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Imaging Spectrometer - Horiba

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Seamless Integration with Synapse<br />

and Symphony ® CCD Detectors<br />

HORIBA Jobin Yvon was the first spectroscopy-based company<br />

to embrace the emerging CCD detector technology and to integrate<br />

the unique two-dimensional capabilities of these detectors<br />

with spectrometer control functions. HORIBA Jobin Yvon has<br />

15 years of experience in manufacturing CCD detectors in-house<br />

and optimizing both our CCD and spectrometer designs for<br />

unmatched spectroscopic performance.<br />

A full line of large and small format CCD chips is available to<br />

work with the spectrometers. Chip innovations from wavelength<br />

optimized back illuminated chips to deep depletion versions are<br />

available in both TE-cooled and LN-cooled housings. Due to<br />

varied parameters of the CCD, spectral coverage and resolution<br />

of the system will depend on the chosen gratings and the<br />

chosen CCD. The following table describes the expected spectral<br />

coverage and resolution of the spectrometers with different<br />

gratings and typical CCD detectors.<br />

Expected Spectral Coverage & Resolution with a Synapse or Symphony CCD **<br />

Grating<br />

(g/mm)<br />

Dispersion<br />

(nm/mm)<br />

<strong>Spectrometer</strong><br />

Mechanical<br />

Range* (nm)<br />

Spectral Coverage<br />

(nm) with<br />

26.7 mm CCD<br />

iHR320<br />

CCDs with 13.5 µm pixels CCDs with 26 µm pixels<br />

Single Pixel<br />

Spectral<br />

Coverage (nm)<br />

Typical<br />

Spectral<br />

Resolution (nm)<br />

Single<br />

Pixel Spectral<br />

Coverage (nm)<br />

Typical Spectral<br />

Resolution (nm)<br />

3600 0.20 0 to 500 5 0.003 0.01 0.005 0.02<br />

2400 0.87 0 to 750 23 0.012 0.04 0.023 0.07<br />

1800 1.38 0 to 1,000 37 0.019 0.06 0.036 0.11<br />

1200 2.31 0 to 1,500 62 0.031 0.09 0.060 0.18<br />

900 3.20 0 to 2,000 85 0.043 0.13 0.083 0.25<br />

600 4.94 0 to 3,000 132 0.067 0.20 0.128 0.39<br />

300 10.12 0 to 6,000 270 0.137 0.41 0.263 0.79<br />

150 20.43 0 to 12,000 545 0.276 0.83 0.531 1.59<br />

Grating<br />

(g/mm)<br />

Dispersion<br />

(nm/mm)<br />

<strong>Spectrometer</strong><br />

Mechanical<br />

Range* (nm)<br />

Spectral Coverage<br />

(nm) with<br />

26.7 mm CCD<br />

iHR550<br />

CCDs with 13.5 µm pixels CCDs with 26 µm pixels<br />

Single Pixel<br />

Spectral<br />

Coverage (nm)<br />

Typical<br />

Spectral<br />

Resolution (nm)<br />

Single<br />

Pixel Spectral<br />

Coverage (nm)<br />

Typical Spectral<br />

Resolution (nm)<br />

3600 0.16 0 to 500 4 0.002 0.01 0.004 0.01<br />

2400 0.53 0 to 750 14 0.007 0.02 0.014 0.04<br />

1800 0.81 0 to 1,000 22 0.011 0.03 0.021 0.06<br />

1200 1.34 0 to 1,500 36 0.018 0.05 0.035 0.10<br />

900 1.84 0 to 2,000 49 0.025 0.07 0.048 0.14<br />

600 2.83 0 to 3,000 76 0.038 0.11 0.074 0.22<br />

300 5.75 0 to 6,000 154 0.078 0.23 0.150 0.45<br />

150 11.58 0 to 12,000 309 0.156 0.47 0.301 0.90<br />

* The system’s optical range will depend not only on the grating groove density, but also the grating blaze angle and the detector’s spectral response.<br />

** Dispersion, Spectral Coverage and Resolution values are given for 500 nm. These values may vary at different wavelengths.

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