Deblurring Sgr A* Images
APA
(2014). Deblurring Sgr A* Images. Perimeter Institute. https://pirsa.org/14110105
MLA
Deblurring Sgr A* Images. Perimeter Institute, Nov. 14, 2014, https://pirsa.org/14110105
BibTex
@misc{ pirsa_PIRSA:14110105, doi = {10.48660/14110105}, url = {https://pirsa.org/14110105}, author = {}, keywords = {Strong Gravity}, language = {en}, title = {Deblurring Sgr A* Images}, publisher = {Perimeter Institute}, year = {2014}, month = {nov}, note = {PIRSA:14110105 see, \url{https://pirsa.org}} }
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Talk Type
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Abstract
Scattering in the tenuous interstellar plasma blurs the image of Sgr A*. This effect decreases steeply with increasing frequency and becomes subdominant to the intrinsic emission structure at wavelengths close to a millimeter. I will discuss recent work that demonstrates how we can invert the blurring when properties of the scattering are known. With this technique, we can reconstruct the unscattered image of Sgr A* using EHT data. I will also show why some EHT observables -- such as closure phase and fractional polarization -- are largely immune to scattering. Finally, despite decades of study, there has been a recent flurry of progress in understanding the scattering properties, including studies of the Galactic Center magnetar and the discovery of refractive substructure in the scattering disk of Sgr A* at 1.3-cm wavelength. I will discuss these recent findings and their implications for imaging Sgr A* with the EHT