Parkes summary for current projects utilising FAST time
| Project Code | PI | Dates | Title |
|---|---|---|---|
| PX500/501 | Taotao Fang | 2018 October Semester (2018OCT) | HI Survey of Nearby Edge-On Galaxies An HI observing campaign of several Chandra-observed nearby edge-on Galaxies, intended to study the correlation between galactic parameters. |
| PX500/501 | George Hobbs | 2018 October Semester (2018OCT) | Analysis of state switching pulsars A small-scale survey of the complete sample of intermittent pulsars. |
| PX500/501 | George Hobbs (Andrew Cameron) | 2018 October Semester (2018OCT) | Mapping the orbit of a nulling, long-period binary pulsar A campaign designed to map and solve the orbit of the pulsar J1812-15, an as-yet unpublished discovery of the HTRU-S Galactic Plane survey which also shows nulling behaviour. |
| PX500/501 | Di Li | 2018 October Semester (2018OCT) | Target of Opportunity observations of transient events We propose to set up a Target of Opportunity (ToO) program within the PX500/501 project to follow up transient events. |
| PX500/501 | Junzhi Wang | 2018 October Semester (2018OCT) | Isotope ratios of 12C/13C from formaldehyde in the Galactic central region We propose detailed mapping observations of the 1_11-1_10 lines of H2CO and H213CO toward significant areas covering characteristic GC clouds. In this way we can determine accurately the isotope ratio of 12C/13C towards the GC region. |
| PX500/501 | Renxin Xu | 2018 October Semester (2018OCT) | Single Pulse Study Search mode observations of bright pulsars, aiming to reveal the radio radiation mechanism of pulsars with their single pulse properties. |
| PX500/501 | Wu Yuefang | 2018 October Semester (2018OCT) | Interaction of pulse nulling and sub-pulse drifting We apply for single pulse observations of seven pulsars, all of which show nulling and three of which appear to show drifting behaviour. |
| PX500/501 | Wu Yuefang | 2018 October Semester (2018OCT) | Linear carbon chain molecules and their formation Observations of Planck cold cores and protostars using lines of HC7N, intended to probe components of stellar formation mechanisms. |
Generated: Jimi Green (13-Nov-2018)