POLARBEAR-2 optical and polarimeter designs

POLARBEAR-2 is a ground based cosmic microwave background (CMB) radiation experiment observing from Atacama, Chile. The science goals of POLARBEAR-2 are to measure the CMB polarization signals originating from the inflationary gravity-wave background and weak gravitational lensing. In order to achieve these science goals, POLARBEAR-2 employs 7588 polarization sensitive transition edge sensor bolometers at observing fre quencies of 95 and 150 GHz with 5.5 and 3.5 arcmin beam width, respectively. The telescope is the off-axis Gregorian, Huan Tran Telescope, on which the POLARBEAR-1 receiver is currently mounted. The polarimetry is based on modulation of the polarized signal using a rotating half-wave plate and the rotation of the sky. We present the developments of the optical and polarimeter designs including the cryogenically cooled refractive optics that achieve the overall 4 degrees field-of-view, the thermal filter design, the broadband anti-reflection coating, and the rotating half-wave plate.

[1]  Edward J. Wollack,et al.  SEVEN-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE (WMAP) OBSERVATIONS: PLANETS AND CELESTIAL CALIBRATION SOURCES , 2010, 1001.4731.

[2]  Gabriel M. Rebeiz,et al.  Multi-Chroic Dual-Polarization Bolometric Detectors for Studies of the Cosmic Microwave Background , 2014 .

[3]  J. J. Bock,et al.  SPIDER: a balloon-borne CMB polarimeter for large angular scales , 2010, Astronomical Telescopes + Instrumentation.

[4]  S. Pancharatnam,et al.  Achromatic combinations of birefringent plates , 1955 .

[5]  Britt Reichborn-Kjennerud,et al.  A cryogenic half-wave plate polarimeter using a superconducting magnetic bearing , 2011, Optical Engineering + Applications.

[6]  M. Lueker,et al.  A MEASUREMENT OF THE DAMPING TAIL OF THE COSMIC MICROWAVE BACKGROUND POWER SPECTRUM WITH THE SOUTH POLE TELESCOPE , 2011, 1105.3182.

[7]  Graeme Smecher,et al.  The POLARBEAR-2 Experiment , 2014 .

[8]  C. B. Netterfield,et al.  Planck early results - I. The Planck mission , 2011, 1101.2022.

[9]  Shaul Hanany,et al.  Performance of three- and five-stack achromatic half-wave plates at millimeter wavelengths. , 2008, Applied optics.

[10]  I. Buder,et al.  FIRST SEASON QUIET OBSERVATIONS : MEASUREMENTS OF CMB POLARIZATION POWER SPECTRA AT 43 GHZ IN THE MULTIPOLE RANGE 25 ≤ l ≤ 475 QUIET Collaboration , 2010 .

[11]  DE P.A.R.A,et al.  MEASUREMENT OF CMB POLARIZATION POWER SPECTRA FROM TWO YEARS OF BICEP DATA , 2009 .

[12]  P. A. R. Ade,et al.  BICEP2 and Keck array operational overview and status of observations , 2012, Other Conferences.

[13]  Peter Ade,et al.  The POLARBEAR experiment , 2012, Other Conferences.

[14]  Adrian T. Lee,et al.  EBEX: a balloon-borne CMB polarization experiment , 2010, Astronomical Telescopes + Instrumentation.