Proto DUNESP First Look at Data Tingjun Yang

  • Slides: 24
Download presentation
Proto. DUNE-SP: First Look at Data Tingjun Yang (Fermilab) LBNC review Oct 15, 2018

Proto. DUNE-SP: First Look at Data Tingjun Yang (Fermilab) LBNC review Oct 15, 2018

What can we learn from Proto. DUNE? DUNE FD Proto. DUNE • Detector Performance

What can we learn from Proto. DUNE? DUNE FD Proto. DUNE • Detector Performance – Signal-to-Noise ratio DQM – Modeling of detector response • LBL Physics Calibration – Electron energy reconstruction – Muon momentum reconstruction • Nucleon Decay Search Reconstruction – Kaon reconstruction • Supernova Neutrino Search – ~10 Me. V electron reconstruction 2 10/15/18 Proto. DUNE-SP: First Look at Data Analysis

The Proto. DUNE SP DRA Organization • DRA – Detector Reconstruction and Analysis •

The Proto. DUNE SP DRA Organization • DRA – Detector Reconstruction and Analysis • DRA Level 1 – overall responsibility on code development and organizing analysis effort - T. Yang (FNAL) - G. Christodoulou (CERN) • DRA Level 2 - Reconstruction – L. Whitehead (CERN) - DQM – M. Potekhin (BNL) - Calibration – M. Mooney (CSU) - Analysis – S. Bordoni (CERN) Weekly meeting on Wednesday 9: 30 am Fermilab time, 4: 30 pm CERN time Mailing list: dune-proto-sp-dra@fnal. gov https: //web. fnal. gov/collaboration/DUNE/Site. Pages/Proto. DUNEs%20 simulation%20 and%20 reconstruction%20 activities. aspx 3 10/15/18 Proto. DUNE-SP: First Look at Data

Proto. DUNE Analysis Goals • Short-term goals – detector performance - Dead channels, noisy

Proto. DUNE Analysis Goals • Short-term goals – detector performance - Dead channels, noisy channels - Noise level, signal to noise ratio - Electron lifetime • Medium-term goals – detector response Information for DUNE physics TDR - d. E/dx of pions, protons, kaons, electrons - Energy and momentum resolutions • Long-term goals – cross sections - Inclusive pion cross section - Exclusive channels – charge exchange, etc. 4 10/15/18 Proto. DUNE-SP: First Look at Data Physics publications

Outline • Results of detector performance - Noise level, signal to noise ratio -

Outline • Results of detector performance - Noise level, signal to noise ratio - Electron lifetime • Preparation for data analysis - Beam-TPC information matching - Sticky code mitigation - Electronics calibration - Space Charge calibration - Muon based calibration - TPC reconstruction - Photon detector analysis • Event displays 5 10/15/18 Proto. DUNE-SP: First Look at Data

Noise level • Noise level - Collection: 3. 5 ADC (500 e) - Induction:

Noise level • Noise level - Collection: 3. 5 ADC (500 e) - Induction: 4. 5 ADC (600 e) • Preliminary results show 99. 7% of 15, 360 channels are alive 6 10/15/18 Proto. DUNE-SP: First Look at Data

Signal-to-noise ratio Beam APA 5 APA 6 APA 4 APA 3 APA 2 APA

Signal-to-noise ratio Beam APA 5 APA 6 APA 4 APA 3 APA 2 APA 1 • Signal to noise ratio from DQM: ~50 in collection channels in all APAs 7 10/15/18 Proto. DUNE-SP: First Look at Data

Electron lifetime Beam APA 5 APA 6 APA 4 APA 3 APA 2 APA

Electron lifetime Beam APA 5 APA 6 APA 4 APA 3 APA 2 APA 1 • Purity monitored by both purity monitors and muons 8 10/15/18 Proto. DUNE-SP: First Look at Data

Outline • Results of detector performance - Noise level, signal to noise ratio -

Outline • Results of detector performance - Noise level, signal to noise ratio - Electron lifetime • Preparation for data analysis - Beam-TPC information matching - Sticky code mitigation - Electronics calibration - Space Charge calibration - Muon based calibration - TPC reconstruction - Photon detector analysis • Event displays 9 10/15/18 Proto. DUNE-SP: First Look at Data

Beamline Information • Beamline information is saved to DIP database at CERN and then

Beamline Information • Beamline information is saved to DIP database at CERN and then copied to IFBeam database at Fermilab. - Save beamline information for online monitoring and offline analysis: particle direction, momentum, PID with Cerenkov Detectors, Time of Flight Measurements. - Matching TPC beam events to tracks in beamline. Mean = 6. 71 Ge. V RMS = 0. 4 Ge. V 8 hrs of data taking at 7 Ge. V. 10 10/15/18 Proto. DUNE-SP: First Look at Data

Sticky Code Mitigation • Sticky code - the 6 LSBs in ADC ASIC was

Sticky Code Mitigation • Sticky code - the 6 LSBs in ADC ASIC was found to be “sticky” around 000000 (0 x 00) or 111111 (0 x 3 F). • Can be mitigated through linear interpolation. • A new method is developed to interpolate through FT. • The current focus is on noise mitigation and deconvolution. 11 10/15/18 Proto. DUNE-SP: First Look at Data

ADC gain and linearity • Using pulser data to measure ADC gain and linearity.

ADC gain and linearity • Using pulser data to measure ADC gain and linearity. • Analysis of a recent pulser run 4565. • Gain variation is ~5% over all channels. 12 10/15/18 Proto. DUNE-SP: First Look at Data

Space Charge Simulation with LAr Flow • We now simulate SCE using the space

Space Charge Simulation with LAr Flow • We now simulate SCE using the space charge density map with LAr flow - first study of LAr flow on SCE • Very different distributions in the two drift volumes • Essential to have data-driven calibration Spatial distortion maps 13 10/15/18 Proto. DUNE-SP: First Look at Data

Detector Calibration with Muons • Similar procedure developed by Micro. Boo. NE: Micro. Boo.

Detector Calibration with Muons • Similar procedure developed by Micro. Boo. NE: Micro. Boo. NE-NOTE 1048 -PUB (2018). d. Q/dx calibration • Tools are developed using MC. • d. Q/dx calibration using throughgoing muons - Remove spatial and temporal variations in detector response - Calibration constants are being uploaded to database by Jon Paley • d. E/dx calibration using stopping muons - Determine absolute energy scale using muon stopping power - More details in DRA meeting next week 14 10/15/18 Proto. DUNE-SP: First Look at Data d. E/dx calibration

Pandora Reconstruction • Pandora pattern recognition algorithms are being optimized for data. Preliminary results

Pandora Reconstruction • Pandora pattern recognition algorithms are being optimized for data. Preliminary results look good. 15 10/15/18 Proto. DUNE-SP: First Look at Data

Photon Detector Analysis • The PDS system is operational: we see both beam particles

Photon Detector Analysis • The PDS system is operational: we see both beam particles and cosmicray muons. • All SSP modules are operational and reading back. • Very few dead/noisy channels. Mean ADC Sum vs. Energy APA 3 Arapuca Mean ADC Sum (x 104) Mean. ADC 5 4, 5 4 3, 5 3 2, 5 2 1, 5 1 0, 5 0 0 16 10/15/18 1 2 3 4 5 6 Beam momentum (Ge. V/c) Proto. DUNE-SP: First Look at Data 7 8

Outline • Results of detector performance - Noise level, signal to noise ratio -

Outline • Results of detector performance - Noise level, signal to noise ratio - Electron lifetime • Preparation for data analysis - Beam-TPC information matching - Sticky code mitigation - Electronics calibration - Space Charge calibration - Muon based calibration - TPC reconstruction - Photon detector analysis • Event displays 17 10/15/18 Proto. DUNE-SP: First Look at Data

Run 5244, Event 10488, 1 Ge. V 18 10/15/18 Proto. DUNE-SP: First Look at

Run 5244, Event 10488, 1 Ge. V 18 10/15/18 Proto. DUNE-SP: First Look at Data

Run 5235, Event 10190, 1 Ge. V 19 10/15/18 Proto. DUNE-SP: First Look at

Run 5235, Event 10190, 1 Ge. V 19 10/15/18 Proto. DUNE-SP: First Look at Data

Run 5240, Event 6656, 1 Ge. V 20 10/15/18 Proto. DUNE-SP: First Look at

Run 5240, Event 6656, 1 Ge. V 20 10/15/18 Proto. DUNE-SP: First Look at Data

Run 5144, Event 47293, 7 Ge. V 21 10/15/18 Proto. DUNE-SP: First Look at

Run 5144, Event 47293, 7 Ge. V 21 10/15/18 Proto. DUNE-SP: First Look at Data

Run 5145, Event 81569, 7 Ge. V 22 10/15/18 Proto. DUNE-SP: First Look at

Run 5145, Event 81569, 7 Ge. V 22 10/15/18 Proto. DUNE-SP: First Look at Data

Run 5203, Event 1290, 7 Ge. V 23 10/15/18 Proto. DUNE-SP: First Look at

Run 5203, Event 1290, 7 Ge. V 23 10/15/18 Proto. DUNE-SP: First Look at Data

Conclusions • The first look at data looks very promising - Very low noise

Conclusions • The first look at data looks very promising - Very low noise level and very high signal-to-noise ratio - Very few dead/bad channels • We are able to reconstruct tracks with just a few tweaks to the reconstruction algorithms. - Current focus is on low level reconstruction • We have developed tools for detector calibration using MC. • More results on calibration and cross sections will arrive. 24 10/15/18 Proto. DUNE-SP: First Look at Data