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2. The WATCH experiment

Four monitors WATCH (Lund 1986), designed at the Danish Space Research Institute, are mounted on board the orbital observatory GRANAT. The field of view of a monitor is a circle 74tex2html_wrap1133 radius. The scintillation detector is made of alternating stripes of NaI and CsI. The full geometrical area of the detector is 47 cm2. The effective area of the detector is dependent on the incident angle of the arriving photons as shown in Fig. 1 (click here): at small angles it declines as a cosine, starting at tex2html_wrap_inline1113tex2html_wrap1133 more steeply, and for a source 65tex2html_wrap1133 off-axis it is one fourth of that for an on-axis source. The fields of view of the four instruments cover different quarters of the sky and partially overlap. Because at the very beginning of the experiment one of the monitors went out of order, tex2html_wrap_inline1119% of the sky can be simultaneously viewed under most favourable conditions. The performance of the WATCH instrument is based on the rotation modulation collimator principle. A point source, provided it is bright enough for at least one rotation of the modulation collimator (tex2html_wrap_inline1121 s), can be localized with an accuracy of tex2html_wrap_inline1123 arcmin (at the tex2html_wrap_inline1069 confidence level), where n10 is the source signal in units of 10 standard deviations (Brandt 1994). The detector count rate is recorded in two energy bands, the boundaries of which were reset several times during the mission and roughly correspond to 8-20 keV and 20-60 keV.

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Figure 1: Detector efficiency as a function of source off-axis angle (same for both WATCH energy bands)



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