WALLABY - an SKA Pathfinder Hi survey
Barbel S Koribalski, L Staveley-Smith, T Westmeier, P Serra, K Spekkens, O Wong, K Lee-Waddell, CDP Lagos, D Obreschkow, E Ryan-Weber, M Zwaan, V Kilborn, G Bekiaris, K Bekki, F Bigiel, A Boselli, A Bosma, B Catinella, G Chauhan, ME Cluver Show all
Astrophysics and Space Science | SPRINGER | Published : 2020
Awarded by European Union's Horizon 2020 research and innovation programme
Awarded by Australian Research Council Future Fellowship - Australian Government
Awarded by MINECO/FEDER, UE
Awarded by MICIU/FEDER, EU
Awarded by State Agency for Research of the Spanish MCIU through the "Center of Excellence Severo Ochoa"
Awarded by Juan de la Cierva formacion fellowship
Awarded by BMBF
Awarded by European Research Council under the European Union's Seventh Framework Programme (FP/2007-2013)/ERC Grant
Awarded by Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D)
The Australian SKA Pathfinder (ASKAP) is part of the Australia Telescope National Facility (ATNF) which is managed by CSIRO. Operation of ASKAP is funded by the Australian Government with support from the National Collaborative Research Infrastructure Strategy (NCRIS). ASKAP uses the resources of the Pawsey Supercomputing Centre. Establishment of ASKAP, the Murchison Radio-astronomy Observatory (MRO) and the Pawsey Supercomputing Centre are initiatives of the Australian Government, with support from the Government of Western Australia and the Science and Industry Endowment Fund. We acknowledge the Wajarri Yamatji as the traditional owners of the Observatory site.FB and DK acknowledge funding from the European Union's Horizon 2020 research and innovation programme; grant agreement No 726384 (FB) and No 679627 (DK).MEC is a recipient of an Australian Research Council Future Fellowship (project number FT170100273) funded by the Australian Government.RKK acknowledges the South African Research Chairs Initiative of the Department of Science and Innovation. RKK and GIGJ acknowledge the South African National Research Foundation for their support.MGJ and LVM acknowledge support from the grants AYA2015-65973-C3-1-R (MINECO/FEDER, UE) and RTI2018-096228-B-C31 (MICIU/FEDER, EU), as well as from the State Agency for Research of the Spanish MCIU through the "Center of Excellence Severo Ochoa" award for the Instituto de Astrofisica de Andalucia (SEV-20170709). MGJ is supported by a Juan de la Cierva formacion fellowship (FJCI-2016-29685).PK is partially supported by the BMBF project 05A17PC2 for D-MeerKAT.DO is a recipient of an Australian Research Council Future Fellowship (FT190100083) funded by the Australian Government.KS acknowledges support from the Natural Sciences and Engineering Research Council of Canada (NSERC).JMvdH acknowledges support from the European Research Council under the European Union's Seventh Framework Programme (FP/2007-2013)/ERC Grant Agreement nr. 291531.Parts of this research were supported by the Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), through project number CE170100013.