In this paper, we use information from the light field to obtain a distribution map of the wavefront phase. This distribution is associated with changes in...
Lightweight metal mirrors manufactured by AM applied to astronomical instrumentation: first steps towards all-in-one opto-mechanical components
Additive Manufacture (AM) comprises a group of technologies that allow to go from a 3D model to manufactured components, creating them layer by layer until the...
LIGO/Virgo S200213t: No notable candidates in GOTO imaging
We report on optical observations with the Gravitational-wave Optical Transient Observer prototype in response to S200213t (GCN #27042).Targeted observations...
LIINUS: a design study for interferometric imaging spectroscopy at the LBT
We present a feasible design concept and the science drivers for the proposed near-infrared interferometric integral field spectrograph at the LBT. Combining...
LiLiMaRlin and applications to OWN, MONOS, and CollDIBs OWN, MONOS, and CollDIBs
LiLiMaRlin is a library of libraries of massive-star high-resolution optical spectra built by collecting data from [a] our spectroscopic surveys (OWN, IACOB...
Limits on the D:H ratio in the interstellar medium from molecular observations
The abundance ratio of D:H in the interstellar medium can be derived either more directly from the UV absorption measurements of HD and H2 in the spectra of...