Virtual Office Hours

Gather on Fridays at 11 AM PST | 2 PM EST for virtual office hours.

We’ll work through a topic of the week (roughly 30 minutes) and discuss any questions that come up along the way. In April & May 2023 we’ll talk about how to care for your SEC-MALS or FFF-MALS system, help you brush up on your ASTRA and DYNAMICS data processing, discuss measuring dn/dc values and why dn/dc is important, and see how stable RI baselines are achievable.

Working with polydisperse samples? We’ll see how to leverage ASTRA’s distribution analysis and results fitting features. Special topics on error analysis, batch MALS work, and more.

Virtual Office Hours are 100% live sessions, with anonymous Q&A welcome during and after the discussion. Free for all Wyatt customers.

Register below! Virtual Office hours are held on select Friday afternoons at 11 AM PST | 2 PM EST.

 
 

Hosted by: Dr. Andy Meyer

Dr. Andy Meyer joined Wyatt Technology in 2001, serving for several years as an Applications Scientist, then as Dean of Wyatt's "Light Scattering University" and as Director of Customer Service & Support. After managing multiple regions in North America, Dr. Meyer is now a Senior Application Scientist for Wyatt. As a Wyatt customer, he completed his Ph.D. in Applied Science – Polymer Chemistry from the College of William and Mary in Virginia.

2023 Dates

Topic

June 9
11 AM PST | 2 PM EST

ASTRA Data Processing: Optimizing Baselines & Peak Settings
- Strategy for drawing baselines & peaks in ideal and non-ideal situations
- Interpreting peaks from MALS, RI, UV detection
- Reviewing ASTRA’s tools for automatic baseline settings and digital noise reduction

Register
June 16
11 AM PST | 2 PM EST

ASTRA Data Processing: System Coefficients (Normalization, Calibration, Alignment and More)
- Normalization, alignment, band broadening: When, why, and how
- Revisiting detector calibration coefficients: When, why, and how

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June 23
11 AM PST | 2 PM EST

ASTRA Data Processing: Light Scattering Plots, Mass Recovery, Data Exporting
- Mass recovery %
- Working with the light scattering plot, slice by slice
- Using Zimm, Debye, and Berry models
- Choosing the best set of detector signals for analysis
- Data exporting tools

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July 14
11 AM PST | 2 PM EST

AAV Characterization via SEC-MALS: Pro Tips & Best Practices

Register
July 21
11 AM PST | 2 PM EST

All About QELS: Flow-related Concepts, QELS Data Processing, and Maximizing Success

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July 28
11 AM PST | 2 PM EST

AAV & LNP Characterization via FFF-MALS: Pro Tips & Best Practices, Co-hosted with John Champagne, Ph.D.

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August 4
11 AM PST | 2 PM EST

Managing UV & RI Data & Instrument Coefficients in ASTRA; Calculating ASTRA Peak Mass Recovery

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August 11
11 AM PST | 2 PM EST

Choosing the Ideal SEC column for SEC-MALS Characterization, Co-hosted with Michelle Chen, Ph.D.

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August 18
11 AM PST | 2 PM EST

All About DLS Temperature Transitions: Thermal Work with the NanoStar-II and DLS Plate Reader

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August 25
11 AM PST | 2 PM EST

DLS Data Interpretation: Regularization vs. Cumulants, Reducing Incomplete Acquisitions; Using Dynamics Data Filters

Register

Register below! Virtual Office hours are held on select Friday afternoons at 11 AM PST | 2 PM EST.