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[vsnet-alert 5382] (fwd) RXTE observations of YY (DO) Dra
- Date: Sat, 18 Nov 2000 15:10:55 +0900 (JST)
- To: vsnet-alert, vsnet-campaign-ip
- From: Taichi Kato <tkato>
- Subject: [vsnet-alert 5382] (fwd) RXTE observations of YY (DO) Dra
- Sender: owner-vsnet-alert@kusastro.kyoto-u.ac.jp
(fwd) RXTE observations of YY (DO) Dra
From: Koji Mukai <mukai@milkyway.gsfc.nasa.gov>
Subject: RXTE observations of YY (DO) Dra
Date: Fri, 17 Nov 2000 13:45:22 -0500 (EST)
Northern Observers,
We have been granted TOO observation of YY (DO) Dra with the RXTE
satellite during the current outburst, as follows (all times UT).
Nov 19 00:34-01:35
02:14-03:16
03:54-04:51
Nov 20: 00:27-01:28
02:06-03:08
03:47-04:43
22:40-23:42
Nov 21: 00:20-01:22
01:58-03:00
We hope to be able to track the X-ray flux and X-ray spin pulse shapes
in decline (unfortunately, spacecraft safety concerns during the Leonids
have prevented earlier RXTE observations --- but we'll still get good
data).
Dr. Szkody has pointed out that, during the last outburst, X-ray and
optical spin pulses were out of phase. We would therefore like to
request all observers capable of fast photometry to obtain as much
data as weather etc. permit --- this system has a 530 s spin period,
but most of the modulations are at 1/2 the spin period and its orbital
sideband. Simultaneous photometry with RXTE would be particularly
valuable; even if not simultaneous, any data that would allow us to
track the evolution of spin modulation during the outburst decay
would be highly useful.
Best wishes,
Koji Mukai
(mukai@milkyway.gsfc.nasa.gov)
Return to Daisaku Nogami
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