The ASML Right Field Detector, part number 874-0084-002 (also identified as 126442), is a precision photodiode‑based sensor module designed to measure the intensity and uniformity of the exposure light field in deep ultraviolet (DUV) lithography systems. It is typically mounted at the edge of the projection field to provide real‑time feedback for dose control and illumination optimization.
The detector uses a silicon PIN photodiode with a custom interference filter that shapes the spectral response to match the DUV wavelength (e.g., 248 nm or 193 nm, depending on system configuration). The photodiode operates in photovoltaic mode, providing excellent linearity over a dynamic range of 1 nW to 10 mW. The detector is temperature‑stabilized by a built‑in thermoelectric cooler (TEC) and a feedback control loop, ensuring that the responsivity drift is less than 0.1% per °C. The output signal is fed to a transimpedance amplifier, producing a voltage proportional to the incident optical power.
Spectral Range: 190 – 400 nm (DUV, with peak at 248 nm and 193 nm options)
Responsivity: 0.25 A/W at 248 nm (typical)
Active Area: 3 mm x 3 mm (square)
Measurement Range: 10 µW to 100 mW (with adjustable gain)
Non‑linearity: < 0.5% over full range
Noise Equivalent Power (NEP): < 1 pW/√Hz at 10 Hz
Temperature Control: 25 °C ± 0.1 °C
Output Signal: 0‑10 V analog (BNC connector)
Power Supply: ±15 V DC @ 0.5 A each, plus 5 V DC @ 0.2 A for TEC
This detector is positioned at the right‑hand side of the exposure field, outside the projection lens aperture, to sample a portion of the illumination beam. It measures the incident power after the reticle and before the wafer, providing a direct indication of the dose delivered to the wafer surface. The signal is used by the dose control loop to adjust the pulse energy of the excimer laser or the exposure time, ensuring that each die receives the exact energy required. Additionally, by scanning the detector across the field (via stage movement), the system can map the illumination uniformity and correct for any gradient via adjustable attenuators.
Mount the detector on the field‑measurement bracket using the two M4 screws. The active area must be precisely positioned at the same height as the wafer plane. Connect the power cable (15‑pin D‑sub) and the BNC signal cable to the corresponding ports on the measurement electronics. After mechanical installation, align the detector by using a visible pilot laser and adjusting the bracket until the beam is centered on the active area. The alignment is critical; a misalignment of more than 0.5 mm can cause significant measurement errors.
The detector is factory‑calibrated against a NIST‑traceable standard photodiode at the specific DUV wavelength. A calibration certificate is provided with the unit. In the field, verification can be performed using a reference light source with a known output; the system software includes a calibration routine that compares the detector reading with the expected value. If the reading deviates by more than 2%, the gain factor can be adjusted via a trim potentiometer on the amplifier board. Recalibration should be carried out annually or whenever the detector is exposed to high‑humidity or contamination.
The detector window (quartz) should be cleaned quarterly with a mixture of isopropanol and deionized water, using a soft swab. Avoid scratching the surface. The TEC and the cooling fan (if present) should be checked for proper operation; if the temperature exceeds 30 °C, the fan may be clogged. Common faults: “No Signal” – check the BNC cable and verify that the power supplies are on; “Unstable Reading” – ensure that the detector is shielded from ambient light and that the grounding is adequate. If the detector response becomes non‑linear, the photodiode may be saturated; reduce the incident power or switch to a lower‑gain range. The detector is not repairable at component level; replace the entire module if performance degrades beyond specifications.



