can we effectively flag with minimal time- series available? • Tests: • Insert transients into existing data. • Experiment with new strategies. (Calvelo,) Cendes Figures: Calvelo
widespread use. • Extensive commissioning at ASTRON through this year to date. • Many TKP members participated! • How can we optimise speed and accuracy for transients? van der Horst, Rowlinson
based on “Grid” technologies. • Data storage. • (Re)processing. • TKP (with help from SARA) pioneered the use of NDPPP in the LTA. • Much of the Bell#1 data (Jess’s talk) was flagged/compressed on the Grid.
CEP Cluster Transients Pipeline Calibration LOFAR Stations • Coming soon: LOFAR 2.0. • Flagging on BlueGene? • How long is calibration valid? • GPU imaging? • BlueGene successor? • ...? • We need to provide input!
both for trap and LOFAR imaging. • Historical duplication: PyBDSM, TKP. • Minimal development recently. • Two pronged approach: • Support for ASTRON sourcefinder comparison project. • Renewed discussion/development on TKP specific requirements. • No firm conclusion yet.
promptly to new events. • Astronomer-defined and (post- MSSS) machine learning. • Both cases start by breaking the lightcurve into “features”. • ➜ Major effort post-MSSS. (Coenen, Rol)
LO FA R 1.0 release Call for proposals LO FA R 2.0 freeze LO FA R 2.0 release A A RTFA AC correlator LO FA R 3.0 release System design Initial “trap” U pgraded “trap” Connect to A A RTFA AC pipeline M ining lightcurve archive BlueG ene/P replacem ent approximate dates LO FA R sending VO Events
up for MSSS. • Still a lot of work to make them suitable for real-time operations. • To capitalize on the upcoming LOFAR 2.0 (and beyond), we need to be prepared provide input now.