Visual magnitude estimates by RASNZ members object YYMMDD(UT) mag code remarks APSAG 010122.838 <153 Pea.RASNZ APSDT 010122.836 <152 Pea.RASNZ ARAAT 010122.844 127 Pea.RASNZ Active ARABF 010122.842 <145 Pea.RASNZ ARAFV 010122.840 <153 Pea.RASNZ CAREP 010122.779 <155 Pea.RASNZ CAROY 010122.778 153 Pea.RASNZ CARV436 010122.769 <155 Pea.RASNZ CENMU 010122.801 148 Pea.RASNZ CENUW 010122.809 <150 Pea.RASNZ CENBV 010122.812 131 Pea.RASNZ CENDY 010122.812 130 Pea.RASNZ CENNN 010122.805 <154 Pea.RASNZ CENV359 010122.802 <154 Pea.RASNZ CENV373 010122.800 <153 Pea.RASNZ CENV436 010122.790 <153 Pea.RASNZ CENV442 010122.789 <155 Pea.RASNZ CENV485 010122.803 <154 Pea.RASNZ CENV591 010122.803 <154 Pea.RASNZ CENV803 010122.782 136 Pea.RASNZ Active CENV803 010122.851 136 Pea.RASNZ CETWW 010120.545 139 Pea.RASNZ Active CETWX 010120.546 <159 Pea.RASNZ CHAZ 010122.746 <150 Pea.RASNZ CHARX 010122.780 <155 Pea.RASNZ CHAST 010122.781 132 Pea.RASNZ CMAWZ 010122.757 145 Pea.RASNZ Active CMACG 010122.756 <153 Pea.RASNZ CMAHL 010122.729 137 Pea.RASNZ Active CMISV 010122.730 136 Pea.RASNZ CNCSY 010122.758 136 Pea.RASNZ CNCYZ 010122.731 <142 Pea.RASNZ CNCAK 010122.760 <150 Pea.RASNZ CNCCC 010122.759 <149 Pea.RASNZ COLTV 010122.734 139 Pea.RASNZ CRTTT 010122.783 <154 Pea.RASNZ CRTTU 010122.785 <154 Pea.RASNZ CRUAP 010122.799 <153 Pea.RASNZ CRUBI 010122.807 110 Pea.RASNZ CRUBP 010122.808 110 Pea.RASNZ CRVTV 010122.806 <150 Pea.RASNZ DORRY 010120.675 <155 Pea.RASNZ DORRY 010122.742 <153 Pea.RASNZ ERIXZ 010120.549 <160 Pea.RASNZ ERIAH 010120.550 <155 Pea.RASNZ ERIAQ 010120.551 <156 Pea.RASNZ ERIBF 010120.551 146 Pea.RASNZ ERIEF 010120.549 <158 Pea.RASNZ FORVX 010120.548 <155 Pea.RASNZ HYAAG 010122.775 145 Pea.RASNZ Active HYACT 010122.761 <153 Pea.RASNZ HYAEX 010122.806 128 Pea.RASNZ HYALY 010122.811 <154 Pea.RASNZ HYAMM 010122.775 <155 Pea.RASNZ HYISY 010120.554 123 Pea.RASNZ HYIWX 010120.547 145 Pea.RASNZ HYIBL 010120.553 157 Pea.RASNZ Definitely visible HYIBL 010122.737 <151 Pea.RASNZ HYIVW 010120.674 138 Pea.RASNZ HYIVW 010122.741 138 Pea.RASNZ LEOT 010122.794 <152 Pea.RASNZ LEOX 010122.776 125 Pea.RASNZ Outburst LEORZ 010122.792 <152 Pea.RASNZ LUPBR 010122.817 <152 Pea.RASNZ MENW 010120.556 145 Pea.RASNZ MENW 010122.740 145 Pea.RASNZ MENTU 010120.555 <154 Pea.RASNZ MENTU 010122.738 <153 Pea.RASNZ MENAH 010122.747 127 Pea.RASNZ MUSSY 010122.851 105 Pea.RASNZ MUSSY 010122.851 110 Pea.RASNZ NORAB 010122.819 <152 Pea.RASNZ NORHP 010122.831 134 Pea.RASNZ Active NORIK 010122.832 <148 Pea.RASNZ ORICN 010120.672 132 Pea.RASNZ Active ORIV1159 010120.674 136 Pea.RASNZ Active PICRR 010122.748 121 Pea.RASNZ PICTW 010122.752 151 Pea.RASNZ PUPRX 010122.771 120 Pea.RASNZ PUPUY 010122.762 139 Pea.RASNZ Active PUPBV 010122.765 150 Pea.RASNZ PUPBX 010122.764 138 Pea.RASNZ Active PUPCL 010122.763 <153 Pea.RASNZ PUPV347 010122.750 135 Pea.RASNZ PUPV445 010122.767 95 Pea.RASNZ PUPVV 010122.769 <155 Pea.RASNZ PYXT 010122.771 150 Pea.RASNZ PYXVZ 010122.772 152 Pea.RASNZ SCOMM 010122.846 <145 Pea.RASNZ SCOV478 010122.850 <145 Pea.RASNZ TRAEK 010122.810 <154 Pea.RASNZ TUCVW 010120.553 <152 Pea.RASNZ TUCVW 010122.736 <145 Pea.RASNZ TUCVZ 010120.552 <152 Pea.RASNZ TUCVZ 010122.735 <145 Pea.RASNZ VELBB 010122.770 <153 Pea.RASNZ VELCU 010122.771 <155 Pea.RASNZ VELV382 010122.776 123 Pea.RASNZ VELV383 010122.777 <155 Pea.RASNZ VIRTW 010122.798 143 Pea.RASNZ Active VIRHS 010122.814 <152 Pea.RASNZ VIRHV 010122.816 <150 Pea.RASNZ VOLRX 010122.774 <153 Pea.RASNZ VOLSY 010122.774 <153 Pea.RASNZ NSV 08383 010122.833 <152 Pea.RASNZ LMC V1341 010120.555 <154 Pea.RASNZ LMC V1341 010122.739 <153 Pea.RASNZ LMC V2724 010120.676 145 Pea.RASNZ LMC V2724 010122.744 145 Pea.RASNZ LMC V3434 010122.746 148 Pea.RASNZ EC10565-2858 010122.787 <152 Pea.RASNZ RXJ0640-24 010122.755 <153 Pea.RASNZ RXJ0643-20 010122.753 <153 Pea.RASNZ RXJ1155.4-56 010122.791 119 Pea.RASNZ HD 5980 010120.551 110 Pea.RASNZ HD 5980 010122.735 111 Pea.RASNZ Observer's code: Pea: Andrew Pearce Nedlands,W.Australia 41cm RASNZ Sequence Note: After correspondence with other observers, it appears that my positive observation of AK Cnc was erroneous which does not surprise me due to the difficult conditions at the time. Above positive observation of BL Hyi was made at dark sky site where the star was seen clearly. Again it may be up to 0.5 mags brighter than this because of poor comparision star mags.