MbrlCatalogueTitleDetail

Do you wish to reserve the book?
VieRDS: A Software to Simulate Raw Telescope Data for very Long Baseline Interferometry
VieRDS: A Software to Simulate Raw Telescope Data for very Long Baseline Interferometry
Hey, we have placed the reservation for you!
Hey, we have placed the reservation for you!
By the way, why not check out events that you can attend while you pick your title.
You are currently in the queue to collect this book. You will be notified once it is your turn to collect the book.
Oops! Something went wrong.
Oops! Something went wrong.
Looks like we were not able to place the reservation. Kindly try again later.
Are you sure you want to remove the book from the shelf?
VieRDS: A Software to Simulate Raw Telescope Data for very Long Baseline Interferometry
Oops! Something went wrong.
Oops! Something went wrong.
While trying to remove the title from your shelf something went wrong :( Kindly try again later!
Title added to your shelf!
Title added to your shelf!
View what I already have on My Shelf.
Oops! Something went wrong.
Oops! Something went wrong.
While trying to add the title to your shelf something went wrong :( Kindly try again later!
Do you wish to request the book?
VieRDS: A Software to Simulate Raw Telescope Data for very Long Baseline Interferometry
VieRDS: A Software to Simulate Raw Telescope Data for very Long Baseline Interferometry

Please be aware that the book you have requested cannot be checked out. If you would like to checkout this book, you can reserve another copy
How would you like to get it?
We have requested the book for you! Sorry the robot delivery is not available at the moment
We have requested the book for you!
We have requested the book for you!
Your request is successful and it will be processed during the Library working hours. Please check the status of your request in My Requests.
Oops! Something went wrong.
Oops! Something went wrong.
Looks like we were not able to place your request. Kindly try again later.
VieRDS: A Software to Simulate Raw Telescope Data for very Long Baseline Interferometry
VieRDS: A Software to Simulate Raw Telescope Data for very Long Baseline Interferometry
Journal Article

VieRDS: A Software to Simulate Raw Telescope Data for very Long Baseline Interferometry

2021
Request Book From Autostore and Choose the Collection Method
Overview
The digital data produced by each telescope within the observation process of Very Long Baseline Interferometry (VLBI) can be referred to as raw data. The raw telescope data represents the initial data stage (Level 0 data) of the VLBI processing chain, consisting of correlation, fringe-fitting, and geodetic/astrometric parameter estimation. Any systematic effects which are compensated and used for parameter estimation within this chain, are present in the raw telescope data streams. The group delay, although the primary geodetic VLBI observable, can be considered to be the most prominent effect. In this publication, we present a new software package implemented in MATLAB that can simulate raw telescope data for VLBI. The software is called VieRDS ( https://github.com/TUW-VieVS/VieRDS ) and features tools to simulate a delay, a delay rate, a phase offset, and a frequency response of arbitrary magnitude for each channel of the telescope data stream. The signal model consists of a radio source component of selectable flux density, a system noise component, and a phase calibration signal. Furthermore, a tool for one and two bit quantization and a module to store the simulated data in VDIF data format is implemented. For the first time, the simulation of a dispersive group delay for a VGOS broadband frequency setup, and the simulation of the characteristic station frequency response of two VGOS telescopes are shown for demonstration purposes. The simulated data can be correlated and fringe-fitted by commonly used VLBI software correlators and fringe-fitting programs. VieRDS is thus an ideal tool for testing hypotheses of adverse observational effects in a controlled environment by deliberately causing these effects and studying the responses in the correlator output. In this article, we focus on the description of the key characteristic of the simulation concept, the digital signal creation, the digital signal processing algorithms, and the software architecture.
Publisher
The Astronomical Society of the Pacific,IOP Publishing