The Voltage Capture System (VCS; Tremblay et al. 2015) provides access to high time and frequency resolution voltage data from the MWA. The data recorded are the critically sampled voltages streaming from the fine-PFB stage of the standard MWA signal chain (i.e. before the correlator), thus the data have 100 μs time resolution and 10 kHz frequency resolution. The primary science driver for the VCS is pulsars, though there are also opportunities in terms of channelised either to 10 kHz resolution (legacy) or 1.28 MHz (MWAX).
The primary science driver for the VCS is the study of pulsars, exploring a frequency range in which the vast majority of pulsars have very little or no published information. Some major themes are:
- The pulsar emission mechanism, i.e. studying phenomena such as giant pulses, sub-pulse drifting, and emission intermittency
- Survey and monitoring science, i.e characterising known pulsars, detection of new pulsars, and regular monitoring of targets of interest, and
- Propagation effects induced by the interstellar medium, i.e pulse broadening/scattering, scintillation and dispersion measure variations (in time and frequency).
Apart from pulsars, VCS data can also be applied to:
- Cosmic rays
- FRBs
- Solar science (e.g. solar bursts, interplanetary scintillation)
...
Please also see the MWA Transients Collaboration for other transient science (e.g. triggering on GRBs, FRBs and other exotic phenomena).Fundamentally, VCS data is much larger than normal MWA observations, providing ~28 TB/hr of data. This also limits the duration of any single observing run to ~1.5 hours. flare stars) which do not necessarily rely on the VCS.
Contents
| Child pages (Children Display) |
|---|