We propose target of opportunity global 3mm-VLBI observations of M87 vital to enhance a scheduled global 1.3mm-VLBI experiment with the EHT in March, 2015. We submit this proposal as ToO, since scheduling and details of the 1.3mm-VLBI run were not known at the previous submission deadline.
Observations could be scheduled either via HSA or GMVA.
The purpose is to obtain a high quality 3mm-VLBI image, to help interpreting results from 1mm-VLBI, which is more sensitivity and
uv-coverage limited.
With the combined 3mm/1mm data we aim at a coherent understanding of
the event horizon-scale structure in M87, and in particular of the jet launching region on scales from about 3-100 Schwarzschild radii.
The proposed observations will allow us to:
(1) determine size and shape of the jet base versus frequency down to about 3 Rs;
(2) study spectral index along the northern and southern
jet sheath and in core;
3) determine VLBI component spectra and their magnetic field strength;
4) test if core and inner jet sheath are polarized; and
5) constrain theoretical GRMHD modeling (eg. BP vs. BZ of jet launching by accurate observational data.
We note that combined 3mm/1.3mm observation can only be done once per year.
Name | Institution |
---|---|
Vincent Fish | Haystack Observatory |
Shep Doeleman | Center for Astrophysics | Harvard & Smithsonian |
Michael Lindqvist | Chalmers University of Technology |
Pablo de Vicente | Yebes, Centro Astronómico de |
David Hughes | Astrofísica, Óptica y Electrónica, Instituto Nacional de |
Masanori Nakamura | Academia Sinica; National Institute of Technology, Hachinohe College |
Keiichi Asada | Academia Sinica |
Michael Bremer | Institut de Radio Astronomique Millimétrique |
Jose L. Gomez | Andalucía, Instituto de Astrofísica de |
R. Craig Walker | National Radio Astronomy Observatory |
Thomas Krichbaum | Max-Planck-Institut für Radioastronomie |
Rusen Lu * | Max-Planck-Institut für Radioastronomie; Shanghai Astronomical Observatory, CAS |
* indicates the PI