Contents 1. ING INSTRUMENTATION IN SEMESTER 2002A 2. EC funding for observers 3. Availability of SARG on the TNG *** NEW! **** ============================================================================== ING INSTRUMENTATION IN SEMESTER 2002A GENERAL INFORMATION Detailed information on ING instrumentation offered for the forthcoming semester can be found in the ING web pages at http://www.ing.iac.es/Astronomy/observing/instruments.html and guidelines for proposal submission can be found at http://www.ing.iac.es/Astronomy/observing/INGinfo_home.html Applicants are recommended to refer to these pages for the latest information. Applicants should be aware that occasionally highly rated proposals may not be awarded time due to scheduling constraints. In 2002A this will be particularly relevant to NAOMI and INTEGRAL programmes competing for access to GHRIL, and to programmes competing for INGRID at Cass and INGRID in GHRIL with NAOMI. NAOMI runs will be restricted second half of the semester while INTEGRAL runs will be scheduled in the first half. An additional constraint is that INGRID will not be available until approximately 22nd March (beginning of bright time) due to essential engineering work. Further, due to planned modifications of the Nasmyth platforms which are due to start in the summer of 2002, UES may not be available towards the end of the semester. ING INSTRUMENTATION IN SEMESTER 2002A WHT - http://www.ing.iac.es/Astronomy/telescopes/wht/ --- Applicants are reminded that to encourage proposals for larger time allocations on the WHT, the PATT2 application form allows a 2-page scientific justification for WHT proposals of six or more nights. The following instrument/detector configurations are available: Instrument + Detector ISIS BLUE + EEV12 ISIS RED + TEK AUX-port/UBVRI + TEK UES + SITe1 or 2xEEV Mosaic PRIME + 2xEEV Mosaic AUTOFIB2/WYFFOS + TEK (small fibres only - shared-risks basis) INTEGRAL/WYFFOS + TEK INGRID + 1kx1k HgCdTe NAOMI/INGRID + 1kx1k HgCdTe (shared-risks basis) Notes: NAOMI/INGRID observations will be carried out in service mode. AUTOFIB2: Only small fibres are available Visitor Instrument Contacts: LDSS2 - Richard Bower, R.G.Bower@durham.ac.uk SAURON - Tim de Zeeuw, tim@strw.leidenuniv.nl S-CAM - Michael Perryman, mperryma@astro.estec.esa.nl TAURUS - Richard McMahon, rgm@ast.cam.ac.uk INT - http://www.ing.iac.es/Astronomy/telescopes/int/ --- Instrument + Detector WFC + 4xEEV IDS 235/500 + EEV10 or TEK Visitor Instrument Contacts CIRSI - Richard McMahon, rgm@ast.cam.ac.uk Observing time is allocated in blocks of one week on average, and observing programmes shorter than *4* nights are not accepted, unless explicitly agreed in advance by the Head of Astronomy or the Director of ING. JKT - http://www.ing.iac.es/Astronomy/telescopes/jkt/ --- Direct imaging (2kx2k SITe2) The JKT only supports one common-user instrument, and private instruments are not accepted. Observing time is usually allocated in blocks of one week, and observing programmes shorter than *5* nights are not accepted, unless explicitly agreed in advance by the Head of Astronomy or the Director of ING. ============================================================================== EC FUNDING FOR ACCESS TO ING TELESCOPES Under the auspices of the EC's Access to Research Infrastructures Programme, EC funding to cover travel, accommodation and subsistence costs will be available to observers meeting certain criteria of eligibility. Refer to http://www.otri.iac.es/eno/ for further details. ============================================================================== Availability of SARG at the TNG As part of a collaboration between ING and TNG, NL and UK observers may apply to use the TNG high resolution spectrograph, SARG. Depending on demand, up to seven nights will be available to the NL & UK communities. SARG is a high efficiency echelle spectrograph designed for the spectral range from 370 up to 900 nm, and for resolutions from R=29,000 up to R=164,000. Both single object and long slit (up to 30 arcsec) observing modes are possible. A dioptric camera images the cross dispersed spectra onto a mosaic of two 2048X4096 CCDs. Note that successful applicants to SARG/TNG will qualify for EC funding. Further details on the TNG and SARG may be found on their web site www.tng.iac.es Please note that NL and UK applicants for SARG should apply using their standard PATT/NL form and should send these to their own national TAGs. Do not apply to the TNG. CAT observers should apply for TNG time in the usual way. ============================================================================== Danny Lennon Head of Astronomy, ING September 10th, 2001 ============================================================= * 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 address in the body of the message, where address 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/ =============================================================