Table 1: Fields identified by our ASTROVIRTEL program. The second column gives the exposure time that went into the coaddition (images with very bad PSF or seeing were rejected). Exposure times in parentheses indicate the total exposure time per association as identified by querator.

Target		 Exposure time Image seeing

B08p3		 4900 (5600) 0 $.\!\!^{\prime\prime}$88
B08p2 4900 (5600) 0 $.\!\!^{\prime\prime}$88
B08p1 4500 (5600) 0 $.\!\!^{\prime\prime}$88
B0800 7200 (8300) 0 $.\!\!^{\prime\prime}$88
B08m1 4500 (6000) 0 $.\!\!^{\prime\prime}$88
B08m2 4000 (5800) 0 $.\!\!^{\prime\prime}$88
B08m3 5400 (6000) 0 $.\!\!^{\prime\prime}$96
Pal3 5000 (6120) 1 $.\!\!^{\prime\prime}$0
AM1 7500 (7620) 1 $.\!\!^{\prime\prime}$0
Comparison1 5300 (9300) 0 $.\!\!^{\prime\prime}$97
C04p1 4000 (5600) 0 $.\!\!^{\prime\prime}$88
C04p3 4000 (5600) 0 $.\!\!^{\prime\prime}$83
C04m2 4000 (4800) 0 $.\!\!^{\prime\prime}$85
C04m3 4000 (4800) 0 $.\!\!^{\prime\prime}$85
NGC 300 15 100 ($\approx$25 000) 1 $.\!\!^{\prime\prime}$06
C04p2 4000 (5600) 0 $.\!\!^{\prime\prime}$86
C04m1 4000 (4800) 0 $.\!\!^{\prime\prime}$86
C04m4 4000 (4800) 0 $.\!\!^{\prime\prime}$86
C0400 4800 (5600) 0 $.\!\!^{\prime\prime}$87


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