Colleagues, Marc Biesmans' analogy of the observations of SV Sge with RX And brings up some interesting questions. However, for me at least, the analogy does not hold. Marc is not aware of the communications between myself and Gary Poyner. As with RX And, SV Sge has a faint companion that can lead to misidentification. However, the problem with RX And as I recall was that the position of the variable was slightly off and it had faded well below the charts many of us were using. When the AAVSO (Charles Scovil) finally issued a smaller field chart with a much fainter sequence, it became very clear which was RX And and which was the close companion star. In the case of SV Sge, however, Gary and I were well aware of the existence of the 149 companion, long before the message from Marc. The reason for my communication with Gary was over this very issue of identification since the 149 star didn't look right to me. Therefore, the similarity with RX And ends there since we both knew about its existence. I don't think it should be surprising that there is disagreement in such a difficult field. There is also a direct relationship to working near the limits of our instruments and uncertainty. I have no direct problem with Marc pointing out the inconsistencies of the SV Sge data. I saw this myself, and I've seen instances of it in the past and we'll see it in the future. Furthermore, I don't personally have a problem with Marc using this as an attack against my visual observations. I made over 15,000 estimates last year and the probability of a gaff here and there is a certainty owing to the sheer number of observations. Looking at the same fields night after night is also problematic in that a field can become too familiar so a mistake can be repeated time and again. But I've been doing this work far too long and I go by the principle that *every* visual observer should adhere: I report what *I* see. Furthermore, I report it daily -- for the whole astronomical community to see and scrutinize. If I make a mistake, it can be very public. But therein lies the problem. What are other observers to think about this public flogging? This will certainly hurt VSNET since any observer who was thinking of submitting data will now be less inclined. I was already aware that my contributions were not only hindering other observers from participating, but in some cases from observing at all! Perhaps I should now think that the drawbacks of contributing outweigh the benefits. The actual number of participants is now only a select few, so maybe there is something to this. I welcome any comments. Regards, Gene P.S. Our summer monsoon has arrived so my contributions will be at a minimum over the next month.