[Message Prev][Message Next][Thread Prev][Thread Next][Message Index][Thread Index]
[vsnet-obs 42824] CCD observations of faint CVs on 2/1/03
- Date: Fri, 03 Jan 2003 09:37:34 +0200
- To: <vsnet-obs@kusastro.kyoto-u.ac.jp>
- From: "Berto Monard" <LAGMonar@csir.co.za>
- Subject: [vsnet-obs 42824] CCD observations of faint CVs on 2/1/03
- Delivered-To: vsnet-obs-archive@ooruri.kusastro.kyoto-u.ac.jp
- Delivered-To: vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
- Delivered-To: vsnet-obs@kusastro.kyoto-u.ac.jp
- Disclaimer: The CSIR exercises no editorial control over E-mail messages and/or attachments thereto/links referred to therein originating in the organisation and the views in this message/attachments thereto are therefore not necessarily those of the CSIR and/or its employees. The sender of this e-mail is, moreover, in terms of the CSIR's Conditions of Service, subject to compliance with the CSIR's internal E-mail and Internet Policy.
- Sender: owner-vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
CCD observations of 02 January 2003
observer: Berto Monard MLF, Pretoria, South Africa
Bronberg observatory / CBA Pretoria
location: -25 º 54' 48", 28º 26' 44"E, altitude 1590m
instrumentation: LX200 12" f/4.2 with ST-7E, unfiltered
conditions: clear
HYIBL 030102.832 169CR MLF
RXSJ0230-6842 030102.835 178CR MLF
SDSSJ015543.0+002807 030102.840 154CR MLF
CETEQ 030102.837 168CR MLF
CET5 030102.838 179CR MLF
RXJ025538.2-224655 030102.842 175CR MLF
ERIEF 030102.844 179CR MLF
FORVY 030102.846 167CR MLF
RXSJ0354-1652 030102.850 171CR MLF
RXSJ0425-1945 030102.852 182CR MLF
PICUW 030102.855 159CR MLF
PYXWX 030102.863 164CR MLF
CARV436 030102.860 143CR MLF
PUPV516 030102.862 181CR MLF
RXJ0600.5-2709 030102.86 <185CR MLF
VELMR 030102.866 159CR MLF
TUCCP 030102.83 <185CR MLF
MCT2347-3144 030102.829 166CR MLF
SCLBW 030102.830 161CR MLF
PICTW from 030102.9 to 030103.05 evolved between 141CR and 151CR
MLF
reported CR magnitudes result from differential photometry to non-red
comparison stars with R magnitudes (directly or derived) from
published
photometric data or traceable to UCAC1 (comparison stars selected from
USNO-A2.0 data on the basis of non-red colour and reliability of the
data).
--
This message has been scanned for viruses and dangerous content by
MailScanner, and is believed to be clean.
"The CSIR exercises no editorial control over E-mail messages and/or
attachments thereto/links referred to therein originating in the
organisation and the views in this message/attachments thereto are
therefore not necessarily those of the CSIR and/or its employees.
The sender of this e-mail is, moreover, in terms of the CSIR's Conditions
of Service, subject to compliance with the CSIR's internal E-mail and
Internet Policy."
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp