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Coldlight

Instruments that measure light by interfering with it.

Est. 1911 · Rotterdam

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Coldlight builds instruments that convert the wave behaviour of light into a number: interferometers, plate cameras, coherence analysers, atmospheric monitors. A 400 mm aperture flat leaves the shop holding its figure to λ/40 at 632.8 nanometres. Below that tolerance a fringe pattern stops describing the wavefront under test and starts describing the errors of the instrument reading it.

No polishing machine finishes that surface. Computer-controlled laps remove material evenly and leave subsurface damage that prints through once the coating goes on; a bench optician reads the live fringe and corrects it by hand, stroke by stroke, until the interferogram goes quiet. The archive’s contact plates are held flat to 2 µm across the holder, because a plate that bows loses fringe order at its edge before the emulsion is exposed. The annealed blanks Coldlight specifies drift 0.9 nm/K, so a lab that cannot hold its air to within a degree cannot hold its glass to within a fringe.

There is no coating, no algorithm and no clever mounting that stands in for a hand that stopped lapping at the correct stroke. An interferometer tells you what the wavefront is doing, or it tells you what the room is doing. It does not do both.

12 accreditations. The earliest granted in 1923, the most recent in 2011. Every one still active on instruments built this year.

  • SINCE 1958
    ICR

    Interlaboratory Calibration Register

    Traceable to national length standard

  • SINCE 1974
    OSC·II

    Optical Standards Consortium

    Class II surface figure accreditation

  • SINCE 1981λ/40

    Wavefront Conformity Board

    Peak to valley across full aperture

  • SINCE 1923
    GMR

    Guild of Metrological Refiners

    Master grade, continuous since admission

  • SINCE 1996ATM-7

    Atmospheric Instrument Panel

    Sealed to 7 bar, salt fog qualified

  • SINCE 1967
    OBS

    Observatory Supply Directorate

    Approved supplier, primary optics

  • SINCE 2004D·9

    Dispersion Test House

    Nine-line spectral verification

  • SINCE 1989VRT

    Vertical Reference Assembly

    Gravimetric alignment, 0.2 arcsec

  • SINCE 2011ECL

    Extreme Conditions Laboratory

    Rated 218 K to 341 K without drift

  • SINCE 1948
    HRT

    Heritage Register of Trades

    Protected workshop, hand-figured optics

  • SINCE 1999CHR

    Coherence Measurement Panel

    Verified to 40 m coherence length

  • SINCE 1986
    A·400

    Aperture Certification Office

    400 mm clear aperture, edge to edge

Facility readout.

Figures as logged this quarter, not projected.

Coldlight / current
Years in operation
115
Instruments in service
640
Oldest under active calibration contract
Delivered 1953
Best wavefront error achieved
λ/40
Largest clear aperture handled
400 mm

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