Fig. 2

Distribution in the sky of the different photometric detections of sub-structures in
the Virgo region. The dotted horizontal line at Dec = −4° represents the rough southern
limit of the SDSS imaging survey. There are also 3 SEGUE imaging stripes that cross
the region at negative declinations as shown by the other dotted lines. Labels
correspond to the following references: N02, Newberg
et al. (2002); V06, Vivas & Zinn
(2006); D06, Duffau et al. (2006);
J08, Jurić et al. (2008); K-A, K-B and K-C,
Keller et al. (2008, 2009); K-VOD, K-VES, K-160 and K-180, Keller (2010). The small squares represent the fields observed by
Jerjen et al. (2013); the one at (RA, Dec)
coincides with the location of Vir
Z (Walsh et al. 2009). The × symbol shows the densest part of the
overdensity as seen in RRLS in the QUEST survey.
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