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Ocean Optics - Inventor of the World's First Miniature Spectrometer
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Jaz Optical Bench Options
Jaz's
spectrometer module is designed to give you options that allow you to configure the bench for your application. Our
Applications Scientists can help you choose the optimum components, or you
can follow this guide to choose an entrance aperture size, detector
accessories, filters, a grating and more. Jaz features an asymmetrical crossed Czerny-Turner optical bench
(which has no moving parts that can wear or break) and an innovative,
replaceable aperture design.
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1 |
SMA 905 Connector |
Light from a fiber
enters the optical bench through the SMA 905 Connector. The SMA 905
bulkhead provides a precise locus for the end of the optical fiber,
fixed slit, absorbance filter and fiber clad mode aperture.
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2 |
Interchangeable Entrance Slit
(specify slit size) |
Light passes through
the installed slit, which acts as the entrance aperture. Slits come in
various widths from 5 µm to 200 µm and can be replaced by qualified
users. The slit is fixed in the SMA 905
bulkhead to sit against the end of a fiber. |
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3 |
Longpass Absorbing Filter
(optional) |
If selected, an
absorbance filter is installed between the slit and the clad mode
aperture in the SMA 905 bulkhead. The filter is used to block second-
and third-order effects or to balance color. |
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4 |
Collimating Mirror
(specify standard or SAG+) |
The collimating mirror
is matched to the 0.22 numerical aperture of our optical fiber. Light
reflects from this mirror, as a collimated beam, toward the grating.
You can opt to install a standard mirror or a UV absorbing SAG+
mirror. |
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5 |
Grating & Wavelength
Range
(specify grating & starting wavelength) |
We install the grating
on a platform that we then rotate to select the starting wavelength
you’ve specified. Then we permanently fix the grating in place to
eliminate mechanical shifts or drift. |
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6 |
Focusing Mirror
(specify standard or SAG+) |
This mirror focuses
first-order spectra on the detector plane. Both the collimating and
focusing mirrors are made in-house to guarantee the highest
reflectance and the lowest stray light possible. You can opt to
install a standard or SAG+ mirror. |
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7 |
L2 Detector Collection
Lens |
This cylindrical lens,
made in-house to ensure aberration-free performance, is fixed to the
detector to focus the light from the tall slit onto the shorter
detector elements. It increases light-collection efficiency. |
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8 |
Detector |
Jaz features the 2048-element Sony ILX511B linear CCD array detector.
Each pixel responds to
the wavelength of light that strikes it. Electronics bring the
complete spectrum to the software. |
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9 |
OFLV Variable Longpass
Order-sorting Filter
(optional) |
Our proprietary filters
precisely block second- and third-order light from reaching specific
detector elements. |
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10 |
UV2
Detector Upgrades |
When selected, the
detector’s standard BK7 window is replaced with a quartz window to
enhance the performance of the spectrometer for applications <340 nm. |
A precision SMA 905 Connector aligns to the
spectrometer’s entrance slit and ensures concentricity of the fiber. For
an upgrade fee that includes the cost of the custom connector and labor,
we will replace the standard SMA 905 Connector with a different connector
of your choice. We also offer connector adapters, such as an SMA-to-ST
Adapter and an SMA-to-FC Adapter. Please call for details on custom
connectors and adapters.
Another Jaz optical bench option is the size of the entrance aperture. Entrance slits are
rectangular apertures, 1-mm tall and various widths from 5 µm to 200 µm,
with the width determining the amount of light entering the bench. Note
that the smallest slit achieves the best optical resolution. (For more on
how your slit choice affects optical resolution,
click
here.) Unlike the fixed slits in most spectrometers, the Jaz slit is
designed to be easily interchangeable by a qualified user. This is a
great convenience for anyone who needs to adjust the amount of signal
entering the spectrometer. Contact an Applications Scientist for
additional information about changing slits in the field. Also, you can
opt against having a slit, in which case the diameter of the fiber
connected to the spectrometer determines the size of the entrance
aperture.
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Slit |
Description |
Pixel Resolution |
Price |
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INTSMA-005 |
5-µm wide x 1-mm high |
~3.0 pixels |
$174 |
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INTSMA-010 |
10-µm wide x 1-mm high |
~3.2 pixels |
$174 |
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INTSMA-010S |
10-µm
wide x 50 µm high |
~3.2
pixels |
$174 |
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INTSMA-025 |
25-µm wide x 1-mm high |
~4.2 pixels |
$174 |
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INTSMA-050 |
50-µm wide x 1-mm high |
~6.5 pixels |
$174 |
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INTSMA-100 |
100-µm wide x 1-mm high |
~12.0 pixels |
$174 |
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INTSMA-200 |
200-µm wide x 1-mm high |
~24.0 pixels |
$174 |
We offer longpass absorbing or blocking
filters; each filter has a transmission band and a blocking band to
restrict radiation to a certain wavelength region for eliminating second-
and third-order effects. These filters are installed permanently between
the slit and the clad mode aperture in the bulkhead of the SMA 905
Connector.
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Item |
Description |
Price |
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OF1-WG305 |
Longpass filter; transmits light >305 nm |
$81 |
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OF1-GG375 |
Longpass filter; transmits light >375 nm |
$59 |
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OF1-GG475 |
Longpass filter; transmits light >475 nm |
$59 |
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OF1-OG515 |
Longpass filter; transmits light >515 nm |
$59 |
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OF1-OG550 |
Longpass filter; transmits light >550 nm |
$59 |
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OF1-OG590 |
Longpass filter: transmits light >590 nm |
$59 |
You can replace standard aluminum-coated
reflective mirrors with our proprietary, UV-absorbing SAG+ Mirrors, which
increase reflectance in the VIS-NIR and, in turn, increase the sensitivity
of the spectrometer. SAG+ Mirrors are often specified for fluorescence.
These mirrors also absorb nearly all UV light, which reduces the effects
of excitation scattering in fluorescence measurements. Unlike typical
silver-coated mirrors, the SAG+ mirrors won't oxidize. They have excellent
reflectivity -- more than 95% across the VIS-NIR. The price of the SAG+UPG
is $290.
You choose from among 14 gratings for each
spectrometer channel. With each grating, you consider its groove density (which
helps determine the resolution), its spectral range (which helps determine
the wavelength range) and its blaze wavelength (which helps determine the
most efficient range). Click here for your Grating & Wavelength Choices.
Predicted Ranges &
Resolutions
See a series of graphs to demonstrate the
predicted Range and Resolution of
your Jaz system (Jas has a USB-series optical bench).
At right is a detector with the L2 lens. This
cylindrical lens, made in-house to ensure aberration-free performance, is fixed
to the detector’s window to focus the light from the tall slit onto the shorter
detector elements. It increases light-collection efficiency and reduces stray
light. It also is useful in a configuration with a large-diameter fiber for low
light-level applications. An L2 Detector Collection Lens is
$174.
The Jaz uses the
Sony ILX511B
linear silicon CCD array detector. This detector has response from
200-1100 nm, with sensitivity of 75 photons/count at 400 nm and 41
photons/count at 600 nm.
Our OFLV Variable Longpass Order-sorting Filters are
applied to the detector’s window to eliminate second- and third-order effects.
We use patented coating technology to apply the filter onto the substrate. In
fact, we are the only miniature spectrometer manufacturer to offer “clean”
first-order spectra.
When you specify a detector with the UV2 Detector Window Upgrade, we replace the
detector’s standard BK7 window with a quartz window to enhance the
spectrometer‘s performance from 200-340 nm. The UV2 is available with the DET2B-UV Detector.
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Detector |
Description |
Detector
Price |
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DET2B-VIS |
2000-series detector installed into a Jaz Spectrometer; best for systems
with wavelength ranges above 350 nm. |
$0
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DET2B-UV |
2000-seres detector with UV2 Detector Window
Upgrade installed into a Jaz
Spectrometer; best for systems with wavelength ranges in
the UV |
$174
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an
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Applications Scientist

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