Table 1: Detections of IGR J00291+5934 by the ISDC QLA pipeline, based on ISGRI data from single GPS pointings during INTEGRAL revolutions 0261 (2nd December 2004), 0263 (8th December 2004) and 0264 (11th December 2004). The detected position, angular distance of the source from the spacecraft pointing axis ( $\theta$ ) and 20-60 keV count-rate (F) are shown. The last line shows the detection by JEM-X1 and the 3-10 keV flux. Pointings marked with * are those where the source was not automatically detected and localised manually.
Pointing UTC Start ( $\alpha$ , $\delta$ ) $\theta$ F_20-60

(Rev-ScW) (hh:mm) ( $^{\circ}$ ) ( $^{\circ}$ ) (cps)

0261-2 06:43 (7.26, 59.57) 3.3 $7.5 \pm 0.5$

0261-3 07:23 (7.24, 59.58) 6.7 $6.1 \pm 0.5$

0261-4* 08:03 (7.3, 59.57) 12.2 $7.9 \pm 1.2$

0263-1* 06:31 (7.3, 59.57) 10.2 $5.5 \pm 0.8$

0263-2 07:10 (7.28, 59.58) 6.7 $4.3 \pm 0.5$

0263-3 07:50 (7.27, 59.58) 7.6 $4.6 \pm 0.6$

0263-4* 08:30 (7.3, 59.57) 11.8 $5.3 \pm 1.0$

0264-2* 06:18 (7.28, 59.59 ) 10.4 $1.9 \pm 0.8$

0264-3* 06:58 (7.4, 59.5) 4.6 $2.2 \pm 0.5$

0264-4* 07:38 (7.29, 59.55) 2.3 $2.6 \pm 0.5$

0264-5* 08:18 (7.2, 59.5) 7.9 $2.4 \pm 0.7$

0261-2 06:43 (7.279, 59.568) 3.3 $1.6 \pm 0.2$

**Table 1:** Detections of IGR J00291+5934 by the ISDC QLA pipeline, based on ISGRI data from single GPS pointings during *INTEGRAL* revolutions 0261 (2nd December 2004), 0263 (8th December 2004) and 0264 (11th December 2004). The detected position, angular distance of the source from the spacecraft pointing axis ( $\theta$ ) and 20-60 keV count-rate (F) are shown. The last line shows the detection by JEM-X1 and the 3-10 keV flux. Pointings marked with * are those where the source was not automatically detected and localised manually.
Pointing	UTC Start	( $\alpha$ , $\delta$ )	$\theta$	F_20-60
(Rev-ScW)	(hh:mm)	( $^{\circ}$ )	( $^{\circ}$ )	(cps)
0261-2	06:43	(7.26, 59.57)	3.3	$7.5 \pm 0.5$
0261-3	07:23	(7.24, 59.58)	6.7	$6.1 \pm 0.5$
0261-4*	08:03	(7.3, 59.57)	12.2	$7.9 \pm 1.2$
0263-1*	06:31	(7.3, 59.57)	10.2	$5.5 \pm 0.8$
0263-2	07:10	(7.28, 59.58)	6.7	$4.3 \pm 0.5$
0263-3	07:50	(7.27, 59.58)	7.6	$4.6 \pm 0.6$
0263-4*	08:30	(7.3, 59.57)	11.8	$5.3 \pm 1.0$
0264-2*	06:18	(7.28, 59.59 )	10.4	$1.9 \pm 0.8$
0264-3*	06:58	(7.4, 59.5)	4.6	$2.2 \pm 0.5$
0264-4*	07:38	(7.29, 59.55)	2.3	$2.6 \pm 0.5$
0264-5*	08:18	(7.2, 59.5)	7.9	$2.4 \pm 0.7$
0261-2	06:43	(7.279, 59.568)	3.3	$1.6 \pm 0.2$

Source LaTeX | All tables | In the text

	1 Introduction
	2 Discovery of IGR J00291+5934
	3 Discussion
	References