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GASKAP-HI pilot survey science I: ASKAP zoom observations of HI emission in the Small Magellanic Cloud
DOI: 10.1017/pasa.2021.59 Bibcode: 2022PASA...39....5P

van Loon, J. Th.; Lee, M. -Y.; Joncas, G. +53 more

We present the most sensitive and detailed view of the neutral hydrogen ( ${H\small I}$ ) emission associated with the Small Magellanic Cloud (SMC), through the combination of data from the Australian Square Kilometre Array Pathfinder (ASKAP) and Parkes (Murriyang), as part of the Galactic Australian Square Kilometre Array Pathfinder (GASKAP) pilo…

2022 Publications of the Astronomical Society of Australia
Gaia Herschel 29
Discovery of the most luminous quasar of the last 9 Gyr
DOI: 10.1017/pasa.2022.36 Bibcode: 2022PASA...39...37O

Fan, Xiaohui; Wolf, Christian; Lai, Samuel +8 more

We report the discovery of a bright ( g = 14.5 mag (AB), K = 11.9 mag (Vega)) quasar at redshift z=0.83 — the optically brightest (unbeamed) quasar at z>0.4. SMSS J114447.77-430859.3, at a Galactic latitude of b=+18.1°, was identified by its optical colours from the SkyMapper Southern Survey (SMSS) during a search for symbiotic binary stars. Op…

2022 Publications of the Astronomical Society of Australia
Gaia 4
First photometric and orbital period investigations of four W UMa-type eclipse binaries
DOI: 10.1017/pasa.2022.53 Bibcode: 2022PASA...39...57H

Meng, Zi-Bin; Wang, Hong-Wei; Yu, Yun-Xia +2 more

We presented the first photometric and orbital period investigations for four W Ursae Majoris-type binaries: V473 And, V805 And, LQ Com, and EG CVn. The photometric solutions suggested that V805 And and LQ Com are two total-eclipse contact binaries, while V473 And and EG CVn are partial-eclipse ones. V473 And and LQ Com belong to the A-subtype con…

2022 Publications of the Astronomical Society of Australia
Gaia 4
HST WFC3/Grism observations of the candidate ultra-high-redshift radio galaxy GLEAM J0917-0012
DOI: 10.1017/pasa.2022.4 Bibcode: 2022PASA...39...16S

Seymour, N.; Drouart, G.; Vernet, J. D. R. +11 more

We present Hubble Space Telescope Wide Field Camera 3 photometric and grism observations of the candidate ultra-high-redshift ( $z>7$ ) radio galaxy, GLEAM J0917-0012. This radio source was selected due to the curvature in its 70-230 MHz, low-frequency Murchison Widefield Array radio spectrum and its faintness in K-band. Follow-up spectroscopic…

2022 Publications of the Astronomical Society of Australia
Gaia eHST 4
Evidence of distant spiral arms in the Galactic disk quadrant IV from VVV red clump giants
DOI: 10.1017/pasa.2022.31 Bibcode: 2022PASA...39...39K

Minniti, D.; Saito, R. K.; Alonso-García, J. +4 more

The discovery of new clear windows in the Galactic plane using the VVV near-IR extinction maps allows the study of the structure of the Milky Way (MW) disk. The ultimate goal of this work is to map the spiral arms in the far side of the MW, which is a relatively unexplored region of our Galaxy, using red clump (RC) giants as distance indicators. W…

2022 Publications of the Astronomical Society of Australia
Gaia 1