Physics Analysis Dataset for Luminosity Normalization

1. Dataset Based Physics Analysis Elizabeth Gallas Oxford University From TOB Task Forces to Final Dress Rehearsal 11 December 2006 Elizabeth Gallas

2. Outline • Start from the End • Luminosity and cross section • Storing Luminosity • Streaming Test (Ayana) • Online System • Assumptions: • inclusive streaming • What happens at Pt 1/Tier0 • What happens at Tier 1/beyond (Jack,Marjorie) • Comments about Exclusive Streaming • Summary • Conclusion Elizabeth Gallas

3. Who needs luminosity (normalization) ? • We all agree: • For ‘physics’ triggers/analysis, • Some to greater precision than others • Think about ‘other’ cases • Calibration – not written to ‘physics’ stream !?! • Might be Luminosity dependent or • worse: BCID dependent (Beam Crossing) • Calibration – written to ‘physics’ stream ? • Create robust system enabling luminosity normalization for many trigger configurations • Must come with ‘Operations Rules’ to insure the necessary booking is recorded • Robustness should include ability to recover a lower precision luminosity should losses occur Elizabeth Gallas

4. Calculating a Physics Cross Section Elizabeth Gallas

5. Physics and Trigger Cross Sections Where f includes • Trigger efficiency • Reconstruction efficiency Assumes: • physics dataset is composed of a all events recorded satisfying a trigger in a well defined set of Luminosity Blocks (LBNs) • We can measure the trigger cross section for each Luminosity Block Elizabeth Gallas

6. Measuring a Trigger Cross Section Elizabeth Gallas

7. Simple Luminosity DB – 2 Tables Run_LBN Table Run_LBN_Trigger Table Run Number LBN Trigger Name L1_EVENTS L2_EVENTS L3_EVENTS L1_PRESCALE L2_PRESCALE L3_PRESCALE Run Number LBN Start Time End Time Duration (seconds) Luminosity (nb-1) Live Fraction Quality Elizabeth Gallas

8. For the Streaming Test • This is a simple Luminosity Database being implemented for the Streaming Test • For each Run_Number,LBN,Trigger we can calculate: • Trigger_Luminosity = DELIVERED_LUM * LIVE_FRACTION / PRESCALE • Trigger_Cross_Section = L3_EVENTS / Trigger_Luminosity Elizabeth Gallas

9. Lum DB–StreamTest Data Sources • Columns populated from Ayana's log files: • RUN_LBNS.RUN_NUMBER, LBN • RUN_LBN_TRIGGERS.TRIGGER_NAME,L3_ACCEPTS. • Other database columns • Start, End_times, prescales, luminosity ... • populated with 'fake' data based on logical assumptions about what we expect the data to look like, will evolve with the Test. • Placeholders for • Deadtime, Prescales, Level 1,2 Accepts, Data Quality, Duration Elizabeth Gallas

10. Lum Database – Real Data Sources • Online Quantities • Run, LBN, Start, End_time - RC(Run Control) • Live Fraction – Level 1 • EVENTS accepted – HLT or EventLossMonitor • Trigger Configuration • Prescales at Level 1, 2, and 3, Trigger Names • Luminosity system Quantities • Acceptance, efficiency corrected Luminosity • Offline – Store in Conditions Database • Richard Hawkings – Trigger/Physics week (3/11/06) Elizabeth Gallas

11. Conditions DB - basic concepts Application • COOL-based database architecture - data with an interval of validity (IOV) Indexed • COOL IOV (63 bit) can be interpreted as: • Absolute timestamp (e.g. for DCS) • Run/event number (e.g. for calibration) • Run/LB number (possible to implement) • COOL payload defined per ‘folder’ • Ttuple of simple types  1 DB table row • Can also be a reference to external data • Use channels (int, soon string) for multiple instances of data in 1 folder • COOL tags allow multiple data versions • COOL folders organised in a hierarchy • Athena interfaces, replication, … COOL C++, python APIs, specific data model SQL-like C++ API Relational Abstraction Layer (CORAL) Oracle DB MySQL DB SQLite File Frontier web Online, Tier 0/1 Small DB replicas File-based subsets http-based Proxy/cache Elizabeth Gallas

12. What happens at Point 1/Tier 0 • Assume • Run Structure as in Run Structure Report. • An Inclusive Streaming model • Complications of Exclusive model – later… • At Point 1 (ATLAS online): • 5-10 data loggers open/close files on LumiBlock boundaries • lots of small files in byte stream format • At Tier 0, small files combined • Files contain one/more complete LBNs • Ignored in this simple model: • BCID, Stream… dependence Elizabeth Gallas

13. What happens at Tier 1, beyond • Pt 1/ Tier 0 makes files respecting LBN boudaries • Subsequent processing must allow us to collect and track complete data sets for physics analysis in well defined sets of LBNs • Our bookkeeping must track LBNs • By EVENT / TAG (Jack) • By Metadata / File (Marjorie) Elizabeth Gallas

14. “Exclusive Streaming” - Online • Online: • More acCOUNTing • Count events by run / lbn / trigger • AND new index: stream • Smooth online running depends on • Accurate predictions of rates and overlaps • Trigger rates depend on fully operational • Triggers and detectors • Balancing streams • Empty file syndrome (empty or lost?) • Special runs with special prescales require stream balance analysis • How do we keep rates to one stream from exceeding ?? % • How do we keep rates to one stream from dropping < ?% • Heightens importance of predictions of rates / overlaps • As trigger configurations evolve • Prescales • Thresholds Elizabeth Gallas

15. “Exclusive Streaming” - Offline • Offline: • Implications for TAG database (Jack). • Splits trigger samples to different Streams • LBNs - distributed onto 1/more file(sets) • Note: a‘topological’ split, not just random • Complicates: tracking of processing history (parentage) • Should processing for different streams occur at different Tier 1 sites • Successful analysis depends on Grid coherence • Robustness should include ability to recover a lower precision luminosity should losses occur Elizabeth Gallas

16. “Exclusive Streaming” (3) • In an ideal world, might be manageable, but infrastructure will be quite complex and day-to-day situations will conspire to foil the best laid plans • Perhaps after a few ‘months?’ of data taking • but bookkeeping much more complicated • The Streaming Test will not answer: • How the system might be actually (ab)used • But has experience with ‘grid coherence’ Make Rules, lots of Rules. Hope people understand, follow, or they will invent their own tools… Elizabeth Gallas

17. Summary • FACT: A physics event dataset comprised of or related to the complete set of events passing a trigger recorded in an LBN has a corresponding measurable integrated luminosity. • Any dataset which does not DOES NOT • Unless that process cross section can be related to a known process cross section taken in the same interval We measure luminosity in Luminosity Blocks (smallest complete fundamental unit of ATLAS data taking) • Pt 1/ Tier 0 makes files respecting LBN boudaries • Subsequent processing must allow us to collect and track complete data sets for physics analysis in well defined sets of LBNs • Our bookkeeping must track LBNs by • EVENT / TAG (Jack) • Metadata / File (Marjorie) • Data Quality • Naturally indexed by Run/LBN (or Run/LBN range) • Any other index must have a direct relationship to Run/LBN Elizabeth Gallas

18. Conclusion • Required: Robust Operational Model including a Luminosity Block based (or aware) • File management and bookkeeping • Data analyses • Data quality • Detector, trigger, reconstruction • Having it from day 1 • Enables us to debug problems faster • Trigger cross sections are constant • Measuring their rates helps monitor stability • Streaming Models • The devil is in the details – ‘exclusive streaming’ by physics / trigger will • Initially make it difficult to find problems • Be an ongoing challenge to operations and bookkeeping Elizabeth Gallas