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Space Infrared Telescope for Cosmology and Astrophysics (SPICA), the cryogenic infrared space telescope recently pre-selected for a ‘Phase A’ concept study as one of the three remaining candidates for European Space Agency (ESA's) fifth medium class (M5) mission, is foreseen to include a far-infrared polarimetric imager [SPICA-POL, now called B-fields with BOlometers and Polarizers (B-BOP)], which would offer a unique opportunity to resolve major issues in our understanding of the nearby, cold magnetised Universe. This paper presents an overview of the main science drivers for B-BOP, including high dynamic range polarimetric imaging of the cold interstellar medium (ISM) in both our Milky Way and nearby galaxies. Thanks to a cooled telescope, B-BOP will deliver wide-field 100–350
m images of linearly polarised dust emission in Stokes Q and U with a resolution, signal-to-noise ratio, and both intensity and spatial dynamic ranges comparable to those achieved by Herschel images of the cold ISM in total intensity (Stokes I). The B-BOP 200
m images will also have a factor
30 higher resolution than Planck polarisation data. This will make B-BOP a unique tool for characterising the statistical properties of the magnetised ISM and probing the role of magnetic fields in the formation and evolution of the interstellar web of dusty molecular filaments giving birth to most stars in our Galaxy. B-BOP will also be a powerful instrument for studying the magnetism of nearby galaxies and testing Galactic dynamo models, constraining the physics of dust grain alignment, informing the problem of the interaction of cosmic rays with molecular clouds, tracing magnetic fields in the inner layers of protoplanetary disks, and monitoring accretion bursts in embedded protostars.
To measure the outcomes of laser treatment of cholesteatoma covering cochlear and vestibular fistulas.
Cholesteatoma matrix over the fistula was denatured; the power density was sufficient only to gradually heat, but not vaporise, the keratin-forming matrix. The denaturing speed was controlled so that the integrity of the fistula cover was maintained. The change in bone conduction threshold and the residual rate of cholesteatoma at the fistula were measured.
Thirty-six fistulas were assessed. There were seven cochlear fistulas. All were 5 mm or less in maximum length. For the entire group, the average change in bone conduction threshold was −0.3 dB. For cochlear fistulas, the average change in bone conduction was + 0.2 dB. The distribution of hearing results for the entire group was Gaussian; the apparent changes in hearing could be attributed to errors associated with testing. All patients underwent second-stage surgery. In all cases, the cholesteatoma was completely cleared from the fistula site. There were no facial palsies.
Laser denaturing of cholesteatoma matrix over fistulas measuring 5 mm or less of vestibular apparatus and the cochlea is effective at eliminating cholesteatoma, and is not associated with cochlear hearing loss or facial palsy.