SPARKESX: Single-dish PARKES data sets for finding the uneXpected -- A data challenge
arXiv:2209.03080 · doi:10.1093/mnras/stac2558
Abstract
New classes of astronomical objects are often discovered serendipitously. The enormous data volumes produced by recent high-time resolution, radio-telescope surveys imply that efficient algorithms are required for a discovery. Such algorithms are usually tuned to detect specific, known sources. Existing data sets therefore likely contain unknown astronomical sources, which will remain undetected unless algorithms are developed that can detect a more diverse range of signals. We present the Single-dish PARKES data challenge for finding the uneXpected (SPARKESX), a compilation of real and simulated high-time resolution observations. SPARKESX comprises three mock surveys from the Parkes "Murriyang" radio telescope. A broad selection of simulated and injected expected signals (such as pulsars, fast radio bursts), poorly characterised signals (plausible flare star signatures) and unknown unknowns are generated for each survey. The goal of this challenge is to aid in the development of new algorithms that can detect a wide-range of source types. We show how successful a typical pipeline based on the standard pulsar search software, PRESTO, is at finding the injected signals. The dataset is publicly available at https://doi.org/10.25919/fd4f-0g20.
Accepted for publication in MNRAS. 18 pages, 8 figures, 4 table
References in corpus (15)
- Array Programming with NumPy
- The NumPy array: a structure for efficient numerical computation
- A bright millisecond radio burst of extragalactic origin
- PSRCHIVE and PSRFITS An Open Approach to Radio Pulsar Data Storage and Analysis
- Fast radio bursts: search sensitivities and completeness
- The SUrvey for Pulsars and Extragalactic Radio Bursts I: Survey Description and Overview
- Discovery of 14 radio pulsars in a survey of the Magellanic Clouds
- Ultra-high-time Resolution Observations of Radio Bursts on AD Leonis
- ASKAP Detection of Periodic and Elliptically Polarized Radio Pulses from UV Ceti
- Discovering the Unexpected in Astronomical Survey Data
- A Search for Technosignatures Around 31 Sun-like Stars with the Green Bank Telescope at 1.15-1.73 GHz
- Detecting Pulsars with Interstellar Scintillation in Variance Images
- Applying saliency-map analysis in searches for pulsars and fast radio bursts
- SETI in 2020
- Detecting Pulsars with Neural Networks: A Proof of Concept