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Can the detection of gws from CCSNe give insights of gravity in the strong regime? Can we test alternative theories to GR from SNs signals? Is this of interest for the group?

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What knowledge can be pulled from understanding supernovae that can impact the general public?

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What will happen after 05? When will we have detectors that are always on?

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Are there multi messenger methods proposed to calculate PNS parameters (mass, rotation, etc) if GW signals are influenced by many parameters?

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Is it really useful to search for SNCC in GW data when this can be detected in neutrino data in essentially zero background?

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What is the maximum distance upto which a GW signal from SN could be detected with current generation or next generation detectors?

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What we need for the detection of failed supernova GW?

And were we able to detect M31-2014-BH1 if Ligo was available on 2014?

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What new data analysis tests or upper limits (if any) would you like to see in the next LVK paper that you haven't seen in past papers?

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If a core-collapse supernova like SN 1987A occurred today at the same distance in the Large Magellanic Cloud, would current gravitational wave detectors such as LIGO, Virgo, or KAGRA be sensitive enough to detect the gravitational wave signal?

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What is the minimum temporal seperation between the beginning of the high frequency feature and the beginning of SASI, if any

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Since we are most confident about detecting CCSN <10 Kpc away, do we have a red flag list for the stars to watch the hardest in case they go supernova? How far out have we confidently catalogued most likely CCSN progenitor candidates?

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What kind of information from the detection side might be helpful for the SN simulations?

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Is it possible to combine the single detector search results with the coincident searches?

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What is the minimum temporal seperation between prompt convection and beginning of high frequency feature

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In Andresen's presentation slide 17, what is the low energy "line" in the spectrograms?

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Being realistic, what are the concrete directions on the theory and detection sides to prepare the ground for a CCSN GW signal?

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What we can learn from Betelgeuse?

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Detecting GW polarizations from CCSN

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What is the SNR needed for a SN detection?

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How to improve the current detection? Any more analysis we can do?

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An astronomer trying to detect a supernova according to AI

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An astronomer trying to detect a supernova