VizieR Online Data Catalog: WALLABY pilot survey: HI gas in Hydra cluster (Wang+, 2021)

  • Jing Wang (Creator)
  • Lister Staveley-Smith (Creator)
  • Tobias Westmeier (Creator)
  • Barbara Catinella (Creator)
  • L. Shao (Creator)
  • Tristan Reynolds (Creator)
  • Bi-Qing For (Creator)
  • Benjamin Lee (Creator)
  • Zibin Liang (Creator)
  • Shun Wang (Creator)
  • Ahmed Elagali (Creator)
  • Helga Dénes (Creator)
  • Dane Kleiner (Creator)
  • Baerbel Koribalski (Creator)
  • Karen Lee-Waddell (Creator)
  • Se-Heon Oh (Sejong University) (Creator)
  • Jonghwan Rhee (Creator)
  • P. Serra (Creator)
  • Kristine Spekkens (Creator)
  • Ivy Wong (Creator)
  • Kenji Bekki (Creator)
  • Frank Bigiel (Creator)
  • Helene M. Courtois (Creator)
  • Kelley M. Hess (Creator)
  • Benne W. Holwerda (Creator)
  • Kristen B W McQuinn (Creator)
  • M Pandey-Pommier (Creator)
  • J.M. Van Der Hulst (Creator)
  • Lourdes Verdes-Montenegro (Creator)

Dataset

Description

Taking advantage of the high survey efficiency of the Australian Square Kilometre Array Pathfinder (ASKAP), the pilot survey of Widefield ASKAP L-band Legacy All-sky Blind surveY (WALLABY; Koribalski+ 2020Ap&SS.365..118K) has been targeting nearby clusters and groups. In this study, we use its second internal data release of the Hydra cluster. WALLABY mapped a 60deg^2^ area around the Hydra cluster center, reaching out to 4r_200_ and fully covering the region within 2r_200_. The WALLABY observation reached a targeted sensitivity of {sigma}_cube_=2.0+/-0.5mJy/beam, with a circular beam FWHM of b_maj_~30" (~7kpc at the distance of Hydra) and a velocity spectral resolution of 4km/s. We use the optical g- and r-band images from the second data release of Pan-STARRS (Waters+ 2020ApJS..251....4W) to derive optical properties. The Hydra cluster has a distance of 47.5+/-3Mpc and based on X-ray data, has a radius r_200_~1.35Mpc, and a mass within this radius, M_200_~3.02x10^14^M_{sun}_ (Reiprich & Bohringer 2002ApJ...567..716R). Its velocity dispersion {sigma}_C_=620km/s is derived from M_200_ using the equation of Evrard+ (2008ApJ...672..122E).
Date made availableNov 2022
PublisherSAO/NASA Astrophysics Data System (ADS)

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