Add to ORKGWe present an overview of the design of IRIS, an infrared (0.85 - 2.5 micron) integral field spectrograph and imaging camera for the Thirty Meter Telescope (TMT). With extremely low wavefront error (<30 nm) and on-board wavefront sensors, IRIS will take advantage of the high angular resolution of the narrow field infrared adaptive optics system (NFIRAOS) to dissect the sky at the diffraction limit of the 30-meter aperture. With a primary spectral resolution of 4000 and spatial sampling starting at 4 milliarcseconds, the instrument will create an unparalleled ability to explore high redshift galaxies, the Galactic center, star forming regions and virtually any astrophysical object. This paper summarizes the entire design and basic capabiliti...
With the successful completion of our preliminary design phase, we will present an update on all des...
With the successful completion of our preliminary design phase, we will present an update on all des...
We present sensitivity estimates for point and resolved astronomical sources for the current design ...
We present an overview of the design of IRIS, an infrared (0.85 - 2.5 micron) integral field spectro...
We present an overview of the design of IRIS, an infrared (0.84 - 2.4 micron) integral field spectro...
We present an overview of the design of IRIS, an infrared (0.84 - 2.4 micron) integral field spectro...
We present an overview of the design of IRIS, an infrared (0.84 - 2.4 micron) integral field spectro...
We present an overview of the design of IRIS, an infrared (0.84 - 2.4 micron) integral field spectro...
IRIS is a near-infrared (0.84 to 2.4 micron) integral field spectrograph and wide-field imager being...
The InfraRed Imaging Spectrograph (IRIS) is a first-light instrument being designed for the Thirty M...
The InfraRed Imaging Spectrograph (IRIS) is a first-light instrument being designed for the Thirty M...
The InfraRed Imaging Spectrograph (IRIS) is a first-light instrument being designed for the Thirty M...
The Infra-Red Imaging Spectrograph (IRIS) is one of the three first light instruments for the Thirty...
The Infra-Red Imaging Spectrograph (IRIS) is one of the three first light instruments for the Thirty...
With the successful completion of our preliminary design phase, we will present an update on all des...
With the successful completion of our preliminary design phase, we will present an update on all des...
With the successful completion of our preliminary design phase, we will present an update on all des...
We present sensitivity estimates for point and resolved astronomical sources for the current design ...
We present an overview of the design of IRIS, an infrared (0.85 - 2.5 micron) integral field spectro...
We present an overview of the design of IRIS, an infrared (0.84 - 2.4 micron) integral field spectro...
We present an overview of the design of IRIS, an infrared (0.84 - 2.4 micron) integral field spectro...
We present an overview of the design of IRIS, an infrared (0.84 - 2.4 micron) integral field spectro...
We present an overview of the design of IRIS, an infrared (0.84 - 2.4 micron) integral field spectro...
IRIS is a near-infrared (0.84 to 2.4 micron) integral field spectrograph and wide-field imager being...
The InfraRed Imaging Spectrograph (IRIS) is a first-light instrument being designed for the Thirty M...
The InfraRed Imaging Spectrograph (IRIS) is a first-light instrument being designed for the Thirty M...
The InfraRed Imaging Spectrograph (IRIS) is a first-light instrument being designed for the Thirty M...
The Infra-Red Imaging Spectrograph (IRIS) is one of the three first light instruments for the Thirty...
The Infra-Red Imaging Spectrograph (IRIS) is one of the three first light instruments for the Thirty...
With the successful completion of our preliminary design phase, we will present an update on all des...
With the successful completion of our preliminary design phase, we will present an update on all des...
With the successful completion of our preliminary design phase, we will present an update on all des...
We present sensitivity estimates for point and resolved astronomical sources for the current design ...