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000472776 0247_ $$2arXiv$$aarXiv:2108.02580
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000472776 041__ $$aEnglish
000472776 082__ $$a530
000472776 088__ $$2arXiv$$aarXiv:2108.02580
000472776 1001_ $$0P:(DE-H253)PIP1089041$$aZhu, Sylvia Jiechen$$b0$$eCorresponding author$$udesy
000472776 1112_ $$a37th International Cosmic Ray Conference$$cBerlin$$d2021-07-15 - 2021-07-22$$gICRC 2021$$wGermany
000472776 245__ $$aThe upgraded Data Acquisition System of the H.E.S.S. telescope array
000472776 260__ $$aTrieste$$bSISSA$$c2021
000472776 300__ $$a8
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000472776 4900_ $$2Author
000472776 520__ $$aThe High Energy Stereoscopic System (H.E.S.S.) is an array of five Imaging Atmospheric Cherenkov Telescopes located in the Khomas Highland of Namibia. H.E.S.S. observes gamma rays above tens of GeV by detecting the Cherenkov light that is produced when Very High Energy gamma rays interact with the Earth’s atmosphere. The H.E.S.S. Data Acquisition System (DAQ) coordinates the nightly telescope operations, ensuring that the various components communicate properly and behave as intended. It also provides the interface between the telescopes and the people on shift who guide the operations. The DAQ comprises both the hardware and software, and since the beginning of H.E.S.S., both elements have been continuously adapted to improve the data-taking capabilities of the array and push the limits of what H.E.S.S. is capable of. Most recently, this includes the upgrade of the entire computing cluster hosting the DAQ software, and the accommodation of a new camera on the large 28m H.E.S.S. telescope. We discuss the performance of the upgraded DAQ and the lessons learned from these activities.
000472776 536__ $$0G:(DE-HGF)POF4-613$$a613 - Matter and Radiation from the Universe (POF4-613)$$cPOF4-613$$fPOF IV$$x0
000472776 588__ $$aDataset connected to CrossRef Conference, INSPIRE
000472776 650_7 $$2INSPIRE$$aenergy: high
000472776 650_7 $$2INSPIRE$$aradiation: Cherenkov
000472776 650_7 $$2INSPIRE$$agamma ray: VHE
000472776 650_7 $$2INSPIRE$$aHESS
000472776 650_7 $$2INSPIRE$$adata acquisition
000472776 650_7 $$2INSPIRE$$aprogramming
000472776 650_7 $$2INSPIRE$$aatmosphere
000472776 650_7 $$2INSPIRE$$aupgrade
000472776 650_7 $$2INSPIRE$$aGeV
000472776 650_7 $$2INSPIRE$$aCherenkov counter
000472776 650_7 $$2INSPIRE$$ahardware
000472776 650_7 $$2INSPIRE$$acluster
000472776 650_7 $$2INSPIRE$$aimaging
000472776 650_7 $$2INSPIRE$$ainterface
000472776 650_7 $$2INSPIRE$$aperformance
000472776 693__ $$0EXP:(DE-H253)HESS-20170101$$5EXP:(DE-H253)HESS-20170101$$eHigh Energy Stereoscopic System$$x0
000472776 7001_ $$0P:(DE-H253)PIP1011667$$aMurach, Thomas$$b1$$udesy
000472776 7001_ $$0P:(DE-H253)PIP1021898$$aOhm, Stefan$$b2$$udesy
000472776 7001_ $$0P:(DE-H253)PIP1017273$$aFüssling, Matthias$$b3
000472776 7001_ $$0P:(DE-H253)PIP1032605$$aKrack, Fabian$$b4$$udesy
000472776 7001_ $$aMosshammer, Klemens$$b5
000472776 7001_ $$0P:(DE-H253)PIP1010717$$aLindemann, Rico$$b6$$udesy
000472776 7001_ $$aHolch, Tim Lukas$$b7
000472776 7001_ $$0M.de.Naurois.1$$ade Naurois, Mathieu$$b8
000472776 773__ $$0PERI:(DE-600)2642026-0$$a10.22323/1.395.0759$$p759$$tProceedings of Science / International School for Advanced Studies$$v(ICRC2021)$$x1824-8039$$y2021
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