Let's see if this works! I took a look in the Archinal and Hynes book 'Star Clusters' (Willmann-Bell, Inc., 2003) and found a description of the cluster as provided by Archinal: "ARCHINAL 1: This likely cluster is listed here for the first time, having been discovered by one of us, see Figure 4.4 on page 113. It was found rather serendipitously while investigating the identity of Graff 1 (= IC 4756) nearby. When Collinder [1931] gave the reference for the Graff discovery paper [Graff 1922], he incorrectly gave the position (in the paper title) as "18h 50m +5º.5." Assuming this was a 1900.0 position (it turns out it was actually an 1855.0 position) the updated position for 2000.0 (18h 55m +05º.6) was examined on the DSS and a star cluster found there. Later, after checking the correct position in a copy of the actual Graff paper, it was realized that this was a previously uncataloged star cluster, and therefore, a new discovery. The cluster itself contains about 24 stars in an area 1.5' in diameter. There are 4 GSC stars included, the brightest of which is GSC 00457-00629 at magnitude 13.4. The center of the group was taken to be the northern component of GSC 0457-00615 The other two GSC stars are 0457-00095 and 0457-00642. The estimated Trumpler type is II2p. A histogram equalization display of the DSS image in the area shows a possible Milky Way star cloud (or large patch of bright nebulosity?) in an approximately 8' diameter area just to the west of the cluster. No check of the colors or proper motion of these stars has been made, so their existence as a cluster has yet to be proven. However, the appearance in the DSS is more 'cluster-like' than many other groups cataloged as star clusters." Searching for the first GSC star on SkyMap Pro took me right to the 3 brightest GSC stars, and a look at the DSS photograph confirmed a small cluster at that location. Hope that helps. Richard Larimer -- See message header for info on list archives or unsubscribing, and please send personal replies to the author, not the list.