A stellar way to overcome barriers for discovery verification
This is the first in a multi-part blog series highlighting the key pillars and impressive benefits of the Stellar mass spectrometer—the first-of-its-kind solution purpose-built for discovery verification. Stay tuned for more blog posts in the series.
If you were a handyman, you wouldn’t dream of using a wrench as a hammer, or a screwdriver as a chisel. You always need the right tool for the job. Same is true for clinical and translational researchers, who depend on having the right solution to maximize their productivity while advancing their research.
The challenge: A missing tool in the discovery-to-validation workflow
For decades, clinical and translational researchers have struggled with biomarker verification workflows due to a technology gap. There’s no current technology that simultaneously addresses the scale, sensitivity and throughput demands without some serious drawbacks. You know this well.
Triple quad technology performing multiple reaction monitoring (MRM) is challenged to keep up with limited capacity to handle massive target lists while quantifying at lower limits using faster LC gradients.
HRAM MS technology performing parallel reaction monitoring (PRM) are challenged to maintain high sensitivity with high acquisition speeds to function with high throughput at experimental scale.
The breakthrough solution: The first-of-its kind verification-class MS
Researchers struggling to fill the technology gap need not struggle any more. The first-to-market Thermo Scientific Stellar mass spectrometer expertly addresses the shortcomings of both ends of the existing verification-based mass spectrometer spectrum with its:
- Expanded scale – The Stellar MS expands biomarker candidate verification per unit time while covering a wider range of compound classes. For proteomics and metabolomics, the expanded scale enables researchers to include more stable isotope labeled standards (SIS) without having to drop endogenous targets, enabling absolute quantitation for better statistical analysis, plus method standardization.
- Higher sensitivity – It generates data incredibly fast, but still maintains excellent sensitivity to enable accurate measurements and better putative biomarker stratification. With its impressive quantitative performance, this mass spectrometer minimizes the risk of false negatives. The sensitivity of quantitation extends dynamic range in association with the expanded scale to provide both breadth and depth of sample analysis.
- Greater specificity – The Stellar mass spectrometer’s ability to acquire full scan MS2 and MS3 enables greater specificity by measuring all product ions associated with the precursor analyte, ensuring quantitative confidence in your targets of interest. It can detect smaller signal changes between donor groups (e.g., diseased and healthy), which ensures your measured expression levels are attributed to your target compound and not to background isomeric/isobaric interferences.
- Massive throughput – It provides the capacity to process all the samples in a study faster, which increases the laboratory capacity for more projects or expand the study size which increases statistical power for more confidence. Combined with the Thermo Scientific Vanquish Neo UHPLC system that delivers chromatographic performance from 0.1 to 100 µL/min, the Stellar MS has the acquisition speed to improve throughput 3-5X compared to methods using existing QQQ and HRAM instrumentation.
- Unrivaled quantitative productivity – Measuring a large number of targets is one thing, but how do researchers build these highly multiplexed methods? Traditionally, this process has been slow, painful and costly, requiring either direct infusion or many replicate injections followed by manual data evaluation. With the Stellar MS, researchers can go from building a method to completing an entire study faster while maintaining high data quality and confidence in results.
Stay tuned for part 2! Find the original article here
Discover more about the one of its kind Stellar Mass Spectrometer here