Parkes observations for project P1171 semester 2023OCTS_07
CSIRO RDS Repository
View Archive InfoField | Value | |
Title |
Parkes observations for project P1171 semester 2023OCTS_07
|
|
Creator |
Florian Eppel
|
|
Subject |
Astronomical sciences not elsewhere classified
|
|
Description |
The origin of Fast Radio Bursts (FRBs) is still unclear with a plethora of theoretical models for their origin. Several models predict associated multi-wavelength emission, but previous searches for optical, X-ray or gamma-ray counterparts of FRBs have not led to any detection. The Galactic magnetar SGR 1935+2154A has been observed to simultaneously emit FRB-like bursts and X-ray flares, which suggests that also extragalactic FRB sources may exhibit X-ray counterparts. Because of the high cost of X-ray satellites and in face of the relatively low FRB detection probability in their small field of view, coordinated radio and X-ray observations are logistically very difficult to set up. We propose a new approach using the X-ray satellite XMM-Newton and the Parkes/Murriyang radio telescope to put constraints on the theoretical models: We aim to conduct shadowing observations with the Parkes telescope to search for new FRBs in fields that are simultaneously covered by XMM-Newton. We hereby target regular XMM observations of nearby (low-z) galaxies, to increase our detection chances of possibly associated X-ray emission. In case of an FRB detection in the radio band, we will have guaranteed simultaneous X-ray coverage and will get detailed information about the associated X-ray spectrum and light curve since all XMM-Newton data will become public a year after the observation. |
|
Publisher |
CSIRO
|
|
Contributor |
Clancy James
Matthias Kadler Joern Wilms Ryan Shannon Laura Spitler Arne Rau Mirko Krumpe Sabina Bahic Marylin Cruces Chenhui Niu |
|
Date |
2023-12-15
|
|
Type |
—
|
|
Format |
—
|
|
Identifier |
csiro:61236
|
|
Language |
—
|
|
Coverage |
—
|
|
Rights |
—
|
|