Abstract The Optical, Spectroscopic, and Infrared Remote Imaging System OSIRIS is the
scientific camera system onboard the Rosetta spacecraft (Figure 1). The advanced high …

▪ Abstract Standard star photometry dominated the latter half of the twentieth century
reaching its zenith in the 1980s. It was introduced to take advantage of the high sensitivity …

Context. The census of stellar and substellar companions of nearby stars is largely
incomplete, in particular toward the low-mass brown dwarf and long-period exoplanets. It is …

The precise localization of the repeating fast radio burst (FRB 121102) has provided the first
unambiguous association (chance coincidence probability p≲ 3× 10− 4) of an FRB with an …

This paper presents and summarizes a software package (" LPipe") for completely
automated, end-to-end reduction of both bright and faint sources with the Low Resolution …

We combine high-redshift Type Ia supernovae from the first three years of the Supernova
Legacy Survey (SNLS) with other supernova (SN) samples, primarily at lower redshifts, to …

Context. In the age of JWST, temperate terrestrial exoplanets transiting nearby late-type M
dwarfs provide unique opportunities for characterising their atmospheres, as well as …

We present distance measurements to 71 high redshift type Ia supernovae discovered
during the first year of the 5-year Supernova Legacy Survey (SNLS). These events were …

ABSTRACT The High-Z Supernova Search is an international collaboration to discover and
monitor Type Ia supernovae (SNe Ia) at z> 0.2 with the aim of measuring cosmic …

Studying quasars at the highest redshifts can constrain models of galaxy and black hole
formation, and it also probes the intergalactic medium in the early universe. Optical surveys …