Data Acquisition Architecture and Online Processing System for the HAWC gamma-ray observatory
HAWC collaboration: A. U. Abeysekara, R. Alfaro, C. Alvarez, J. D., \'Alvarez, R. Arceo, J. C. Arteaga-Vel\'azquez, H. A. Ayala Solares, A. S., Barber, B. M. Baughman, N. Bautista-Elivar, J. Becerra Gonzalez, E., Belmont-Moreno, S. Y. BenZvi, D. Berley, M. Bonilla Rosales

TL;DR
This paper describes the design and implementation of a data acquisition and real-time processing system for the HAWC gamma-ray observatory, enabling efficient handling of high-volume data for TeV gamma-ray astronomy.
Contribution
It introduces a novel high-throughput data acquisition architecture and a real-time processing system using off-the-shelf hardware and open-source software for the HAWC observatory.
Findings
System produces ~500 MB/s raw data
Real-time analysis with <5 seconds latency
Flexible software framework for multiple algorithms
Abstract
The High Altitude Water Cherenkov observatory (HAWC) is an air shower array devised for TeV gamma-ray astronomy. HAWC is located at an altitude of 4100 m a.s.l. in Sierra Negra, Mexico. HAWC consists of 300 Water Cherenkov Detectors, each instrumented with 4 photomultiplier tubes (PMTs). HAWC re-uses the Front-End Boards from the Milagro experiment to receive the PMT signals. These boards are used in combination with Time to Digital Converters (TDCs) to record the time and the amount of light in each PMT hit (light flash). A set of VME TDC modules (128 channels each) is operated in a continuous (dead time free) mode. The TDCs are read out via the VME bus by Single-Board Computers (SBCs), which in turn are connected to a gigabit Ethernet network. The complete system produces ~ 500 MB/s of raw data. A high-throughput data processing system has been designed and built to enable real-time…
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