Publication | Closed Access
Commissioning and performances of the VLT-VIMOS
300
Citations
0
References
2003
Year
EngineeringMicroscopyOptical TestingInstrumentation EngineeringOptical CharacterizationMulti-slit SpectroscopyVirtual InstrumentationOptical DiagnosticsIntegral Field SpectroscopyInfrared OpticComputational ImagingInstrumentationRadiation ImagingRadiologyHealth SciencesAccelerator TechnologyElectrical EngineeringOphthalmologyImaging SpectroscopySpectral ImagingSynchrotron RadiationMicroelectronicsSpectroscopyIntegral Field Unit
The Visible Multi‑Object Spectrograph VIMOS is a wide‑field survey instrument currently being commissioned for operations at the ESO‑VLT. VIMOS is expected to be offered to the ESO community for regular observations in early 2003. During its first commissioning period, VIMOS confirmed excellent performance in direct imaging, multi‑slit spectroscopy, and integral field spectroscopy, delivering the largest imaging field at the VLT (224 arcmin²), an unprecedented multiplex of ~800 slits, a 54×54 arcsec² integral field unit with 6400 spectra, and image quality limited only by natural seeing.
The Visible Multi-Object Spectrograph VIMOS is a wide field survey instrument in the process of being commissioned for operations at the ESO-VLT. During the first commissioning period, the instrument has confirmed its excellent performances in its three basic modes of operation: direct imaging, multi-slit spectroscopy, and integral field spectroscopy. VIMOS provides the largest imaging field at the VLT with 224 arcmin<sup>2</sup>. It offers an unprecedented multiplex gain in multi-slit spectroscopy, with on order 800 slits which can be observed simultaneously. The integral field unit has a field up to 54x54 arcsec<sup>2</sup>, with 6400 spectra recorded at once. The overall efficiency of VIMOS combined to the Melipal unit #3 is confirmed to be as computed on the basis of the measured transmission of optical elements. Image quality is confirmed to be excellent, providing images limited by natural seeing in most conditions. High quality slit masks cut by the laser machine coupled to excellent geometric mask to CCD mapping lead to multi-slit spectra of excellent quality. VIMOS is expected to be offered to the ESO community for reguglar observations in early 2003.