V1  found in region of high background and likely contaminated; the light 
V1   curve is noisy. 
V2  located five pixels from a very bright star; the resulting bias in the 
V2   photometry might be responsible for the low amplitude of the light curve. 
V3  found in a crowded region. 
V4  it appears to be a blend from visual inspection. 
V5  V5, V6, V7 all found in a crowded region.
V6  V5, V6, V7 all found in a crowded region.
V7  V5, V6, V7 all found in a crowded region.
V8  it appears to be a blend based on visual inspection, possibly resulting in 
V8   a light curve with low amplitude. 
V9  found in a crowded region; the resulting bias in the photometry might be 
V9   responsible for the low amplitude of the light curve. 
V10 V10 and V11: the light variations are not entirely convincing from a visual
V10   inspection; the light curve has small amplitude. 
V11 V10 and V11: the light variations are not entirely convincing from a visual
V11   inspection; the light curve has small amplitude. 
V12 found in a crowded region. 
V13 located 2 pixels away from a bright star. 
V14 found in a crowded region. 
V15 the light variations are not entirely convincing from a visual inspection. 
V16 found in a crowded region; the resulting bias in the photometry might be 
V16  responsible for the low amplitude of the light curve. 
V17 V17-V21: found in a crowded region; the light curve of V20 is symmetric. 
V18 V17-V21: found in a crowded region; the light curve of V20 is symmetric. 
V19 V17-V21: found in a crowded region; the light curve of V20 is symmetric. 
V20 V17-V21: found in a crowded region; the light curve of V20 is symmetric. 
V21 V17-V21: found in a crowded region; the light curve of V20 is symmetric. 
V22 located close to the diffraction spike of a bright star; the light curve 
V22  is noisy. 
V23 it appears to be a blend on visual inspection. 
V24 located 10 pixels away from a bright star; the resulting bias in the 
V24  photometry might be responsible for the symmetric nature of the light curve
V25 found in a crowded region. 
V26 the light variations are not entirely convincing from a visual inspection. 
V27 the light curve appears to be rather symmetric. 
V28 V28-V34: found in a crowded region; the light curves are symmetric 
V28  and/or noisy. 
V29 V28-V34: found in a crowded region; the light curves are symmetric 
V29  and/or noisy. 
V30 V28-V34: found in a crowded region; the light curves are symmetric 
V30  and/or noisy. 
V31 V28-V34: found in a crowded region; the light curves are symmetric 
V31  and/or noisy. 
V32 V28-V34: found in a crowded region; the light curves are symmetric 
V32  and/or noisy. 
V33 V28-V34: found in a crowded region; the light curves are symmetric 
V33  and/or noisy. 
V34 V28-V34: found in a crowded region; the light curves are symmetric 
V34  and/or noisy. 
V35 the light curve appears to be rather symmetric. 
V36  and V37: found in a crowded region; the light curve of V36 is noisy. 
V37  and V36: found in a crowded region; the light curve of V36 is noisy. 
V38 it appears to be a blend on visual inspection. 
V39 V39-V44: found in a crowded region; the light curves are noisy
V39  and/or symmetric. 
V40 V39-V44: found in a crowded region; the light curves are noisy
V40  and/or symmetric. 
V41 V39-V44: found in a crowded region; the light curves are noisy
V41  and/or symmetric. 
V42 V39-V44: found in a crowded region; the light curves are noisy
V42  and/or symmetric. 
V43 V39-V44: found in a crowded region; the light curves are noisy
V43  and/or symmetric. 
V44 V39-V44: found in a crowded region; the light curves are noisy
V44  and/or symmetric. 
V45 the light curve is noisy. 
V46 found in a crowded region. 
V47 it appears to be a blend on visual inspection. 
V48 V48 and V49: found in a crowded region; the light curves are noisy. 
V49 V48 and V49: found in a crowded region; the light curves are noisy. 
V50 the light curve is noisy. 
V51 it appears to be a blend on visual inspection. 
V52 found very close to the edge of the chip; the photometry might be 
V52  contaminated, possibly resulting in the flat minimum of the light curve. 
V53 V53-V56: found in a crowded region; some light curves are noisy 
V53  or symmetric. 
V54 V53-V56: found in a crowded region; some light curves are noisy 
V54  or symmetric. 
V55 V53-V56: found in a crowded region; some light curves are noisy
V55  or symmetric. 
V56 V53-V56: found in a crowded region; some light curves are noisy
V56  or symmetric. 
V57 the light variations are not entirely convincing from a visual inspection. 
V58 found in a crowded region; the light curve has small amplitude. 
V59 the light variations are not entirely convincing from a visual inspection. 
V60 found in a crowded region; the light curve has small amplitude. 
V61 located 4 pixels away from a bright star; the photometry might be 
V61  contaminated, possibly resulting in the small amplitude observed for the 
V61  light curve. 
V62 it appears to be a blend on visual inspection. 
V63 found in a crowded region, the light curve has slow ascent. 
V64 V64 and V65: the light variations are not entirely convincing from a visual
V64  inspection. 
V65 V64 and V65: the light variations are not entirely convincing from a visual
V65  inspection. 
V66 found in a crowded region. 
V67 the light curve has very sparse phase coverage; the nature of the 
V67   variations could not be established. 
V68 V68-V70: found in a crowded region.
V69 V68-V70: found in a crowded region.
V70 V68-V70: found in a crowded region.