LIGHTS: A robust technique to identify galaxy edges
The LIGHTS survey is imaging galaxies at a depth and spatial resolution comparable to what the Legacy Survey of Space and Time (LSST) will produce in 10 years...
Line-of-sight velocity distributions of elliptical galaxies from collisionless mergers
We analyse the skewness of the line-of-sight velocity distributions in model elliptical galaxies built through collisionless galaxy mergers. We build the models...
Linearization versus Preconditioning: Which Approach Is Best for Solving Multilevel Transfer Problems?
We present a critical analysis of linearization and preconditioning, the two most used approaches proposed for achieving the required linearity in the iterative...
Localization and Broadband Follow-up of the Gravitational-wave Transient GW150914
A gravitational-wave (GW) transient was identified in data recorded by the Advanced Laser Interferometer Gravitational-wave Observatory (LIGO) detectors on 2015...
Long-lasting activity of asteroid (248370) 2005 QN<SUB>173</SUB>
We present the results of observations of asteroid (248370) QN 173 obtained during July 2021-January 2022 with three telescopes. Our analysis revealed the...
Long-term eclipse timing of white dwarf binaries: an observational hint of a magnetic mechanism at work
We present a long-term programme for timing the eclipses of white dwarfs in close binaries to measure apparent and/or real variations in their orbital periods...
Long-term Monitoring, Time Delay, and Microlensing in the Gravitational Lens System Q0142-100
We present 12 yr of monitoring of the gravitational lens Q0142-100 from the Teide Observatory. The data, taken from 1999 to 2010, comprise 105 observing nights...
Low Surface Brightness Galaxies in the Sloan Digital Sky Survey. I. Search Method and Test Sample
In this paper we present results of a pilot study to use imaging data from the Sloan Digital Sky Survey (SDSS) to search for low surface brightness (LSB)...
Lower atmosphere and pressure evolution on Pluto from ground-based stellar occultations, 1988-2016
Context. The tenuous nitrogen (N2) atmosphere on Pluto undergoes strong seasonal effects due to high obliquity and orbital eccentricity, and has recently (July...