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July 2003

Overview

This month I found free software for synchronizing my computer's clock with an atomic clock in the US and found a way to determine a site's latitude and longitude using a Ontario & Canadian Government websites.

The MX916 is the imaging camera, with exposures for variable stars of 30 seconds at 2x2 binning (unguided). This month's session notes are below the overview section.

Monthly Statistics, July 2003
Night Imaging
Time (s)
Exposure
Time (s)
#
Targets
#
Exposures
7/14/03 12074 5880 17 196
7/28/03 17849 8670 21 289
7/29/03 2421 1680 3 56
7/30/03 19698 10350 19 345
4 nights 52042
(14.46 hr)
26580
(7.38 hr)
60 886

Session Notes

Mon/Tue, July 14/15, 2003

Session from 23:30 to 03:45. I did variables again with the MX916 and a Johnson V filter:
1 V759 Oph 5 DH Aql 9 RV Aql 13 SS Del
2 BC Oph 6 UU Aql 10 TV Aql 14 AN Peg
3 V1493 Aql 7 RS Aql 11 SY Aql 15 RR Equ
4 FO Aql 8 TU Aql 12 XZ Del 16 SX Cyg
17 EY Cyg

Mon/Tue, July 28/29, 2003

Session from 22:45 to 03:45. I did variables with the MX916 and a Johnson V filter:

1 BC Oph 6 UW Lyr 11 AY Lyr 16 V516 Cyg
2 SV Her 7 EL Lyr 12 EY Cyg 17 EF Peg
3 CY Lyr 8 RS Lyr 13 SX Cyg 18 AN Peg
4 UV Lyr 9 AB Lyr 14 V503 Cyg 19 V368 Peg
5 TY Lyr 10 SU Lyr 15 DG Cyg 20 FF Peg
21 IP Peg

In addition to reporting observations electronically, the AAVSO web site has a "Quick Look" page which allows me to see which stars are not well observed -- these will get higher priority from me in the future.

For example: my "fainter than" observations of V368 Peg are almost two magnitudes fainter than the visual observers'. If I can increase my exposure enough, I may be able to see the star and measure its brightness, further enhancing the value of the observation.

Tue/Wed, July 29/30, 2003

Session from 23:30 to 00:30. I did variables with the MX916 and a Johnson V filter. At 00:24 clouds moved over the sky and ended my session. Only 3 variables were imaged tonight: CY Lyr, RX Lyr, and AY Lyr.

Wed/Thu, July 30/31, 2003

Session from 22:15 to 04:15. I did variables with the MX916 and a Johnson V filter, utilized about 1¼ hours of astronomical twilight, and visited the following variables:
1 V970 Oph 6 V344 Lyr 11 V503 Cyg 16 SW Peg
2 V759 Oph 7 RW Lyr 12 V516 Cyg 17 RT Peg
3 CY Lyr 8 V493 Lyr 13 RR Equ 18 IP Peg
4 AY Lyr 9 ST Lyr 14 EF Peg 19 V368 Peg
5 LL Lyr 10 EY Cyg 15 AS Peg

This morning I found some Internet software from the US National Institute of Standards and Technology which sets my computer's clock accurately (see here). Now my image file datetime stamps will be reasonably accurate!

I was also able to get reasonably accurate latitude & longitude for Winchester Observatory (since I don't have a GPS unit). This involved the following steps:

So now I know that Winchester Observatory is located at 75deg 21' 6" W longitude, 45deg 5' 25" N latitude.