Description
Specifications Table
| Product Name | Stray light filter, 200 nm (RSPEC00411) UV-VIS spectroscopy stray light standard | VWRC84789.180 | Avantor |
|---|---|
| Quantity/Pack Size | 100 ml |
| Form | Liquid |
| Grade | Spectroscopy Grade |
| Application | UV-VIS spectroscopy stray light calibration |
Product Description
When it comes to UV-VIS spectroscopy, accuracy is everything. Even the smallest amount of stray light can skew your results, leading to unreliable data. That’s where the Stray Light Filter, 200 nm (RSPEC00411) comes in. Designed specifically for UV-VIS spectroscopy, this high-quality standard helps you measure and correct stray light in your instruments, ensuring your readings are as precise as possible.
Whether you’re a student working on a research project, an educator setting up lab experiments, or a researcher fine-tuning your spectroscopy methods, this stray light filter is an essential tool. It’s formulated to meet strict spectroscopy-grade standards, so you can trust it to deliver consistent performance every time. The 100 ml pack size is perfect for regular lab use, giving you enough volume for multiple calibrations without frequent reordering.
Using this filter is straightforward. Simply follow your instrument’s calibration protocol, and you’ll be able to detect and compensate for stray light interference. This is especially important when working with samples that have low absorbance or when you need to measure trace components. With this filter, you can be confident that your UV-VIS spectroscopy results are free from the errors that stray light can introduce.
At eqipped, we understand the importance of reliable lab supplies. That’s why we offer this stray light filter from Avantor, a brand known for its commitment to quality and precision. When you buy from us, you’re not just getting a product—you’re getting a tool that helps you achieve accurate, reproducible results in your lab work.
Need a stray light filter for your UV-VIS spectroscopy setup? Order the Stray Light Filter, 200 nm online today and ensure your instrument is calibrated for precision.
This filter is particularly useful for applications where even minor deviations can impact your findings. Whether you’re analyzing pharmaceutical compounds, environmental samples, or conducting academic research, having a reliable stray light standard is crucial. It’s also a great addition to any lab that wants to maintain the highest standards of instrument performance.
If you’re unsure about how to use this filter or need guidance on integrating it into your workflow, our team at eqipped is here to help. We’re committed to supporting students, researchers, and educators with the right tools and knowledge to succeed in their work.
FAQs
What is a stray light filter used for in UV-VIS spectroscopy?
A stray light filter is used to measure and correct the amount of unwanted light that reaches the detector in a UV-VIS spectrometer. This ensures that your absorbance readings are accurate, especially at low wavelengths like 200 nm.
How often should I calibrate my UV-VIS spectrometer with this filter?
It’s recommended to calibrate your instrument with a stray light filter whenever you notice inconsistencies in your results or as part of your regular maintenance schedule, typically every few months depending on usage.
Can this filter be used with any UV-VIS spectrometer?
Yes, this stray light filter is designed to be compatible with most standard UV-VIS spectrometers. However, always check your instrument’s manual for specific calibration requirements.
What is the shelf life of this stray light filter?
When stored properly in a cool, dry place and kept sealed, this filter has a long shelf life. However, it’s best to use it within a year of opening for optimal performance.
Is this filter suitable for educational labs?
Absolutely. This stray light filter is ideal for educational settings where students are learning about UV-VIS spectroscopy and the importance of instrument calibration. It’s a great tool for teaching accurate measurement techniques.
