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[vsnet-newvar 298] New Bernhard variable (BeV43)
- Date: Tue, 14 Mar 2000 20:01:41 -0800
- To: "dubois@simbad.u-strasbg.fr" <dubois@simbad.u-strasbg.fr>, "gerard@simbad.u-strasbg.fr" <gerard@simbad.u-strasbg.fr>, "samus@sai.msu.ru" <samus@sai.msu.ru>, "vsnet-newvar@kusastro.kyoto-u.ac.jp" <vsnet-newvar@kusastro.kyoto-u.ac.jp>
- From: Klaus Bernhard <klaus.bernhard@vpn.at>
- Subject: [vsnet-newvar 298] New Bernhard variable (BeV43)
- CC: Wolfgang Moschner <wolfgang.moschner@t-online.de>, Herbert Raab <herbert.raab@ris.at>, Chris Lloyd <cl@astro1.bnsc.rl.ac.uk>, Andreas Berthold <andreasberthold@hotmail.com>, "101763.3365@compuserve.com" <101763.3365@compuserve.com>
- Sender: owner-vsnet-newvar@kusastro.kyoto-u.ac.jp
Dear colleagues!
I would like to send you observations of a new variable star (BeV43),
which I have discovered in a systematic CCD-based search for new
variables.
In each observing run typically 400 images are taken of several survey
fields.
The frames are processed automatically.
Instruments:
CCD-camera:Starlight Xpress SX (unfiltered)
Telescope: Celestron-8 (20 cm Schmidt-Cassegrain)
New variable star:
new BeV43 051244.8 +101510 (J2000) 11.9 12.4(CCD)
comments:
BeV43: GSC 702 1892
Comparison star was for all measurements GSC 702 1438 (12.4 mag),
which was checked to be constant.
Data analysis was made by Chris Lloyd, UK. His comment:
There is a strong series of spikes in the periodogram with 1.3034
and 0.10966 being the strongest. It could be almost any type of variable
at this stage.
object YYMMDD(UT) mag (CCD) code
BeV43 000111.8847 11.98 BRH.BAV
BeV43 000124.8618 11.90 BRH.BAV
BeV43 000125.8910 12.43 BRH.BAV
BeV43 000126.8882 12.23 BRH.BAV
BeV43 000204.8285 11.87 BRH.BAV
BeV43 000210.8660 11.92 BRH.BAV
BeV43 000227.8201 11.90 BRH.BAV
Regards,
Klaus Bernhard
Klaus Bernhard
Kafkaweg 5
A-4030 LINZ
AUSTRIA
e-mail:
klaus.bernhard@vpn.at
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