The galaxy cluster mass scale and its impact on cosmological constraints from the cluster population

GW Pratt, M Arnaud, A Biviano, D Eckert, S Ettori… - Space Science …, 2019 - Springer
The total mass of a galaxy cluster is one of its most fundamental properties. Together with
the redshift, the mass links observation and theory, allowing us to use the cluster population …

Surveying the reach and maturity of machine learning and artificial intelligence in astronomy

CJ Fluke, C Jacobs - Wiley Interdisciplinary Reviews: Data …, 2020 - Wiley Online Library
Abstract Machine learning (automated processes that learn by example in order to classify,
predict, discover, or generate new data) and artificial intelligence (methods by which a …

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 …

The weak lensing radial acceleration relation: Constraining modified gravity and cold dark matter theories with KiDS-1000

MM Brouwer, KA Oman, EA Valentijn, M Bilicki… - Astronomy & …, 2021 - aanda.org
We present measurements of the radial gravitational acceleration around isolated galaxies,
comparing the expected gravitational acceleration given the baryonic matter (g bar) with the …

Astronomical big data processing using machine learning: A comprehensive review

S Sen, S Agarwal, P Chakraborty, KP Singh - Experimental Astronomy, 2022 - Springer
Astronomy, being one of the oldest observational sciences, has collected a lot of data over
the ages. In recent times, it is experiencing a huge data surge due to advancements in …

Machine learning for observational cosmology

K Moriwaki, T Nishimichi… - Reports on Progress in …, 2023 - iopscience.iop.org
An array of large observational programs using ground-based and space-borne telescopes
is planned in the next decade. The forthcoming wide-field sky surveys are expected to …

The Fornax Deep Survey with the VST-IV. A size and magnitude limited catalog of dwarf galaxies in the area of the Fornax cluster

A Venhola, R Peletier, E Laurikainen, H Salo… - Astronomy & …, 2018 - aanda.org
Context. The Fornax Deep Survey (FDS), an imaging survey in the u′, g′, r′, and i′-
bands, has a supreme resolution and image depth compared to the previous spatially …

Machine learning in astronomy: A practical overview

D Baron - arxiv preprint arxiv:1904.07248, 2019 - arxiv.org
Astronomy is experiencing a rapid growth in data size and complexity. This change fosters
the development of data-driven science as a useful companion to the common model-driven …

Galaxy And Mass Assembly (GAMA): assimilation of KiDS into the GAMA database

S Bellstedt, SP Driver, ASG Robotham… - Monthly Notices of …, 2020 - academic.oup.com
ABSTRACT The Galaxy And Mass Assembly Survey (GAMA) covers five fields with highly
complete spectroscopic coverage (> 95 per cent) to intermediate depths (r< 19.8 or i< 19.0 …

4MOST consortium survey 7: wide-area vista extragalactic survey (WAVES)

SP Driver, J Liske, LJM Davies, ASG Robotham… - arxiv preprint arxiv …, 2019 - arxiv.org
WAVES is designed to study the growth of structure, mass and energy on scales of~ 1 kpc
to~ 10 Mpc over a 7 Gyr timeline. On the largest length scales (1-10 Mpc) WAVES will …