Table B.1

All XMM survey-type observations in the XXL fields, integrated with astrometric correction offsets.

(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13) (14)
ObsId FieldName RA Dec MOS1 MOS2 pn Quality Badfield db Cat ΔRA ΔDec Corr
0037980101 XXLn000-01a 35.68970 −3.84966 14.1 14.4 10.0 0 0 X X − 1.072 ± 0.428 − 1.072 ± 0.395 CFHTLS
0037980201 XXLn000-02a 36.02333 −3.85000 13.1 13.3 8.8 0 0 X X − 1.072 ± 0.383 − 0.528 ± 0.381 CFHTLS
0037980301 XXLn000-03a 36.35712 −3.84977 13.4 13.4 9.1 0 0 X X − 0.544 ± 0.421 − 0.528 ± 0.422 CFHTLS
0037980401 XXLn000-04a 36.68933 −3.85002 5.3 4.9 3.6 0 2 X X − 0.528 ± 0.543 0.528 ± 0.687 CFHTLS
0404960101 XXLn000-04b 36.64175 −3.81891 8.9 9.0 3.3 0 2 X X − 1.072 ± 0.635 − 0.528 ± 0.602 CFHTLS
0553910101 XXLn000-04c 36.64454 −3.81438 11.2 11.5 8.6 0 2 X X − 1.072 ± 0.516 − 0.528 ± 0.435 CFHTLS
0037980401 XXLn000-04z 36.64454 −3.81891 25.3 25.4 15.5 0 0 X X − 1.072 ± 0.356 − 0.528 ± 0.386 CFHTLS
0037980501 XXLn000-05a 37.02270 −3.85013 15.9 15.9 11.8 0 0 X X 0.528 ± 0.340 0.000 ± 0.295 CFHTLS
0037980601 XXLn000-06a 35.52316 −3.51672 13.0 13.0 8.8 0 0 X X − 0.528 ± 0.578 − 0.528 ± 0.507 CFHTLS
0037980701 XXLn000-07a 35.85716 −3.51575 12.3 12.3 7.8 0 0 X X − 0.528 ± 0.487 0.528 ± 0.486 CFHTLS

Notes. The full table is available at the CDS, and replaces the one published in XXL Paper I. FieldName is the internal XXL labelling; n(s) stands for the XXL-N (XXL-S) field; a, b, c... tags indicate that the same sky position has been observed several times in different AOs (consult the ESA XMM log using the ESA ObsId)because the quality of earlier pointings was insufficient; the z tag means that a fictitious pointing has been created combining the events of all usable repeated pointings in order to improve the quality. In total there are 542 and 81 a, b, c, and z pointings, respectively. In case of repeated fields, and of overlaps from adjacent fields, the X-ray catalogue will remove overlapping detections, and consider only the one from the better pointing, or, in case of equal quality, the object with the smallest off-axis angle. Columns 5–7 give the remaining exposure (in ks) after selection of the good-time intervals, for the MOS and pn detectors. Quality flag: 0 = good quality; 1 = low exposure; 2 = high background; 3 = 1 and 2. Badfield flag: 0 for best acceptable observation at a given position, 1 for deep/good observation from the archives, not part of XXL proper, 2 other acceptable XXL observation at same position, 3 bad pointings, i.e. quality = 3. This flag is used in the overlap removal procedure. Column 10 is ticked if XAMIN detected at least one object in this pointing. Column 11 is ticked if at least one source in this pointing survived the overlap removal procedure and hence entered the X-ray source catalogue. Columns 12 and 13 (new in this version) report the astrometric offsets (in′′) computed by EPOSCORR and Col. 14 indicates whether the correction was applied, and from which reference catalogue (see Sect. 2.1.3 for details).

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.