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Armagh, 19 February 2008
This session:
MuSiCoS, Narval & ESPaDONs archive (James)
DAO (Jason) Archive observations (Luca)
Armagh, 19 February 2008
Low res. spectropolarimetry:Advantages and drawbacks
Extremely efficient on hot and fast rotating stars
No additional use other than for field determinations
Armagh, 19 February 2008
FLAMESFiber Large Array Multi-Element Spectrograph
132 GIRAFFE Medusa buttons
30 GIRAFFE IFU buttons
8 UVES buttons
Armagh, 19 February 2008
FLAMESFiber Large Array Multi-Element Spectrograph
NAMENAME min min (Ǻ)(Ǻ) max max ((ǺǺ)) ((ǺǺ)) RR
H 379.0 3700 3867 167 22500
H395 3854 4049 195 19600
… … … … …
H627.3 6120 6405 285 22500
… … … … …
H920.5 8960 9419 459 19000
FLAMES high resolution settings
Armagh, 19 February 2008
FLAMESFiber Large Array Multi-Element Spectrograph
NAMENAME min min (Ǻ)(Ǻ) max max ((ǺǺ)) ((ǺǺ)) RR
L385.7 3620 4081 461 8000
L427.2 3964 4567 603 6400
… … … … …
L614.2 6438 7148 746 8600
… … … … …
L881.7 8206 9400 1190 6500
FLAMES low resolution settings
Armagh, 19 February 2008
From less obvious to exotic
Photometry Multi-objects vs. 3D spectroscopy IR Imaging and spectroscopy Interferometry Radio X-rays, UV Astrometry (Gaia)
Armagh, 19 February 2008
NIR high resolution spectroscopy:CRIRES @ VLT
R=100,000 Spectral coverage = 5 nm!
Armagh, 19 February 2008
Future instruments: SPIROU@CHFT
Spectral coverage: 0.9 to 2.5 m Spectral resolution: R=50,000 15% throughput S/N ratio = 100 with 1h exp on a J=13 star Commissioning on 2013
Armagh, 19 February 2008
GIANO @ TNG
Similar to Spirou Commissioning in 2009 Attached at the Nasmith