Copy of Ben Burningham's old page, which I hope to update...
PATT Observatories:
(deadlines for proposals are 15/9 for A session and
15/3 for B session)
Site
|
Telescope
|
Instrument
name
|
description
|
notes
|
Mauna
Kea, Hawaii, USA
|
UKIRT
(3.8m)
|
MICHELLE
|
10-20
micron imaging (67".2 x 50".4 FOV), long slit
spectroscopy, echelle spectroscopy and
imaging/spectro-polarimetry.
|
Until
September 30th
|
UIST
|
1-5
micron imaging (2'x 2' FOV) and long slit spectroscopy;
cross-dispersed (JHK) and integral field spectroscopy; imaging
and spectropolarimetry.
|
Not available?
|
?CGS-4
|
1-5
micron long slit grating spectroscopy with 4 gratings (R ~
400-40000).
|
Echelle
and 40l/mm grating from mid-October
|
IRCAM/TUFTI
|
1-5
micron camera (20".8 FOV), L-band imaging polarimetry
available.
|
Not Available
|
UFTI
|
1-2.5
micron camera (92" FOV), imaging polarimetry and K-band FP.
|
more
sensitive than IRCAM at all JHK for 0.5" images
|
IRPOL2
|
Polarimetry
facility for UKIRT
|
|
Gemini
N (8 m)
|
NIRI
|
near-IR
imager and low res spectrograph
|
AVAIL
Q. O only in 2002b
|
GMOS
|
optical
imager, integral field, long-slit and multi-object spectrograph
|
AVAIL
Q.O only in 2002b
|
Hokupa'a+
QUIRC
|
natural
guide star AO system with QUIRC near-IR camera
|
Not
available in 2002b
|
CIRPASS
|
near-IR
integral field spectrograph
|
Not
available in 2002b
|
Cerro
Pachon, Chile
|
Gemini
S (8 m)
|
T-ReCS
|
mid-IR
imager and spectrograph
|
AVAIL
Q.O only in 2002b
|
AcqCam
|
acquisition
camera offered for broadband BVRI imaging
|
AVAIL
Q.O only in 2002b
|
Flamingos
I
|
near-IR
imager and multi-object spectrograph
|
AVAIL
S.O only in 2002b.
|
Phoenix
|
near-IR
spectrograph (high res - R= 50,000
|
AVAIL
S.O only in 2002b.
|
ING,
La Plama, Spain
|
WHT
(4.2 m)
|
ISIS
|
2
armed medium res. spectrograph with imaging and
spectro-polarimetry available
|
AVAIL
|
UES
|
High
res. echelle spectrograph (R>85000)
|
AVAIL
|
AF2/WYFFOS
|
Automatic
fibre positioner feeding WYFFOS spectrograph (up to 150 objects)
|
AVAIL
|
INTEGRAL/WYFFOS
|
Integral
field spectrograph (upto 6 bundles) feeding WYFFOS
|
AVAIL
|
PFIP
|
Prime
focus imaging (16'.2 x 16'.2 FOV)
|
AVAIL
|
AUX
|
Auxilary
port camera at Cassegrain focus (1'.8 x 1'.8 FOV)
|
AVAIL
|
INGRID
|
near-IR
(0.8-2.5micron) camera (4'.06x4'.06 FOV)
|
AVAIL
|
NAOMI/INGRID
|
Adaptive
optics system for use with INGRID
|
AVAIL
|
INT
(2.5 m)
|
IDS
|
long
slit spectrograph
|
AVAIL
|
WFC
|
Wide
field imaging (34'.2 FOV)
|
AVAIL
|
JKT
(1.0m)
|
CCD
imager
|
10'x
10' FOV imaging
|
AVAIL
|
AAO,
NSW, Aus.
|
AAT
(3.9 m)
|
2dF
|
2
degree field multi-object fibre-fed spectrograph (up to 400
objects)
|
|
IRIS2
|
IR
imager (8'x 8'? FOV) and medium res. spectrograph,
cross-dispersion and multi-slit spectroscopy; spectro- and
imaging polarimetry available.
|
|
LDSS++
|
Low
res. multi-object multi-slit wide field (12') spectrograph
|
Expert
user instrument
|
RGO
|
Long
slit spectroscopy and spectropolarimetry
|
|
SPIRAL
|
Optical
integral field unit (22" x 11" FOV)
|
Expert
user instrument
|
TAURUS
II
|
FP
interferometer with tunable narrow band imaging, narrow band
imaging, polarimetry (expert) and low res. long- and multi-slit
spectroscopy (expert)
|
|
UHRF
|
Ultra-high
res. (R~300000, 600000, 940000) spectrograph at coude focus
|
|
UCLES
|
Cross-dispersed
echelle spectrograph
|
|
WFI
|
Wide
field imager
|
|
UKST
(1.2 m)
|
6dF
|
6
degree field multi-object fibre-fed spectrograph (up to 750
spectra per night)
|
|
ESO
Sites
(deadlines are normally around 31/3 and 31/9, check
the ESO proposals page for current deadlines)
Site
|
Telescope
|
Instrument
name
|
description
|
notes
|
La
Silla, Chile
|
3.6
m
|
ADONIS
|
Near-IR
(1-5 micron) adaptive optics system for use with one of two
cameras: SHARPII+, COMIC
|
|
SHARPII+
|
1-
2.5 micron camera (FOV's: 25".6 x 25".6, 12".8 x
12".8, 8".5 x 8".5
|
|
COMIC
|
1-5
micron camera (FOV's: 12".8 x 12".8 (L, L', M), 4".5
x 4".5 (J, H, K', K))
|
|
CES
|
High
resolution (R~235000) echelle spectroscopy at Coude focus
|
|
EFOSC-2
|
Faint
object spectrograph and camera with polarimetry (FOV 5'.2 x 5'.2)
|
|
TIMMI-2
|
Mid-infrared
spectrograph/imager in N, M and Q bandpasses (5-24 micron)
|
|
NTT
(3.5 m)
|
EMMI
|
multi-mode
instrument with wide-field imaging; low res. multi-object or long
slit grism spectroscopy; medium res. long slit grating
spectroscopy; echelle spectroscopy.
|
|
SUSI-2
|
High
resolution imaging, optimised for good seeing, complementing that
of EMMI
|
|
SOFI
|
IR
(0.9-2.5 micron) imaging with low and medium res. spectroscopy
and polarimetry
|
|
2.2
m
|
WFI
|
Wide
field imaging (FOV 34' x 33') with slitless field spectroscopy
|
|
1.54m
Danish
|
DFOSC
|
Faint
object spectroscopy and imaging
|
|
1.52
m
|
B&C
spectrograph
|
Low
and medium resolution spectrograph
|
|
FEROS
|
Fibre-fed
echelle spectroscopy of entire optical range @R ~48000.
|
|
VLT,
Paranal, Chile
|
Antu,
UT1 (8.2 m)
|
ISAAC
|
IR
(0.9-5 micron) low and medium res. spectroscopy, imaging (FOV 's
SW: 2'.5x2'.5, LW: 72"x72") and polarimetry.
|
AVAIL
|
FORS1
|
Imaging,
long slit and multi-object spectroscopy, polarimetry
|
AVAIL
|
Keuyen,
UT2 (8.2 m)
|
FLAMES
|
Fibre
positioner and fibres feeding to either UVES (8 objects) or
GIRAFFE (130, 15 or 1 objects)
|
Not Available
|
UVES
|
UV
and optical cross-dispersed echelle spectrograph, R~ 40000 (1"
slit)
|
AVAIL
|
GIRAFFE
|
High
and medium res. spectrograph with 3 modes: MEDUSA: single fibre
mode, ~130 objects; IFU: 15 objects, 2"x3" apertures;
ARGUS: single object, array of microlenses (FOV's 12"x7",
6".6x4".2)
|
Not Available
|
FORS2
|
As
for FORS1, but no polarimetry, does have short slit, medium res.
echelle grism spectroscopy
|
AVAIL
|
Melipal,
UT3 (8.2 m)
|
VISIR
|
Imaging
(w/ variable magnification) and long slit spectroscopy (8-25
micron)
|
Not Available
|
VIMOS
|
Visible
multi-object spectrograph (150 slits w/ R~2000, 750 slits w/ R~
200), with imaging (FOV 4 x 7'x8') and IFU.
|
Not Available
|
Yepun,
UT4 (8.2 m)
|
NIRMOS
|
Near-IR
(1.0-1.8 micron) multi object spectrograph (150 slits w/ R~2000),
with imaging (FOV 4 x 6'x8').
|
Not Available
|
SINFONI
|
integral
field spectrograph with AO module, 32 x32 spatial pixels
(8"x8",3.2"x3.2", 0.8"x0.8")
|
Not Available
|
NAOS/CONICA
|
Adaptive
optics system with imaging and spectroscopy and polarimetry
|
AVAIL
|
SAAO
(deadlines
18/12 for April/June, 1/4 for July/ September, 1/7 for October/
December, 1/10 for January/ March)
|