rebecca K. Webb, Siddharth Gandhi, Matteo Brogi +4

Characterising the atmospheres of hot Jupiters is important in understanding the formation and migration of these exotic planets. However, there are still many open questions about…

astro-ph.EP2020★ 9 cited

A search for He I airglow emission from the hot Jupiter tau Boo b

Yapeng Zhang, I. A. G. Snellen, P. Mollière +4

The helium absorption line at 10830 Å, originating from the metastable triplet state 2S, has been suggested as an excellent probe for the extended atmospheres of hot Jupiters a…

astro-ph.EP2020★ 55 cited

Seeing above the Clouds with High Resolution Spectroscopy

Siddharth Gandhi, Matteo Brogi, Rebecca K. Webb

In the last decade ground based high resolution Doppler spectroscopy (HRS) has detected numerous species in transiting and non-transiting hot Jupiters, and is ideally placed for at…

astro-ph.EP2020★ 74 cited

Molecular Cross Sections for High Resolution Spectroscopy of Super Earths, Warm Neptunes and Hot Jupiters

Siddharth Gandhi, Matteo Brogi, Sergei N. Yurchenko +9

High resolution spectroscopy (HRS) has been used to detect a number of species in the atmospheres of hot Jupiters. Key to such detections is accurately and precisely modelled spect…

astro-ph.EP2020★ 27 cited

A weak spectral signature of water vapour in the atmosphere of HD 179949 b at high spectral resolution in the L-band

Rebecca K. Webb, Matteo Brogi, Siddharth Gandhi +5

High resolution spectroscopy (R > 20,000) is currently the only known method to constrain the orbital solution and atmospheric properties of non-transiting hot Jupiters. It does so…