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[vsnet-chat 2287] Re: FASTT, OGLE variable star survey area
- Date: Tue, 07 Sep 1999 16:14:58 +0900
- To: vsnet-chat@kusastro.kyoto-u.ac.jp
- From: Seiichi Yoshida <seiichi@muraoka.info.waseda.ac.jp>
- Subject: [vsnet-chat 2287] Re: FASTT, OGLE variable star survey area
- cc: kenic-k@astroarts.co.jp
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
Dear Dr. Henden,
[vsnet-chat 2199]:
> >Anybody knows where is the survey area of OGLE or
> >FASTT projects?
> For the FASTT SDSS equatorial zones, you can look in
> the Henden/Stone AJ article or download the .tex file at
> http://ftp.nofs.navy.mil/pub/outgoing/aah/fastt1/henden.tab1.tex
> For OGLE, go to either princeton or warsaw and look at
> http://vsnet.astrouw.edu.pl/~ftp/ogle/ogle2/fields.html
> http://vsnet.astro.princeton.edu/~ogle/ogle2/fields.html
Many thanks for your information.
> If the star is identified as a variable in any of these
> publications, then it should not be considered a 'new variable'
> by MISAO.
Yes, one of our new variable stars (MisV objects), MisV0130 is
identified with HS1332 discovered by FASTT. Therefore, the number of
MisV objects is 336 now, but the number of real new objects is 335,
except for MisV0130.
In order to avoid confusion, we will never modify the number. But in
the recent article for IBVS, we mentioned about the identification.
We added all FASTT-1 data into our database. So we will never attach
MisV number for HS objects. Actually, we have discovered the following
variable stars. But we did not announce them as MisV objects because
they are identified with HS objects.
(1)
GSC5128.0947 19 00 09.56 -01 34 57.1 11.05
USNO-A1.0_0825.14018550 19 00 09.508 -01 34 56.99 99.9R 15.3B
IRAS 18575-0139 R.A.=19 00 08.85 Decl.=-01 34 59.5 (20 x 6", p.a.=81) flux(12)=16.14 flux(25)=5.61 flux(60)=1.72 flux(100)=<99.10 98% variable
1999 Apr 14.76013 8.3C
1999 Apr 14.76057 8.3C
1999 May 8.71331 8.3C
1999 May 8.71374 8.3C
1999 Jul 24.51586 9.2C
1999 Jul 24.51653 9.1C
--> HS1466
(2)
USNO-A1.0_0825.14175450 19 02 12.807 -00 44 21.28 12.9R 16.6B
IRAS 18596-0048 R.A.=19 02 12.50 Decl.=-00 44 22.7 (21 x 4", p.a.=81) flux(12)=7.74 flux(25)=4.42 flux(60)=<5.89 flux(100)=<84.67 99% variable
1999 Apr 14.75911 12.8C
1999 Apr 14.75954 12.8C
1999 May 8.71193 13.1C
1999 May 8.71236 13.2C
1999 Jul 24.51391 14.0C
1999 Jul 24.51481 13.8C
--> HS1330
(3)
USNO-A1.0_0825.13934521 18 59 11.277 -01 19 09.83 12.4R 15.9B
IRAS 18565-0123 R.A.=18 59 10.26 Decl.=-01 19 13.6 (42 x 6", p.a.=81) flux(12)=2.48 flux(25)=1.07 flux(60)=<1.06 flux(100)=<63.24 20% variable
1999 May 8.71193 10.0C
1999 May 8.71236 10.0C
1999 Jul 24.51391 11.7C
1999 Jul 24.51481 11.6C
--> HS1463
We found that the star (1) and (3) can be identified with GCVS stars,
VX AQL (=HS1466) and V886 AQL (=HS1463). The identifications were
reported in [vsnet-id 100]. We also write an IBVS article about it soon.
Because we added HS objects into our database, we will report the
magnitude data of them to VSNET after this.
By the way, some HS objects can be identified with known variable
stars in the GCVS. Isn't it a list of NEW variable stars discovered in
the FASTT-1 project?
Best regards,
--
Seiichi Yoshida
seiichi@muraoka.info.waseda.ac.jp
http://vsnet.info.waseda.ac.jp/muraoka/members/seiichi/index.html
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