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[vsnet-chat 2331] Re: GSC1.2 magnitudes near V844 Her
- Date: Fri, 1 Oct 1999 13:33:15 -0700
- To: aavso-discussion@informer2.cis.McMaster.CA, vsnet-chat@kusastro.kyoto-u.ac.jp
- From: aah@nofs.navy.mil
- Subject: [vsnet-chat 2331] Re: GSC1.2 magnitudes near V844 Her
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
Not to keep harping on sequences, but Hazel McGee
mentioned the AAVSO preliminary chart magnitudes.
I quote from Bruce Sumner's sequence notes for V844 Her
but after correcting star 2's magnitude:
"There is a Preliminary AAVSO 'e' chart dated 06/1997, with six PEP(V)
magnitudes included. These magnitudes are from S. Antipin (IBVS 4360).
Five of the magnitudes are common to both sequences:
ID Henden AAVSO Antipin
2 12.310 13.1 13.14
3 12.517 13.8 13.86
4 12.834 14.1 14.10
7 14.083 14.9 14.92
8 14.995 16.2 16.15
Antipin's (and hence the AAVSO) magnitudes are 1 magnitude or more
fainter than those derived here. This results from Antipin's magnitudes
being misinterpreted as V magnitudes, when it fact they are photographic
magnitudes derived from photographic plates taken in Crimea and now in
the Moscow plate collection. In actual fact Antipin's magnitudes are
closely related to B magnitudes."
Arne
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