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VPH grism for Subaru Telescope Diffraction Efficiency of Gratings Diffraction Efficiency of Gratings Noboru Ebizuka, Shuji Sato, Kaoru Nakajima, Keiko Oka, Akiko Yamada, Masako Kashiwagi, Kashiko Kodate, Kohtaro Ichiyama, Takashi Ichikawa,


  1. VPH grism for Subaru Telescope Diffraction Efficiency of Gratings Diffraction Efficiency of Gratings Noboru Ebizuka, Shuji Sato, Kaoru Nakajima, Keiko Oka, Akiko Yamada, Masako Kashiwagi, Kashiko Kodate, Kohtaro Ichiyama, Takashi Ichikawa, Chihiro Tohkoku, Toru Yamada, Masakazu Harashima, Tsutomu Okura, Koji Kawabata, Kazuhiro Shimasaku, Takashi Hattori, Nobunari Kashikawa, Masanori Iye Nagoya University, Japan Women's University, Tohoku University, Soma Optics Co.Ltd., Hiroshima University, University of Tokyo, National Astronomical Observatory of Japan Surface relief grating VPH grating May 17 - 21, 2009, Kyoto Joint Subaru/Gemini Science Conference [K. Oka et. al., SPIE 5005, 2003] Resin for Volume Hologram Grism with High Index Prisms Grism with High Index Prisms Resin for Volume Hologram RPM: Radical polymerization monomer, Polymerized by UV and 460 - 600 nm. CPM: Cation polymerization monomer, Polymerized by UV. RPP: Radical polymerization polymer. CPP: Cation polymerization polymer. " Laser Exposure ! Critical angle of refractive indices 2.6 and 1.5 is 35.2 degree ( � in = 0, � = 35.2). # UV exposure $ Laser Exposure Grism with VPH or Quasi-Bragg grating is less sensitive to critical angle. # [Ebizuka et. al., SPIE 4842, 2002] Nippon Paint Co.Ltd. Optical System for Holographic Exposure Holographic Exposure Hologram Plate Making Hologram Plate Making Optical System for Cleaning of glass substrates. Dropping resin (liquid) on a substrate, View 2 heating up to 80 !" View 1 Hologram resin Glass substrates (Nippon Paint Co. Ltd.) Sandwich resin with View 2 substrate. Thickness is adjusted by glass beads. Glass beads View 1

  2. VPH VPH Grisms Grisms for FOCAS for FOCAS Efficiencies of FOCAS VPH Efficiencies of FOCAS VPH Grisms Grisms (Faint Object CAmera and Spectrograph) 100 Band Blaze Range R ( � / �� # Developer [nm] [nm] @0.4” Slit I band B-V band 80 R band U-B 450 346 – 522 2,600 JWU z band B-V 520 432 – 606 3,000 JWU U-B band V-R 650 516 – 781 2,500 Ralcon Efficiency [%] 60 R* 680 631 – 725 7,200 JWU V-R band R-z** 800 550 – 1,047 1,600 Nagoya Univ. I* 800 741 – 856 7,000 Ralcon 40 I-Y** 950 792 – 1,104 3,100 JWU Mid 300 z* 950 879 – 1,027 6,400 Ralcon Mid 300 Red blue ________________________________________________________________________________________ 20 * ZnSe prisms. ** Under development. JWU: Japan Women’s University Size: 110 x 106 x 106 (max) mm 0 300 400 500 600 700 800 900 1000 1100 Wavelength [nm] [M. Kashiwagi et. al., SPIE 5494, 2004; K.S. Kawabata et. al. SPIE 4841, 2003] VPH Grisms VPH Grisms for for MOIRCS MOIRCS Efficiencies of FOCAS Efficiencies of FOCAS R-z R-z Band Band Grism Grism (Multi-Object InfraRed Camera and Spectrograph) VPH grating Band Blaze Range [ µ m] R@0.5” Slit Efficiency Developer (360 g/mm, Blaze: 800nm ) [ µ m] (Max) Y 1.02 0.94 – 1.09 3,200 ~ 0.80 ~ 0.80 Soma Optics J 1.25 1.13 – 1.37 3,100 0.82, 0.74 Tohoku Univ. H 1.65 1.52 – 1.78 3,000 ~ ~ 0.75 0.75 Surface relief grating Tohoku Univ. K* 2.20 2.00 – 2.40 2,600 > 0.90 JWU (300 g/mm, Blaze: 750 nm) * Under development. 100 Incident 7576_45 7576_50 7576_55 8384_45 8384_50 8384_55 82% angle 80 74% Efficiency [%] 60 40 -4.0° 0° +4.4° 20 J band VPH grisms 0 700 800 900 1000 1100 1200 1300 VPH grism grism is versatile for is versatile for mideum mideum dispersion ! dispersion ! VPH Wavelength [nm] Y band VPH grisms Spectrum of a galaxy (z = 1.618) Spectrum of a galaxy (z = 1.618) Quasi-Bragg grating Quasi-Bragg grating • Echelle mode, a higher order grating with a cross disperser, 70 effectively utilizes 2 dimensional detector. • Diffraction efficiency of a VPH grating decreases at higher orders. • Diffraction efficiency of a surface relief grating changes slightly. 57 70 Size: 70 x 70 x 57 (max) mm. Diffraction efficiency of VPH Diffraction efficiency of MOIRCS, J band VPH grism, 0”.8 slit grating of higher order Quasi-Bragg Quasi-Bragg [Onodera in private communication]. [K. Oka et. al., SPIE 5290, 2004] [T. Ichikawa et. al., SPIE 7014, 2008]

  3. Diffraction of Quasi-Bragg Grating Trial Fabrication of Quasi-Bragg Grating Diffraction of Quasi-Bragg Grating Trial Fabrication of Quasi-Bragg Grating � = 0 � = 0.6 A: 10 x 10 x 0.2 x 40 pcs (left), B: 1.5 x 10 x 0.2 x 40 pcs (right) Cutting Laminating of Mirror � = 1.2 Plate Lapping and Polishing � = 1.8 for Wave Guide [N. Ebizuka et. al., SPIE 6273, 2006] Conclusions Conclusions • U-B, B-V, V-R, R, I and z band grisms for FOCAS, and J and H band grism for MOIRCS are available. • Y band grism for MOIRCS is ready for installation. • R-z and I-Y band grisms for FOCAS, and K band grism for MOIRCS are under development. We appreciate Mr. Kawabata and Mr. Teranishi of Nippon Paint Co.Ltd. for providing hologram resin. These works had partially supported by the grant-in- aid of RIKEN for practical use of research results.

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