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[vsnet-campaign-xray 235] Re: new transient source IGR J18539+0727



Dear all,

I have analyzed my last night (April 22.0 UT) images and blink compared the
combined  unfiltered 9 x 60s and Rc-filtered 4 x 60s frames with DSS2R. No
new objects found within 3 arc minutes radius from the reported IGR
J18539+0727 position. Only the previously reported object is much brighter
in unfiltered frame. 

Refined (USNOA2.0 reference) astrometry:

RA = 18 53 59.82 Decl = +07 25 38.5  (2000.0)  CR=14.3

This is identified to be the infrared source IRAS18515+0721.

The unfiltered frame has limiting magnitude about CR=18.5 and the Rc frame
about R=17.9.
Morning sky was already very light so deeper images were not possible to get
in order to search possibly fainter optical transient.

I have placed also JPEG versions of the combined frames into web:

http://nyrola.jklsirius.fi/ccd/2003/data0421/IGRJ18539+0727C.jpg
http://nyrola.jklsirius.fi/ccd/2003/data0421/IGRJ18539+0727R.jpg

best regards,

arto
--
Arto Oksanen                       mailto:arto.oksanen@jklsirius.fi
Jyvaskylan Sirius ry, Kyllikinkatu 1, FIN-40100 Jyväskylä,  Finland 
Tel. +358-14-4157852, Mobile: +358-40-5659438, Fax: +358-14-4157803
Nyrola Observatory    http://www.ursa.fi/sirius/nytt/nytt_info.html 

-----Original Message-----
From: Taichi Kato [mailto:tkato@kusastro.kyoto-u.ac.jp] 
Sent: 22. huhtikuuta 2003 5:14
To: vsnet-campaign-xray@ooruri.kusastro.kyoto-u.ac.jp
Cc: vsnet-newvar@ooruri.kusastro.kyoto-u.ac.jp
Subject: Ävsnet-campaign-xray 233Å (fwd) Re: new transient source IGR
J18539+0727


Date: Tue, 22 Apr 2003 05:10:59 +0300
From: Arto Oksanen <oksanenÉnyrola.jklsirius.fi>
Subject: Re: new transient source IGR J18539+0727

Photometry of the suspect:

20030422.04 UT CR=14.2 R=16.2 V<17 B<14 

Plate solved combined images:

http://nyrola.jklsirius.fi/ccd/2003/data0421/IGRJ18539+0727V.fit
http://nyrola.jklsirius.fi/ccd/2003/data0421/IGRJ18539+0727R.fit
http://nyrola.jklsirius.fi/ccd/2003/data0421/IGRJ18539+0727C.fit

I have not checked the images for other possible optical transients.


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