OPPORTUNITY TO USE S-CAM ON THE WHT S-CAM ON THE WHT IN SEMESTER 2003B Michael Perryman (ESA) advises that he will make the new 10x12-pixel S-CAM available on the WHT in 2003B. Observers interested in collaborative use of the instrument are invited to contact him before the end of 2002. His email is: mperryma@rssd.esa.int The S-CAM web page is on: http://astro.estec.esa.nl/SA-general/Research/Stj/ S-CAM is based on the principle that a UV/optical/IR photon can break Cooper pairs in a superconductor and release an electron packet of size proportional to the photon energy. This makes possible high-speed photon counting, in which the arrival time and the photon energy are measured simultaneously. The system provides high QE over a broad wavelength range, with zero readout noise. Summary of detector properties: Detector area: 10 x 12 pixels, 0.8 arcsec/pixel Wavelength coverage: 350-750 nm Wavelength resolution: ~10 at 500 nm Photon arrival time tagging to about 1 microsec Count rate: (very approx) 200 counts/s at V=18 in V band Bright magnitude limit: about V = 14 (brighter requiring ND filters) Publications: Optical STJ Observations of the Crab Pulsar, Perryman et al, 1999, AA, 346, L30 S-Cam: an Imaging Spectrophotometer Based on Superconducting Tunnel Junctions, Rando et al, 2000, Experimental Astronomy, 10, 499 High-Speed Energy-Resolved STJ Photometry of the Eclipsing Binary UZ For, Perryman et al, 2001, MNRAS, 324, 899 Direct Determination of Quasar Redshifts, de Bruijne et al., 2002, AA, 381, L57 Eclipse Mapping of HU Aqr from STJ Observations, Bridge et al., 2002, MNRAS, in press High-speed energy-resolved STJ photometry of the eclipsing dwarf nova IY UMa, Steeghs et al., 2002, MNRAS, in press ING-IAC CONFERENCE ON SATELLITES AND TIDAL STREAMS ING-IAC joint conference SATELLITES AND TIDAL STREAMS May 26-30, 2003 La Palma, Canary Island, Spain * Scientific Advisory Committee: A. Burkert (Germany), M. Irwin (UK), A. Klypin (USA), D. Martinez-Delgado (Spain, co-chair), S. Majewski (USA), M. Mateo (USA), F. Prada (Spain, co-chair), R. Rebolo (Spain), P. Schneider (Germany) and R. Zinn (USA) * Local Organizing Committee: F. Prada (chair), D. Martinez-Delgado, R. Corradi, J. Mendez, A. Zurita J. de Araoz, T. Karthaus, E. Bejarano * Principal Topics: - Satellites of galaxies: bright and dark - The dark matter content of dSph and LSB galaxies - Tidal streams: probes of the structure and formation of the Milky Way and other Nearby Large Galaxies - Predictions of Cold Dark Matter models on small scales - Compact HVCs and galactic substructure - Mass substructure from gravitational lensing * Contact: Francisco Prada & David Martinez-Delgado. Email: sattail@iac.es * 1st announcement due to November 12th, 2002 ============================================================= * To unsubscribe from [INGNEWS] send to majordomo@ing.iac.es the command "unsubscribe ingnews" in the body of the message. Please don't type in the quotation marks and leave the subject field and the rest of the body empty. * You can subscribe to this mailing list by sending an email to majordomo@ing.iac.es with the message "subscribe ingnews " in the body of the message, where should contain your email address, e.g. einstein@xyz.ac.uk. You can subscribe a colleague in the same way if you have subscribed your address previously. * For further information on ING, point your browser to: http://www.ing.iac.es/ =============================================================