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This report outlines the detailed steps for the 2021 AFP SiT installation and performance testing, including pedestal tuning, shielding requirements, and readout tests. Need a timeline, checklists, and manpower allocation plan
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AFP@FWD-IB SiT p ALFA ALFA AFP station ALFA ATLAS Roman Pot DetectorsMichael Rijssenbeek ALFA Fiber Detectors ToF AFP ALFA – Beam View AFP – Beam View ALFA Single Diffraction @ Standard Optics Elastics @ β*=2.5 km Optics
AFP 2018 Data Loss • Report written; submitted to FWD Management and IB AFP@FWD-IB
Roman Pots TC • Responsibility (1 FTE): Marko M, Giulio A. AFP@FWD-IB
SiT • Responsibility (1 FTE): Marko M, IFAE: Sebastian G + …, • missing manpower at IFAE • help from pixels? 0.2 FTE consultation from Martin K? • Need detailed step-by-step plan for AFP SiT Installation and Start-up in 2021 • Performance test: pedestal tuning, noisy pixs map, Ileak vs V, Vbreakdown, … • laptop with readout connection for single plane pixel detector • sign-off sheets with results • SiT: height calibration • Final readout test before installation (via LTB-VLDB) • Readout test after pot closing (via LTB-VLDB) • Shielding • EMF shielding of flexes/feedthroughs • Cooling • metal foam HE prototype testing (Jun-Aug 2019) • flange cooling • Checklists AFP@FWD-IB
ToF/ToF Trigger • ToF Responsibility: MR; Olomouc/Bohemia: Tom S, Libor N, Tomas K, Vlada U, Vjaceslav G, …Alberta: Jim P, Paul D. • Manpower OK • Need detailed step-by-step plan for AFP ToF Installation and Start-up in 2021 • PMT long-term HV-in-vacuum test (as is ongoing; need a 2nd PMT!) • PMT Performance test: 1) gain vs. HV, 2) gain vs rate, 3) cross talk • needs fast LED/Laser pulser, dark box (can be done in air) • Electronics Performance test: channel-by-channel gain, noise, resolution (pulser) • needs fast electronics pulser; several output form factors (e.g. like PMT) • sign-off sheets with results • Need a time line (MS Project or similar) • Need Checklists AFP@FWD-IB
TDAQ/DCS TDAQ: • Responsibility (0.5 FTE): IFJ PAN: Krzysztof K, Bartosz D, + …? • manpower OK for now, but need to train new experts • need ~0.5 FTE during run3 DCS: • Responsibility (0.5 FTE): IFJ-PAN:Elzbieta B, Jolanta O; LIP: Luis S. • manpower OK for now • need ~0.5 FTE during run3 AFP@FWD-IB
RC/Trigger/DQ/TB RC: • RC Coordinator (0.1-0.2 FTE): IFJ-PAN: Maciej T • manpower OK now (LS2) • need ~0.3 FTE during run3 Trigger: • TB Coordinator (0.2 FTE): IFJ-PAN: Maciej T; LIP: Patricia C, Nuno C, Tiago V, Ana P? • manpower OK now (LS2) • need ~0.3 FTE during run3 DQ: • DQ Coordinator (0.5 FTE):CTU: Andre S? Olomouc: Karel C? CU: Marek T? IFJ-PAN: Maciej T? • Need detailed step-by-step plan for readiness in 2021 • first version tests on recorded data (?) in Spring 2020? • need ~0.2 FTE during run3 Test Beam (TB): • TB Coordinator (0.3 FTE): Olomouc: Tomas K (Libor N, MR) AFP@FWD-IB
DP, Soft/Sim, Optics, Forward p CP DP: • DP Coordinator (0.2 FTE): AGH-UST: Leszek A, … • manpower OK now (LS2), but need ~0.5 FTE for run3! Soft/Sim: • Soft/SimCoordinator (0.2 FTE): AGH-UST: Leszek A, … • need ~0.2-0.5 FTE in addition Optics: • Optics Coordinator (0.3 FTE): Peter B, Janusz C, Rafal S, Maciej T. • manpower OK now (LS2) Forward Proton Combined Performance: • CP Coordinator (0.3 FTE): Paul N, Rafal S; Hasko S (ALFA). • manpower OK for now: +1 FTE (Lydia B, Jesse L); but could always use more AFP@FWD-IB
Example Checkist Checklist Readout Timing Date/Time ___________ Run#___________ Expert(s):_____________ Beam: Lum_________ Current ___________ BX Pattern___________ RP: Inserted Y / N Comments________________________________ Trigger Type: __________________ DAQ mode: STAA / COMB Current NBX= 1 / 2 / 3 / 4 / 5 BX first_____ BX last_____ SiT: HV________________ Noisy Pixels masked Y / N Comments__________________________________________________________ Timing Scan Results: File___________________ Date/Time ___________ AF AN CN CF P1 _____ _____ _____ _____ P2 _____ _____ _____ _____ P3 _____ _____ _____ _____ P4 _____ _____ _____ _____ Comments__________________________________________________________ ReadoutDelay chosen________ Implemented on Date/Time_________________ Checked: Single bunch B#____________ First & Last bunch in train Bfirst#________ Blast#_________ Comments__________________________________________________________ ELISA Entry #______________ Sign-off Expert:__________________ TC:__________________ AFP@FWD-IB
What Physics with 2017 AFP Data It is even more important now to show physics results (from 2017 data) • Physics with 32 fb–1 of 2017 is the ~same as what could have been done with the full 80 fb–1 • aQGC limits will be a bit worse (2× ?) but still 10× better than with standard methods … • concentrate on the ongoing analyses: • ultra-fast ToF (technical paper) • special low-μ runs: Diffractive studies, DPE di-jets • high-μ runs: exclusive CED μμ; aQGD with exclusive γγ, ZZ, Zγ(and possibly WW) production • new analyses (CED ttbar, CED single top, ...) AFP@FWD-IB
Upcoming Events • 29-30 April: ATLAS Forward Physics Workshop (ALFA-AFP) at CERN • https://indico.cern.ch/event/813544/ • discussion about Data Loss and remedies … • discussion about ToF and ToF performance paper • discussion about Exclusive Di-Muon papers (Performance & Physics) • everyone is strongly encouraged to participate ! • 7 May: ATLAS Weekly • LS2 status - Forward Detectors (Marco B – 15’) • Forward Physics - status and plans (Rafal S or Maciej T – 20’) • 3 June: LHCC Meeting with Forward Physics presentations • FWD, ALFA, and AFP Detector status and Physics • speakers: FWD: Marco B; ARP: MR; Forward Physics: Rafal S • ATLAS Internal rehearsals in mid-May AFP@FWD-IB
Long-term MCP-PMT HV Test in Vacuum p (0-1 bar) Test setup in 180/R-F05 Plan (actual): • Start 16-19 March (19.03.2019 12:17) • operation: • LED pulsing at ~0.1 Hz (actual: 5 Hz) • light yield ~15 p.e./channel? (??) • at STP: • test at 2.5 kV for ~15’ OK • at p=20-40 mbar: (25 mbar) • test at 2.5 kV for ~15’ OK • reduce to 2.2 kV and monitor for ~ 1 month … OK for 5 weeks so far … • at the end, operate PMT at 2.5 kV for ~1 weekNO pulser, just monitoring thermal p.e.s. LeyboldDIAVAC 1000 Screenshot_2019-04-24T12-48-47 DN 40 ISO-K 2×20 k KF25 KF25 KF25 KF25 Oscilloscope nXDS6i Edwards Scroll Pump 0.02 – 1 mbar 10 M 3 kV Reg?? 10 M3 kV 100 M3 kV PAa SHV SHV HV Div 1 nF4 kV 2019-04-24 12:48 BNC/LEMO Pickoff PMTAmp Scaler CAEN N1470 Timer CFD PAb 2-Ch HV PICK-OFF in metal box 36Blue LED • Remote connection & monitoring: • Oscilloscope: http://pool04830003.cern.ch/ • IP webcam: http://128.141.178.108:8080/ AFP@FWD-IB
BackUps AFP@FWD-IB
Publications • AFP ToF Performance in 2017 by Karel Cerny: • Plots (efficiency, time resolution/bar) were approved for public useATL-COM-FWD-2019-002 • next: • finalize the zToF – zVTX distributions for double-tag events; is the rate of ‘signal’ over background as expected? • finalize & approve PUB note (ATL-COM-FWD-2018-027) as CONF or SLIDE • ATLAS Forward Proton Detector Alignment with Exclusive Di-Muon Events by Vlasios and Andre: • Implement comments and finalize the note on CDS ATL-COM-FWD-2019-005 (2017 data) • submit for approval as Performance Plots, and CONF or SLIDE Note • In parallel, continue towards a Physics Note/Paper • 2018 data – first look by Rafal with signal and background simulations! • ALFA 8 TeV Elastics publication (Jorgen & Simon): finalize it in April: • quite good progress – Jorgen is currently performing the many cross checks for the last section of the note • Kick-off of the 900 GeV elastic analysis (ρ, σtot) last week … Tasklist given; needs help with lumi determination once this gets critical AFP@FWD-IB
Run3 Beam Optics • ATLAS & LPC Request on ARP’s opinion on the beam optics (round vs flat; V vs H) • my personal answer: • ALFA has its “own” special optics (β*≲20 m, 3 km) and is not concerned • AFP prefers round optics, i.e. V crossing (VC) plane: • H crossing (HC) worsens the ξ, pT resolution (I think) • irradiation pattern will be flat must shift the detectors vertically during YETS to expose fresh SiT regions • low-mass acceptance is probably a bit smaller • LPC meeting (25 Mar): CMS-PPS said they prefer to keep HC plane in IP5 (narrow vertical acceptance of diamond ToF) ! • We must make our argument to keep VC harder on the timescale of weeks • Plots of round vs flat beam proton hitx,y ellipses at ξ=0.015, 0.020, …, pT=0, 0.3, 1.0 GeV • Pure ξ-acceptance plots using 11σ + 0.5 mm closest beam approach; TCL4/5=20/40σ (?) • Peter B. is working on this; status report this TM ? AFP@FWD-IB
AFP 2018 Data Loss 2 Apr, evening, a 2018 data disaster was reported by Rafal, Maciej, and Kris: wrong BX read out in SiT • high-μ data – no AFP trigger, so 2018 high-μ track data is irretrievably lost • low-μdata – only AFP trigger information • clearly an unmitigated disaster : waste of time, effort, money, lumi, and prestige ! 2-3 Apr Janusz and Marco were informed and they and I informed ATLAS Management on 3 Apr 4 Apr the collaboration was also informed Next steps: • Investigation: How did this escape detection for so long • an investigation by committee will surely be launched • investigate consequences for physics with AFP • Prevention: • design better monitoring (gnam, DQ) to prevent recurrence; shifter protocol • check list procedure after all TDAQ changes • tell “the world” – write a short “report” • in any case, I bear full responsibility for this disaster and submitted my resignation to FWD management AFP@FWD-IB
Timeline (condensed from ~600 entries in MatterMost) Participants: Maciej, Krzysz, Fabian (Chiara, Sune, Elzbieta, Giulio, Bartosz, MR) • Sat, Apr 14, 2018: set up extended readout. STAA. FE tuning in steps of 1/8 BX • Sun, Apr 15, 2018: Collisions Garage. STAA. Change config.sys for SiT with 2017 values. • Mon, Apr 16, 2018: STAA Garage. Finding out tune procedure from Ivan. VLDB tests. Insert 40’: STAA timing scan • Tue, Apr 17, 2018: STAA Coll Garage. Timing scan in garage. 5 BX readout. Some confusion about TiggerLatency/TriggerDelay parameters in STAA and COMB. Noisy pixels and SiT HV. Run COMB Inserted with extended readout. • Wed, Apr 18, 2018: access. Change LTB FS-C. • Thu, Apr 19, 2018: CTP trigger window adjust. Overnight Coll, AFP in garage. • Fri, Apr 20, 2018: Trigger timing adjust (cabling @CTP). Prepare for COMB. Setup TriggerLatency to 100 and 1 BX readout. CollGarage. No check on RO timing. AFP@FWD-IB
Diagnosis • Not enough expertise apart from Krzysz (TDAQ) and Maciej (TC, OnCall) on the SiT FE masking, tuning: only Fabian with some remote help from Ivan. • we lost Joern Lange, Ivan Lopez, Martin Kocian … • I think that Phase II work has taken essential people away from Operations … • Many issues arose at the same time: noisy pixels, HV settings, non working planes, suspected LTB problem (HitBus chip?), trigger rate fluctuations. • Difference between readout tune settings (and their names) for STAA and COMB configs lead to confusion. • Not enough stable beam with pots inserted: need Pots inserted to tune trigger and readout latency; it does not work well in garage … • The various tunings were all intermingled and this leads to confusion of issues. AFP@FWD-IB
Remedy/Prevention • Need new and shadow experts (Trigger, SiT FE, RCE DAQ, gnam, DQ) • Institutes must step up identifying new candidates for TDAQ (1 FTE), SiT (1 FTE), DQ (0.5 FTE) tasks. • More help from Pixel Group? • DQ Task Coordinator needs to be found … • subsistence at CERN can be provided from M&O • Separate the procedures of HV setting & noisy pixel masking, trigger tuning, and readout tuning. • A master “start-up plan” and step-by-step procedures are needed (twiki) • Mandatory checklists for critical tasks (trigger tuning, readout tuning, masking, critical equipment changes in tunnel, …) with sign-off by responsible expert (twiki?) • Need DQ histograms and automated warnings for shifter and On Call • we should demonstrate DQ operation already in LS2 • Weekly run report also at TM with discussion of quality histograms and checklists AFP@FWD-IB
ATLAS Software Development Grants • As announced in the ATLAS Weekly last Tuesday, ATLAS decided to introduce “ATLAS Software Development Grants“ as a measure to mitigate the shortage of developers in critical ATLAS software areas. • ATLAS solicits applications for such positions from members of the ATLAS Collaboration: email Davide.Costanzo and Karl.Jakobs AFP@FWD-IB
To Do List • Start of long-term HV test of potted PMT #2110 in vacuum • ongoing at CERN … • monitor LED pulses, HV current, … • next MCP-PMTs to repair? • Collect BBA data and survey data from 2017-2018 • Budget for LS2 • best split between 2019-2020 • to be presented at April 04 FWD-IB meeting • Planning of Test beam campaigns • ALFA ECR AFP@FWD-IB
ALFA ECR • Marko: modification of ECR almost ready • FLUKA simulation of reduced height (–80 cm) 1st shielding wall by Francesco Cerutti; results in early April • 20 cm high shielding blocks are available(Michael Lazzaroni); replace second block with half-height block … blocked sight lines AFP@FWD-IB
SiT • Requested the SiT work by IFAE as an in-kind M&O contribution (for 2020?) • to be requested by Marco to ATLAS • Work has started by Sebastian, possibly first sensors available by September • Manpower needed to help at IFAE • SiT Cooling: Heat Exchanger upgrade test this Summer AFP@FWD-IB
ToF PMT-in-vacuum: • From Ludo (as chair of ToF Review Committee): • the committee considers the PMT-in-vacuum as the baseline; only if that does not work will they consider the alternative solution. • build and study prototype back-up solution: quartz window effects, behavior of flange and tube, etc. • study heating of PMT-in-vacuum using the current setup, as function of rate • long-term PMT-in-vacuum test was started in 180/R-F05 on 19.03.2019 12:17 – still fine • get #2096 and #2097 long-life MCP-PMTs for repair & potting from Olomouc by end-May picoTDC: • chips still under test at CERN • some issue seen with fine inter-polator: resolution ~10 ps? • more news in ~1-2 months AFP@FWD-IB
PMT #2110: Preparation and Potting • Clean sides of PMT (acetone seems to remove silicone smudges) • Use gloves in all work … • cut ~half the epoxy HV tab with the PC and MCPin lines) • mount PC and MCPin connections: • Axial Lead 50mW 20kΩ resistors • solder PeeWeeleadwire on the cable-side of resistor • drop of silver epoxy 8331-14G on the PMT contact side • PolyUrethane potting … • was done • PMT seems to work under HV and in vacuum (Sept 2018 Beam test) Epoxied resistors PMT in Potting Mold AFP@FWD-IB
Long-Duration Test PHOTONIS MCP-PMT #2110 Tested in STP air: no problems at 2.5 kV (15’) 19.03.2019 12:17 (start): • CAEN HV0=2.2kV, IHV=363μA • Vacuum: p=26mbar(knob=510), T=22°C • LED pulser=–2.0V×15ns, ~5Hz, • PAb: PH0=–1.0V, PH3=–0.9V • HV pick-off: quiet (0.4V,20ns/div) 19.03.2019 14:09 HV0=2.5kV, IHV=416μA; OK 19.03.2019 14:25 HV0=2.2kV, IHV=364μA … HV0=-2.2kV, IHV=363μA pulser -2.0V on 20 ns/div HV0=2.5kV, IHV=416μA pulser off Thanks to Marko and Giulio for crucial help! 4 ns/div AFP@FWD-IB
June Beam Test @ DESY http://testbeam.desy.de • TB22, Mo 24 Jun 8:00 – Mo 31 Jun 8:00 (wk 26) (and TB21, 16-22 Sep (wk 38)) • TB Coordinator: Tomas Komarek; back-up Libor & MR status report at this meeting? • twiki set-up (example https://twiki.cern.ch/twiki/bin/view/Atlas/AFPIntegrationTBNov14) • registration at least 2 weeks in advance ! • safety training Mondays 13:00 in ATLAS Conf. Rm, Bat 1c/room O1.310 (1st floor) • Goals: • To be refined: Q window, HV scans, Hamamatsu vs Photonis, … • Equipment: (Epool) • Trigger counters(?) • Flange, Pot, Vac pump, stand • ?Tracker/telescope + readout? radiation? • fast scope (LecroyWR8104 1GHz 20GS/s or Agilent DSO9254A 2.5 GHz 10/20 GS/s, or TektronicsMSO64 6GHz 25GS/s) • HV and LV PSs • NIM Crate and modules • PAa, PAb, PAc, CFD • ?HPTDC? • cables, laptops, … Low-E e’s check material effects ! AFP@FWD-IB
Estimated ARP Expenditures over LS2 • Estimated for all of LS2 – many cost items can be shifted between 2019 and 2020 (maybe some to 2021) • Divided into ALFA and AFP expenditures as requested by Marco • Divided “reasonably” between 2019 and 2020 (nothing yet to 2021) • Estimated “Manpower at CERN” • NOT including “Common Manpower” (e.g. Giulio), nor Marko ! • Notes: • costs tend only to go up – new items are “discovered” along the way … • should one build in an “unforeseen” or “miscellaneous” for unforeseen costs? • identified items are not all priced with certainty; ultimate costs tend to be different … • “manpower at CERN” (subsistence) is the largest single cost item and should be considered carefully … AFP@FWD-IB
ARP/ALFA Expenditures for LS2 (2019 – 2020) AFP@FWD-IB
AFP Expenditures for LS2 (2019 – 2020) AFP@FWD-IB
Backup AFP@FWD-IB
Conferences & Meetings • Meetings: (http://atlas-project-lumi-fphys.web.cern.ch/atlas-project-lumi-fphys/FWD_SSC/conferences.html) • 20-25 May, 7th Large Hadron Collider Physics Conference, Puebla, Mexico • 09-13 Jun, LHC Forward Physics WG mtg, Dublin. https://indico.cern.ch/event/807740/ • Register for dorm lodging soonest! • 10-14 Jun, RAD2019, Herceg Novi, Montenegro. http://www.rad2019.rad-conference.org • presentation by Marko on ALFA and AFP radiation damage • 17-21 Jun, ANIMMA2019, Portorož, Slovenia. www.animma.com, abst<20Nov • 10-17 Jul, EPS-HEP2019, Ghent, Belgium, http://eps-hep2019.eu/ • 21-30 Aug, New Frontiers in Phys ICNFP 2019, Kolymbari, Crete. https://indico.cern.ch/event/754973/ • 26 Aug – 1 Sep, Low-x 2019 Workshop on DIS, Nicosia, Cyprus. https://indico.cern.ch/event/795601/ • registration open, limited number of registrants … • 05-11 Oct, Acceland Large Exp’l Phys ContrlSysts ICALEPCS2019, New York. https://icalepcs2019.bnl.gov/ AFP@FWD-IB
ToF Ultra-Low Efficiency in 2017 (Review 6 June) Reasons: • PMT life time (≲1 C/cm2) was exceeded: ~3-6 C/cm2 gain deterioration • PMTs gain goal was 5×104: actual gain @2 kV was 1-2×104 CFD threshold inefficiency … • Glue transparency deteriorated by <20% (measurements): expectation for 2018 is same … Cure: • ALD coating = long-life • Gain goal: ~104 high rate capability to ~8 MHz • must measure the PMT gain vs HV (ToT) !! In situ !! • reduce noise/pick-up to ≲10 mV for MIP=~30 mV at PAb out: 08.05 Report by Plzen : 5 mVpp • add 3rd stage amplifier PAc + inverter (need ~10× gain): 08.05 Report by Giulio: OK Note: Log(Gain) is not linear with HV. Also, at low HV, special HV divider ratios apply to maintain p.e. collection eff. In B180 there are 6 PMTs, 3 unknown (1 unmarked, 2 in ToF holders on flanges) AFP@FWD-IB
LS2 Cost Estimates (Feb 2019) AFP@FWD-IB
ALFA Status and Plans for LS2 • Fiber Detector and PMTs will survive until end of Run3 (with shielding in place) • Electronics is expected to (just) survive; prefer 14 TeV large β* run early in Run3 • ALFA Shielding: • alignment in Q5-Q6 requires removal of top two blocks • these will be (partially) re-installed at the end of LS2 … • alignment in Q6-Q7: special procedure using survey wires • ECR LHC-JS-EC-0001 must be changed and re-submitted … • Current detector status: operational (e.g. for 900 GeV run at end-2018) • NO PXI/FESA replacement (only for AFP) – by EP-DT • 2019: Start production of spare Motherboards (no spares left) • ALFA_CTPin input extension, needed to share with CAL-TOPO: software work still needed • 2020: Preventive replacement of all HOME switch optocouplers • Separate LVDT and vacuum pump wires (as was done for AFP) cure LVDT glitches may need to pull new cable … • 2021 Install flow meters • Alignment and commissioning AFP@FWD-IB
AFP Plans for LS2: SiT • Measure SiT efficiency (for Combined FP Performance) • 2017 mostly done (Chiara Grieco); to be documented and completed • 2018 ongoing (Fabian Forster); to be finished in April 2019 • must define what we need and in what form … • New SiT planes for Run3 (16 new needed, + spares): • ~20 good-quality 3D sensors available at IFAE; FE-I4b chips available too • need UBM (@IZM; 5-10kEUR?), dicing, bump-bonding, mounting, wire-bonding to Flex … • (Partial) in-kind contribution by IFAE? • Timeline: production in 2019 (start now); ready by Spring 2020. • Manpower: IFAE (1 person); AFP (Marko M.); Could use help (0.2 FTE / 2 years) AFP@FWD-IB
AFP Plans for LS2: ToF PMT in Potting Mold • Critical: PMT operating at ~2kV in vacuumTwo options: • Improve HV insulation of the PMT: pot ‘bare’ PMTs ourselves • Done for 1 PMT so far: No long-term testing yet … • Pros: no changes w.r.t. current situation • Cons: insulation and long-term testing required • Mount the PMT in air and do the light reception through Q window … • option being designed (help from G. Mladenovic, Belgrade) • Pros: operation in air; exchangeability of PMT; no feedthroughs; … • Cons: changes to Flange, window causes light loss, light spreading, leaks … • Time-line: decision in ~1 month; order PMTs; Production: 2019; Install mid-2020 • Other items: • ToF trigger: digital trigger unit must be thoroughly tested • picoTDC: TDC resolution from 18 ps/channel 3 ps/channel.Is being designed and must be thoroughly tested • Manpower: OK: Alberta, Cracow, Olomouc, Plzen, Prague CU, Stony Brook Anodes MCPout MCPin PC Bare PMT PMT in air to PAb Screw Ring O-rings Flange … PAa PMT Q Window LQ-bars AFP@FWD-IB
AFP Plans for LS2: TDAQ, DCS, Software • Data Preparation: supervising/preparing the AFP data reconstruction • Manpower lacking: 0.2 FTE / 2 years • Soft/Sim: update the AFP detector description for simulations • Full detector simulation • Fast detector simulation • Manpower lacking: 0.5 FTE / 2 years • Forward Proton Combined Performance: • Tools for alignment, calibration, and analysis as discussed above … • Manpower lacking: ~1-2 FTE / 2 years • DAQ: • VLDB testing • Transition to ATCA-RCE-HSIO (firmware/software) • Manpower: OK; but help welcome • DCS: maintenance & upgrades: • LV powering, trigger control, … • Detector conditions from data stream to DCS, … • Manpower: OK • Data Quality: monitoring and alerting • Online monitoring of SiT, ToF, and Trigger efficiencies, Sit distributions, ToF distributions, etc. (gnam software development and maintenance) • Filling DQ histograms and alerting shifter/experts; • Manpower lacking: 0.5 FTE / 2 years AFP@FWD-IB