Click here to view this collection in the new DAP user interface
Parkes observations for project P1067 semester 2020APRS_01
The Parkes Ultra-wide-bandwidth receiver enables, for the first time with the Parkes telescope, a commensal high time and high frequency resolution survey. We will observe Baade's window in which we are guaranteed detections of pulsars and spectral lines. Our science drivers are diverse and range from understanding scattering, to detecting new pul... moresars, to searching for galaxies in the zone of avoidance, probing the globular cluster at the centre of the window and studying OH circumstellar masers and CO-dark molecular gas. The observing strategy and processing software developed for this survey will be applicable to all future Parkes surveys with the wide-band receiver or cyrogenically-cooled phased array feed. less
Astronomical and Space Sciences not elsewhere classified
01 Apr 2020
30 Sep 2020
masers (Galactic and extragalactic)
star formation (Galactic)
interstellar medium in and around the Milky Way
surveys and studies of distant galaxies
Creative Commons Attribution 4.0 International Licence
Hobbs, George; Green, James; Sadler, Elaine; Dawson, Joanne; Li, Di; Cameron, Andrew; Moss, Vanessa; Kaczmarek, Jane; Dai, Shi; Zhang, Lei; Zhang, Songbo (2020): Parkes observations for project P1067 semester 2020APRS_01. v1. CSIRO. Data Collection.
All Rights (including copyright) CSIRO 2020.
Access to this collection's metadata and/or files (if any) are restricted until 30 Mar 2022.
Australia Telescope National Facility
P1067 - A wide-band survey of Baade's Window in the time and frequency domains
The Parkes telescope has been used for numerous surveys. For instance, the telescope has found more than half of the known pulsars. It has also been used to discover new spiral arms in our Galaxy. Parkes has also identified masers. Previously, all these surveys were carried out independently. We are proposing a new survey, which uses the new c... moreapability of the Parkes ultra-wide-bandwidth receiver, that will enable to discovery of both pulsars and spectral features. less