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[vsnet-obs 44463] CCD observations of 31/03/03



CCD observations of 31 March 2003 / UT
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   030331.718   147CR   MLF  brightened
HYIBL   030403.700   140CR   MLF  
RXSJ0230-6842   030331.720   170CR   MLF
HORWW    030331.72   <180CR   MLF
RXJ025538.2-224655   030331.73   <175CR   MLF   
ERIEF   030331.73   <170CR   MLF
FORVY   030331.727   168CR   MLF
RXSJ0354-1652   030331.73   <170CR   MLF
RXSJ0425-1945   030331.73   <180CR   MLF  
EC04030-5801   030331.735   183CR   MLF
EUVEJ0425-5714   030331.74   <180CR   MLF
COLTX   030331.743   141CR   MLF
PICTW   030331.740   145CR   MLF
PICUW   030331.742   158CR   MLF    bright
PUPVV   030331.753   153CR   MLF    bright
PYXWX   030331.756   165CR   MLF
PYXT   030331.758   153CR   MLF
CARV436   030331.748   146CR   MLF
CAR2   030331.750   155CR   MLF
PUPV516   030331.751   175CR   MLF
PUPV445   030331.75   <185CR   MLF
RXJ0600.5-2709   030331.74   <185CR   MLF
MUSGU   030331.79   <180CR   MLF
MUSGQ   030331.80   <185CR   MLF
VELMR  030331.762   158CR   MLF
HYAMN   030331.79   <185CR   MLF
RXJ1002-1925   030331.789   189:CR   MLF
RXJ1007-2016   030331.786   175CR   MLF
VELV381   030331.79   <180CR   MLF
EC10565-2858   030331.774   145CR   MLF    bright
EC10566-3120   030331.772   154CR   MLF
RXJ105010-140431   030331.780   167CR   MLF
CENV1033   030331.796   165CR   MLF
CENV1025   030331.805   157CR   MLF
CENV834   030331.813   148CR   MLF    bright
RXJ1313.2-3259   030331.802   154CR   MLF
CE-315   030331.808   171CR   MLF
CENV822   030331.817   174CR   MLF
CENV895   030331.812   170CR   MLF
4U1543-62   030331.821   150CR   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).


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