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[vsnet-alert 2126] V592 Her CCD photometric run
- Date: Wed, 02 Sep 1998 15:43:51 +0200
- To: vsnet-alert@kusastro.kyoto-u.ac.jp, vsnet-obs@kusastro.kyoto-u.ac.jp
- From: Gianluca Masi <gianmasi@fr.flashnet.it>
- Subject: [vsnet-alert 2126] V592 Her CCD photometric run
- Sender: owner-vsnet-alert@kusastro.kyoto-u.ac.jp
Dear Colleagues,
I attach below a recent photometric run I got on V592 Her. I used these
reference stars:
C1= GSC 1518:1312 RA:16h 30m 48.1s Dec:+21d 20' 37" (2000) mag: 11.6
C2= GSC 1518:1421 RA:16h 31m 13.9s Dec:+21d 20' 45" (2000) mag: 13.0
I'm going to post a light curve at :
http://vsnet.eurolink.it/comets/v592her.gif
Best Regards,
Gianluca Masi
CBA-Italy
--
***********************************************************************
* Gianluca Masi "Two things fill the soul *
* Via Madonna de Loco, 47 with awe and reverence [...]: *
* 03023 Ceccano (FR) the starry sky above me and *
* ITALY the moral law within me" *
* email: gianmasi@fr.flashnet.it *
* http://vsnet.eurolink.it/comets/ I. Kant *
***********************************************************************
Star: V592 Her
Observer: Gianluca Masi, Ceccano (FR) - IT
Telescope: SC 280mm f/6.3
Detector: ** UNFILTERED ** CCD SBIG ST-7 with KAF0400. ABG
Reduction: QMiPS32 and data organization with IDL
JD (UT, 2451057+) V-C1 C1-C2
0.30828717 3.2917595 -1.4948072
0.31006917 3.2835388 -1.4707155
0.31177117 3.2600403 -1.4638042
0.31339117 3.2028837 -1.4840841
0.31498817 3.1514835 -1.4739017
0.31662017 3.2310123 -1.4753675
0.31826417 3.2297497 -1.4869270
0.31988417 3.2073727 -1.4578266
0.32142317 3.2867937 -1.4647675
0.32307917 3.2149916 -1.4849157
0.32473417 3.2222176 -1.4662209
0.32627317 3.2175493 -1.4739532
0.32805517 3.2282906 -1.4500256
0.32957217 3.3307352 -1.4650774
0.33112317 3.3422709 -1.4844227
0.33280117 3.2415428 -1.4673424
0.33444417 3.2207813 -1.4680386
0.33596017 3.1688204 -1.4729052
0.33762717 3.1858501 -1.4792757
0.33915517 3.2352943 -1.4865999
0.34077517 3.2257032 -1.4744167
0.34234917 3.1489668 -1.4907742
0.34387717 3.3567572 -1.4583549
0.34549817 3.3248682 -1.4994297
0.34704817 3.2940197 -1.4716587
0.34864617 3.3012552 -1.4717159
0.35025417 3.3080025 -1.4675426
0.35184017 3.1966381 -1.4692402
0.35341417 3.3340454 -1.4828634
0.35550917 3.2284346 -1.4883690
0.35704817 3.2938490 -1.4592133
0.35871517 3.2682152 -1.4714956
0.36035917 3.1828651 -1.4540691
0.36207217 3.2083673 -1.4676857
0.36384217 3.3223820 -1.4376812
0.36539317 3.3515615 -1.4687376
0.36700217 3.1846914 -1.4557209
0.36878517 3.3050365 -1.4677639
0.37061317 3.3313332 -1.5101566
0.37219917 3.2832985 -1.4626188
0.37378517 3.1758518 -1.4962578
0.37535917 3.1910954 -1.4895039
0.37721017 3.3004408 -1.4843950
0.37875017 3.3124065 -1.4906101
0.38045117 3.2626572 -1.4473352
0.38229217 3.3003521 -1.4610310
0.38392317 3.2311192 -1.5034761
0.38572917 3.2524147 -1.4749355
0.38726817 3.3036489 -1.4506979
0.38885417 3.2567501 -1.4629898
0.39069417 3.3063831 -1.4695787
0.39229217 3.2651310 -1.4911089
0.39397017 3.3000107 -1.4446545
The date is relative to the MID-EXPOSURE.
Add the value reported over the JD column to get the complete JD
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp