Published June 1, 2015 | Version v1
Journal article

Micro-source development for XMASS experiment

  • 1. Department of Physics, Sejong University, Seoul 143-747 (Korea, Republic of)
  • 2. Korea Research Institute of Standards and Science, Daejeon 305-340 (Korea, Republic of)
  • 3. Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo, Kashiwa, Chiba 277-8582 (Japan)
  • 4. Kamioka Observatory, Institute for Cosmic Ray Research, The University of Tokyo, Higashi-Mozumi, Kamioka, Hida, Gifu 506-1205 (Japan)

Description

XMASS is a multipurpose liquid-xenon detector that currently aims to directly detect dark matter. In this paper, we describe the fabrication and characterization of reference sources used for the energy calibration and position reconstruction of the present XMASS detector. Several gamma-ray sources were produced in the form of a sealed needle-source. A thin-wall tube with a diameter of approximately 0.2 mm was sealed at both ends, with the 241Am or 57Co source material contained inside. The active region of the source was observed to be 1–2 mm long, close to the tip of the needle. These sources were tested in the XMASS detector, and the results were compared with Monte-Carlo simulations

Availability note (English)

Available from http://dx.doi.org/10.1016/j.nima.2014.11.012

Additional details

Identifiers

DOI
10.1016/j.nima.2014.11.012;
PII
S0168-9002(14)01276-5;

Publishing Information

Journal Title
Nuclear Instruments and Methods in Physics Research. Section A, Accelerators, Spectrometers, Detectors and Associated Equipment
Journal Volume
784
Journal Page Range
p. 499-503
ISSN
0168-9002
CODEN
NIMAER

Conference

Title
15. symposium on radiation measurements and applications
Acronym
SORMA XV
Dates
9-12 Jun 2014
Place
Ann Arbor, MI (United States)

Optional Information

Copyright
Copyright (c) 2014 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.