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[vsnet-alert 2321] Re: BL2005-489
- Date: Thu, 29 Oct 1998 11:10:16 +0200
- To: observations@aavso.org, vsnet-alert@kusastro.kyoto-u.ac.jp
- From: Berto Monard <lagmonar@csir.co.za>
- Subject: [vsnet-alert 2321] Re: BL2005-489
- Disclaimer: The CSIR exercises no editorial control over E-mail messages originating in the organisation and the views in this message are therefore not necessarily those of the CSIR and/or its employees.
- Sender: owner-vsnet-alert@kusastro.kyoto-u.ac.jp
Hi,
for those interested in monitoring this blazar, I like to share the
sequences I use. They were calibrated against nearby GSPC fields using
USNO-A1.0 as the transfer medium and verified using USNO-A2.0.
In the table are USNO-A1.0 codes for the comparison stars, (2000)
coordinates in RA and DE (in HHMMSS and DDMMSS respectively) and
positions in arcminutes relative to PKS 2005-489.
Code Name : RA / DE (2000) : Pos. relative to PKS : Magn (Berto)
0375-38752207 : 200949-484852 : 4.0' E, 1.0' N : 11.9
0375-38749537 : 200939-484618 : 2.4' E, 3.5' N : 13.5
0375-38745438 : 200923-484459 : 0.4' W, 5.0' N : 12.7
These sequences were sufficient to monitor PKS 2005-489 through its
stages. Hopefully there isn't a variable amongst them...
Regards,
Berto Monard
Pretoria
>>> Ron Remillard <rr@space.mit.edu> 10/28 6:46 PM >>>
X-ray outburst in BL2005-489
The RXTE All Sky Monitor has detected increased X-ray flux
from the BL Lac object 2005-489 (J2000, degrees: 302.3558 -48.8316).
During the interval 1998 Oct 11-28, the flux has been in the range of
4 to 10 mCrab at 2-12 keV, which is a factor of 2 to 3 above the
its typical intensity during 1996-1998. Observations at other
wavelengths are strongly encouraged.
Ron Remillard (rr@space.mit/edu)
for the ASM instrument teams at MIT and GSFC
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