review of vimos and its
TRANSCRIPT
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ESO Spectroscopic Surveys Workshop. Garching 9-10 March 2009
LA SILLAPARANAL
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Review of VIMOS and itsFuture
LA SILLAPARANAL
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F. Selman, the IOT teamand many others…
Colless 2007
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ESO Spectroscopic Surveys Workshop. Garching 9-10 March 2009
LA SILLAPARANAL
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The VIMOS IOT
• Michael Hilker User Support, Garching
• Carlo Izzo Pipeline development, Garching
• Jean-Luis Lizon Engineering, Garching
• Eduardo Peña Software, Paranal
• Marina Rejkuba User Support, Garching
• Pascal Robert Engineering, Paranal
• Burkhard Wolff Quality Control, Garching
• Fernando Selman Instrument Scientist, Paranal
• Gianni Marconi Instrument Scientist Emeritus, Paranal
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ESO Spectroscopic Surveys Workshop. Garching 9-10 March 2009
LA SILLAPARANAL
OBSERVATORY
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VIMOS in a nutshell
FoV= 1/16.5 deg^2
840 slits, 10” at long R=200210 slits, 10” long at R=2000
Multiplex
Passive compensation: ±2 pixels peak-to-valley
Flexures
6 per channelGrisms
UBVRIz OS-red, OS-blue, GG435,GG475, 170mm φ
Filters
180 - 2500R
0.37-1.0 µmλ range
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ESO Spectroscopic Surveys Workshop. Garching 9-10 March 2009
LA SILLAPARANAL
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VIMOS in a nutshell
• 4 2k x 4k CCDs• 0.205 um pixels
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ESO Spectroscopic Surveys Workshop. Garching 9-10 March 2009
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VIMOS MOS Configurations
0.8510.625004096630-870GG475HR_red
0.5510.621504096520-760GG435HR_orange
0.5010.520504096415-620FreeHR_blue
22.55802000550-970OS-redMR
0.8022.55802000480-1000GG475MR
0.7547.3210550550-950OS-redLR_red
0.8045.3180550370-670OS-blueLR_blue
Peak effgris. only
muxDisp.Å/pix
1” RnpixΔλ
[nm]OS FiltGrism
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ESO Spectroscopic Surveys Workshop. Garching 9-10 March 2009
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VIMOS improvement/recovery project
• RELIABILITY– Lower failure rate
• STABILITY– Focal plane stability– Flexures
• SENSITIVITY– Detector upgrade in the red
• Overall efficiency (VMMPS?)
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ESO Spectroscopic Surveys Workshop. Garching 9-10 March 2009
LA SILLAPARANAL
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Improve reliability by reducing therate of failures
10% ----> ~2%
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ESO Spectroscopic Surveys Workshop. Garching 9-10 March 2009
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• Redesign of Mask Exchange Unit(MEU)clamp/translator/blocker.
• Redesign of Grism Exchange Unit (GEU). Ifpossible to permit the insertion of grisms atany angle.
• Filter Exchange Unit (FEU)• New shutters• Pick-up noise/connector overhaul• Software (possibly implied by the above)
Improve reliability by reducing therate of failures
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ESO Spectroscopic Surveys Workshop. Garching 9-10 March 2009
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Focal Plane StabilityFocal plane is stable, but insertion can be unreliable.
Y[pix]= a(yx)x + a(yy)y + y(0)
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ESO Spectroscopic Surveys Workshop. Garching 9-10 March 2009
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Flexures
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ESO Spectroscopic Surveys Workshop. Garching 9-10 March 2009
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But remember that there is a limit…
VIMOS does not have anADC
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ESO Spectroscopic Surveys Workshop. Garching 9-10 March 2009
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Nevertheless…
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ESO Spectroscopic Surveys Workshop. Garching 9-10 March 2009
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Red detector upgrade (Q2 2010)
• - E2V deep depletion2kx4k CCDs, reducefringes, increases redresponse (and CRcontamination).
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ESO Spectroscopic Surveys Workshop. Garching 9-10 March 2009
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Should we get new NIR grisms?
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ESO Spectroscopic Surveys Workshop. Garching 9-10 March 2009
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Conclusions: what can be expected
8.86.7Obs/10h66%43%Efficiency41056193Total
(2%) 80(10%) 563Tech40255630Sub Total(?) 0510NightCal30253115OBS10001150ACQ(?) 0855PRE-IMG
On-target time: 2700s