ESO Spanish Users : Instruments P90

TheEuropean Southern Observatory(ESO)invites proposals for observations at ESO telescopes during Period 90 (1 October 2012- 31 March 2013). The follo

TheEuropean Southern Observatory(ESO)invites proposals for observations at ESO telescopes during Period 90 (1 October 2012- 31 March 2013). The following instruments are offered in this period: La Silla EFOSC-2(ESO Faint Object Spectrograph -2) NTT telescope FEROS(Fibre-fed Extended Range Optical Spectrograph) 2.2m telescope HARPS(High Accuracy Radial velocity Planetary Searcher; See Recent changes) 3.6m telescope SofI(Son of ISAAC)NTT telescope WFI(Wide Field Imager)2.2m telescope Paranal AMBER(Near-infrared interferometric instrument; SeeRecent changes)VLTI CRIRES(Cryogenic high-resolution IR Echelle Spectrograph; SeeRecent changes)VLT-UT1 FLAMES(Fibre Large Array Multi Element Spectrograph) VLT-UT2 FORS2(FOcal Reducer/low dispersion Spectrograph 2)VLT-UT1 HAWK-I(High Acuity Wide field K-band Imager; SeeRecent changes) VLT-UT4 ISAAC(Infrared Spectrometer And Array Camera; SeeRecent changes) VLT-UT3 MIDI(MID-infrared Interferometric instrument; SeeRecent changes) VLTI NAOS-CONICA(High Resolution NIR Camera and Spectrograph; SeeRecent changes)VLT-UT4 OmegaCAM (Wide Field Imager for the VST at Paranal; SeeRecent changes) VST SINFONI(Spectrograph for INtegral Field Obs. in the NIr)VLT-UT4 UVES(UV-Visual Echelle Spectrograph)VLT-UT2 VIMOS(Visual Multi Object Spectrograph; SeeRecent changes)VLT-UT3 VIRCAM(VISTA InfraRed CAMera; SeeRecent changes) VISTA VISIR(VLT Imager and Spectrometer for mid Infra Red; SeeRecent changes)VLT-UT3 XSHOOTER (UV-Visual-NIR medium resolution echelle spectrograph; SeeRecent changes)VLT-UT2 2nd Generation VLT Instruments: The KMOS commissioning will start in Period 89 and extend to at least Period 90. The installation of SPHERE on the UT3 Nasmyth A platform is expected to take placeduring Period 90, followed by its commissioning, which will extend to at least Period 91. The installation of MUSE on the UT4 Nasmyth B platform is expected to take place inthe course of 2013. Chajnantor LABOCA(Large Apex BOlometer CAmera; See) Apex SABOCA(Submillimetre APEX Bolometer CAmera)Apex SHFI(Swedish Heterodyne Facility Instrument; SeeRecent changes)Apex FLASH (First Light APEX Submillimeter Heterodyne receiver; SeeRecent changes)Apex ESO Instruments Summary Table Information partially extracted from the pdf document:ESO Call for Proposals –P90

Instruments P90

The European Southern Observatory (ESO) invites proposals for observations at ESO telescopes during Period 90 (1 October 2012 - 31 March 2013). The following instruments are offered in this period:

La Silla

EFOSC-2 (ESO Faint Object Spectrograph -2) NTT telescope

FEROS (Fibre-fed Extended Range Optical Spectrograph) 2.2m telescope

HARPS (High Accuracy Radial velocity Planetary Searcher; See Recent changes) 3.6m telescope

SofI (Son of ISAAC) NTT telescope

WFI (Wide Field Imager) 2.2m telescope

Paranal

AMBER (Near-infrared interferometric instrument; See Recent changes) VLTI 

CRIRES (Cryogenic high-resolution IR Echelle Spectrograph; See Recent changes) VLT-UT1

FLAMES (Fibre Large Array Multi Element Spectrograph) VLT-UT2

FORS2 (FOcal Reducer/low dispersion Spectrograph 2) VLT-UT1

HAWK-I (High Acuity Wide field K-band Imager; See Recent changes) VLT-UT4

ISAAC (Infrared Spectrometer And Array Camera; See Recent changes) VLT-UT3

MIDI (MID-infrared Interferometric instrument; See Recent changes)   VLTI 

NAOS-CONICA (High Resolution NIR Camera and Spectrograph; See Recent changes) VLT-UT4

OmegaCAM (Wide Field Imager for the VST at Paranal; See Recent changes) VST

SINFONI (Spectrograph for INtegral Field Obs. in the NIr) VLT-UT4

UVES (UV-Visual Echelle Spectrograph)  VLT-UT2

VIMOS (Visual Multi Object Spectrograph; See Recent changes) VLT-UT3

VIRCAM (VISTA InfraRed CAMera; See Recent changes) VISTA

VISIR (VLT Imager and Spectrometer for mid Infra Red; See Recent changes) VLT-UT3

XSHOOTER (UV-Visual-NIR medium resolution echelle spectrograph; See Recent changes)  VLT-UT2

2nd Generation VLT Instruments:
  • The KMOS commissioning will start in Period 89 and extend to at least Period 90.
  • The installation of SPHERE on the UT3 Nasmyth A platform is expected to take place during Period 90, followed by its commissioning, which will extend to at least Period 91.
  • The installation of MUSE on the UT4 Nasmyth B platform is expected to take place in the course of 2013.

Chajnantor

LABOCA (Large Apex BOlometer CAmera; See ) Apex

SABOCA (Submillimetre APEX Bolometer CAmera) Apex

SHFI (Swedish Heterodyne Facility Instrument; See Recent changes) Apex

FLASH (First Light APEX Submillimeter Heterodyne receiver; See Recent changes) Apex

ESO Instruments Summary Table

 

 

Information partially extracted from the pdf document:  ESO Call  for Proposals – P90