Data

ASKAP/WALLABY Early Science Project AS035 - HI Spectral Cube of the Lyon Group of Galaxies 351

The University of Western Australia
For, Bi-Qing ; Staveley-Smith, Lister ; Westmeier, Tobias ; Whiting, Matthew ; Oh, Se-Heon ; Koribalski, Baerbel ; Wang, Jing ; Wong, Ivy ; Bekiaris, Georgios ; Cortese, Luca ; Elagali, Ahmed ; Kleiner, Dane ; Lee-Waddell, Karen ; Madrid Gamboa, Juan ; Popping, Attila ; Rhee, Jonghwan ; Reynolds, Tristan ; Collier, Jordan ; Phillips, Chris ; Voronkov, Max ; Mueller, Oliver ; Jerjen, Helmut
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ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Adc&rfr_id=info%3Asid%2FANDS&rft_id=info:doi10.25919/5dbb90180b902&rft.title=ASKAP/WALLABY Early Science Project AS035 - HI Spectral Cube of the Lyon Group of Galaxies 351&rft.identifier=10.25919/5dbb90180b902&rft.publisher=CSIRO Publishing&rft.description=This collection contains two spectral image cubes of the LGG 351 group. The image cubes consist of 23 ASKAP beams and 7 MHz of bandwidth (1396.57 to 1403.56 MHz, with a resolution of 18.5 kHz). The sky coverage is 13:24:00 < RA < 13:38:00 and -26:30:00 < DEC < -33:30:00. One of the spectral cubes has 45x35 synthesized beam, which is used in For et al. 2019, MNRAS DOI: 10.1093/mnras/stz2501 . The other spectral cube has synthesized beam of 26x19.&rft.creator=For, Bi-Qing &rft.creator=Staveley-Smith, Lister &rft.creator=Westmeier, Tobias &rft.creator=Whiting, Matthew &rft.creator=Oh, Se-Heon &rft.creator=Koribalski, Baerbel &rft.creator=Wang, Jing &rft.creator=Wong, Ivy &rft.creator=Bekiaris, Georgios &rft.creator=Cortese, Luca &rft.creator=Elagali, Ahmed &rft.creator=Kleiner, Dane &rft.creator=Lee-Waddell, Karen &rft.creator=Madrid Gamboa, Juan &rft.creator=Popping, Attila &rft.creator=Rhee, Jonghwan &rft.creator=Reynolds, Tristan &rft.creator=Collier, Jordan &rft.creator=Phillips, Chris &rft.creator=Voronkov, Max &rft.creator=Mueller, Oliver &rft.creator=Jerjen, Helmut &rft.date=2019&rft.type=dataset&rft.language=English Access the data

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This collection contains two spectral image cubes of the LGG 351 group. The image cubes consist of 23 ASKAP beams and 7 MHz of bandwidth (1396.57 to 1403.56 MHz, with a resolution of 18.5 kHz). The sky coverage is 13:24:00 < RA < 13:38:00 and -26:30:00 < DEC < -33:30:00. One of the spectral cubes has 45"x35" synthesized beam, which is used in For et al. 2019, MNRAS DOI: 10.1093/mnras/stz2501 . The other spectral cube has synthesized beam of 26"x19".

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Associated Persons
Se-Heon Oh (Creator); Jing Wang (Contributor)Matthew Whiting (Creator); Baerbel Koribalski (Creator); Georgios Bekiaris (Creator); Dane Kleiner (Creator); Juan Madrid Gamboa (Creator); Jordan Collier (Creator); Chris Phillips (Contributor); Max Voronkov (Contributor); Oliver Mueller (Creator); Helmut Jerjen (Creator)

Issued: 2019-12-12

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