Version 5 (modified by smm, 13 years ago) (diff)



These tests are aimed at determining how to partition the Object and DIASource tables to support efficient operation of the Association Pipeline (AP). The task of the AP is to take new DIASources produced by the Detection Pipeline (DP), and compare them with everything LSST knows about the sky at that point. This comparison will be used to generate Alerts that LSST and other observatories can use for followup observations, and is also used to bring LSSTs knowledge of the sky up to date.

The current AP design splits processing of a Field-of-View (FOV) into 3 phases. For context, here is a brief summary:

prepare phase
This phase of the AP is in charge of loading information about the sky that falls within (or is in close proximity to) a FOV into memory. We will know the location of a FOV roughly 30 seconds in advance of actual observation, and this phase of the AP will start when this information becomes available. The Object, DIASource, and Alert tables contain the information we will actually be comparing new DIASources against. Of these, Object is the largest, DIASource starts out small but becomes more and more significant towards the end of a release cycle, and Alert is relatively trivial in size.
compare-and-update phase
This phase takes new DIASources (produced by the DP) and performs a distance based match against the contents of Object and DIASource. The results of the match are then used to retrieve historical Alerts for any matched Objects. The results of all these matches and joins are sent out to compute nodes for processing - these compute nodes decide which Objects must be changed (or possibly removed), which DIASources correspond to previously unknown Objects, and which of them are cause for sending out an Alert. At this point, the AP enters its final phase.
The responsibility of this phase is to make sure that changes to Object (inserts, updates, possibly deletes), DIASource (inserts only), and Alert (inserts only) are present on disk. There is some (TODO: what is this number) amount of time during which we are guaranteed not to revisit the same FOV.

Note that LSST has a requirement to send out alerts within 60 seconds of performing an observation. Of the 3 AP phases, only compare-and-update is in the critical timing path. This is illustrated by the following (greatly simplified) diagram:

Association Pipeline Phase Timeline

In this diagram, processing of a FOV starts right after observation, with the image processing pipeline (IPP) which is followed by the DP, and finally the AP. The yellow and red boxes together represent processing which must happen in the 60 second window.

The database tests are currently focused on how to partition Object and DIASource such that the prepare phase is as fast as possible, and on how to perform the distance based crossmatch of the compare-and-update phase. Tests of database updates, inserts, and of how quickly such changes can be moved from in-memory tables to disk based tables will follow.

The tests are currently being performed using the USNO-B catalog as a standin for the Object table. USNO-B contains 1045175763 objects, satsifying the DC2 requirement of simulating LSST operations at 10% scale.


The code for the tests is available here.

Partitioning Approaches


In this approach, e


Performance Results