# Description of the FITS files

pn.fits			Raw EVT file (0.3-10 keV) of the pn camera. EXPOSURE_TIME=77002.9 s
pn_filt.fits		Cleaned EVT file (0.3-10 keV) of the pn camera, filtered for the background flares. EXPOSURE_TIME=50804.2 s
pn_im_300_1000.fits	pn image of the field in the 0.3-1 keV band
pn_im_500_2000.fits	pn image of the field in the 0.5-2 keV band
pn_im_2000_7000.fits	pn image of the field in the 2-7 keV band
mos1.fits		Raw EVT file (0.3-10 keV) of the MOS1 camera. EXPOSURE_TIME=86227.2 s
mos1_filt.fits		Cleaned EVT file (0.3-10 keV) of the MOS1 camera, filtered for the background flares. EXPOSURE_TIME=70638.8 s
mos1_im_300_1000.fits	MOS1 image of the field in the 0.3-1 keV band
mos1_im_500_2000.fits	MOS1 image of the field in the 0.5-2 keV band
mos1_im_2000_7000.fits	MOS1 image of the field in the 2-7 keV band
mos2.fits		Raw EVT file (0.3-10 keV) of the MOS2 camera. EXPOSURE_TIME=86238.2 s
mos2_filt.fits		Cleaned EVT file (0.3-10 keV) of the MOS2 camera, filtered for the background flares. EXPOSURE_TIME=71017.6 s
mos2_im_300_1000.fits	MOS2 image of the field in the 0.3-1 keV band
mos2_im_500_2000.fits	MOS2 image of the field in the 0.5-2 keV band
mos2_im_2000_7000.fits	MOS2 image of the field in the 2-7 keV band

For further information on the filtering procedure and data reduction please refer to Nanni et al. 2017 (Astronomy & Astrophysics, 603, A128) and to Nanni et al. 2018 (Astronomy & Astrophysics, 614, A121).