There are only 3 rules for this observing event:
1. Every member from the proposers must try to observe his/her personal target double.
2. The "observing Period" is from September 15th to September 30th.
3. The observing logs must
be first class. That is, a short comment like "Easy split
at 30x" will not calify as a good Olympic record. Don't be
shy and feel free to describe difficulty on finding the double, tell us
about the spectral class, consult other catalogs, measure it if you
can, describe the coloration and of course, don't forget the ambience!.
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Every Olimpics are used always to show some new technologies, so I must to include here some words about the "Difficulty Index" column in the following table: I've designed a Fuzzy-Logic based (a branch of Artificial Intelligence) system in order to give an index between 1 and 100 that expreses how difficult is to split a double. An index of 1 means it is splittable by virtually every telescope or observing instrument, while an index of 100 means you need a first class telescope, aperture and first class skies. First results with a list of doubles shown to me by Paolo Morini (data from Raffaello Brago) show that a good 4" refractor is able to reach a D.I. of about 85-90. An article I've written about this has been accepted for publication in the Spanish magazine "Tribuna de Astronomia y Universo" in December.
The actual prototype has some limitations: First it works only for doubles with separation bounded between 1.0 and 10 seconds of arc, and second, it needs an improving dealing with stars with a faint primary. Actually it only takes into account separation and difference in magnitude. In the future it will have also into account magnitude of the primary and seeing.
We officially declare opened
this 2000, Olympic doubles celebration.
Luis Argüelles
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| 107
Aquarius |
6" | 5.7 | 6.7 | 23h 46min | -18º 40' |
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Richard Harshaw (USA) |
| STF3050
Andromeda |
1.8" | 6.5 | 6.7 | 23h 59min | +33º 43' |
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Luis Argüelles (Spain, EU) |
| 1
Pegasus |
36" | 4.1 | 8.2 | 21h 22min | +19º 48' |
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Tim Leese (UK, EU) |
| 70
Ophiuchius |
3.9" | 4.3 | 6.2 | 18h 05.5 m | +02º 30' |
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Tom Teague (UK, EU) |
| Theta (17) Sagittae | 11.9"-83" | 6.5 | 9.0 - 7.4 | 20h 10min | +20º 55' |
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Eddy O'connor (Australia) |
| Omicron
Capricornius |
21.9" | 5.9 | 6.7 | 20h 30min | -18º 35' |
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Mary Flanagan (USA) |
| Zeta
Aquarius |
1.9" | 3.65 | 3.85 | 22h 28min | -00º 02' |
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PJ Anway (USA) |
| 4
Vulpecula |
18.9" | 5.16 | 10 | 19h 25.5m | +19º 48' |
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William Schart (USA) |
| HN 84 Sagitta | 28.2" | 6.5 | 8.9 | 19h 39.4m | +16º 34' |
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John Ryan
(Spain) |
| HJ
2940
TYC 2260-167-1 (PPM 65055) (And) |
8.40" | 9.64 | 10.6 | 00h 10m | +30º 14' |
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Chuck Shinn (USA) |
| Struve
2737
(Epsilon Equ) |
9.9" (A-B 0.8") | A/B 5.42 | 7.35 | 20h 59m | +04º 18' |
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Tim Leese (UK, EU) |
| Struve
2523
(Vulpecula) |
6.2" | 7.4 | 7.5 | 19h 27m | +21º 20' |
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Jim Jones (USA) |
| 55 Pisces | 6.5" | 5.4 | 8.7 | 00h 40m | +21º 26' |
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Eddy O'connor (Australia) |
| HJ
882
(Aquila) |
6.8" | 9.5 | 10.4 | 19h 20m | +10º 37' |
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Fco. Manuel Rica (Spain.EU) |
| Otto
Struve 525
(Lyra) |
45.4" | 6 | 7.7 | 18h 55m | +33º 58' |
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Paolo Morini (Italy, EU) |
| Gamma Delfinus | 9.6" | 4.3 | 5.1 | 20h 47m | +16º 07' |
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Illario Melandri
(Italy, EU) |
| h2866
Sagittarius |
22.9"-34.8" | 9.2 | 9.3-9.7 | 19h23min | -18º 00' |
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PJ Anway (USA) |
| Alfa CVn (Cor Caroli) | 19.4" | 2.9 | 5.5 | 12h 56m | +38º 19' |
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PinoBandini (Italy, EU) |
| h5003
(Piazzi 6) |
5.5" | 5.2 | 6.9 | 17h 59m | -30º 15' |
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Mary Flanagan (USA) |
| Alpha Pisces | 1.8" | 3.8 | 4.9 | 02h 02m | +02º 46' |
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Tom Teague (UK, EU) |
| Alpha1+2 Capricorni | 378" | 3.6 | 4.2 | 20h 18.1m | -12º 33' |
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Cristina Cellini
(Italy, EU) |