Florian Briegel
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View article: SHINS: the SHARK-NIR instrument control software
SHINS: the SHARK-NIR instrument control software Open
SHARK-NIR is a new compact instrument for coronagraphic imaging, direct imaging, and coronagraphic spectroscopy in the near-infrared wavelengths mounted at LBT. Taking advantage of the telescope's adaptive optics system, it provides high c…
View article: The SDSS-V Local Volume Mapper Telescope System
The SDSS-V Local Volume Mapper Telescope System Open
This paper presents the Local Volume Mapper (LVM) telescope system. LVM is one of three surveys that form the fifth generation of the Sloan Digital Sky Survey (SDSS-V), and it employs a coordinated network of four, 16 cm diameter telescope…
View article: How to make METIS SCAO work
How to make METIS SCAO work Open
Instrumentation
View article: Telescope control software and proto-model siderostat for the SDSS-V Local Volume Mapper
Telescope control software and proto-model siderostat for the SDSS-V Local Volume Mapper Open
The fifth Sloan Digital Sky Survey (SDSS-V) Local Volume Mapper (LVM) is a wide-field integral field unit (IFU) survey that uses an array of four 160 mm fixed telescopes with siderostats to minimize the number of moving parts. Individual t…
View article: METIS AOCS at the beginning of MAIT
METIS AOCS at the beginning of MAIT Open
editorial reviewed
View article: SHARK-NIR, first results of the commissioning at LBT
SHARK-NIR, first results of the commissioning at LBT Open
SHARK-NIR is an instrument which provides direct imaging, both coronagraphic and non-coronagraphic and with the possibility to perform dual-band imaging and low-resolution spectroscopy in Y, J and H bands, with the main scientific goal of …
View article: METIS SCAO -- implementing AO for ELT
METIS SCAO -- implementing AO for ELT Open
METIS, the Mid-infrared ELT Imager and Spectrograph is among the first-generation instruments for ESO\'s 39m Extremely Large Telescope (ELT). It will provide diffraction-limited spectroscopy and imaging, including coronagraphic capabilitie…
View article: NirvanaVIS, an AO-assisted speckle holography add-on for visible wavelengths
NirvanaVIS, an AO-assisted speckle holography add-on for visible wavelengths Open
NirvanaVIS project proposes a visible-wavelength imaging channel upgrade for LINC-NIRVANA (LN), the Italian-German high angular resolution imager installed on the Large Binocular Telescope (LBT). LN is a near-infrared imager operating in t…
View article: Validating the Local Volume Mapper acquisition and guiding hardware
Validating the Local Volume Mapper acquisition and guiding hardware Open
The Local Volume Mapper (LVM) project is one of three surveys that form the Sloan Digital Sky Survey V. It will map the interstellar gas emission in a large fraction of the southern sky using wide-field integral field spectroscopy. Four 16…
View article: LINC-NIRVANA Commissioning at the Large Binocular Telescope -- Lessons Learned
LINC-NIRVANA Commissioning at the Large Binocular Telescope -- Lessons Learned Open
LINC-NIRVANA (LN) is one of the instruments on-board the Large Binocular Telescope (LBT). LN is a high-resolution, near-infrared imager equipped with an advanced adaptive optics module. LN implements layer-oriented Multi-Conjugate Adaptive…
View article: LINC-NIRVANA Commissioning at the Large Binocular Telescope -- Lessons\n Learned
LINC-NIRVANA Commissioning at the Large Binocular Telescope -- Lessons\n Learned Open
LINC-NIRVANA (LN) is one of the instruments on-board the Large Binocular\nTelescope (LBT). LN is a high-resolution, near-infrared imager equipped with an\nadvanced adaptive optics module. LN implements layer-oriented Multi-Conjugate\nAdapt…
View article: The SDSS-V local volume mapper telescope system
The SDSS-V local volume mapper telescope system Open
The Sloan Digital Sky Survey V (SDSS-V) is an all-sky spectroscopic survey of <6 million objects, designed to decode the history of the Milky Way, reveal the inner workings of stars, investigate the origin of solar systems, and track the g…
View article: Operation of a layer-oriented multiconjugate adaptive optics system in the partial illumination regime
Operation of a layer-oriented multiconjugate adaptive optics system in the partial illumination regime Open
Multiconjugate adaptive optics (MCAO) promises uniform wide-field atmospheric correction. However, partial illumination of the layers at which the deformable mirrors are conjugated results in incomplete information about the full turbulenc…
View article: The calibration procedure of the LINC-NIRVANA ground and high layer WFS
The calibration procedure of the LINC-NIRVANA ground and high layer WFS Open
LINC--NIRVANA (LN) is an MCAO module currently mounted on the Rear Bent Gregorian focus of the Large Binocular Telescope (LBT). It mounts a camera originally designed to realize the interferometric imaging focal station of the telescopes. …
View article: The measurement of the Interaction Matrices for the LINC-NIRVANA MCAO
The measurement of the Interaction Matrices for the LINC-NIRVANA MCAO Open
The commissioning of LINC-NIRVANA (LN) is ongoing at the Large Binocular Telescope (LBT).LN provides Multi-Conjugate Adaptive Optics (MCAO) correction for each side of the telescope using the Layer Oriented technique and using Natural Guid…
View article: Aligning the LINC-NIRVANA Natural Guide Stars MCAO system
Aligning the LINC-NIRVANA Natural Guide Stars MCAO system Open
LINC-NIRVANA (LN) is an instrument built to be a Fizeau interferometric imager for the Large Binocular Telescope that will achieve ELT-like spatial resolution. Of course achieving this outstanding resolution requires a very complex instrum…