REVIEW 3 cited by
General-Purpose Software for Managing Astronomical Observing Programs in the LSST Era
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
Signed reviews
read the original abstract
Modern astronomical surveys such as the Large Synoptic Sky Survey (LSST) promise an unprecedented wealth of discoveries, delivered in the form of ~10 million alerts of time-variable events per night. Astronomers are faced with the daunting challenge of identifying the most scientifically important events from this flood of data in order to conduct effective and timely follow-up observations. Several ongoing observing programs have proven databases to be extremely valuable in conducting efficient follow-up, particularly when combined with tools to select targets, submit observation requests directly to ground- and space-based facilities (manual, remotely-operated and robotic), handle the resulting data, interface with analysis software and share information with collaborators. We draw on experience from a number of follow-up programs running at LCOGT, all of which have independently developed systems to provide these capabilities, including the Microlensing Key Project (RoboNet, PI: Tsapras, Co-I: Street), the Global Supernovae Project (SNEx, PI: Howell), and the Near-Earth Object Project (NEOExchange, PI: Lister). We refer to these systems in general as Target and Observation Managers, or TOMs. Future projects, facing a much greater and rapidly-growing list of potential targets, will find such tools to be indispensable, but the systems developed to date are highly specialized to the projects they serve and are not designed to scale to the LSST alert rate. We present a project to develop a general-purpose software toolkit that will enable astronomers to easily build TOM systems that they can customize to suit their needs, while a professionally-developed codebase will ensure that the systems are capable of scaling to future programs.
Forward citations
Cited by 3 Pith papers
-
Is the Symbiotic Recurrent Nova T CrB Late? Recent Photometric Evolution and Comparison with Past Pre-Outburst Behaviour
The 2023 decline of T CrB is not a reliable pre-eruption dip, so the nova could erupt soon with little or no photometric warning.
-
Infrastructure and Strategies for Time Domain and MMA and Follow-Up
A community white paper proposing a funded, coordinated follow-up network of brokers, TOMs, schedulers, and data reduction tools for the LSST alert era.
-
New Regimes in the Observation of Core-Collapse Supernovae
A concise expert review of how wide-field surveys and rapid follow-up are opening new observational windows on core-collapse supernovae.
Discussion (0). Continue with ORCID to comment.