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[vsnet-obs 34771] S obs of 25/07/01



Visual observations of 25 July 2001 
observer: Berto Monard  MLF, Pretoria, South Africa
location: -25 º 54' 48", 28º 26' 44"E
instrument: 32cm /f4.8 Newtonian
conditions: clear and windy
 
VELCU   010725.71   <126   MLF   
VELV383   010725.71   <137   MLF
CRTTU   010725.71   <137   MLF
EC10560-2902   010725.713   144   MLF
EC10565-2858   010725.71   <144   MLF
EC10578-2935   010725.71   <142   MLF
CENV442   010725.71   <137   MLF
CENV436   010725.71   <137   MLF
CENV803   010725.707   140   MLF
RXJ1155.4-5641   010725.71   <140   MLF
RXJ1313.2-3259   010725.71   <148   MLF
CE-315   010725.72   <141   MLF
CENV822   010725.72   <144   MLF
CENV895   010725.72   <146   MLF
4U1543-62   010725.72   <146   MLF
LIBHP   010725.731   137   MLF
LIBGW   010725.73   <143   MLF
LIBAP   010725.730   149   MLF
SCOV893   010725.711   144   MLF
SCOV818   010725.710   122   MLF   still bright
SCOV1033   010725.73   <146   MLF
OPHV2295   010725.73   <145   MLF
OPHV2527   010725.73   <146   MLF
OPHV2400   010725.726   140   MLF 
ARAFV   010725.73   <148   MLF
ARAV877   010725.73   <147   MLF
SGRV4641   010725.734   134   MLF
SGRV1223   010725.734   131   MLF
SGEWZ   010725.772   88   MLF  Tycho II seq / apogee telescope 20x120
SGEWZ   010725.813   86   MLF

CAReta   010725.72   55   MLF  *  RASNZ seq

PKS2005-489   010725.74   132   MLF

* This observation fails to confirm the reported brightness of eta Car. How much does telescope aperture play a rhole in distinguishing the light from the actual star and that of the 'homunculus'. Using the lowest magnification (at 64X) I still see the homunculus separate and its light is not included in the estimate, which only compares the brightness (glare) of eta Car to that of neighbouring stars. 

I also saw Ceres moving near V1223 Sgr.

Kind regards,

Berto Monard 
Pretoria

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