Diagnostics

Scanning Autocorrelators

Input wavelength range Input pulse duration Sensitivity Input rep. rate Temporal resolution
AA-DD 450-3200 nm 10 fs - 30 ps 100 mW^2 >10 Hz 0.09...1.22 fs
AA-M 450-2000 nm 20 fs - 12 ps 100 mW^2 >10 kHz 0.16...0.64 fs
IRA 450 nm - 11 um 50 fs - 250 ps from 1 nJ from 10 Hz 8.3 fs

Single-Shot Autocorrelators

Input wavelength range Input pulse duration Sensitivity Input rep. rate Temporal resolution
ASF 400-2200 nm 5 fs...15 ps 1 uJ in single-shot mode single...150 MHz 2.3...4 fs

SPIDER

Input wavelength range Input pulse duration Sensitivity Input rep. rate Spectrometer
SPIDER 550-1100 nm 5-320 fs 100 mW or 1 uJ any built-in 2-channel

Third-Order Cross-Correlators

Input wavelength range Scan range Sensitivity Dynamic range Delay resolution
COMET 700-1500 nm up to 4 ns 50-100 uJ 10^10 100 fs

Spectrometers

Spectral range Spectral resolution Dynamic range Focal distance Dimensions
ASP-75 190-1100 nm 0.05...1 nm 1000:1 75 mm 126x68x53 mm
ASP-150 190-1100 nm 0.017...0.6 nm 1000:1 150 mm 205...242x115x76 mm
ASP-IR 500-1700 / 900-2600 / 1200-3450 nm 0.5...1.2 nm 3x10^5...6x10^4 150 mm 225...295x136x81 mm

Latest News

Ultrafast Phenomena 2018 in Hamburg (15-20 July)

Avesta is participating in Ultrafast Phenomena 2018 conference and tabletop exhibition in Hamburg, Germany (15-20 July). We would be glad to discuss any of the ongoing and future projects with the ultrafast community at our tabletop. Hope to see you soon!

New Year Holidays: 30 Dec 2017 – 08 Jan 2018

Avesta’s facilities will be closed for the New Year break from 30 Dec 2017 till 08 Jan 2018. We will resume all operations on 09 Jan 2018. However, we hope to provide periodic e-mail correspondence during the holidays. We wish you a fruitful and prosperous Year 2018!

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