First on-sky results of ERIS at VLT
arXiv:2301.01580 · doi:10.1117/12.2629258
Abstract
ERIS (Enhanced Resolution Imager and Spectrograph) is a new adaptive optics instrument installed at the Cassegrain focus of the VLT-UT4 telescope at the Paranal Observatory in Chile. ERIS consists of two near-infrared instruments: SPIFFIER, an integral field unit (IFU) spectrograph covering J to K bands, and NIX, an imager covering J to M bands. ERIS has an adaptive optics system able to work with both LGS and NGS. The Assembly Integration Verification (AIV) phase of ERIS at the Paranal Observatory was carried out starting in December 2021, followed by several commissioning runs in 2022. This contribution will describe the first preliminary results of the on-sky performance of ERIS during its commissioning and the future perspectives based on the preliminary scientific results.
arXiv commentProceeding of SPIE Astronomical Telescopes + Instrumentation 2022
References in corpus (6)
- Monitoring stellar orbits around the Massive Black Hole in the Galactic Center
- The orbit of the star S2 around SgrA* from VLT and Keck data
- SINFONI - Integral Field Spectroscopy at 50 milli-arcsecond resolution with the ESO VLT
- The SINS/zC-SINF survey of z~2 galaxy kinematics: SINFONI adaptive optics-assisted data and kiloparsec-scale emission line properties
- New observations of the gas cloud G2 in the Galactic Center
- L'-band AGPM vector vortex coronagraph's first light on VLT/NACO: Discovery of a late-type companion at two beamwidths from an F0V star