Dear Chris: I and my co-authors are confused by the second report from the referee. The comments in his first report helped us to improve the presentation of the paper significantly, we really appreciate that. In the second report, he completely mis-understood us. I trust that the referee did a careful job in going through literatures to prove that the delayed filament eruption is not a new result. Unfortunately, he only came out with the Svestka book that was published over 30 years ago. We studied the Svestka book carefully, found that it has not relevance to our study. The book talked about a curved neutral line for a single event, while our event clearly has two eruption cenetrs. We therefore request a review by a second refree. We do not see that we can improve the paper further based on this report, can you send the current version to the second referee? We give our response to each of the comments below. In addition, I attach a TRACE 195A movie for you and the new referee. Two eruption centers are evident. "The term 'delayed filament eruption' is misleading for the presented observation. A flare starts at places A,B with ribbon motions (Fig. 2). A second single ribbon is traced in Fig. 2 (and not a pair as written in the abstract) at another site along a strongly curved neutral line, and later." Reply: The 2nd flare can be seen as another PAIR of ribbons, not a single one. Fig.2 only plots one because another one is not very clear, embedding in the already-brightened first flare ribbon. TRACE movie shows this pair. "Such observations are not new (as several times claimed in the text). It is a piecewise filament eruption, propagating with its onset, along a (here curved) neutral line, compare, e.g. Svestka, Solar Flares. Reidel 1976, p. 46, Fig. 22. It seems to me that much related findings are already described in the Chapter II.E of this old but still useful book. The absence of an observed filament between A and B is no problem (see also page 43 above Fig. 20a in Svestka) the nicely correlated ribbon expansion reveals that there is a dynamic flare ongoing between A and B. The ribbon evolution is influenced by flux concentrations which decelerate or stop the ribbon motion (see Svestka, same chapter). That seems to happen at 19:30 UT: the radio data in Fig. 2 show a fine peak at 19:30 UT, directly in the time interval of Figs. 1 and 3. This remains completely uncommented in the manuscript despite of rough coincidence with the kink in the 1a,1b positions. We trust that the referee did a careful job in going through literatures to prove that the delayed filament eruption is not a new result. Unfortunately, he only came out with a book chapter that was published over 30 years. We studied the Svestka book carefully, found that it has not relevance to our study. The book talked about a curved neutral line for a single event, while our event clearly has two eruption centers. The attached mpeg TRACE 195A movie demonstrates these two centers clearly, as well as the eruption of filament is related to heating of a hot loop. All Svestka discussed is the dynamics of separating ribbons along a curved neutral line. "The whole discussion would be on a much safer ground if the ribbon evolution would be carefully compared with the magnetic flux distribution. I recomnmend the authors to do it (MDI)." Reply This is not relavent to the main conclusion of the paper. "I am surprised about an evident discrepancy in the Summary and Discussion. Here the authors suggest a magnetic connection AD and BC as a start configuration for the flare (if I understood correctly the third sentence before the end). On the other hand, they show in Fig. 2 that A and B have associated ribbon motion. Moreover, the authors claim to have seen the flare core between A and B (Figs. 1 and 5). So: what is true? I can not see in the paper that the authors have much argument for the discussion with regard to the points C and D. The whole discussion of the loop brightening near the later destabilized filament F and references to ongoing reconnection is vague, at least for the referee." Reply: The referee probably is unaware of the Moore's tether-cutting model, where the flare core may be later linked to moving ribbon. This is actually the NEW thing unmentioned by others, e.g., Svestka's previous obs." "I believe it was a bad decision of the authors to skip the RHESSI imaging data (the old Fig. 2). May be its careful analysis helps to better understand the presented (and not yet properly explained) data." Reply: Because the referee had objection to the loop connection issue based on the Hessi image, thus what we did is what he wanted, i.e., to concentrate our discussion on event evolution. Because hessi entered into night at 19:20:30, we do not think that Hessi can provide more helpful information for this event. "I suggest to show in Fig. 5 a reference field so that the reader can be convinced that the transversal field is really changing only in the box drawn in Fig. 1." Reply: This can be done easily and we have data to prove. However, because of the page limit, we want to wait for the second referee's comments to see if other more important things need to be added.