| Atlantis |
| type | lenses |
| telescope | GranTeCan 10m |
| wv range | 1-2.4 micron |
| lens scale | 0.25", 0.1", 0.07", 0.03" |
| number of lenses | 1024 |
| field of view | 8"x8", 3.2"x3.2", 2.4"x2.4", ~1"x1" |
| spectral resolution | 2000, 5000 |
| detector | maybe HAWAII |
| sensitivity | |
| web pages | IAC |
| papers | |
| status | can't find whether it's approved or not |
| people | Almudena Prieto (PI) |
| software | |
| CIRPASS |
| type | lenses |
| telescope | Gemini North |
| wv range | 0.85-1.8 micron |
| lens scale | 0.36", 0.25", 0.12", 0.05" |
| number of lenses | 499 |
| field of view | (all "x") 13.3x4.1, 9.3x2.9, 4.4x1.4, 1.9x0.6 |
| spectral resolution | 3000 at 1.35 micron |
| detector | HAWAII 2k square |
| sensitivity | S/N=5 for J~21.5 in 10800 s |
| web pages | Cambridge |
| papers | |
| status | shipping early 2001 |
| people | IoA, Cambridge |
| software | package in early development |
| GOHSS |
| type | lenses |
| telescope | Galileo |
| wv range | 0.8-1.8 micron |
| lens scale | |
| number of lenses | |
| field of view | |
| spectral resolution | 3000 |
| detector | |
| sensitivity | |
| web pages | TWG, Observatory of Capodimente, Naples |
| papers | |
| status | |
| people | Naples |
| software | |
| GNIRS |
| type | slicer |
| telescope | Gemini |
| wv range | 0.9-2.5, 2.9-5.5 micron |
| slit width | |
| field of view | |
| spectral resolution | 600, 1800, 5400, 6000, 18000 |
| detector | 1Kx1K InSb (ALADDIN) |
| sensitivity | |
| web pages | Gemini pages |
| papers | |
| status | Oct-Dec 2002 (for GNIRS but IFU is an upgrade.......) |
| people | NOAO |
| MPE-3D |
| type | slicer |
| telescope | AAT (3.9m) |
| wv range | (all micron) 1.48-1.78 (Hlow), 1.55-1.75 (Hhigh), 1.94-2.41 (K), 1.95-2.18 (Kshort), 2.17-2.43 (Klong) |
| slit width | uses grisms |
| field of view | ~6"x6" (depends on telescope) |
| spectral resolution | 1250 (Hlow), 2100 (Hhigh), 1100 (K), 2100 (Kshort), 2100 (Klong) |
| detector | 256x256 NICMOS-3 Rockwell |
| sensitivity | H=17.5, K=17 in 9400 s if 1" seeing and 0.4" pixels |
| web pages | MPE |
| papers | |
| status | commissioned |
| people | |
| NIFS |
| type | slicer |
| telescope | Gemini (+A/O) |
| wv range | 1-2.5 micron |
| slit width | 0.1" |
| field of view | 3.2"x3.2" |
| spectral resolution | 5400 |
| detector | HAWAII 2K |
| sensitivity | |
| web pages | ANU |
| papers | |
| status | commissioning August 2002 |
| people | ANU, U of Hawaii, Gemini |
| NIRMOS |
| type | lenses |
| telescope | VLT - UT4 |
| wv range | 1-1.8 micron |
| lens scale | |
| number of lenses | 1600 |
| field of view | 28"x28", 14"x14" |
| spectral resolution | 2500 |
| detector | |
| sensitivity | |
| web pages | Marseille |
| papers | |
| status | due 2002 |
| people | Olivier Le Fevre (PI) P Vettolani (Co-PI), Paris, Marseille, OHP, Toulouse, Bologna, Milan, Naples, ESO |
| software | |
| PIFS |
| type | slicer |
| telescope | Palomar 200 inch |
| wv range | 1-2.5 micron, 1-5 micron |
| slit width | 0.67" |
| field of view | 5.5"x9.5" |
| spectral resolution | 600,1300 |
| detector | 256x256 |
| sensitivity | K=18, 5sigma in 1 hour (high resolution) |
| web pages | Caltech |
| papers | Murphy et al., PASP, 111, 1176, 1999 |
| status | first use Sep 1998 |
| people | Tom Murphy, Caltech |
| SINFONI |
| type | slicer |
| telescope | VLT UT3 (with SPIFFI spectrograph) |
| wv range | 1-2.5 micron |
| slit width | |
| field of view | 32x32 pixels (11"x11" - 1.6"x1.6") |
| spectral resolution | <4500 |
| detector | 1024 Rockwell |
| sensitivity | |
| web pages | ESO |
| papers | |
| status | Sept 2002 |
| people | MPE-Garching, ESO |
| SMIRFS |
| type | lenses |
| telescope | UKIRT (CGS4) |
| wv range | 1-2.5 micron |
| lens scale | 0.63" |
| number of lenses | 72 |
| field of view | 6"x4" |
| spectral resolution | 300-6000 |
| detector | 256x256 InSb |
| sensitivity | |
| web pages | Durham instrumentation group |
| papers | Haynes et al, to be published in PASP, astro-ph/9909017 |
| status | commissioned June 1997 |
| people | Durham |
| software | James Turner (Durham) has some, but instrument makes reduction difficult |
| UIST - slicer |
| type | slicer |
| telescope | UKIRT (UIST spectrograph) |
| wv range | 1-5 micron |
| slit width | 0.24 |
| field of view | 29 arcsec2 |
| spectral resolution | |
| detector | ALADDIN 1024x1024 InSb |
| sensitivity | |
| web pages | Durham, Edinburgh |
| papers | |
| status | delivery April 2001 (UIST), IFU detailed design complete |
| people | Durham for IFU, Edinburgh for spectrograph |
| FLAMES - GIRAFFE |
| type | lenses |
| telescope | VLT - UT2 |
| wv range | 3700-9000 A |
| lens scale | IFU is 0.52"/lens, ARGUS is 0.52"/lens or 0.27"/lens |
| number of lenses | 2 IFU each with 20 fibres, or one with 300 fibres (ARGUS mode) |
| field of view | each IFU is 2.1"x3.1", ARGUS mode is 11.5"x7.3" or 5.3"x3.7" |
| spectral resolution | 7500-25000 |
| detector | 2x4K EEV CCDs |
| sensitivity | |
| web pages | ESO, Paris-Meudon |
| papers | |
| status | end 2001 |
| people | Paris-Meudon (F.Hammer), Geneva (A.Blecha) |
| software | |
| FMOS |
| type | lenses |
| telescope | Subaru |
| wv range | optical |
| lens scale | |
| number of lenses | |
| field of view | |
| spectral resolution | |
| detector | |
| sensitivity | |
| web pages | |
| papers | |
| status | |
| people | |
| software | |
| GMOS |
| type | lenses |
| telescope | Gemini |
| wv range | 3600-11000 A |
| lens scale | 0.2 |
| number of lenses | 1000 (object) 500 (background) |
| field of view | 5"x7" (object) 5"x3.5" (background) |
| spectral resolution | 670-4400 |
| detector | 3x2048x4608 |
| sensitivity | |
| web pages | Gemini pages |
| papers | |
| status | shipping December 2000, available 2001B |
| people | ATC, Durham, Canada |
| software | |
| INTEGRAL |
| type | lenses |
| telescope | WHT (with WYFFOS spectrograph) |
| wv range | optical |
| lens scale | 0.7" (bundle1), 1.4" (bundle2), 4.0" (bundle3) |
| number of lenses | 205 (bundle1), 219 (bundle2), 135 (bundle3) |
| field of view | 7.8"x6.4" (bundle1), 16"x12.3" (bundle2), 33.6"x29.4" (bundle3) |
| spectral resolution | 550-2200 (bundle1), 455-2000 (bundle2), 225-967 (bundle3) |
| detector | |
| sensitivity | |
| web pages | ING |
| papers | |
| status | available on WHT |
| people | IAC-ING |
| software | basic data reduction available, based on IRAF |
| MPFS |
| type | lenses |
| telescope | SAO 6m (Russia) |
| wv range | 3600-9600 A |
| lens scale | 0.5 x 0.5", 0.75 x 0.75", 1x1" |
| number of lenses | 16x16 |
| field of view | 8x8", 12x12", 16x16" |
| spectral resolution | 1.35-5 A/pix |
| detector | CCD 1024x1024 |
| sensitivity | |
| web pages | SAO |
| papers | |
| status | available |
| people | |
| software | |
| OASIS |
| type | lenses |
| telescope | CFHT |
| wv range | 4500-10000 A |
| lens scale | 0.04,0.11,0.16,0.27,0.3,0.41 |
| number of lenses | |
| field of view | 1.6x1.2 - 11x9 |
| spectral resolution | 1000-2000 |
| detector | Loral |
| sensitivity | |
| web pages | CFHT OASIS information, the same page at Lyon |
| papers | |
| status | available on CFHT |
| people | Pierre Martin - Instrument Scientist (martin@cfht.hawaii.edu)
Roland Bacon - software (bacon@cumulus.univ-lyon1.fr) |
| software | |
| PMAS |
| type | lenses |
| telescope | Calar Alto, LBT |
| wv range | optical |
| lens scale | |
| number of lenses | 16x16 |
| field of view | |
| spectral resolution | |
| detector | |
| sensitivity | |
| web pages | AIP |
| papers | |
| status | commissioning 2001 |
| people | AIP |
| software | |
| SAURON |
| type | lenses |
| telescope | WHT |
| wv range | 4800-5400 A |
| lens scale | 0.26, 0.94 |
| number of lenses | 1520 |
| field of view | 9x11, 33x41 |
| spectral resolution | 1600 |
| detector | |
| sensitivity | |
| web pages | |
| papers | Miller et al, ASP conf series ?? (Imaging the Universe in 3D), p??, 2000 |
| status | commissioned 1-5 Feb 1999 |
| people | |
| software | adapting OASIS procedure |
| Spiral B |
| type | lenses |
| telescope | AAT |
| wv range | 4800-10000 A |
| lens scale | 0.7" |
| number of lenses | 512 |
| field of view | 22"x11" |
| spectral resolution | 1150-11000 (all at 5000A) |
| detector | |
| sensitivity | |
| web pages | AAO |
| papers | |
| status | commissioned March 2000, available as expert user instrument |
| people | David Lee, AAO |
| software | |
| TEIFU |
| type | lenses |
| telescope | WHT (with WYFFOS spectrograph and ELECTRA A/O) |
| wv range | optical |
| lens scale | 0.25, 0.13 |
| number of lenses | 1000 |
| field of view | 2x(7x3.9), 2x(3.5x1.9) |
| spectral resolution | |
| detector | 1024x1024 (Tek6) CCD |
| sensitivity | |
| web pages | Durham instrumentation group |
| papers | Haynes et al, SPIE, 1998 postscript |
| status | commissioned WHT June and Sept 1999, foreoptics modified during 2000 to work with new WHT AO system, NAOMI |
| people | Durham |
| software | imspec IRAF package in development |
| VIMOS |
| type | lenses |
| telescope | VLT - UT3 |
| wv range | 3700-10000 A |
| lens scale | 0.67"/lens, 0.33"/lens |
| number of lenses | 6400 |
| field of view | 54"x54", 27"x27" |
| spectral resolution | 180-2520 |
| detector | |
| sensitivity | |
| web pages | Marseille |
| papers | Prieto et al, SPIE, 2000 |
| status | IFU completed May 2000, commissioning early 2001 |
| people | Olivier Le Fevre (PI) P Vettolani (Co-PI), Paris, Marseille, OHP, Toulouse, Bologna, Milan, Naples, ESO |
| software | |