The Hyper Suprime-Cam SSP survey: overview and survey design
H Aihara, N Arimoto, R Armstrong… - Publications of the …, 2018 - academic.oup.com
Abstract Hyper Suprime-Cam (HSC) is a wide-field imaging camera on the prime focus of
the 8.2-m Subaru telescope on the summit of Mauna Kea in Hawaii. A team of scientists from …
the 8.2-m Subaru telescope on the summit of Mauna Kea in Hawaii. A team of scientists from …
The galaxy in context: structural, kinematic, and integrated properties
J Bland-Hawthorn, O Gerhard - Annual Review of Astronomy …, 2016 - annualreviews.org
Our Galaxy, the Milky Way, is a benchmark for understanding disk galaxies. It is the only
galaxy whose formation history can be studied using the full distribution of stars from faint …
galaxy whose formation history can be studied using the full distribution of stars from faint …
[HTML][HTML] The art of measuring physical parameters in galaxies: a critical assessment of spectral energy distribution fitting techniques
C Pacifici, KG Iyer, B Mobasher… - The Astrophysical …, 2023 - iopscience.iop.org
The study of galaxy evolution hinges on our ability to interpret multiwavelength galaxy
observations in terms of their physical properties. To do this, we rely on spectral energy …
observations in terms of their physical properties. To do this, we rely on spectral energy …
How to measure galaxy star formation histories. II. Nonparametric models
J Leja, AC Carnall, BD Johnson, C Conroy… - The Astrophysical …, 2019 - iopscience.iop.org
Nonparametric star formation histories (SFHs) have long promised to be the" gold standard"
for galaxy spectral energy distribution (SED) modeling as they are flexible enough to …
for galaxy spectral energy distribution (SED) modeling as they are flexible enough to …
KiDS+ VIKING-450: Cosmic shear tomography with optical and infrared data
H Hildebrandt, F Köhlinger, JL Van den Busch… - Astronomy & …, 2020 - aanda.org
We present a tomographic cosmic shear analysis of the Kilo-Degree Survey (KiDS)
combined with the VISTA Kilo-Degree Infrared Galaxy Survey. This is the first time that a full …
combined with the VISTA Kilo-Degree Infrared Galaxy Survey. This is the first time that a full …
KiDS-450: cosmological parameter constraints from tomographic weak gravitational lensing
H Hildebrandt, M Viola, C Heymans… - Monthly Notices of …, 2017 - academic.oup.com
We present cosmological parameter constraints from a tomographic weak gravitational
lensing analysis of∼ 450 deg2 of imaging data from the Kilo Degree Survey (KiDS). For a …
lensing analysis of∼ 450 deg2 of imaging data from the Kilo Degree Survey (KiDS). For a …
CosmoPower: emulating cosmological power spectra for accelerated Bayesian inference from next-generation surveys
We present CosmoPower, a suite of neural cosmological power spectrum emulators
providing orders-of-magnitude acceleration for parameter estimation from two-point statistics …
providing orders-of-magnitude acceleration for parameter estimation from two-point statistics …
[HTML][HTML] The fourth data release of the Kilo-Degree Survey: ugri imaging and nine-band optical-IR photometry over 1000 square degrees
K Kuijken, C Heymans, A Dvornik… - Astronomy & …, 2019 - aanda.org
Context. The Kilo-Degree Survey (KiDS) is an ongoing optical wide-field imaging survey
with the OmegaCAM camera at the VLT Survey Telescope, specifically designed for …
with the OmegaCAM camera at the VLT Survey Telescope, specifically designed for …
[HTML][HTML] From galactic bars to the hubble tension: Weighing up the astrophysical evidence for milgromian gravity
Astronomical observations reveal a major deficiency in our understanding of physics—the
detectable mass is insufficient to explain the observed motions in a huge variety of systems …
detectable mass is insufficient to explain the observed motions in a huge variety of systems …
emerge – an empirical model for the formation of galaxies since z ∼ 10
We present emerge, an E mpirical M od E l for the fo R mation of G alaxi E s, describing the
evolution of individual galaxies in large volumes from z∼ 10 to the present day. We assign a …
evolution of individual galaxies in large volumes from z∼ 10 to the present day. We assign a …