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Training Session, Tucson

The Pan-STARRS Moving Object Processing System. Training Session, Tucson. Thanks. LSSTC. Introductions. Policies. Tuesday No cell phones, laptops, etc. Wednesday, Thursday, Friday Whatever Parking Passes. Schedule. Tuesday Morning MOPS Overview Tuesday Afternoon

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Training Session, Tucson

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  1. The Pan-STARRS Moving Object Processing System Training Session, Tucson MOPS Training Session, Tucson, AZ

  2. Thanks • LSSTC MOPS Training Session, Tucson, AZ

  3. Introductions MOPS Training Session, Tucson, AZ

  4. Policies • Tuesday • No cell phones, laptops, etc. • Wednesday, Thursday, Friday • Whatever • Parking Passes MOPS Training Session, Tucson, AZ

  5. Schedule • Tuesday Morning • MOPS Overview • Tuesday Afternoon • MOPS Simulation Training • Wednesday, Thursday, Friday • MOPS Simulation running MOPS Training Session, Tucson, AZ

  6. MOPS Collaborating Institutions • Institute for Astronomy (IfA) • Large Synoptic Survey Telescope (LSST) • University of Pisa • Jet Propulsion Lab (JPL) • Carnegie Mellon University, Robotics Institute AUTON Laboratory • Minor Planet Center (MPC) • Spacewatch • University of Helsinki MOPS Training Session, Tucson, AZ

  7. MOUs (existent) • JPLDifferential Orbit Determination & Ephemeris Generation • LSSTTwo year software engineer (Pierfederici) • NEODysIOD and 2-night linking • SpacewatchTargeted follow-up of interesting objects MOPS Training Session, Tucson, AZ

  8. MOUs (in negotiations) • MROTargeted follow-up of interesting objects MOPS Training Session, Tucson, AZ

  9. The MOPS Team (IfA) Larry DenneauSenior Software Engineer Tommy GravJunior Scientific Researcher now at JHU Joe MasieroGraduate Student Robert JedickeMOPS Manager, IfA Specialist MOPS Training Session, Tucson, AZ

  10. The MOPS Team (IfA) Jim HeasleySenior Professor David TholenSenior Professor Richard WainscoatSpecialist, UH Telescope Support, Associate Chair MOPS Training Session, Tucson, AZ

  11. The MOPS Team (extended) Francesco PierfedericiLSST Software Engineer Daniel ChangUH ICS Graduate Student MOPS Training Session, Tucson, AZ

  12. The MOPS Team (External) Steven ChesleyJet Propulson Laboratory Jeremy KubicaCarnegie Mellon Robotics Institute Mikko KaasalainenUniversity of Helsinki Andrea MilaniUniversity of Pisa MOPS Training Session, Tucson, AZ

  13. MOPS Workload Pan-STARRS Management MOPS Training Session, Tucson, AZ

  14. Pan-STARRS Solar System MOPS Training Session, Tucson, AZ

  15. Asteroids • PS4 will find as many asteroids in one lunation as have been identified since the discovery of Ceres in 1801 MOPS Training Session, Tucson, AZ

  16. PS4 & NEOs • Tens of thousands of NEOs MOPS Training Session, Tucson, AZ

  17. PS4 & the Main Belt • 10,000,000 MB objects in ten years MOPS Training Session, Tucson, AZ

  18. PS4 & Comets • Pan-STARRS will find ~10X as many comets per year as all existing surveys • 1,000’s of comets in ten years operation • INTERSTELLAR ! ! ! MOPS Training Session, Tucson, AZ

  19. PS4 & TNOs • ~20,000 TNOs MOPS Training Session, Tucson, AZ

  20. PS4 & Distant Planets Jewitt 2003, ‘Project Pan-STARRS and the Outer Solar System,’ EMP New Plutos320AU New Earths620AU (50AU) New Neptunes1230AU (130AU) New Jupiters2140AU (340AU) MOPS Training Session, Tucson, AZ

  21. PS4 Minor Planet Summary 10,000,000 1,000,000 100,000 Known 10,000 PS 1 Year PS 10 Years 1,000 100 10 1 TNOs Comets Centaurs Main Belt NEO / PHO Companions Other Trojans Jovian Trojans Interstellar Visitors Wide TNO Binaries MOPS Training Session, Tucson, AZ

  22. MOPS Overview • Identify known objects • Discover new objects • Derive observable parameters • Catalogue objects • Enable solar system science MOPS Training Session, Tucson, AZ

  23. Terminology Review: • Single Occurrence Transient = SOT • A detection that is not at the same position as any other known stationary object in the past 30 (TBR) days • High S/N (HSD) Detection • A detection that has a high probability of being a real object (~>5) • Low S/N (LSD) Detection • A detection that has a low probability of being a real object (~>3) • Data Collection = DC = DB = Database • A generalized database MOPS Training Session, Tucson, AZ

  24. Terminology Review: • Observing Cycle = OC • Integer number incrementing @ 0 UT on day closest to full moon • Synthetic Object • An artificial object with orbital and shape parameters • Derived Object • A synthetic or real object and its parameters derived from observations MOPS Training Session, Tucson, AZ

  25. Terminology Review: • Detection (not an SOT) • A statistically significant collection of pixels after image convolution with a shape kernel • Tracklet • A set of 2 detections that may be observations of the same object • Track • A set of 2 tracklets that may be observations of the same object • Orbit • A six parameter representation of the heliocentric path of an object MOPS Training Session, Tucson, AZ

  26. Terminology Review: MOPS Training Session, Tucson, AZ

  27. Terminology Review: Evening Sweet Spot Opposition Morning Sweet Spot MOPS Training Session, Tucson, AZ

  28. MOPS Top Level Design Seamlessly combine existing softwareinto an operational system. MOPS Training Session, Tucson, AZ

  29. MOPS Top Level Design TransientDetections Intra-night Linking Inter-night Linking OrbitDetermination Meta-data SyntheticSolar System Database Identification Attribution Precovery Two-Night Linking Impact RiskAnalysis PublishedObjects GUI Users MPC MOPS Training Session, Tucson, AZ

  30. Stationary Combined Static Transients Moving Transient Detection (IPP) 4 Telescopes + + + MOPS Training Session, Tucson, AZ

  31. Intra-Night Linking (Tracklets) First exposure Second exposure • 250 realdetections / deg2 • 250 false detections / deg2 MOPS Training Session, Tucson, AZ

  32. Attributions Legend Tracklets Known Objects MOPS Training Session, Tucson, AZ

  33. Inter-Night Tracklet Linking (tracks) Legend FirstNight SecondNight ThirdNight FourthNight FifthNight MOPS Training Session, Tucson, AZ

  34. Multiple Hypothesis Testing O(n2) MOPS Training Session, Tucson, AZ

  35. kd-tree solution O(n log n) MOPS Training Session, Tucson, AZ

  36. Initial Orbit Determination Good IOD Bad IOD Legend First Night Second Night Third Night MOPS Training Session, Tucson, AZ

  37. Differential Orbit Determination OD IOD Legend First Night Second Night Third Night MOPS Training Session, Tucson, AZ

  38. Orbit Identification MOPS Training Session, Tucson, AZ

  39. PS1 Review: DRM Surveys DRM = PS1Design Reference Mission MOPS Training Session, Tucson, AZ

  40. PS1 Review: DRM Surveys >61% of time amenable to discovery of solar system objects. Some of the other surveys can also identify solar system objects. MOPS Training Session, Tucson, AZ

  41. PS1 Review: Filters g r i z y MOPS Training Session, Tucson, AZ

  42. PS1 Review: w filter w~g+r+i g r i MOPS Training Session, Tucson, AZ

  43. PS1 Review: Bandpasses MOPS Training Session, Tucson, AZ

  44. PS1 Review: Sensitivities The trailed NEO single exposure sensitivityis equivalent to V=23 in g, r, and i bands. The discovery of ‘tracklets’ is equivalentto a 5 sigma limiting magnitude of V=22.8 MOPS Training Session, Tucson, AZ

  45. PS1 Review: Sky-Plane Tesselation Outside view of the celestial sky tesselated into 6252 fields. Of these fields, 5464 have boresight centers > -30° Declination. The 3° field of view of PS1 with an inscribed hexagon of 5.84 square degrees. The twenty percent overlap from a single tesselation due to the circular field of view. MOPS Training Session, Tucson, AZ

  46. PS1 Review: Sky-Plane Tesselation Outside view of the celestial sky tesselated into 6252 fields. Of these fields, 5464 have boresight centers > -30° Declination. The 3° field of view of PS1 with an inscribed hexagon of 5.84 square degrees. The twenty percent overlap from a single tesselation due to the circular field of view. MOPS Training Session, Tucson, AZ

  47. PS1 Review: Sky-Plane Tesselation Outside view of the celestial sky tesselated into 6252 fields. Of these fields, 5464 have boresight centers > -30° Declination. The 3° field of view of PS1 with an inscribed hexagon of 5.84 square degrees. The twenty percent overlap from a single tesselation due to the circular field of view. MOPS Training Session, Tucson, AZ

  48. Observing Strategy • Every survey mode obtains at least twoimages at each location separated by a Transient Time Interval (15-30 minutes) • serendipitous positions & colours • Solar system survey re-visits each location after 3-6 days • obtain 3-4 nights/month • ~12 day arc MOPS Training Session, Tucson, AZ

  49. PS1 Review: 3p Survey 210 deg = 14 hrs Opposition 15 deg = 1 hr +90 dec Equator -30 dec MOPS Training Session, Tucson, AZ

  50. PS1 Review: 3p Survey MOPS Training Session, Tucson, AZ

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