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BEGIN:VEVENT
SUMMARY:General discussion
DTSTART;VALUE=DATE-TIME:20230320T170000Z
DTEND;VALUE=DATE-TIME:20230320T173000Z
DTSTAMP;VALUE=DATE-TIME:20261014T004855Z
UID:indico-contribution-3045-20324@indico.ific.uv.es
DESCRIPTION:https://indico.ific.uv.es/event/6923/contributions/20324/
LOCATION:Universe 1001-Primera-1-1-1 - Paterna. Seminario
URL:https://indico.ific.uv.es/event/6923/contributions/20324/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Performance of the trigger system for displaced muons in CMS
DTSTART;VALUE=DATE-TIME:20230320T163000Z
DTEND;VALUE=DATE-TIME:20230320T165000Z
DTSTAMP;VALUE=DATE-TIME:20261014T004855Z
UID:indico-contribution-3045-20246@indico.ific.uv.es
DESCRIPTION:Speakers: Alejandro Soto Rodriguez (University of Oviedo)\nThe
  performance of the HLT and OMTF for displaced muons is presented. In Run3
 \, new HLT paths designed to trigger on displaced muons have been added. I
 n addition to the displaced standalone muon paths that were present in Run
 2\, these new paths are designed to trigger on displaced global muons. Sev
 eral improvements have also been made in the L1 trigger system to identify
  displaced muons. A new algorithm is currently being developed for the OMT
 F\, its preliminary performance is also presented.\n\nhttps://indico.ific.
 uv.es/event/6923/contributions/20246/
LOCATION:Universe 1001-Primera-1-1-1 - Paterna. Seminario
URL:https://indico.ific.uv.es/event/6923/contributions/20246/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Early Run 3 Trigger Menu and Operations in ATLAS
DTSTART;VALUE=DATE-TIME:20230320T160000Z
DTEND;VALUE=DATE-TIME:20230320T162000Z
DTSTAMP;VALUE=DATE-TIME:20261014T004855Z
UID:indico-contribution-3045-20247@indico.ific.uv.es
DESCRIPTION:Speakers: Varsha Senthilkumar (IFIC (CSIC-UV))\nThe online eve
 nt selection in ATLAS takes place in two stages. At the first level trigge
 r (Level-1)\, hardware-based\, custom electronics and information from the
  calorimeters and muon spectrometer are used to select events. At the seco
 nd and final stage\, the High Level Trigger (HLT)\, software-based\, vario
 us object-specific algorithms as required by different analysis groups app
 ly further selections to filter events. The HLT algorithms\, represented a
 s “trigger chains” are collectively known as the “trigger menu”. T
 herefore\, the ATLAS trigger menu encapsulates the selections used by all 
 ATLAS physics analyses and detector studies. This talk covers the trigger 
 menu and its performance in the first year of Run 3 operations. During the
  second long shut down of the LHC (LS2\, 2019-2021)\, various upgrades wer
 e made to the ATLAS trigger system\, including new triggers to optimize th
 e data collection. These upgrades have either been deployed in 2022 or hav
 e been tested to be implemented for data taking in 2023. The upgraded trig
 ger system will be able to cope with the much higher levels of pileup expe
 cted in Run 3\, which reached an average number of interactions per bunch 
 crossing of 40.9 in 2022.\n\nhttps://indico.ific.uv.es/event/6923/contribu
 tions/20247/
LOCATION:Universe 1001-Primera-1-1-1 - Paterna. Seminario
URL:https://indico.ific.uv.es/event/6923/contributions/20247/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Inclusive radiative lines for run 3 in LHCb
DTSTART;VALUE=DATE-TIME:20230320T153000Z
DTEND;VALUE=DATE-TIME:20230320T155000Z
DTSTAMP;VALUE=DATE-TIME:20261014T004855Z
UID:indico-contribution-3045-20289@indico.ific.uv.es
DESCRIPTION:Speakers: Aniol Lobo Salvia (Universitat de Barcelona)\nThe LH
 Cb detector has undergone a large update during Long Shutdown 2 involving 
 both subdetectors and the Trigger and Data acquisition systems. This talk 
 will briefly cover the most important upgrades in the Trigger system and p
 resent how the inclusive radiative lines have been modernized to run optim
 ally in the new conditions.\nEmphasis will be given to:\n - Evolving to a 
 ‘hardware-less’ trigger\n - Use of GPUs for the first stage of the tri
 gger\n - Benefits of running an offline-quality reconstruction in the HLT2
  stage\n - Real time calibration\n - Increased instantaneous luminosity\n 
 - Selective persistence\nand particular to the radiative inclusive lines:\
 n - Inclusive lines: particularities\n - Implementation and optimization\n
  - Performance\n\nhttps://indico.ific.uv.es/event/6923/contributions/20289
 /
LOCATION:Universe 1001-Primera-1-1-1 - Paterna. Seminario
URL:https://indico.ific.uv.es/event/6923/contributions/20289/
END:VEVENT
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