2014 Sep 08 光赤外天連シンポ @ 国立天文台三鷹

Progress with the Prime Focus Spectrograph for the Subaru Telescope:a massively multiplexed optical and near-infrared fiber spectrographHajime Sugai (PFS Project Manager; Kavli IPMU (WPI)), PFS Collaboration

2014年12月に台湾(ASIAA)で第6回コラボレーションミーティングが行われます。

Wide Field
Corrector

PFI部分に一部HSC team作成の図が使われています（WFC,POpt2部分。次ページ参照）

Prime Focus Instrument

Spectrograph

Wide Field
Corrector

Fiber Cable

Wide Field
Corrector

Metrology camera

Wide Field
Corrector

Fiber Positioner(from bottom)

Sharing WFC & POpt2 with HSC
Prime Focus Spectr.
(PFS)
Hyper Suprime-Cam(HSC)PFS case:
Optical interface with Wide Field Corrector
Field element= 54-mm thickness flat plate
substitutes for filter + dewar window

Prime Focus Unit POpt2
Wide Field Corrector (WFC)

HSC from http://www.eso.org/sci/facilities/eelt/fp7-elt-pub/wfi_workshop/pdffile/SMiyazaki.pdf

Science targets
9.3 h-3 Gpc3 in 0.8<z<2.4
1400 deg2 HSC Wide field
Dark Energy
Test General Relativity

Cosmology

HSC Deep field
Milky Way 17<V<21.5 390 deg2
M31halo 21.5<V<22.5 65 deg2

Dark Matter HSC sample

Credit: Gen Chiaki, Atsushi Taruya

Galactic Archaeology

1<z<2 16 deg2 to JAB~23.4
Chemical Evolution
Star Formation

Galaxy/AGN evolution

SF rate figure: Hopkins & Beacom
Image: Belokurov et al.

“Extragalactic science, cosmology, and Galactic archaeology
with the Subaru Prime Focus Spectrograph”,
Takada et al., 2014, PASP, 66, R1

2014 Jun SPIE papers from PFS
Instrument overview
Progress with the Prime Focus Spectrograph for the Subaru Telescope:a massively multiplexed optical and near-infrared fiber spectrograph (Sugai et al.)MicrolensDesign and performance of a F/#-conversion microlens for Prime Focus Spectrograph at Subaru Telescope (Takato et al.)Fiber system
Fiber Optical Cable and Connector System (FOCCoS) for PFS/ Subaru (Cesar Oliveira et al.)Studying focal ratio degradation of optical fibers with a core size of 128 microns for FOCCoS/ PFS/ Subaru (dos Santos et al.)Slit device for FOCCoS – PFS – Subaru (Cesar Oliveira et al.)Polish device for FOCCoS/PFS slit system (Cesar Oliveira et al.)Multi-fibers connectors systems for FOCCoS-PFS-Subaru (Cesar Oliveira et al.)Fiber positioner
Developing Engineering Model Cobra fiber positioners for the Subaru Telescope’s Prime Focus Spectrometer (Fisher et al.)

PFI, Metrology camera
Prime Focus Instrument of Prime Focus Spectrograph for Subaru Telescope (Wang et al.)Metrology camera system of Prime Focus Spectrograph for Subaru telescope (Wang et al.)Spectrograph
Current status of the Spectrograph System for the SuMIRe/PFS (Vivès et al.)
Optical design of the SuMiRe/PFS Spectrograph (Pascal et al.)Integration and test activities for the SUMIRE Prime Focus Spectrograph at LAM : first results (Madec et al.)Dewar & Detector
Focal Plane Alignment and Detector Characterization for the Subaru Prime Focus Spectrograph (Barkhouser et al.)
CCD readout electronics for the Subaru Prime Focus Spectrograph (Hope et al.)(Cryocooler vibration damping for the Subaru Prime Focus Spectrograph (Hope et al.))VPH gratings for the Subaru PFS: performance measurements of the prototype grating set (Barkhouser et al.)The near infrared camera for the Subaru Prime Focus Spectrograph (Gunn et al.)Updates on income
Presently drastic phase: 2014 March - end of FIRST fund- updates after 2013 Dec negotiation with NAOJ
(1) Further contribution from IPMU determined(2) Borrowed money from University of Tokyo(3) Contribution from NAOJ in addition to Subaru modification(4) MPA as new partner(5) Negotiating with new partner candidates(6) Negotiating with smaller partner candidates(7) Budget request of PFS submitted from University of Tokyo

現在、contingencyを含めないと、必要なトータル額に対して4%不足。
Contingencyも含めると8%不足。もちろん、cost reductionも実行中。

PFS Basic Characteristics
Optical + NIR Multi-object fiber spectrograph- Number of science fibers (Polymicro, Fujikura): 2394
600 or 597 per module X 4 Spectrograph modules- Fiber core diameter 127,128,129mm
Microlens (PID Nitto) attached to fiber input edge
fiber input F/2.2 -> F/2.8 (1”.1 diameter per fiber)- Field of view: 1.3 deg diameter- Wavelength: 0.38 - 1.26 μm

PFS Basic Characteristics- Each spectrograph module: 3-color-arm design
Arm Coverage[nm] Resolution[l/dl] (Kaiser VPHG)-----------------------------------------------------Blue 380 - 650
2500(Medium res. 710-885nm, R=5000
Red 630 - 9703200 Ohara prisms glued)
NIR 940-1260
4500------------------------------------------------------Spectrograph collimator F/2.5, camera F/1.1
Detector pixel 15mm
(2Kx4K x 2 Hamamatsu FDCCDs for each Blue/Red arm,
4Kx4K Teledyne HgCdTe(1.7mm cutoff) for NIR arm)

Major milestones (events)
Endorsement by Japanese community
MOU between NAOJ and IPMU

2011 Jan2011 Dec

Project CoDR (Conceptual Design)
Project RR (Requirement)
Project PDR (Preliminary Design)
Subsystem CDRs (Critical Design)First Light (Engineering)Subaru Strategic Program

2012 Mar2012 Oct2013 Feb
various
S17B
S19A-S23B

Microlens at fiber entrance
Challenge
withinput
Microlens
fast
telesope
Transforms
f-ratio on(F/2.2F/2.8) F-ratio.
(1) to reduce light loss caused by over-filling
After successful
productions
Mechanical & Optical samples,
acceptanceangle ofof
fiber
Mass production of 3500 microlenses completed.
(2) to ease difficulties of spectrograph design
PID Nitto:
K-VC82(nd=1.75),
4.8643-mm
concave
Moldinga suitablemicrolensout of curvature-radiusglass
molding - uniform lens dimensions
outer diameter = 1.486 mm +/- 1.2 mm (1s)glass - variety of refractive-index selection(specification 1.482-1.490 mm).
thickness 3mm within +/- 10mm (as specified).
Fiber core
Superbroad AR coating by NAOJ ATC (Waseda et al.)3 mm

Fiber positioner
Phi Stage(2.4 mmradius)

movie1

movie2

movieold

1.3°Field of View

Cobra Positioner
Patrol Area
(9.5 mm dia.)

Theta Stage
(2.4 mmradius)

After Generation 3,Engineering Model (EM: one module with a halfof 57 fiber positioners) tested.

0510150Iteration

Fiber positioner
Convergence to target

Theta Error
5um Cumulative Convergence400100105um Convergence9110010-110706050402001000 6-50 5302050 7Iterations

21030080

100 8% Converged95%

J2 Error (deg)Percentage Convergence (%)

10Dist to Target (um)

15090

3

J1 Error (deg)40-100 4

10-2100510Iteration

150-1005
1 2 3 4 05 6 7 8 9101112131415
Iterations Iterations

10-150 30 0

Convergence to target for the best (among five at the time) EM fiber positioner.
For randomly selected 100 target points within 9.5 mm diameter patrol area.
Left) Fiber position
is convergedwith iteration. For each of 100
5um Cumulative
Convergence
Phitarget
Error positions (cases).
9100Right) Fractionof cases where the fiber positions 150
are converged within 5 mm.
90Fiber Positioner (Cobra) Contract
EM試験を通した改良・価格削減をもとにfixed price contract
Sep 03 – starting contract with NewScalewith a half of Non Recurring Cost (NRC)
Nov 01 – another half of NRC
NRCにより量産体制 200 cobras per month 体制整うと~2400 cobrasを１年間で。

Basic Concept of the Slit Device

Fiber-slit Prototype

実際に使用するスリットも製作開始。

Spectrograph modules
Measurements on “prototype” VPHGs
Wavefront error measurements: e.g., 0.4 waves RMS for 280mm clear aperturefor blue VPHG prototype

Volume Phase Holographic Grating
Wave front error 改善策
改善案１：
原因究明し製作工程を治す。
難しいが、できれば、きれいはＶＰＨができてベスト。
改善案２：
カバープレートを研磨する。ＶＰＨによるＷＦＥをキャンセルするように。
研磨代・時間がかかる。エレガントでない。


実際とったのは、改善案１
ＪＨＵ,ＰＵががんばって、カイザーにも行って原因究明。
ホログラフィック作成光学系のアラインメント改善。
実際使用するＶＰＨＧを製作開始するところ。

CCD Pin bases製作
NAOJ ATC Nishino et al.
http://atc.mtk.nao.ac.jp/~yukiko/FDCCD_Manual/Astronomer/PinBase_etc/pinbase.png
AlN pin bases
placing Ti pins with positional accuracy s=1.4mm in each of x,y.
pin-diameter accuracy of 0.4mm.

 Accurate alignment of a pair CCDs

in Sugai et al. 2014, SPIE

location for setting four spectrograph modules- now fourth floor of the infrared instrument side (IR4), following decisions by SAC basedon Subaru UM 2014 Jan discussion.
(1) much less work/cost of reinforcement for IR4, compared with IR3;(2) less effects on operations of Nasmyth-floor instruments since IR4 floor is farther;(3) more space available on IR4 floor compared with IR3 floor with an elevator etc.
disadvantage on IR4: slightly longer Cable B fibers are necessary (connecting through the second floor, close to tel. elevation axis).

Floor / spectrograph clean roomdesigns on IR4prototypes / mockups