Towards a Real-time Transient Classification Engine

TL;DR

This paper discusses the development of a real-time transient classification system for astronomical data, emphasizing the importance of temporal features and standard data formats to enhance understanding of transient phenomena.

Contribution

It introduces a new system for near real-time classification of astronomical transients using time series features and advocates for a standardized data representation format.

Findings

Development of a near real-time classification system

Use of features from time series and static data

Call for community adoption of VOTimeseries standard

Abstract

Temporal sampling does more than add another axis to the vector of observables. Instead, under the recognition that how objects change (and move) in time speaks directly to the physics underlying astronomical phenomena, next-generation wide-field synoptic surveys are poised to revolutionize our understanding of just about anything that goes bump in the night (which is just about everything at some level). Still, even the most ambitious surveys will require targeted spectroscopic follow-up to fill in the physical details of newly discovered transients. We are now building a new system intended to ingest and classify transient phenomena in near real-time from high-throughput imaging data streams. Described herein, the Transient Classification Project at Berkeley will be making use of classification techniques operating on ``features'' extracted from time series and contextual (static) information. We also highlight the need for a community adoption of a standard representation of astronomical time series data (i.e., ``VOTimeseries'').