La Silla Instruments Summary Table
| Instrument | Spectral Coverage | Observing Mode | Spectral Resolution | Multiplex | Note | Telescope |
|---|---|---|---|---|---|---|
| HARPS | optical 378-691nm |
echelle, polarimetry | 120,000 | no | 2 fibres, high accuracy; 2 fibers, high efficiency |
3.6m |
| EFOSC-2 | optical 350 - 1100nm |
imaging, spectroscopy, polarimetry, coronagraphy | ~1000 | yes | imaging and spectroscopic polarimetry | NTT |
| SOFI | near-IR 1-2.5 µm |
imaging, spectroscopy | 600-2200 | no | - | NTT |
| ULTRACAM | optical: u',g',r' or u',g',i' or u',g',z' |
3-channel, high-speed CCD camera | - | no | frame rate up to 300Hz; field-of-view of 6 arcmin |
NTT |
Paranal Instruments Summary Table
| Instrument | Spectral Coverage | Observing Mode | Spectral Resolution | Multiplex | Note | Telescope |
|---|---|---|---|---|---|---|
| FORS2 | optical 330 - 1100 nm |
imaging (incl. configurable occulting bars), long slit and multi-object spectroscopy, spectropolarimetry, imaging polarimetry | 260 - 2600 | yes | Spectroscopy with ~7' long slit, ~20" multi-slit, and laser-cut slit masks; multiple object spectroscopy; RRM | VLT UT1 |
| KMOS | near-IR 0.8 - 2.5 µm |
multi-object integral field spectroscopy (24 arms) | 1800 - 4000 | yes | 24-arms Integral Field Spectroscopy; 2.8x2.8", 0.2" sampling IFU over a 7.2' field; | VLT UT1 |
| FLAMES | optical 370 - 950 nm |
multi-fibre echelle,integral field spectroscopy | 6000 - 47000 | yes | 132 Medusa fibres; 15 deployable IFUs, one large IFU; GIRAFFE: single echelle order; 8 fibres to UVES | VLT UT2 |
| VISIR | mid-IR: 4.5 - 21 µm | M, N and Q band normal and burst-mode imaging; coronagraphy (Angular Groove Phase Mask, 4-Quadrant Phase Mask); N band low resolution long slit spectroscopy; high-resolution long slit and cross-dispersed spectroscopy | ~400, 20000 | no |
pixel size of 0.045 and 0.076 arcsec in imaging, and 0.076 arcsec in spectroscopy | VLT UT2 |
| UVES | optical 300 - 1100 nm |
echelle, image slicer, slit spectroscopy | up to 80,000 (blue arm) / 110,000 (red arm) | no | long slit capability in single order; iodine cell; RRM | VLT UT2 |
optical: 500 - 900 nm near-IR: 0.95 - 2.32 µm |
high-contrast imaging, dual-band imaging, integral field spectroscopy, differential-polarimetric imaging with or without classical, apodized pupil Lyot coronagraphs, sparse aperture mask | ~30, 50, 400 | no | extreme AO with optical wave-front sensor; fast star hopping; RRM | VLT UT3 | |
| X-SHOOTER | UV-optical-NIR |
echelle, slit and integral field spectroscopy | ~5000-17000 |
no | full spectral coverage with one pointing; slit + IFU; RRM |
VLT UT3 |
| HAWK-I | near-IR 0.85-2.5 µm | broand and narrow band imaging, fast photometry | - | - | pixel size of 0.106"; field: 7.5'x7.5', subwindow readout capability; GLAO; RRM | VLT UT4 |
| MUSE |
465 - 930 nm |
integral field spectroscopy | 1770 @ 480nm 3590 @ 930nm |
no | IFU size on sky 60"x60" with spaxel size 0.2" (WFM) or 7.5"x7.5" with spaxel size 0.025" (NFM); GLAO, LTAO, no AO; RRM. |
VLT UT4 |
| ESPRESSO | optical 380 - 788 nm |
fibre-fed échelle spectroscopy | 140,000, 190,000, or 70,000 (median) | no | 2 fibres (1 object, 1 sky or simultaneous reference); RV precision < 1 m/s (with the ultimate goal of reaching 10 cm/s); 1-UT and 4-UT modes |
VLT UT3, or/and |
| GRAVITY | near-IR 2.05 - 2.45 µm |
spectro-interferometry | R ~ 20, 500, & 4000 |
no |
4 beam combiner - delivers spectrally dispersed visibilities, differential and closure phases |
VLTI - ATs VLTI - UTs |
| MATISSE | mid-IR 2.8 - 4.1 µm 4.5 - 5 µm 8 - 13 µm |
spectro-interferometry | R ~ 30 (covers L&M-band) R ~ 506, 959, 3666 (L or M band) R ~ 30, 218 (N band) |
no | 4 beam combiner - delivers spectrally dispersed visibilities, differential and closure phases |
VLTI - ATs VLTI - UTs |
| PIONIER | near-IR 1.65 µm |
spectro - interferometry | R ~ 5 or 40 |
no | 4 beam combiner - delivers spectrally dispersed visibilities, differential and closure phases |
VLTI - ATs VLTI - UTs |
| VIRCAM | near-IR 0.8-2.2 µm |
imaging | - | - | 1.5 degree x 1 degree field of view with 0.34" average pixel size | VISTA |
| OmegaCAM | optical 350-910 nm | imaging | - | - | 1 degree x 1 degree unvignetted field of view with 0.21" pixel size | VST |
APEX Instruments Summary Table
| Instrument | Spectral Coverage | Observing Mode | Spectral Resolution | Multiplex | Note | Telescope |
|---|---|---|---|---|---|---|
| LABOCA | 870 µm | bolometer array | - | - | 295 pixels | APEX |
| SEPIA | 159-211 GHz 272-376 GHz 578-738 GHz |
heterodyne receiver | - |
- |
Sideband separating receiver with instantaneous coverage in 2 bands of 4 GHz in both polarizations (for SEPIA180) or 8 GHz in both polarizations (for SEPIA345 and SEPIA660). | APEX |
| ARTEMIS | 350 µm 450 µm |
bolometer array | - |
- | FoV: 4' x 2'; 2304 pixels (fully sampled) | APEX |
| nFLASH |
200-270 GHz 385-500 GHz |
heterodyne receiver |
- | - | Sideband separating receiver with instantaneous coverage in 2 bands of 4 GHz in both polarizations (for nFLASH460) or 8 GHz in both polarizations (for nFLASH230).
|
APEX |