An optical biosensor is a specialized analytical device that utilizes the principles of optics
and light in bimolecular processes. Localized surface plasmon resonance (LSPR) is a …

Transport-induced quenching, ie the homogenization of chemical abundances by
atmospheric advection, is thought to occur in the atmospheres of hot gas giant exoplanets …

We report transmission spectroscopy of the bloated hot Jupiter WASP-74b in the wavelength
range from 4000 to 6200 Å. We observe two transit events with the Very Large Telescope …

We have performed low-resolution ground-based spectroscopy of HATS-46 b in
transmission, using the EFOSC2 instrument on the ESO New Technology Telescope (NTT) …

One of the strongest Na i features was observed in WASP-96b. To confirm this novel
detection, we provide a new 475–825 nm transmission spectrum obtained with …

We present a new optical transmission spectrum of the hot Jupiter HAT-P-1b based on two
transits observed with the Double Spectrograph (DBSP) on the Palomar 200-inch (P200) …

We present the optical transmission spectrum of the hot Jupiter WASP-104b based on one
transit observed by the blue and red channels of the Double Spectrograph (DBSP) at the …

We present new optical transmission spectra for two hot Jupiters: WASP-25b (M= 0.56 MJ;
R= 1.23 RJ; P= 3.76 days) and WASP-124b (M= 0.58 MJ; R= 1.34 RJ; P= 3.37 days), with …

High-precision transit photometry supplies ideal opportunities for detecting new exoplanets
and characterizing their physical properties, which usually encode valuable information for …

Transiting planets provide unique opportunities for the atmospheric characterization of
exoplanets as they can reveal composition and the temperature structures at the day–night …