  The joint observation of core-collapse supernovae with gamma-ray bursts shows
that jets can be launched in the aftermath of stellar core collapse, likely by
a newly formed black hole that accretes matter from the star. Such gamma-ray
bursts have only been observed accompanying Type Ibc supernovae, indicating a
stellar progenitor that lost its Hydrogen envelope before collapse. According
to recent hypothesis it is possible that jets are launched in core-collapse
events even when the progenitors still retain their Hydrogen envelopes,
however, such jets are not able to burrow through the star and will be stalled
into the interior of the progenitor star before escaping. These jets are called
chocked jets. High-energy neutrinos produced by such choked jets could escape
the stellar envelope and could be observed. Here we examine how multi-messenger
searches for high-energy neutrinos and core-collapse supernovae can detect or
limit the fraction of stellar collapses that produce jets. We find that a high
fraction of jet production is already limited by previous observational
campaigns. We explore possibilities with future observations using LSST,
IceCube and Km3NET.
