*From: *Enrique de Miguel <edmiguel63@xxxxxxxxx
<mailto:edmiguel63@xxxxxxxxx>>
*Date: *13 April 2011 19:16:08 GMT+02:00
*To: *cba-chat@xxxxxxxxxxx <mailto:cba-chat@xxxxxxxxxxx>
*Subject: **BK Lyn*
As Joe pointed out, this star is persistently showing negative
superhumps. Currently peak-to-peak variations are ~0.20 mag,
but they used to be as large as ~0.6 mag 20-30 days ago.
Nice target ......
I've proceeded to calibrate a number of stars in the field of BK Lyn
in the B and V bands. For BK Lyn followers, appropriate values
and comments are given below, along with a DSS chart. Keep
in mind that I'm not a "calibrator" and these values should be
regarded as a guide. The bluest "bright" target in the field (apart
from BK Lyn) is #4 (GSC 2496-0893), with B-V=0.53. This is the one
I'm using as comp star for BK Lyn.
Note that star #9 (GSC 2496-0739) seems to be a (non-catalogued)
variable (details below). Incidentally, this seems to have been
used as comp star in Skillman and Patterson A&A 417, 298 (1993).
Enrique
Calibrating BK Lyn field
#label name V B-V erV erBV
2 GSC 2496-1004 14.950 0.714 0.004 0.005
3 GSC 2496-1453 14.890 0.925 0.004 0.004
4 GSC 2496-0893 13.897 0.533 0.003 0.004
5 GSC 2496-0769 13.991 0.610 0.003 0.004
6 GSC 2496-1173 14.010 0.783 0.001 0.004
7 GSC 2496-1374 14.286 0.672 0.007 0.003
8 GSC 2496-0907 13.529 0.839 0.002 0.006
9 GSC 2496-0739 13.262 0.941 0.006 0.012
10 GSC 2496-1579 14.260 0.773 0.005 0.003
11 GSC 2496-1060 14.852 0.620 0.009 0.008
Comments:
1. Values based on measurements carried out on 4 nights (8, 9, 10, 12
April 2011) under excellent conditions.
2. Errors indicate standard deviations about the mean value
calculated over the 4 nights and do not include errors
associated with the transformation. The latter are less
than 0.012 in B band and less than 0.010 in V band.
3. Star #12 is NSVS 7454553 (pulsating RRab Lyr).
4. The bright star in the SE is WASP-13 (star hosting an exoplanet).
5. Star #9 is a non-catalogued low-amplitude variable star, with peak-
to-peak variations of ~0.06-0.07. The periodicity is still uncertain,
but very likely P=0.741(9) d (if pulsating) or multiples of P if
eclipsing.
6. Nightly values of B-V for BK Lyn show slight variations. For
the 4 calibration nights these values are: 0.025, -0.048, 0.036,
and 0.059, values which are otherwise expected for a target of
this nature. These are instantaneous values and not nightly
averages.