Upgrade to Pro — share decks privately, control downloads, hide ads and more …

Ideas for Metrology of Silicon Diffractive Optics

gully
November 01, 2013

Ideas for Metrology of Silicon Diffractive Optics

This talk was given around November of 2013 to members of the Si Diffractive Optics Group at UT Austin. The talk highlights summarizes the 27 tasks or ideas our group was working on at that moment in time, and details one specific idea for enhanced metrology of Si immersion gratings.

gully

November 01, 2013
Tweet

More Decks by gully

Other Decks in Science

Transcript

  1. ideas for Si diffractive optics
    UT Austin Silicon Diffractive Optics Group

    View Slide

  2. michael gully-santiago
    astronomer, engineer, graduate
    student, bicycle rider

    View Slide

  3. I made a list of 27 ideas.
    There were so many that I gave them all id #’s.

    View Slide

  4. The goal of this presentation is to inform you about the ideas.

    View Slide

  5. Rank ID Idea
    # # -
    1 Si01 Measure the ICP etch time – phase relation
    2 Si02 Predict and characterize the effect of poor lithographic contacting
    3 Si03 Measure the UV exposure dose – phase relation
    4 Si04 High spatial resolution measurements of bonded Si pucks
    5 Si05 Characterization of heritage grating surfaces
    6 Si23 Improve UV illumination uniformity
    7 Si22 Reduce the dose-phase curve
    8 Si21 Reduce the UV fringe amplitude
    9 Si07 e-beam silicon immersion grating production
    10 Si06 A contacted grism for Mimir
    11 Si08 Does thermal anneal eliminate IR bubbles in bonded Si?
    12 Si09 L- and M- band immersion grating for iSHELL
    13 Si10 J-, H-, and K- band immersion grating for iSHELL
    14 Si11 ACT immersion grating prototype
    15 Si12 Internal transfer of skills and knowledge I-VI
    16 Si13 Directly measured moderate order HeNe spectral purity of photo masks
    17 Si14 Characterization of stock lab optics with Cary 5000
    18 Si15 The geometrical efficiency loss from dispersion at high λ and m
    19 Si16 SPIE paper idea: applications and specifications for immersion gratings
    20 Si17 A higher performance immersion grating for IGRINS
    21 Si18 Robust inventory and travelers for silicon and optical parts
    22 Si19 Quantify vendor provided defect density, compare to specifications
    23 Si20 Improve Si wafer mounting strategy to better simulate optical surfaces
    24 Si24 Directly measure blaze angle in reflection
    25 Si25 Directly measure on-blaze efficiency in reflection
    26 Si26 Characterize the effect of high temperature annealing on precision optics
    27 Si27 Quantify the Fabry-Pèrot effect of finite thickness Si optics
    All 27 ideas

    View Slide

  6. 1 Si01 Measure the ICP etch time – phase relation
    2 Si02 Predict and characterize the effect of poor lithographic contacting
    3 Si03 Measure the UV exposure dose – phase relation
    The ones we’ve done
    4 Si04 High spatial resolution measurements of bonded Si pucks
    5 Si05 Characterization of heritage grating surfaces
    6 Si23 Improve UV illumination uniformity
    7 Si22 Reduce the dose-phase curve
    8 Si21 Reduce the UV fringe amplitude
    9 Si07 e-beam silicon immersion grating production
    10 Si06 A contacted grism for Mimir
    11 Si08 Does thermal anneal eliminate IR bubbles in bonded Si?
    12 Si09 L- and M- band immersion grating for iSHELL
    13 Si10 J-, H-, and K- band immersion grating for iSHELL
    14 Si11 ACT immersion grating prototype
    15 Si12 Internal transfer of skills and knowledge I-VI
    16 Si13 Directly measured moderate order HeNe spectral purity of photo masks
    17 Si14 Characterization of stock lab optics with Cary 5000
    18 Si15 The geometrical efficiency loss from dispersion at high λ and m
    19 Si16 SPIE paper idea: applications and specifications for immersion gratings
    20 Si17 A higher performance immersion grating for IGRINS
    21 Si18 Robust inventory and travelers for silicon and optical parts
    22 Si19 Quantify vendor provided defect density, compare to specifications
    23 Si20 Improve Si wafer mounting strategy to better simulate optical surfaces
    24 Si24 Directly measure blaze angle in reflection
    25 Si25 Directly measure on-blaze efficiency in reflection
    26 Si26 Characterize the effect of high temperature annealing on precision optics
    27 Si27 Quantify the Fabry-Pèrot effect of finite thickness Si optics
    The ones we haven’t

    View Slide

  7. 1 Si01 Measure the ICP etch time – phase relation
    2 Si02 Predict and characterize the effect of poor lithographic contacting
    3 Si03 Measure the UV exposure dose – phase relation
    The ones we’ve done
    Let’s recap

    View Slide

  8. 1 Si01 Measure the ICP etch time – phase relation
    2 Si02 Predict and characterize the effect of poor lithographic contacting
    3 Si03 Measure the UV exposure dose – phase relation
    Si03 Measure the UV exposure dose – phase relation
    We measured the UV exposure dose-phase relation:
    dL/dE ~ 1000 ± 250 nm/E0
    It is important to distinguish between phase and line-
    edge position.
    -1000
    -500
    0
    500
    1000
    1500
    2000
    0 2 4
    dL / dE
    E/E
    0
    wafer 081213_01 Zygo Results
    UTexas 30 micron
    S1800 0.6 micron
    Linear(UTexas 30
    micron)
    Linear(S1800 0.6
    micron)
    There are clearly horizontal discontinuities in the
    Zygo interferometry. The regions pictured received
    discrete UV exposure doses of 60 – 80 s.

    View Slide

  9. 1 Si01 Measure the ICP etch time – phase relation
    2 Si02 Predict and characterize the effect of poor lithographic contacting
    3 Si03 Measure the UV exposure dose – phase relation
    Si01 Measure the ICP etch time – phase relation
    dn
    !3"
    w
    h
    Silicon nitride
    Silicon
    Photoresist
    xs
    xn
    Sidewall etching can arise from a sloped
    photoresist or isotropic chemical etching.
    Zygo interferometry constrains the ICP
    sidewall etch rate from t = 55-125 s
    dL/dt < 5 nm/s
    Image:
    cbrooks
    We predicted 4 horizontal discontinuities in
    the below image. We see only 1 discontinuity,
    so the ICP etch has negligible effect on phase.

    View Slide

  10. 1 Si01 Measure the ICP etch time – phase relation
    2 Si02 Predict and characterize the effect of poor lithographic contacting
    3 Si03 Measure the UV exposure dose – phase relation
    Si02 Predict and characterize the effect of poor
    lithographic contacting
    25 nm undulations measured w/ Zygo are consistent with
    fringe amplitude = 2.5 ± 1.6%
    Directly measured resist reflectivity integrated against the
    UV lamp spectrum are consistent with 1% fringe amplitude.
    Not shown: grayscale lithography with Dektak measured
    film thickness is consistent with 2% fringe amplitude.

    View Slide

  11. 4 Si04 High spatial resolution measurements of bonded Si pucks
    5 Si05 Characterization of heritage grating surfaces
    6 Si23 Improve UV illumination uniformity
    7 Si22 Reduce the dose-phase curve
    8 Si21 Reduce the UV fringe amplitude
    9 Si07 e-beam silicon immersion grating production
    10 Si06 A contacted grism for Mimir
    11 Si08 Does thermal anneal eliminate IR bubbles in bonded Si?
    12 Si09 L- and M- band immersion grating for iSHELL
    13 Si10 J-, H-, and K- band immersion grating for iSHELL
    14 Si11 ACT immersion grating prototype
    15 Si12 Internal transfer of skills and knowledge I-VI
    16 Si13 Directly measured moderate order HeNe spectral purity of photo masks
    17 Si14 Characterization of stock lab optics with Cary 5000
    18 Si15 The geometrical efficiency loss from dispersion at high λ and m
    19 Si16 SPIE paper idea: applications and specifications for immersion gratings
    20 Si17 A higher performance immersion grating for IGRINS
    21 Si18 Robust inventory and travelers for silicon and optical parts
    22 Si19 Quantify vendor provided defect density, compare to specifications
    23 Si20 Improve Si wafer mounting strategy to better simulate optical surfaces
    24 Si24 Directly measure blaze angle in reflection
    25 Si25 Directly measure on-blaze efficiency in reflection
    26 Si26 Characterize the effect of high temperature annealing on precision optics
    27 Si27 Quantify the Fabry-Pèrot effect of finite thickness Si optics
    The ones we haven’t
    Now let’s
    look at

    View Slide

  12. 4 Si04 High spatial resolution measurements of bonded Si pucks
    5 Si05 Characterization of heritage grating surfaces
    6 Si23 Improve UV illumination uniformity
    7 Si22 Reduce the dose-phase curve
    8 Si21 Reduce the UV fringe amplitude
    9 Si07 e-beam silicon immersion grating production
    10 Si06 A contacted grism for Mimir
    11 Si08 Does thermal anneal eliminate IR bubbles in bonded Si?
    12 Si09 L- and M- band immersion grating for iSHELL
    13 Si10 J-, H-, and K- band immersion grating for iSHELL
    14 Si11 ACT immersion grating prototype
    15 Si12 Internal transfer of skills and knowledge I-VI
    16 Si13 Directly measured moderate order HeNe spectral purity of photo masks
    17 Si14 Characterization of stock lab optics with Cary 5000
    18 Si15 The geometrical efficiency loss from dispersion at high λ and m
    19 Si16 SPIE paper idea: applications and specifications for immersion gratings
    20 Si17 A higher performance immersion grating for IGRINS
    21 Si18 Robust inventory and travelers for silicon and optical parts
    22 Si19 Quantify vendor provided defect density, compare to specifications
    23 Si20 Improve Si wafer mounting strategy to better simulate optical surfaces
    24 Si24 Directly measure blaze angle in reflection
    25 Si25 Directly measure on-blaze efficiency in reflection
    26 Si26 Characterize the effect of high temperature annealing on precision optics
    27 Si27 Quantify the Fabry-Pèrot effect of finite thickness Si optics
    Some ideas are innovative metrology techniques
    metrology

    View Slide

  13. 4 Si04 High spatial resolution measurements of bonded Si pucks
    5 Si05 Characterization of heritage grating surfaces
    6 Si23 Improve UV illumination uniformity
    7 Si22 Reduce the dose-phase curve
    8 Si21 Reduce the UV fringe amplitude
    9 Si07 e-beam silicon immersion grating production
    10 Si06 A contacted grism for Mimir
    11 Si08 Does thermal anneal eliminate IR bubbles in bonded Si?
    12 Si09 L- and M- band immersion grating for iSHELL
    13 Si10 J-, H-, and K- band immersion grating for iSHELL
    14 Si11 ACT immersion grating prototype
    15 Si12 Internal transfer of skills and knowledge I-VI
    16 Si13 Directly measured moderate order HeNe spectral purity of photo masks
    17 Si14 Characterization of stock lab optics with Cary 5000
    18 Si15 The geometrical efficiency loss from dispersion at high λ and m
    19 Si16 SPIE paper idea: applications and specifications for immersion gratings
    20 Si17 A higher performance immersion grating for IGRINS
    21 Si18 Robust inventory and travelers for silicon and optical parts
    22 Si19 Quantify vendor provided defect density, compare to specifications
    23 Si20 Improve Si wafer mounting strategy to better simulate optical surfaces
    24 Si24 Directly measure blaze angle in reflection
    25 Si25 Directly measure on-blaze efficiency in reflection
    26 Si26 Characterize the effect of high temperature annealing on precision optics
    27 Si27 Quantify the Fabry-Pèrot effect of finite thickness Si optics
    Some ideas are for improving our process
    metrology
    process

    View Slide

  14. 4 Si04 High spatial resolution measurements of bonded Si pucks
    5 Si05 Characterization of heritage grating surfaces
    6 Si23 Improve UV illumination uniformity
    7 Si22 Reduce the dose-phase curve
    8 Si21 Reduce the UV fringe amplitude
    9 Si07 e-beam silicon immersion grating production
    10 Si06 A contacted grism for Mimir
    11 Si08 Does thermal anneal eliminate IR bubbles in bonded Si?
    12 Si09 L- and M- band immersion grating for iSHELL
    13 Si10 J-, H-, and K- band immersion grating for iSHELL
    14 Si11 ACT immersion grating prototype
    15 Si12 Internal transfer of skills and knowledge I-VI
    16 Si13 Directly measured moderate order HeNe spectral purity of photo masks
    17 Si14 Characterization of stock lab optics with Cary 5000
    18 Si15 The geometrical efficiency loss from dispersion at high λ and m
    19 Si16 SPIE paper idea: applications and specifications for immersion gratings
    20 Si17 A higher performance immersion grating for IGRINS
    21 Si18 Robust inventory and travelers for silicon and optical parts
    22 Si19 Quantify vendor provided defect density, compare to specifications
    23 Si20 Improve Si wafer mounting strategy to better simulate optical surfaces
    24 Si24 Directly measure blaze angle in reflection
    25 Si25 Directly measure on-blaze efficiency in reflection
    26 Si26 Characterize the effect of high temperature annealing on precision optics
    27 Si27 Quantify the Fabry-Pèrot effect of finite thickness Si optics
    Some ideas are not ideas at all- they are
    commitments we have to make devices
    metrology
    process
    make devices

    View Slide

  15. 4 Si04 High spatial resolution measurements of bonded Si pucks
    5 Si05 Characterization of heritage grating surfaces
    6 Si23 Improve UV illumination uniformity
    7 Si22 Reduce the dose-phase curve
    8 Si21 Reduce the UV fringe amplitude
    9 Si07 e-beam silicon immersion grating production
    10 Si06 A contacted grism for Mimir
    11 Si08 Does thermal anneal eliminate IR bubbles in bonded Si?
    12 Si09 L- and M- band immersion grating for iSHELL
    13 Si10 J-, H-, and K- band immersion grating for iSHELL
    14 Si11 ACT immersion grating prototype
    15 Si12 Internal transfer of skills and knowledge I-VI
    16 Si13 Directly measured moderate order HeNe spectral purity of photo masks
    17 Si14 Characterization of stock lab optics with Cary 5000
    18 Si15 The geometrical efficiency loss from dispersion at high λ and m
    19 Si16 SPIE paper idea: applications and specifications for immersion gratings
    20 Si17 A higher performance immersion grating for IGRINS
    21 Si18 Robust inventory and travelers for silicon and optical parts
    22 Si19 Quantify vendor provided defect density, compare to specifications
    23 Si20 Improve Si wafer mounting strategy to better simulate optical surfaces
    24 Si24 Directly measure blaze angle in reflection
    25 Si25 Directly measure on-blaze efficiency in reflection
    26 Si26 Characterize the effect of high temperature annealing on precision optics
    27 Si27 Quantify the Fabry-Pèrot effect of finite thickness Si optics
    Two ideas are about investing in organization
    metrology
    process
    make devices
    organization

    View Slide

  16. 4 Si04 High spatial resolution measurements of bonded Si pucks
    5 Si05 Characterization of heritage grating surfaces
    6 Si23 Improve UV illumination uniformity
    7 Si22 Reduce the dose-phase curve
    8 Si21 Reduce the UV fringe amplitude
    9 Si07 e-beam silicon immersion grating production
    10 Si06 A contacted grism for Mimir
    11 Si08 Does thermal anneal eliminate IR bubbles in bonded Si?
    12 Si09 L- and M- band immersion grating for iSHELL
    13 Si10 J-, H-, and K- band immersion grating for iSHELL
    14 Si11 ACT immersion grating prototype
    15 Si12 Internal transfer of skills and knowledge I-VI
    16 Si13 Directly measured moderate order HeNe spectral purity of photo masks
    17 Si14 Characterization of stock lab optics with Cary 5000
    18 Si15 The geometrical efficiency loss from dispersion at high λ and m
    19 Si16 SPIE paper idea: applications and specifications for immersion gratings
    20 Si17 A higher performance immersion grating for IGRINS
    21 Si18 Robust inventory and travelers for silicon and optical parts
    22 Si19 Quantify vendor provided defect density, compare to specifications
    23 Si20 Improve Si wafer mounting strategy to better simulate optical surfaces
    24 Si24 Directly measure blaze angle in reflection
    25 Si25 Directly measure on-blaze efficiency in reflection
    26 Si26 Characterize the effect of high temperature annealing on precision optics
    27 Si27 Quantify the Fabry-Pèrot effect of finite thickness Si optics
    Two ideas are about the design of gratings
    metrology
    process
    make devices
    organization
    design

    View Slide

  17. 4 Si04 High spatial resolution measurements of bonded Si pucks
    5 Si05 Characterization of heritage grating surfaces
    6 Si23 Improve UV illumination uniformity
    7 Si22 Reduce the dose-phase curve
    8 Si21 Reduce the UV fringe amplitude
    9 Si07 e-beam silicon immersion grating production
    10 Si06 A contacted grism for Mimir
    11 Si08 Does thermal anneal eliminate IR bubbles in bonded Si?
    12 Si09 L- and M- band immersion grating for iSHELL
    13 Si10 J-, H-, and K- band immersion grating for iSHELL
    14 Si11 ACT immersion grating prototype
    15 Si12 Internal transfer of skills and knowledge I-VI
    16 Si13 Directly measured moderate order HeNe spectral purity of photo masks
    17 Si14 Characterization of stock lab optics with Cary 5000
    18 Si15 The geometrical efficiency loss from dispersion at high λ and m
    19 Si16 SPIE paper idea: applications and specifications for immersion gratings
    20 Si17 A higher performance immersion grating for IGRINS
    21 Si18 Robust inventory and travelers for silicon and optical parts
    22 Si19 Quantify vendor provided defect density, compare to specifications
    23 Si20 Improve Si wafer mounting strategy to better simulate optical surfaces
    24 Si24 Directly measure blaze angle in reflection
    25 Si25 Directly measure on-blaze efficiency in reflection
    26 Si26 Characterize the effect of high temperature annealing on precision optics
    27 Si27 Quantify the Fabry-Pèrot effect of finite thickness Si optics
    The rest are ongoing experimental R&D efforts
    metrology
    process
    make devices
    organization
    design
    R&D

    View Slide

  18. 4 Si04 High spatial resolution measurements of bonded Si pucks
    5 Si05 Characterization of heritage grating surfaces
    6 Si23 Improve UV illumination uniformity
    7 Si22 Reduce the dose-phase curve
    8 Si21 Reduce the UV fringe amplitude
    9 Si07 e-beam silicon immersion grating production
    10 Si06 A contacted grism for Mimir
    11 Si08 Does thermal anneal eliminate IR bubbles in bonded Si?
    12 Si09 L- and M- band immersion grating for iSHELL
    13 Si10 J-, H-, and K- band immersion grating for iSHELL
    14 Si11 ACT immersion grating prototype
    15 Si12 Internal transfer of skills and knowledge I-VI
    16 Si13 Directly measured moderate order HeNe spectral purity of photo masks
    17 Si14 Characterization of stock lab optics with Cary 5000
    18 Si15 The geometrical efficiency loss from dispersion at high λ and m
    19 Si16 SPIE paper idea: applications and specifications for immersion gratings
    20 Si17 A higher performance immersion grating for IGRINS
    21 Si18 Robust inventory and travelers for silicon and optical parts
    22 Si19 Quantify vendor provided defect density, compare to specifications
    23 Si20 Improve Si wafer mounting strategy to better simulate optical surfaces
    24 Si24 Directly measure blaze angle in reflection
    25 Si25 Directly measure on-blaze efficiency in reflection
    26 Si26 Characterize the effect of high temperature annealing on precision optics
    27 Si27 Quantify the Fabry-Pèrot effect of finite thickness Si optics
    Let’s talk about the metrology ones
    metrology

    View Slide

  19. 5 Si05 Characterization of heritage grating surfaces
    16 Si13 Directly measured moderate order HeNe spectral purity of photo masks
    17 Si14 Characterization of stock lab optics with Cary 5000
    24 Si24 Directly measure blaze angle in reflection
    25 Si25 Directly measure on-blaze efficiency in reflection
    27 Si27 Quantify the Fabry-Pèrot effect of finite thickness Si optics
    Let’s talk about the metrology ones

    View Slide

  20. 5 Si05 Characterization of heritage grating surfaces
    16 Si13 Directly measured moderate order HeNe spectral purity of photo masks
    17 Si14 Characterization of stock lab optics with Cary 5000
    24 Si24 Directly measure blaze angle in reflection
    25 Si25 Directly measure on-blaze efficiency in reflection
    27 Si27 Quantify the Fabry-Pèrot effect of finite thickness Si optics
    Let’s talk about the metrology ones
    specifically these two

    View Slide

  21. Si24 Directly measure blaze angle in reflection
    A typical grating has 3 blaze angles.
    The width of the facet is inversely related
    to the breadth of the blaze envelope.

    View Slide

  22. Si24 Directly measure blaze angle in reflection
    A typical grating has 3 blaze angles.
    The width of the facet is inversely related
    to the breadth of the blaze envelope.
    0 degree (groove tops)

    View Slide

  23. Si24 Directly measure blaze angle in reflection
    A typical grating has 3 blaze angles.
    The illuminated width of the facet
    depends on viewing orientation
    Shallow facet
    (e.g. 38° for complement of R3)
    Front surface
    illumination in air

    View Slide

  24. Si24 Directly measure blaze angle in reflection
    A typical grating has 3 blaze angles.
    The illuminated width of the facet
    depends on viewing orientation
    Steep facet
    (e.g. 71.6° for R3)
    Front surface
    illumination in air

    View Slide

  25. Si24 Directly measure blaze angle in reflection
    A typical grating has 3 blaze angles.
    By the way:
    The illuminated width of the facet
    depends on viewing orientation
    Steep facet
    (e.g. 71.6° for R3)
    Front surface
    illumination in air Immersed in Si

    View Slide

  26. Si24 Directly measure blaze angle in reflection
    A typical grating has 3 blaze angles.
    The width of the facet is inversely related
    to the breadth of the blaze envelope.

    View Slide

  27. Si24 Directly measure blaze angle in reflection
    A typical grating has 3 blaze angles.
    The width of the facet is inversely related
    to the breadth of the blaze envelope.
    1
    2
    3
    1.  Groove tops (always 0°)
    2.  Shallow facet (e.g. 38° for complement of R3)
    3.  Steep facet (e.g. 71.6° for R3)

    View Slide

  28. Si24 Directly measure blaze angle in reflection
    A typical grating has 3 blaze angles.
    The width of the facet is inversely related
    to the breadth of the blaze envelope.
    1
    2
    3
    1.  Groove tops (always 0°)
    2.  Shallow facet (e.g. 38° for complement of R3)
    3.  Steep facet (e.g. 71.6° for R3)
    What Astronomers want:
    -know the realized* R3 blaze angle and its uncertainty
    -a small** uncertainty
    -no avoidable*** efficiency loss
    *the realized blaze angle may differ from the design blaze angle since it depends
    intimately on the Si cutting angle (well known) and the anisotropic KOH wet etch
    rates (poorly known, variable)
    **small means negligible contribution to the overall uncertainty in the alignment of
    the spectrograph during integration and testing. Ask Dan Jaffe what X is.
    ***geometrical efficiency loss comes from groove shadowing, which can be
    anticipated in the design.
    δ=
    71.6 ± ε°
    ε << X

    View Slide

  29. Si24 Directly measure blaze angle in reflection
    A typical grating has 3 blaze angles.
    The width of the facet is inversely related
    to the breadth of the blaze envelope.
    Depending on the illumination angle,
    some facets are shadowed.
    shadowed







    What Astronomers want:
    -know the realized* R3 blaze angle and its uncertainty
    -a small** uncertainty
    -no avoidable*** efficiency loss
    *the realized blaze angle may differ from the design blaze angle since it depends
    intimately on the Si cutting angle (well known) and the anisotropic KOH wet etch
    rates (poorly known, variable)
    **small means negligible contribution to the overall uncertainty in the alignment of
    the spectrograph during integration and testing. Ask Dan Jaffe what X is.
    ***geometrical efficiency loss comes from groove shadowing, which can be
    anticipated in the design.

    View Slide

  30. Si24 Directly measure blaze angle in reflection
    A typical grating has 3 blaze angles.
    The width of the facet is inversely related
    to the breadth of the blaze envelope.
    Depending on the illumination angle,
    some facets are shadowed.
    shadowed





    What Astronomers want:
    -know the realized* R3 blaze angle and its uncertainty
    -a small** uncertainty
    -no avoidable*** efficiency loss
    *the realized blaze angle may differ from the design blaze angle since it depends
    intimately on the Si cutting angle (well known) and the anisotropic KOH wet etch
    rates (poorly known, variable)
    **small means negligible contribution to the overall uncertainty in the alignment of
    the spectrograph during integration and testing. Ask Dan Jaffe what X is.
    ***geometrical efficiency loss comes from groove shadowing, which can be
    anticipated in the design.


    Immersed in Si

    View Slide

  31. Si24 Directly measure blaze angle in reflection
    A typical grating has 3 blaze angles.
    The width of the facet is inversely related
    to the breadth of the blaze envelope.
    Depending on the illumination angle,
    some facets are shadowed.
    shadowed





    What Astronomers want:
    -know the realized* R3 blaze angle and its uncertainty
    -a small** uncertainty
    -no avoidable*** efficiency loss
    *the realized blaze angle may differ from the design blaze angle since it depends
    intimately on the Si cutting angle (well known) and the anisotropic KOH wet etch
    rates (poorly known, variable)
    **small means negligible contribution to the overall uncertainty in the alignment of
    the spectrograph during integration and testing. Ask Dan Jaffe what X is.
    ***geometrical efficiency loss comes from groove shadowing, which can be
    anticipated in the design.


    Immersed in Si
    GROOVE TOP SHADOWING MEMO
    MICHAEL GULLY-SANTIAGO
    1. Introduction
    This document describes the geometry of micromachined silicon immersion gratings
    being developed at the University of Texas Department of Astronomy Silicon Diffractive
    Optics Group and the MIT Nanoruler Group. Specifically, we calculate the acceptable
    groove top to pitch length ratio above which the efficiency of the devices is degraded. This
    information is useful for the design of gratings using direct writing systems, where the
    groove width is a free parameter. Maintaining a large groove top to pitch length ratio is
    important to avoid failures during processing, such as undercutting or over etching.
    2. Geometry
    Figure 1 shows an overview of a silicon immersion grating. Figure 2 shows a detail of a
    single groove, chronicling the relevant geometry; the parameters are listed below.
    t is the groove top width
    p is the groove spacing (also called the groove pitch)
    δ is the blaze angle
    a is the silicon etch angle; for this document we adopt a = 70.53

    ,
    the maximum allowable ratio of
    t
    p is given by:
    t
    p =
    1
    1 +
    tan(a)
    tan(δ)
    ,
    So, for the adopted value of a, and tan(δ) = 2 (i.e. an R2 echelle), we have
    t
    p

    = 0.41.
    For an R3 echelle, we have
    t
    p

    = 0.51.
    References
    [Marsh et al.(2007)] Marsh, J. P., Mar, D. J., & Jaffe, D. T. 2007, Applied Optics, 46, 3400
    MICHAEL GULLY-SANTIAGO
    1. Introduction
    This document describes the geometry of micromachined silicon immersion gratings
    being developed at the University of Texas Department of Astronomy Silicon Diffractive
    Optics Group and the MIT Nanoruler Group. Specifically, we calculate the acceptable
    groove top to pitch length ratio above which the efficiency of the devices is degraded. This
    information is useful for the design of gratings using direct writing systems, where the
    groove width is a free parameter. Maintaining a large groove top to pitch length ratio is
    important to avoid failures during processing, such as undercutting or over etching.
    2. Geometry
    Figure 1 shows an overview of a silicon immersion grating. Figure 2 shows a detail of a
    single groove, chronicling the relevant geometry; the parameters are listed below.
    t is the groove top width
    p is the groove spacing (also called the groove pitch)
    δ is the blaze angle
    a is the silicon etch angle; for this document we adopt a = 70.53

    ,
    the maximum allowable ratio of
    t
    p is given by:
    t
    p =
    1
    1 +
    tan(a)
    tan(δ)
    ,
    So, for the adopted value of a, and tan(δ) = 2 (i.e. an R2 echelle), we have
    t
    p

    = 0.41.
    For an R3 echelle, we have
    t
    p

    = 0.51.
    References
    [Marsh et al.(2007)] Marsh, J. P., Mar, D. J., & Jaffe, D. T. 2007, Applied Optics, 46, 3400
    Date: May 27, 2009.
    1
    δ is the blaze angle
    a is the silicon etch angle; for this document we adopt a = 70.53

    ,
    the maximum allowable ratio of
    t
    p is given by:
    t
    p =
    1
    1 +
    tan(a)
    tan(δ)
    ,
    So, for the adopted value of a, and tan(δ) = 2 (i.e. an R2 echelle), we have
    t
    p

    = 0.41.
    For an R3 echelle, we have
    t
    p

    = 0.51.
    References
    [Marsh et al.(2007)] Marsh, J. P., Mar, D. J., & Jaffe, D. T. 2007, Applied Optics, 46, 3400
    Date: May 27, 2009.
    1
    GROOVE TOP SHADOWING MEMO
    MICHAEL GULLY-SANTIAGO
    1. Introduction
    This document describes the geometry of micromachined silicon immersion
    being developed at the University of Texas Department of Astronomy Silicon Di
    Optics Group and the MIT Nanoruler Group. Specifically, we calculate the ac
    groove top to pitch length ratio above which the efficiency of the devices is degrad
    information is useful for the design of gratings using direct writing systems, w
    groove width is a free parameter. Maintaining a large groove top to pitch length
    important to avoid failures during processing, such as undercutting or over etchin
    2. Geometry
    Figure 1 shows an overview of a silicon immersion grating. Figure 2 shows a de
    single groove, chronicling the relevant geometry; the parameters are listed below.
    t is the groove top width
    p is the groove spacing (also called the groove pitch)
    δ is the blaze angle
    a is the silicon etch angle; for this document we adopt a = 70.53

    ,
    the maximum allowable ratio of
    t
    p is given by:
    t
    p =
    1
    1 +
    tan(a)
    tan(δ)
    ,
    So, for the adopted value of a, and tan(δ) = 2 (i.e. an R2 echelle), we have
    t
    p
    For an R3 echelle, we have
    t
    p

    = 0.51.
    References
    [Marsh et al.(2007)] Marsh, J. P., Mar, D. J., & Jaffe, D. T. 2007, Applied Optics, 46, 3400
    Date: May 27, 2009.
    1

    View Slide

  32. Si24 Directly measure blaze angle in reflection
    A typical grating has 3 blaze angles.
    The width of the facet is inversely related
    to the breadth of the blaze envelope.
    1
    2
    3
    1.  Groove tops (always 0)
    2.  Shallow facet (e.g. 38° for complement of R3)
    3.  Steep facet (e.g. 71.6° for R3)
    What Astronomers want:
    -know the realized* R3 blaze angle and its uncertainty
    -a small** uncertainty
    -no avoidable*** efficiency loss
    *the realized blaze angle may differ from the design blaze angle since it depends
    intimately on the Si cutting angle (well known) and the anisotropic KOH wet etch
    rates (poorly known, variable)
    **small means negligible contribution to the overall uncertainty in the alignment of
    the spectrograph during integration and testing. Ask Dan Jaffe what X is.
    ***geometrical efficiency loss comes from groove shadowing, which can be
    anticipated in the design.
    δ=
    71.6 ± ε°
    ε << X


    View Slide

  33. Si24 Directly measure blaze angle in reflection
    A typical grating has 3 blaze angles.
    The blaze angle is encoded in the
    measured brightness of diffraction orders
    3

    View Slide

  34. Si24 Directly measure blaze angle in reflection
    A typical grating has 3 blaze angles.
    The blaze angle is encoded in the
    measured brightness of diffraction orders
    3
    Figure 9 from Marsh, Mar, and Jaffe 2007.
    Jasmina Marsh (a former grad student) did this all the time.
    This technique fell out of favor because the measurement
    was time-consuming and subject to a major systematic
    uncertainty.

    View Slide

  35. Si24 Directly measure blaze angle in reflection
    A typical grating has 3 blaze angles.
    The illuminated width of the facet is
    inversely related to the breadth of the
    blaze envelope.
    Figure 9 from Marsh, Mar, and Jaffe 2007.
    Jasmina Marsh (a former grad student) did this all the time.
    This technique fell out of favor because the measurement
    was time-consuming and subject to a major systematic
    uncertainty.
    3

    View Slide

  36. Si24 Directly measure blaze angle in reflection
    A typical grating has 3 blaze angles.
    The blaze angle of the facet is at the peak
    of the blaze envelope.
    Figure 9 from Marsh, Mar, and Jaffe 2007.
    Jasmina Marsh (a former grad student) did this all the time.
    This technique fell out of favor because the measurement
    was time-consuming and subject to a major systematic
    uncertainty.
    3

    View Slide

  37. Si24 Directly measure blaze angle in reflection
    Figure 9 from Marsh, Mar, and Jaffe 2007.
    Jasmina Marsh (a former grad student) did this all the time.
    This technique fell out of favor because the measurement
    was time-consuming and subject to a major systematic
    uncertainty.
    How do you know which order
    you are in?
    How confident are you that you
    are not off-by-one? (or two or three…)
    For example, how do you know you are
    measuring order #426 and not #427?
    For 426th order, off-by-one means
    uncertainty in blaze angle is ± ε = 1/426
    =0.002 radians
    =0.13°

    View Slide

  38. Si24 Directly measure blaze angle in reflection
    Figure 9 from Marsh, Mar, and Jaffe 2007.
    Jasmina Marsh (a former grad student) did this all the time.
    This technique fell out of favor because the measurement
    was time-consuming and subject to a major systematic
    uncertainty.
    How do you know which order
    you are in?
    How confident are you that you
    are not off-by-one? (or two or three…)
    For example, how do you know you are
    measuring order #426 and not #427?
    For 426th order, off-by-one means
    uncertainty in blaze angle is ± ε = 1/426
    =0.002 radians
    =0.13°
    The solution to this problem is that you
    have to find zero order and start counting
    from zero to 426.

    View Slide

  39. Si24 Directly measure blaze angle in reflection
    We need a rotation stage to rotate the many (~80)
    diffraction orders onto a detector. The detector will
    detect and measure the brightness of every order.
    detector
    Figure 9 from Marsh, Mar, and Jaffe 2007.
    Jasmina Marsh (a former grad student) did this all the time.
    This technique fell out of favor because the measurement
    was time-consuming and subject to a major systematic
    uncertainty.

    View Slide

  40. Si24 Directly measure blaze angle in reflection
    We need a rotation stage to rotate the many (~80)
    diffraction orders onto a detector. The detector will
    detect and measure the brightness of every order.
    This is definitely
    zero order. No
    doubt there.
    0° 71.6°
    We can centroid
    wicked good dude!
    -38°

    View Slide

  41. Si24 Directly measure blaze angle in reflection
    We need a rotation stage to rotate the many (~80)
    diffraction orders onto a detector. The detector will
    detect and measure the brightness of every order.
    BOOM
    shakalaka! This is definitely
    zero order. No
    doubt there.
    0° 71.6°
    We can centroid
    wicked good dude!
    -38°

    View Slide

  42. Si24 Directly measure blaze angle in reflection
    We need a rotation stage to rotate the many (~80)
    diffraction orders onto a detector. The detector will
    detect and measure the brightness of every order.
    0° 71.6°
    -38°
    Actually there are a few challenges:
    Measurements must be done in Littrow, which means
    the non-constant illuminated groove width is a
    nuisance parameter. So results are model-dependent.
    You need huge dynamic range. Like ~ 80 dB?
    You need very-high-precision clocking with a goniometer.
    I don’t actually know how well you can centroid… probably
    depends on the groove spacing and blaze angle.
    Is a bare laser beam OK or do you need to collimate and
    focus? Collimating gives spurious secondary images.

    View Slide

  43. Si24 Directly measure blaze angle in reflection
    We need a rotation stage to rotate the many (~80)
    diffraction orders onto a detector. The detector will
    detect and measure the brightness of every order.
    0° 71.6°
    -38°
    Actually there are a few challenges:
    Measurements must be done in Littrow, which means
    the non-constant illuminated groove width is a
    nuisance parameter. So results are model-dependent.
    You need huge dynamic range. Like ~ 80 dB?
    You need very-high-precision clocking with a goniometer.
    Is a bare laser beam OK or do you need to collimate and
    focus? Collimating gives spurious secondary images.
    I don’t actually know how well you can centroid… probably
    depends on the groove spacing and blaze angle.
    Lock-in amplifier + ND filter + HDR repeats
    Just buy a goniometer!
    Might not be better than Џ= 0.2° which isn’t good enough
    Extra alignment/dithering work.
    See memo.

    View Slide

  44. Si24 Directly measure blaze angle in reflection
    So I actually already did this for CA1.
    Sorta.

    View Slide

  45. Si24 Directly measure blaze angle in reflection
    !"!#$
    $
    %&"$'()'*+$,-./01,$02$01/"13"3$/#$4"$!"5$2#$/.1678!9:;5$.13$!:<7=>?>@=$$A"$B#1/-#C$/&"$4C.
    4#FC"$G0/&$-"2H"B/$/#$/&"$+0C0B#1$B-E2/.C$HC.1"2=$$%&"$I0,F-"$#1$/&"$4"C#G$-0,&/$02$B#H0"3$I-
    /-0.1,C"$02$2K"/B&"3$I#-$.1$!"(,"#!"/-E$#1$/&"$C"I/=$$L"-"5$01!:<7=>?>@5$.13$M$02$/&"$#H/0B
    !"#$%&'()#*#$&'+,),-.#/(0(1,)#2(33+41'(56#78'(1 +,%8#
    %#Y$ +F1,$Z""5$A"02#1,$A.1,5$[.1$\.II"$
    O-#!Y$ U0B&."C$(FCCE6+.1/0.,#$
    MMY$ '()'*+$/".!$
    [./"Y$ SV;VSQ77$
    )"Y$ M]67$4C.D"$.1,C"$
    M#!!"1/2Y$
    $
    %&02$3#BF!"1/$2F!!.-0D"2$/&"$4C.D"$.1,C"$!".2F-"!"1/2$#I$M]75$/&"$'()
    ,-./01,=$$'$!".2F-"$/&"$4C.D"$.1,C"$.2$!:;<=>?#@AB#C=DCE$8G&0B&$&.2$"!:Q=<
    /#$G0/&01$/&"$"--#-2=$
    $
    %&"$'()'*+$,-./01,$02$01/"13"3$/#$4"$!"5$2#$/.1678!9:;5$.13$!:<7=>?>@=$$A"$B#1/-#C$/&"$4C.D"$.1,C"$4E$BF//01,$/&"$+0$
    4#FC"$G0/&$-"2H"B/$/#$/&"$+0C0B#1$B-E2/.C$HC.1"2=$$%&"$I0,F-"$#1$/&"$4"C#G$-0,&/$02$B#H0"3$I-#!$#$%&'()*($+,(-../J$/&"$
    /-0.1,C"$02$2K"/B&"3$I#-$.1$!"(,"#!"/-E$#1$/&"$C"I/=$$L"-"5$01!:<7=>?>@5$.13$M$02$/&"$#H/0B.CCE$.B/0N"$2F-I.B"=$
    $
    $
    %&"-"$.-"$/G#$G.E2$I#-$4$/#$30II"-$!01F/"CE$I-#!$!",$$$
    O0-2/5$/&"$I010/"$.102#/-#H0B$G"/$"/B&$-./0#$#I$20C0B#1$H-#3FB"2$.$2!.CC$01B-".2"5$"!,$01$/&"$,-##N"$.H"P$8.1,C"$
    $$01$/&"$.4#N"$C"I/9=$$O#-$.1$01I010/"$.102#/-#H0B$"/B&$-./0#5$$1;@$02$3"I01"3$4E$/&"$+0$B-E2/.C$2/-FB/F-"$HC.1"2=$$
    A"02#1,$A.1,$.13$#/&"-2$"PH"-0!"1/.CCE$!".2F-"3$.1$.102#/-#H0B$-./0#$#I$>Q67QQ5$.13$.:;@RS"!, G0/&$"!:[email protected]$
    .13$"!$3"I01"3$01$O0,F-"$>$I-#!$U.-2&$"/$.C=$SQQ<$8B#H0"3$#1$/&"$1"P/$H.,"$I#-$B#1N"10"1B"9=$
    +"B#135$/&"$+0$4#FC"$B#FC3$4"$BF/$0!H-"B02"CE=$$'1$/&./$B.2"5$/&"$-"3$C01"$!.-K"3$S$01$/&"$I0,F-"$01$/&"$.4#N"$
    -0,&/$H-#3FB"2$.13$.1,C"$4:3$G&0B&$02$/##$2!.CC$#-$C.-,"=$$%&"$2H"B0I0B./0#1$#1$/&"$.1,C"$I-#!$/&"$N"13#[email protected]$
    G&0B&$02$N"-E$2!.CC5$2#$G"$.-"$B#1I03"1/$/&./$/&"$4#FC"$BF//01,$02$1#/$#F-$40,,"2/$H-#4C"!=$$$A"$.1/0B0H./"3$/&"$
    .102#/-#H0B$"/B&$.1,C"$G&"1$-"XF"2/01,$/&"$+0$4#FC"$BF/$.1,C"5$2#$#F-$I01.C$3"N0B"$G#FC3$4"$);$.I/"-$BF//01,$.13$
    "/B&01,=$
    !"#$%&'()#*#$&'+,),-.#/(0(1,)#2(33+41'(56#78'(1 +,%8#
    %#Y$ +F1,$Z""5$A"02#1,$A.1,5$[.1$\.II"$
    O-#!Y$ U0B&."C$(FCCE6+.1/0.,#$
    MMY$ '()'*+$/".!$
    [./"Y$ SV;VSQ77$
    )"Y$ M]67$4C.D"$.1,C"$
    M#!!"1/2Y$
    $
    %&02$3#BF!"1/$2F!!.-0D"2$/&"$4C.D"$.1,C"$!".2F-"!"1/2$#I$M]75$/&"$'()'*+$H-#/#/EH"$0!!"-20#1$
    ,-./01,=$$'$!".2F-"$/&"$4C.D"$.1,C"$.2$!:;<=>?#@AB#C=DCE$8G&0B&$&.2$"!:Q=<;?EF5$.13$.,-""2$G0/&$!:!"(
    /#$G0/&01$/&"$"--#-2=$

    View Slide

  46. Si24 Directly measure blaze angle in reflection
    !"!#$
    $
    %&"$'()'*+$,-./01,$02$01/"13"3$/#$4"$!"5$2#$/.1678!9:;5$.13$!:<7=>?>@=$$A"$B#1/-#C$/&"$4C.
    4#FC"$G0/&$-"2H"B/$/#$/&"$+0C0B#1$B-E2/.C$HC.1"2=$$%&"$I0,F-"$#1$/&"$4"C#G$-0,&/$02$B#H0"3$I-
    /-0.1,C"$02$2K"/B&"3$I#-$.1$!"(,"#!"/-E$#1$/&"$C"I/=$$L"-"5$01!:<7=>?>@5$.13$M$02$/&"$#H/0B
    !"#$%&'()#*#$&'+,),-.#/(0(1,)#2(33+41'(56#78'(1 +,%8#
    %#Y$ +F1,$Z""5$A"02#1,$A.1,5$[.1$\.II"$
    O-#!Y$ U0B&."C$(FCCE6+.1/0.,#$
    MMY$ '()'*+$/".!$
    [./"Y$ SV;VSQ77$
    )"Y$ M]67$4C.D"$.1,C"$
    M#!!"1/2Y$
    $
    %&02$3#BF!"1/$2F!!.-0D"2$/&"$4C.D"$.1,C"$!".2F-"!"1/2$#I$M]75$/&"$'()
    ,-./01,=$$'$!".2F-"$/&"$4C.D"$.1,C"$.2$!:;<=>?#@AB#C=DCE$8G&0B&$&.2$"!:Q=<
    /#$G0/&01$/&"$"--#-2=$
    $
    $
    %&$!'($)"*"!+",-$./0/-$%$*#1,2"34$!"125,"($67"$+318"$1&93"$+4$*#5&6'&9$67"$#,(",2$:,#!$8",#$6#$67"$+318";$$
    %$:#5&($6716$#,(",$<.$'2$67"$+,'976"26$#,(",$'&$='66,#>$,":3"*6'#&$!"125,"!"&62$"!?3#4'&9$31!+([email protected];<&!$C"D"$
    312",;$$E716$!"125,"!"&6$?31*"($67"$+318"$1&93"$:',!34$'&$67"$,1&9"$F.;A$G$($G$F/;H-$2'&*"$#67",>'2"$#,(",2$>#53($+"$+,'976"26;$$
    I&$J"+,51,4$B-$./00-$%$!"125,"($67"$,"316'K"$'&6"&2'6'"2$#:$67"$#,(",2$25,,#5&('&9$67"$+318";$$E7"$,"316'K"$
    '&6"&2'6'"2$#:$67"2"$#,(",2$1,"$2"&2'6'K"$6#$67"$+318"$1&93";$$%$*#&26,5*6"($1$2*131,$+318"($9,16'&9$!#("3-$>7'*7$
    '&*35("($67"$='66,#>$9"#!"6,4$#:$67"$!"125,"!"&62-$1&($67"$:#,"27#,6"&'&9$#:$67"$#?6'*1334$1*6'K"$25,:1*"$L!$'&$
    J'95,"$0M-$:#,$*12"2$>7"&$67"$9,##K"$:1*"6$'2$271(#>"($+4$67"$9,##K"$6#?;$$E7"$+"26$19,""!"&6$#:$!#("3$1&($
    #+2",K16'#&$#**5,2$:#,$!!"#$%&'()*'+$,+-$L>7'*7$712$"[email protected]/;FBA-.;$$/0121'314256131782'461'9:72;28178'<;80'
    !!=&!"#$>"-?'L>7'*7$712$"[email protected]/;/-.'
    $$
    $

    View Slide

  47. Si24 Directly measure blaze angle in reflection
    !"!#$
    $
    %&"$'()'*+$,-./01,$02$01/"13"3$/#$4"$!"5$2#$/.1678!9:;5$.13$!:<7=>?>@=$$A"$B#1/-#C$/&"$4C.
    4#FC"$G0/&$-"2H"B/$/#$/&"$+0C0B#1$B-E2/.C$HC.1"2=$$%&"$I0,F-"$#1$/&"$4"C#G$-0,&/$02$B#H0"3$I-
    /-0.1,C"$02$2K"/B&"3$I#-$.1$!"(,"#!"/-E$#1$/&"$C"I/=$$L"-"5$01!:<7=>?>@5$.13$M$02$/&"$#H/0B
    !"#$%&'()#*#$&'+,),-.#/(0(1,)#2(33+41'(56#78'(1 +,%8#
    %#Y$ +F1,$Z""5$A"02#1,$A.1,5$[.1$\.II"$
    O-#!Y$ U0B&."C$(FCCE6+.1/0.,#$
    MMY$ '()'*+$/".!$
    [./"Y$ SV;VSQ77$
    )"Y$ M]67$4C.D"$.1,C"$
    M#!!"1/2Y$
    $
    %&02$3#BF!"1/$2F!!.-0D"2$/&"$4C.D"$.1,C"$!".2F-"!"1/2$#I$M]75$/&"$'()
    ,-./01,=$$'$!".2F-"$/&"$4C.D"$.1,C"$.2$!:;<=>?#@AB#C=DCE$8G&0B&$&.2$"!:Q=<
    /#$G0/&01$/&"$"--#-2=$
    $$
    $
    0.2° uncertainty isn’t good enough as it stands.
    We need:
    1)  more better data (i.e. more orders, lower uncertainty)
    2)  Better model

    View Slide

  48. Si24 Directly measure blaze angle in reflection
    The main reason the uncertainty is so large is
    that my scalar diffraction model is bad.
    But of course it is.
    I am most excited about this idea because it is an easy
    experimental way to constrain non-scalar diffraction effects
    that we only ever speculate about.
    Rank gratings in ascending blaze angle much better than 0.2°.
    We will then have a data-driven model.
    Intermediate phases of wet etching- anisotropic etch rate.
    We could pin this relation to CA1, and bootstrap.
    Monitor before and after thermal cycling / aluminization, etc.
    Evidence for groove bottom completion.
    $$
    $

    View Slide

  49. An advert for the other metrology ideas

    View Slide

  50. Si25 Directly measure on-blaze
    efficiency in reflection
    Above: Cary 5000 breadboard accessory with
    custom optical layout. A reference mirror is shown
    on the left. We can put an immersion grating here to
    rapidly measure the near-blaze efficiency.
    Right: Plots from CROWBAR. The top scan was
    taken near Littrow only.
    1.0 1.5 2.0 2.5 3.0
    h (!m)
    0.0
    0.2
    0.4
    0.6
    0.8
    1.0
    Raw efficiency
    70
    75
    80
    85
    90
    95
    100
    110
    120
    130
    140
    150

    View Slide

  51. Si13 Directly measured moderate order HeNe
    spectral purity of photo masks
    Amanda Turbyfill demonstrating the HeNe laser beam
    position at the photo mask. The photomask is
    challenging to measure because it is an unblazed grating.
    Figure 13 from Marsh, Mar, and Jaffe 2007.
    Monochromatic spectral purity can reveal ghosts in
    photomasks down to the 5 nm level, if moderate orders at
    steep enough incidence angles can be reliably measured.
    “Steep enough” is ~10-30°

    View Slide

  52. Si05 Characterization of heritage grating surfaces
    !""#$%%"!&'()'#*(+&,"-,(.
    /!&01()'02*(+&,"
    3,('0/&.#45"&
    6&.7'8&*9
    :"*(;&9
    /*<0"(0;& "*(;&905"0=#>
    ?7'7.).09"*(;&[email protected]&7A!"0790B#>
    C(*0"!7,;&*09"*(;&90)9&0&D&'0
    ').E&*9$0F#>G0H#>0&",-
    6&.&.E&*0"(0&>#5'809"*(;&90
    E&I(*&095D7'A05905'0:JK0
    :7L&
    M5''("0E&[email protected]&*0(*0"544&*0"!5'0
    NOO#>0P5*"E(5*8097L&Q
    :,54&0<()*07,('0"(0I7440590.),!0(I0
    "!&05*"E(5*80590#(997E4&
    R'A*()#
    3I0<()*08&97A'0!590.(*&0"!5'0('&0
    9!5#&G0.5;&09)*&0"(0)'A*()#
    :5D&059
    :5D&0590-:JK05'80.5;&09)*&0
    SR9&0T*"E(5*89U0790,!&,;&8
    NOO#>
    -:JK
    Amanda and I are working on this, and I’m giving a separate presentation on it.

    View Slide

  53. Si27 Quantify the Fabry-Pèrot effect of finite
    thickness Si optics
    This is too complicated to get into right now. Ask Dan Jaffe.

    View Slide

  54. Si14 Characterization of stock lab
    optics with Cary5000
    FEL1450
    0
    10
    20
    30
    40
    50
    60
    70
    80
    90
    1400 1450 1500 1550 1600 1650
    Wavelength (nm)
    Transmission%
    Very simple.
    Our stock lab filters and mirrors will be much more
    useful if we know and verify their properties.

    View Slide

  55. [email protected] |
    astronomer and engineer
    attribution to:
    les vieux garçons, from The Noun Project
    Pierre TORET, from The Noun Project
    Sá Ferreira - Purple Matter, from The Noun Project
    !""#$%%"!&'()'#*(+&,"-,(.
    /!&01()'02*(+&,"
    3,('0/&.#45"&
    6&.7'8&*9
    :"*(;&9
    /*<0"(0;& "*(;&905"0=#>
    ?7'7.).09"*(;&[email protected]&7A!"0790B#>
    C(*0"!7,;&*09"*(;&90)9&0&D&'0
    ').E&*9$0F#>G0H#>0&",-
    6&.&.E&*0"(0&>#5'809"*(;&90
    E&I(*&095D7'A05905'0:JK0
    :7L&
    M5''("0E&[email protected]&*0(*0"544&*0"!5'0
    NOO#>0P5*"E(5*8097L&Q
    :,54&0<()*07,('0"(0I7440590.),!0(I0
    "!&05*"E(5*80590#(997E4&
    R'A*()#
    3I0<()*08&97A'0!590.(*&0"!5'0('&0
    9!5#&G0.5;&09)*&0"(0)'A*()#
    :5D&059
    :5D&0590-:JK05'80.5;&09)*&0
    SR9&0T*"E(5*89U0790,!&,;&8
    NOO#>
    -:JK
    Adriano Emerick, from The Noun Project
    Renee Ramsey-Passmore, from The Noun Project
    Nherwin Ardoña, from The Noun Project
    Thank you.
    Please ask me about the ideas.

    View Slide