Polarimetric Calibration for Nasmyth instrument HiCIAO Jun Hashimoto (National Astronomical Observatory of Japan) and SEEDS, HiCIAO, AO team 1/13 What is HiCIAO ? • Near-infrared high contrast imaging instrument with a linear polarimetor at the 8.2m Subaru telescope. • Targets: exoplanets and proto-planetary disks GJ758 (Thalmann et al. 2009) HiCIAO results k And SAO206462 ~10-30MJ 30AU 52AU Carson+12 PDS 70 Muto+12 100AU Hashimoto+12 • We use linear polarization for the detection of disks • Required polarimetric accuracy: 0.1-0.3 % – 20-30 % polarization in disks 2/13 Nasmyth polarimetor HiCIAO • HiCIAO is mounted on Nasmyth platform. SUBARU unpolarized light HiCIAO polarized light 45º Nasmyth focus Tertiary mirror • Instrumental polarization comes from the telescope and instruments. • Correcting with Correction Matrix, not standard star. What is instrumental polarization ? 3/13 • The amplitude and phase of incident light are changed at mirrors (Fresnel reflection). Reflectance – Rs and Rp: the reflection coefficient of perpendicular and parallel wave to the plane of incidence. refractive index Mirror case of a bare silver mirror 4/13 Conceptual figure of the optical path • Instrumental polarization in HiCIAO mainly comes from Tertiary Mirror and Image Rotator. – Rotating during tracking objects, thus, time variable. • Other optics generate static instrumental polarization. – Corrected by flat-fielding uging non-polarized light. 5/13 Instrumental polarization from Tertiary mirror • Bare silver mirror – n=0.3+11.7i @ 1.6um • Tertiary mirror rotates with the telescope elevation Q/I (unpolarized light) ~0.3% instrumental polarization is generated by Tertiary Mirror 6/13 Instrumental polarization from Image Rotator • Three silver mirrors to derotate images • Over coating (SiO2) Conceptual figure of Image Rotator – multi-reflection Phase Difference • Wavelength dependency • Linear polarization is changed to circular polarization at 1.6 um Conceptual figure of multi-reflection 7/13 Cross talk (Q , U => V) in Image Rotator Observed linear polarization with a rotation angle Angle of Image rotator (degree) • Most incident linear polarization is changed to circular polarization at 45 degrees 8/13 Correction • Construction of the matrix between observed values and true Stokes parameters – no need of observations for polarized standard star Observed Jones matrix HiCIAO matrix observed values Incident Jones matrix Incident Stokes parameters linear combination of IQUV Deriving incident stokes QU by linear transformation. 9/13 Matrix between observed values and Stokes parameter observable incident Stokes parameters • p, q, u, v are functions of refractive indecs of Tertiary Mirror and Image Rotator Constant Values • A, B, C, D are functions of parallactic angle and Telescope Elevation, Image Rotator angle, and wave-plate angle. Variable values 10/13 Stabilize instrumental polarization • Optimizing the tracking of half-waveplate to stabilize time-variable instrumental polarization star • Two tracking mode Sidereal – Sidereal tracking – Pupile tracking (ADI mode) time dependency of instrumental polarization Q/I ADI telescope spider Tracking half-waveplate Tracking half-waveplate Q/I No tracking half-waveplate No tracking half-waveplate 11/13 Performance • Polarimetric standard star – Elias 16 • Instrumental polarization is corrected by our model. • 4.22% +- 0.07%, 71.1º +- 0.5º (HiCIAO) • 4.09% +- 0.02%, 71.0º +- 1.0º (Hough+88) – HDE 283809 • 2.67% +- 0.13%, 63.0º +- 3.1º (HiCIAO) • 2.59% +- 0.07%, 58.0º +- 1.0º (Whittet+92) • Photometric standard star (not nearby star, may have interstellar polarization) – SAO93770 • <P>=0.70%, <sigmaP>=0.20% – GSC01804 • <P>=0.52%, <sigmaP>=0.13% • Accuracy of polarization in HiCIAO PDI is sigmaP < ~0.2%, sigmaθ < ~5º. 12/13 Known problem • Large wavelength dependency in Image Rotator MKO H band filter • Blue or red sources may have large uncertainty. • Tracking Image Rotator around ‘0’ degree. 13/13 Conclusion • HiCIAO is the Nasmyth polarimetor at the Subaru telescope. • Instrumental polarization including cross talk is corrected by Correction Matrix. • For better correction, half-waveplate is tracked to stabilize the variable instrumental polarization • Accuracy: a few 0.1% Thank you! 14/13 15/13 Performance • Polarization vector pattern of AB Aur. – Detecting polarization at the vicinity of the mask edge (r >0.15" : 22 AU) – Center: 90.1º +- 0.2º ,FWHM: 4.3º +- 0.4º • Instrumental Polarization is corrected. • The PI image of AB Aur is less affected by speckle noise. 600 400 (number) 85 90 95 (degree)