







|
EXAGE
Wafer Defect Inspection System |
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Union Optical EXAGE
Wafer Defect Inspection System (IWR-200) |

System 3 & 4 shown.
The Union Optical EXAGE IWR-200 Wafer Defect Inspection
System has been designed to achieve an overall system performance that requires an
accuracy of 0.2µm or less by making use of the world's highest level of technology.
The EXAGE system flexibly responds to the thorough and stringent inspection requirements
in industry.
The EXAGE has a high degree of expandability so that the
most up-to-date inspection system can be customized by utilizing a variety of optional
accessories. This is an inspection system that can be upgraded depending on how it is
used.

Many functions to prevent
overlooking even minor defects
- Brightfield observation
- Darkfield observation
- Brightfield Polarized Light observation
- Brightfield Transmitted Light observation
- Nomarski Interference Contrast observation
Wide selection of
magnification changes: 50X to 9400X
Sophisticated Software
- Windows NT®
- Various observation modes can be selected from the recipe
and set electronically and instantly.
- High speed communications between the microscope and PC.
- Observational images can be transferred to optional PCs in a
network.
- Defects can be promptly identified by linking them with the
coordinate systems of related inspection equipment.
Shelter design to perfectly protect
wafers from static electricity and contamination
- Dust-protective body shape and anti-static coating prevent
dust accumulation.
- Operations to be performed on the stage, such as changing
the objective, selecting the speculum, adjusting the aperture diaphragm, etc., are
electrically performed so that dust falling onto a specimen can be avoided.
Operation board to prevent useless
motions
- User interface to make the setting of observation modes
easy.
- The software control system makes all operational modes
simple, increasing the efficiency of inspection works.
The system table has been
ergonomically designed so as to be operator-friendly


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Hardware |
Software |
| Manual
Stage |
Auto
Stage |
Wafer
Transport System |
Optional
Equipment |
Online
Communication |
| System 1 |
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|
|
|
|
| System 2 |
|
 |
|
Stage |
|
| System 3 |
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|
 |
Stage Wafer
Transport System |
|
| |
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| System 4 |
|
 |
 |
Stage Wafer
Transport System |
Related Inspection System, etc. |

The magnification change system and the speculum selecting
system required for metallographic observations have been realized by adopting the
infinity-corrected optical system. The system incorporates the plan apochromatic
objectives having high-resolution, high-contrast, and long working distance, manufactured
based on the fusion of the optical design and lens manufacturing technologies that Union
Optical had been developing for many years. The combination of widefield eyepieces and
various kinds of photographic lenses makes it possible to deal with all kinds of
observation methods and the output of image information.
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Plan
apochromatic objectives, and objectives of SPLIC series and Epi-SPLIC series, with
high-resolution, high-contrast, and long working distance, have been installed. The system
incorporates newly-designed objectives with super-high magnifications, such as 150X (NA
0.95) series and 250X (NA 0.95) series, covering the inspection works for all sorts of
specimens.
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The
field diameter of 26mm is secured by using the newly-designed widefield eyepiece, HUW10X.
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Intermediate
magnification changers including 1.25X, 1.6X, 2.0X, and 2.5X are now available, and the
observation at the maximum magnification of 9400X was made possible by combining the 250X
objective lens with the 15X eyepieces.
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When
CCD cameras of various sizes are used, by using 0.3X and 0.5X photographic lenses, an
image having almost the same field of view as seen through the eyepieces can be observed.
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The
coaxial incident-light illuminator and the transmitted light illuminator (optional) have
been installed. By advancing the concept of Union Optical's unique multi-image modular
system further, respective observation methods based on various systems including
Brightfield, Darkfield, Polarization, Nomarski Interference Contrast, and Transmitted
Light illumination (optional) systems can now be controlled by the controller in one
compact area.
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For further information and specifications on the EXAGE
Wafer Defect Inspection System, please contact us.
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Copyright © 1998,
Terran Technology, Inc.; Labtek Division
Last modified: November 06, 2012 |