Observational probes of cosmic acceleration
DH Weinberg, MJ Mortonson, DJ Eisenstein, C Hirata… - Physics reports, 2013 - Elsevier
The accelerating expansion of the universe is the most surprising cosmological discovery in
many decades, implying that the universe is dominated by some form of “dark energy” with …
many decades, implying that the universe is dominated by some form of “dark energy” with …
Cosmological parameters from observations of galaxy clusters
Studies of galaxy clusters have proved crucial in helping to establish the standard model of
cosmology, with a Universe dominated by dark matter and dark energy. A theoretical basis …
cosmology, with a Universe dominated by dark matter and dark energy. A theoretical basis …
Planck 2015 results-XXVII. The second Planck catalogue of Sunyaev-Zeldovich sources
PAR Ade, N Aghanim, M Arnaud, M Ashdown… - Astronomy & …, 2016 - aanda.org
We present the all-sky Planck catalogue of Sunyaev-Zeldovich (SZ) sources detected from
the 29 month full-mission data. The catalogue (PSZ2) is the largest SZ-selected sample of …
the 29 month full-mission data. The catalogue (PSZ2) is the largest SZ-selected sample of …
redmapper. i. algorithm and sdss dr8 catalog
ES Rykoff, E Rozo, MT Busha, CE Cunha… - The Astrophysical …, 2014 - iopscience.iop.org
We describe redMaPPer, a new red sequence cluster finder specifically designed to make
optimal use of ongoing and near-future large photometric surveys. The algorithm has …
optimal use of ongoing and near-future large photometric surveys. The algorithm has …
Planck 2015 results-III. LFI systematic uncertainties
PAR Ade, J Aumont, C Baccigalupi, AJ Banday… - Astronomy & …, 2016 - aanda.org
We present the current accounting of systematic effect uncertainties for the Low Frequency
Instrument (LFI) that are relevant to the 2015 release of the Planck cosmological results …
Instrument (LFI) that are relevant to the 2015 release of the Planck cosmological results …
LOFAR observations of galaxy clusters in HETDEX-Extraction and self-calibration of individual LOFAR targets
RJ Van Weeren, TW Shimwell, A Botteon… - Astronomy & …, 2021 - aanda.org
Diffuse cluster radio sources, in the form of radio halos and relics, reveal the presence of
cosmic rays and magnetic fields in the intracluster medium (ICM). These cosmic rays are …
cosmic rays and magnetic fields in the intracluster medium (ICM). These cosmic rays are …
Nine new repeating fast radio burst sources from CHIME/FRB
E Fonseca, BC Andersen, M Bhardwaj… - The Astrophysical …, 2020 - iopscience.iop.org
We report on the discovery and analysis of bursts from nine new repeating fast radio burst
(FRB) sources found using the Canadian Hydrogen Intensity Mapping Experiment (CHIME) …
(FRB) sources found using the Canadian Hydrogen Intensity Mapping Experiment (CHIME) …
The Atacama Cosmology Telescope: Sunyaev-Zel'dovich selected galaxy clusters at 148 GHz from three seasons of data
We present a catalog of 68 galaxy clusters, of which 19 are new discoveries, detected via
the Sunyaev-Zel'dovich effect (SZ) at 148 GHz in the Atacama Cosmology Telescope (ACT) …
the Sunyaev-Zel'dovich effect (SZ) at 148 GHz in the Atacama Cosmology Telescope (ACT) …
Supplement:“localization and broadband follow-up of the gravitational-wave transient GW150914”(2016, ApJL, 826, L13)
BP Abbott, R Abbott, TD Abbott… - The Astrophysical …, 2016 - iopscience.iop.org
This Supplement provides supporting material for Abbott et al.(2016a). We briefly summarize
past electromagnetic (EM) follow-up efforts as well as the organization and policy of the …
past electromagnetic (EM) follow-up efforts as well as the organization and policy of the …
A catalog of 132,684 clusters of galaxies identified from Sloan Digital Sky Survey III
ZL Wen, JL Han, FS Liu - The Astrophysical Journal Supplement …, 2012 - iopscience.iop.org
Using the photometric redshifts of galaxies from the Sloan Digital Sky Survey III (SDSS-III),
we identify 132,684 clusters in the redshift range of 0.05⩽ z< 0.8. Monte Carlo simulations …
we identify 132,684 clusters in the redshift range of 0.05⩽ z< 0.8. Monte Carlo simulations …