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MK Equinox Meeting March 2008 Cassegrain upgrades UIST Controller upgrade: EDICT replaced by ARC Improved performance in all modes; Full-array readout.

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Presentation on theme: "MK Equinox Meeting March 2008 Cassegrain upgrades UIST Controller upgrade: EDICT replaced by ARC Improved performance in all modes; Full-array readout."— Presentation transcript:

1 MK Equinox Meeting March 2008 Cassegrain upgrades UIST Controller upgrade: EDICT replaced by ARC Improved performance in all modes; Full-array readout in thermal bands 1kx 1k 4-point mosaic M’ (4.8 microns) Original readout method Saturated toward centre of array 1kx 1k 4-point mosaic M’ (4.8 microns) Row-reset readout No saturation More headroom, so Improved sensitivity BEFOREAFTER

2 MK Equinox Meeting March 2008 Cassegrain Upgrades Full commissioning of UIST coronagraphic imaging and imaging polarimetry Target behind the wider (1.3 arcsecond) occulting wire Slot 1 Slot 2 o o e e

3 MK Equinox Meeting March 2008 Cassegrain Science Highlights Radial Profile Null Profile (psf-psf) First Science Use of Coronagraphic Imaging Polarimetry - Wisniewski et al. 2008 in prep - Herbig Ae proroplanetary disk: HD 163296 - Variable outer structure in HST optical coronagraphy - UIST Coronagraphic Polarimetry: subarcsecond disk structure

4 MK Equinox Meeting March 2008 Cassegrain Science Highlights Cloud spectrum modelled with cloud layer at 200-400mbar Uranus + Moons + cloud Uranus + Moon – UIST imaging, CH 4 filter UIST Narrow-Band Imaging and Long-slit spectroscopy - Irwin et al. 2008 in prep - First data taken with new ARC controller - Uranus cloud circulation spectroscopy and context imaging - Cloud feature discovered at 200-400mBar level

5 MK Equinox Meeting March 2008 UKIDSS UKIDSS LAS passes z=6 for QSOs Gemini-S / GMOS Warren et al. 2008 in prep UKIDSS + SDSS izYJ (initial candidate list) LT I (remove M dwarfs) UKIRT YJ (confirm high QSO probability) 8-m spectroscopy (final confirmation & z)

6 MK Equinox Meeting March 2008 UKIDSS Zoomable mosaic of the GPS http://surveys.roe.ac.uk:8080/wsa/gps_mosaic.jsp

7 MK Equinox Meeting March 2008 Campaigns U/CMP/1 - Coma Cluster of Galaxies (Mouhcine) - 12 nights U/CMP/2 - WFCAM Transit Survey (Hodgkin, Pinfield) - 200 nights U/CMP/3 - High-z Elliptical Galaxies (Best, Smail) – 45 nights U/CMP/4 – GRB monitoring (Tanvir) – 235 hours Total time allocations All but U/CMP/1 are under way.

8 MK Equinox Meeting March 2008 Campaigns Example: U/CMP/3 (HIZELS) – looking for H-alpha at z~2 Geach et al. 2008 in prep.

9 MK Equinox Meeting March 2008 Campaigns Example: U/CMP/3 (HIZELS) – looking for H-alpha at z~2 Geach et al. 2008 in prep.


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