Telescopes
Fermi LAT Performance
Reference Information - Roman Space Telescope/NASA
Effective area of the mini-telescope as a function of the energy of... | Download Scientific Diagram
Monte Carlo design studies for the Cherenkov Telescope Array - ScienceDirect
XMM-Newton Guest Observer Facility
XRT Effective Area
eROSITA-DE:EarlyDataRelease:eROSITACalibration
Technical Details - Mirrors - XMM-Newton - Cosmos
The effective area functions used in this work. Solid red is the... | Download Scientific Diagram
NuSTAR (Nuclear Spectroscopic Telescope Array)
3.3.6 EPIC filters and effective area
Resources – Colibrì Telescope
Effective area for two telescopes as a function of energy compared with... | Download Scientific Diagram
5 XRT
File:Comparison optical telescope primary mirrors.svg - Wikimedia Commons
CTA-Performance-prod3b-v2-South-20deg-EffectiveArea - Cherenkov Telescope Array
The effective area of an instrument with five 1-meter diameter... | Download Scientific Diagram
14FEB2005/KWCAE2-UsersGroup Astro-E2 X-Ray Telescopes XRT Setup & Structure Performance Characteristics –Effective Area –Angular Resolution –Optical Axes. - ppt download
Researchers | NuSTAR
WFXT collecting effective area (goal) compared with Chandra and... | Download Scientific Diagram
Swift: About Swift - XRT Instrument Description
The effective area of one telescope | Download Scientific Diagram
Lynx X-Ray Observatory: an overview
Effective area of the instrument after considering the optics... | Download Scientific Diagram
![2021 Effective Area calibration of the Nuclear Spectroscopic Telescope ARray (NuSTAR) [IMA] | arXiver](https://i1.wp.com/arxiver.moonhats.com/wp-content/uploads/2021/10/MadsenEtAl-2110.11522_f10.jpg?w=312&h=311&ssl=1 "2021 Effective Area calibration of the Nuclear Spectroscopic Telescope ARray (NuSTAR) [IMA] | arXiver")
2021 Effective Area calibration of the Nuclear Spectroscopic Telescope ARray (NuSTAR) [IMA] | arXiver
The eROSITA X-ray telescope on SRG
An analysis method for data taken by Imaging Air Cherenkov Telescopes at very high energies under the presence of clouds - ScienceDirect
