L Band Starlight Speckles with the MMT Adaptive Optics System

L Band Starlight Speckles with the MMT Adaptive Optics System

MMT M-band speckles computed from AO WFS vs actual Clio2 images.Подробнее

MMT M-band speckles computed from AO WFS vs actual Clio2 images.

dOTF Wavefront Sensor simulation using the 6.5m MMTПодробнее

dOTF Wavefront Sensor simulation using the 6.5m MMT

Illustration of AO Lag Error.Подробнее

Illustration of AO Lag Error.

SJAA SIG Adaptive Optics Elinor GatesПодробнее

SJAA SIG Adaptive Optics Elinor Gates

Speckle imaging over a 4.25 km horizontal pathПодробнее

Speckle imaging over a 4.25 km horizontal path

A starlight wind sensor derived from MMT adaptive optics wavefront sensor dataПодробнее

A starlight wind sensor derived from MMT adaptive optics wavefront sensor data

30 fps residual MMT AO average speckle intensityПодробнее

30 fps residual MMT AO average speckle intensity

AO on offПодробнее

AO on off

Adaptive Optics SystemПодробнее

Adaptive Optics System

Adaptive optics Top # 6 FactsПодробнее

Adaptive optics Top # 6 Facts

Magellan Adaptive Optics Loop Closing In The Test TowerПодробнее

Magellan Adaptive Optics Loop Closing In The Test Tower

A snippet of raw Fomalhaut data using the VLT NACO APP coronagraphПодробнее

A snippet of raw Fomalhaut data using the VLT NACO APP coronagraph

Lab Demonstration of DMPAC Antihalo servo in the labПодробнее

Lab Demonstration of DMPAC Antihalo servo in the lab

Adaptive Optics | Introductory Astronomy Course 3.04Подробнее

Adaptive Optics | Introductory Astronomy Course 3.04

VLT APP Test image of a bright starПодробнее

VLT APP Test image of a bright star

Closing the Adaptive Optics Loop with Magellan AO systemПодробнее

Closing the Adaptive Optics Loop with Magellan AO system