Dear ISN members, the CBAT members, and SNe enthusiasts, I appreciate the efforts of the ISN staff, and at least welcome they continue (even in restricted form) providing images of suspect SNe. 1) Regarding images of suspect SNe on-line: First to mention, I still see no problem with publicly posting possible SNe images (I perfectly agree with Geltner), as long as the ISN staff can reach the server access log to avoid unscrupulous purposes. If it isn't the case, the choice of the new ISN Web feature may be acceptable from the side of regular subscribers. However, it should be noted potential confirmatory observers may not be always on the usual subscription list; such observer may be a visiting astronomer who can spend little time in the annoying process of newly obtaining a password, or who may too remote to access the Web directly (some observatories restrict the internet usage to visiting astronomers). Another solution may be to construct an automatic e-mail responding service. Potentially interested observers are publicly notified of the presence of a new object (using some alert networks, allowing redistribution of messages), if an observer is interested, he or she simply have to send a request e-mail to some specific e-mail address, which then returns some uuencoded image of the object. The sender of the mail can be identified, and the request can be easily logged. Remote observers who have no direct access to the Web can also reach the information. What about this idea? 2) joining form, 3) discovery form: nothing to comment on. 4) ISN mailing lists The idea of creating isn-alert and isn-chat may be appreciated, depending on the philosophy of the ISN. The "emulated" lists, VSNET, have the same nomenclature, but we have a philosophy to make _everything_ open to the public worth notifying. While responsibility to provide adequate follow-up information accompanies those who make alerts (true or false), the same responsibility applies to the public who share and appreciate the information. This is our public (if not shown explicitly) rule. This is the point the ISN proposal seems to be a bit different from the VSNET custom, despite its structural similarity. I think the newly suggested feature may be another option for this kind of mailing lists, but I hope the ISN not to become a "too closed community", from which potential researchers may remain unnotified. I have another fear of the fate of "unconfirmed" suspects, which regretable condition quite easily occurs due to the interference by the Moon, the proximity to the Sun, or by local weather conditions. Even if the objects may have faded beyond the detectability of most amatuer's instruments, there may be a chance more powerful instruments may save. I have seen similar occasions in some novae, which were failed to be confirmed at the time of discovery, but were recovered later by powerful instruments, sometimes even by those who are "chance" astronomers who took the field for other purposes. If the original information was made open at earlier time, these objects might have been followed in more adequate way. The suggested new features of the ISN lists and Web seem to confine such unconfirmed information within the list, which feature may eliminate the possibility of "chance rediscovery" or chance identification (e.g. as a new variable star, or as an unknown minor planet -- researcher of these categories of objects are not always interested in joining SN-dedicated lists). I believe the public availability is essential. If reasons exist to do otherwise, I would recommend the ISN to publish in some manner the record of these unconfirmed objects (or images) for the potential future users. Best regards, Taichi Kato