Conveners
The Time-Varying mm-Wave Sky: Plenary Introduction
- Anna Ho (UC;LBL)
- Gregg Hallinan (Caltech)
The Time-Varying mm-Wave Sky: Parallel
- Anna Ho (UC;LBL)
- Gregg Hallinan (Caltech)
The Time-Varying mm-Wave Sky: Plenary Summary Report
- Anna Ho (UC;LBL)
- Gregg Hallinan (Caltech)
In this talk I will give a brief description of the gamma-ray burst phenomena, will introduce the different types of progenitors, and the model that defines the electromagnetic emission of GRBs. I will focus particularly on the emission in the millimetre range and place this into the context of CMB-S4, giving examples of what we may expect to gain through the observations performed by the new...
The mm-band presents an exciting new discovery space for extragalactic transients, including supernovae, gamma-ray bursts, tidal disruption events, and fast & blue optical transients. I will set the stage via glimpses through the new window opened up by ALMA into the science of such transients, followed by prospects for their detection and characterization with upcoming CMB surveys.
For GRB science, what do we need in terms of:
- Alert stream contents & timescale
- Additional technical infrastructure / data products
Do we benefit from a higher-cadence experiment from the Pole? (Higher depth, higher cadence, longer revisit time)
- Review recent results from SPT & ACT
- Questions to bear in mind during the talks
For stellar-flare science, what do we need in terms of:
- Alert stream contents & timescale
- Additional technical infrastructure / data products
Do we benefit from a higher-cadence experiment from the Pole? (Higher depth, higher cadence, longer revisit time)
