David G. Bramall
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View article: Overview of the Fiber System for the Dark Energy Spectroscopic Instrument
Overview of the Fiber System for the Dark Energy Spectroscopic Instrument Open
The Dark Energy Spectroscopic Instrument (DESI) is a revolutionary instrument designed for precise measurements of cosmic distances and the investigation of dark energy. DESI utilizes 5000 optical fibers to simultaneously measure the spect…
View article: Overview of Space-Based Laser Communication Missions and Payloads: Insights from the Autonomous Laser Inter-Satellite Gigabit Network (ALIGN)
Overview of Space-Based Laser Communication Missions and Payloads: Insights from the Autonomous Laser Inter-Satellite Gigabit Network (ALIGN) Open
This paper examines the growing adoption of laser communication (lasercom) in space missions and payloads for identifying emerging trends and key technology drivers of future optical communications satellite systems. It also presents a com…
View article: MOSAIC GLAO performance and system architecture: AO for the entire ELT focal plane
MOSAIC GLAO performance and system architecture: AO for the entire ELT focal plane Open
International audience
View article: MOSAIC at the ELT: a unique instrument for the largest ground-based telescope
MOSAIC at the ELT: a unique instrument for the largest ground-based telescope Open
Pelló, Roser et al.-- Full list of authors: Pelló, Roser; Puech, Mathieu; Prieto, Éric; Rodrigues, Myriam; Sanchez-Janssen, Rubén.; Dalton, Gavin B.; Ducret, Franck; El Hadi, Kacem; García-Vargas, María. L.; Lynn, Jeff; Bharmal, Nazim A.; …
View article: Steering Mirror System with Closed-Loop Feedback for Free-Space Optical Communication Terminals
Steering Mirror System with Closed-Loop Feedback for Free-Space Optical Communication Terminals Open
Precision beam pointing plays a critical role in free-space optical communications terminals in uplink, downlink and inter-satellite link scenarios. Among the various methods of beam steering, the use of fast steering mirrors (FSM) is wide…
View article: Topology Optimization of a Single-Point Diamond-Turning Fixture for a Deployable Primary Mirror Telescope
Topology Optimization of a Single-Point Diamond-Turning Fixture for a Deployable Primary Mirror Telescope Open
CubeSats, known for their compact size and cost effectiveness, have gained significant popularity. However, their limited size imposes restrictions on the optical aperture and, consequently, the Ground Resolution Distance in Earth Observat…
View article: Topology Optimization Of A Single Point Diamond Turning Fixture For A Deployable Primary Mirror Telescope
Topology Optimization Of A Single Point Diamond Turning Fixture For A Deployable Primary Mirror Telescope Open
CubeSats, known for their compact size and cost-effectiveness, have gained significant popularity. However, their limited size imposes restrictions on optical aperture and, consequently, Ground Resolution Distance in Earth Observation miss…
View article: Advances with the WIVERN laboratory experiment for testing novel laser-based wavefront sensing techniques
Advances with the WIVERN laboratory experiment for testing novel laser-based wavefront sensing techniques Open
In order to overcome some existing challenges with the use of laser guide stars (LGS), including complexity,expense, and implementation challenges, we describe in this work WIVERN which is a testbed for laboratoryexperiments in laser-based…
View article: WIVERN: a laboratory experiment for testing novel laser-based wavefront sensing techniques
WIVERN: a laboratory experiment for testing novel laser-based wavefront sensing techniques Open
WIVERN is a testbed for laboratory experiments in laser-based wavefront sensing. It emulates laser uplink from a 4m telescope with 1.6 arcsec seeing and laser back-scattering from up to 20 km. Currently there are three current wavefront se…
View article: Performance of the Dark Energy Spectroscopic Instrument (DESI) fiber system
Performance of the Dark Energy Spectroscopic Instrument (DESI) fiber system Open
The recently commissioned Dark Energy Spectroscopic Instrument (DESI) will measure the expansion historyof the universe using the Baryon Acoustic Oscillation technique. The spectra of 35 million galaxies and quasarsover 14000 sq deg will b…
View article: A four mirror anastigmat collimator design for optical payload calibration
A four mirror anastigmat collimator design for optical payload calibration Open
We present here a four mirror anastigmatic optical collimator design intended for the calibration of an earth observation satellite instrument. Specifically, the collimator is to be applied to the ground based calibration of the Sentinel-4…
View article: An efficient stable optical polariser module for calibration of the S4UVN earth observation satellite
An efficient stable optical polariser module for calibration of the S4UVN earth observation satellite Open
We describe here an optical polariser module intended to deliver well characterised polarised light to an imaging spectrometer instrument. The instrument in question is the Sentinel-4/UVN Earth observation imaging spectrometer due to be de…