The origin of the highest energy cosmic rays is still unknown. The discovery of their sources
is expected to reveal the workings of the most energetic astrophysical accelerators in the …

The epoch of galaxy assembly from 2⩽ z⩽ 4 marks a critical stage during the evolution of
today's galaxy population. During this period, the star-formation activity in the Universe was …

Fast radio bursts (FRBs) are brief, bright, extragalactic radio flashes,. Their physical origin
remains unknown, but dozens of possible models have been postulated. Some FRB sources …

We use 26× 10 6 galaxies from the Dark Energy Survey (DES) Year 1 shape catalogs over
1321 deg 2 of the sky to produce the most significant measurement of cosmic shear in a …

Gravitational waves (GWs) from compact binary coalescences allow for the direct
measurement of the luminosity distance to their source. This makes them standard-distance …

During the second observing run of the Laser Interferometer Gravitational-wave Observatory
(LIGO) and Virgo Interferometer, a gravitational-wave signal consistent with a binary neutron …

This paper presents a table with estimates of the absolute magnitude of the Sun and the
conversions from vegamag to the AB and ST systems for several wide-band filters used in …

ABSTRACT The remarkable Hubble Space Telescope (HST) data sets from the CANDELS,
HUDF09, HUDF12, ERS, and BoRG/HIPPIES programs have allowed us to map the …

We explore the simple inter-relationships between mass, star formation rate, and
environment in the SDSS, zCOSMOS, and other deep surveys. We take a purely empirical …

In the companion Paper XV of this series, we derive accurate total mass-to-light ratios within
a sphere of radius centred on the galaxy, as well as stellar (M/L) stars (with the dark matter …