VSnet folks, Here's a sequence for R Cancri, with stars chosen from the AAVSO (d)-scale chart. N.B. that the chart magnitudes for stars fainter than "81" are substantially in error, being too bright by 0.5 - 0.8 mag. \Brian ******************************************** Photometry of Stars in the Field of R Cancri Name RA (2000) Dec V b-y n spec Remarks HD 69243 8 16 33.8 +11 43 34 10.830 2.031 M7IIIe (1) 6.619 1.465 (2) HD 69365 8 17 07.4 +11 21 04 7.699 0.615 2 K0 (3) .004 .002 HD 69630 8 18 08.3 +11 39 24 8.141 0.034 2 A2 .007 .001 BD+12 1806 8 17 08.2 +12 02 16 9.410 0.723 2 (4) .004 .011 BD+12 1801 8 15 50.7 +12 08 43 10.271 0.280 2 F2 .013 .018 BD+12 1805 8 16 40.1 +11 39 11 10.738 0.165 2 F0 .016 .006 AG+11 0960 8 16 38.8 +11 44 31 11.351 0.329 2 G5 .015 .036 Remarks: (1) R Cnc = HR3248; observation on 28 Mar 1994UT. (2) observation on 31 Oct 1994UT. (3) V = 7.71 (1979 Ann. Tokyo Astron. Obs., 174, 221). (4) GSC 8020-1384.