Abstract

After the first three years of the LHC running, the ATLAS experiment extracted its pixel detector system to refurbish and re-position the optical readout drivers and install a new barrel layer of pixels. The experiment has also taken advantage of this access to install a set of beam monitoring telescopes with pixel sensors, four each in the forward and backward regions. These telescopes are based on chemical vapor deposited (CVD) diamond sensors to survive in this high radiation environment without needing extensive cooling. This paper describes the lessons learned in construction and commissioning of the ATLAS Diamond Beam Monitor (DBM). We show results from the construction quality assurance tests and commissioning performance, including results from cosmic ray running in early 2015.

Highlights

  • The Diamond Beam Monitor (DBM) [1] collects data from the Large Hadron Collider (LHC) collisions inside ATLAS [2]

  • The DBM FE-I4 data is readout as the 15th-stave of the Insertable b-Layer (IBL) [3], and a data stream using the hitbus data is used for luminosity estimates

  • The chip/sensor assemblies are glued to a flexible PCB, and the readout chip is wire bonded to the pads on the PCB

Read more

Summary

Introduction

The Diamond Beam Monitor (DBM) [1] collects data from the LHC collisions inside ATLAS [2]. Each telescope consists of 3 layers of diamond/silicon sensors with FE-I4 readout chips. Each pair of telescopes is connected through a hitbus chip to allow specialized triggering and readout. The DBM FE-I4 data is readout as the 15th-stave of the Insertable b-Layer (IBL) [3], and a data stream using the hitbus data is used for luminosity estimates

Construction and Installation
DBM Layout in the ATLAS Detector
Diamond vs Silicon and Luminosity Measurements
Tuning Modules
Tracking and Luminosity
Conclusion
Full Text
Published version (Free)

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call