Table 4: X-ray parameters of targets in XEST (1): Positions and count rates [first ten entries].
XEST Name RA$_{\rm X}$ Dec$_{\rm X}$ Poserr Offset ML $_{\rm det}^a$ Scts $T_{\rm exp}$ Rate Varb
    h m s $\deg\ \ \hbox{$^\prime$ }\ \ \hbox{$^{\prime\prime}$ }$ ( $\hbox{$^{\prime\prime}$ }$) ( $\hbox{$^{\prime\prime}$ }$)     (s) (ct s-1)  
27-115 HBC 352 3 54 29.54 32 03 02.2 1.04 0.89 9395 3832 15 776 0.2429 0
27-000 HBC 353 3 54 30.17 32 03 04.3 0.00 0.00 0 <183 14 469 <0.0127 0
06-005 HBC 358 AB 4 03 49.27 26 10 53.1 1.48 1.22 1073 879 7361 0.1194 0
06-007 HBC 359 4 03 50.82 26 10 53.0 1.46 0.34 2921 1605 7664 0.2094 0
06-059 L1489 IRS 4 04 43.07 26 18 56.3 1.46 0.10 7632 3336 46 853 0.0712 0
20-001 LkCa 1 4 13 14.03 28 19 09.9 1.58 1.71 455 336 7813 0.0430 0
20-005 Anon 1 4 13 27.28 28 16 23.3 1.53 1.64 24658 8299 21 634 0.3836 0
20-000 IRAS 04108+2803 A 4 13 53.29 28 11 23.4 0.00 0.00 0 <26 29 957 <0.0009 0
20-022 IRAS 04108+2803 B 4 13 54.72 28 11 32.2 1.55 0.70 1145 696 30 660 0.0227 1
20-000 2M J04141188+28 4 14 11.88 28 11 53.5 0.00 0.00 0 <54 48 645 <0.0011 0
a Maximum likelihood for detection for XMM-Newton data, CIAO WAVDETECT "Significance'' for Chandra data.
b Variability flag: 0 = no or only low-level variability; 1 = clear flaring, flare intervals removed in spectral fit; 2 = clear flaring observed but flare intervals not removed; 3 = slow decay of flare throughout observation, all data used.

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