First light of SINFONI at the VLT

H Bonnet, R Abuter, A Baker, W Bornemann… - The …, 2004 - ui.adsabs.harvard.edu
SINFONI is an Adaptive Optics assisted cryogenic Near Infrared Spectrograph developed by
ESO and MPE in collaboration with NOVA. It was successfully commissioned between June …

First light of SINFONI AO-module at VLT

H Bonnet, R Conzelmann, B Delabre… - … in Adaptive Optics, 2004 - spiedigitallibrary.org
… Hall were needed to prepare the AO-Module for first light at UT4 on May 31st, with the ESO
… the first commissioning, the AO-Module was integrated with SPIFFI3,8 to form SINFONI in its …

Implementation of MACAO for SINFONI at the cassegrain focus of VLT in NGS and LGS modes

H Bonnet, S Strobele… - Adaptive Optical …, 2003 - spiedigitallibrary.org
… of SINFONI for the VLT, a Cassegrain facility, merging into one instrument two recently
developed technologies: Adaptive Optics and Integral Field Spectrometry [1]. SINFONI will …

On-sky performance of SPIFFI: the integral field spectrometer for SINFONI at the VLT

C Iserlohe, M Tecza, F Eisenhauer… - Ground-based …, 2004 - spiedigitallibrary.org
… instrument for the ESO VLT in summer 2004 as part of the SINFONI (SINgle Faint Object …
VLT. In this paper we discuss the performance of SPIFFI during the guest-instrument phase. First

SINFONI: integral field spectroscopy at 50-milli-arcsecond resolution with the ESO VLT

F Eisenhauer, R Abuter, K Bickert… - … for Optical/Infrared …, 2003 - spiedigitallibrary.org
… development of SINFONI started in late 1999 with the … with first light at the telescope in
2004. The Adaptive Optics Module of SINFONI is based on MACAO [8,9], developed for the VLT

THE VLT SINFONI Mg ii PROGRAM FOR LINE EMITTERS (SIMPLE). II. BACKGROUND QUASARS PROBING GALACTIC WINDS

I Schroetter, N Bouché, C Péroux… - The Astrophysical …, 2015 - iopscience.iop.org
… 2 describes the sample and the new Very Large Telescope (VLT) SINFONI/UVES data
acquired. In Section 3, we present the analysis of the SINFONI and UVES data together with the …

Improving the observing efficiency of SINFONI and KMOS at the VLT by factors of 2 to 4: sophisticated sky subtraction algorithms

NA Thatte, N Scott, R Houghton… - … , and Systems IV, 2012 - spiedigitallibrary.org
… the SINFONI IFS at the ESO-VLT, we have been able to hyper-sample the spectral PSF and
reconstruct detailed LSF profiles for all wavelengths and all field points for SINFONISINFONI

VLT/SINFONI study of black hole growth in high-redshift radio-loud quasars from the CARLA survey

M Marinello, RA Overzier… - Monthly Notices of …, 2020 - academic.oup.com
… CARLA sources targeted with SINFONI are indicated with … The right-hand side and top
histograms show that our SINFONI … the SINFONI sample covers a more limited range in redshift. …

The design of ERIS for the VLT

P Amico, E Marchetti, F Pedichini… - Ground-based and …, 2012 - spiedigitallibrary.org
… • SPIFFI’s entrance window is located at the edge of the cryostat and it is the dichroic
beamsplitter in SINFONI. It is reasonable to maintain the direct light feed of SPIFFI, replacing the …

Instrumentation at the ESO VLT

A Moorwood - Ground-based and Airborne Instrumentation for …, 2006 - spiedigitallibrary.org
first light in Jan 2006 and will be used to generate artificial stars for the adaptive optics assisted
instruments NACO and SINFONI. … achieve first light on the VLT in the first quarter of 2008. …