Return-Path: 100316.3710@CompuServe.COM Return-Path: <100316.3710@CompuServe.COM> Received: by hil-img-4.compuserve.com (8.6.10/5.950515) id UAA14169; Wed, 13 Nov 1996 20:16:12 -0500 Date: 13 Nov 96 20:14:29 EST From: A C Pickwick <100316.3710@CompuServe.COM> To: Richard West Subject: Observing Proposal Message-ID: <961114011428_100316.3710_JHF55-1@CompuServe.COM> Dear Richard, Please find below an observing proposal for the Dutch Telescope. Regards, Alan. *************************************************************************** Binary Star System 66 Cet To obtain images of the well documented binary star system, 66 Cet, using a range of filters. To process the data and compare it to the published data. To use the data to make a colour image of the system. Manchester Grammar School, Sixth Form Astronomy 02hrs 12.8min, -02deg 24min (J2000) 66 Cet also known as ADS 1703 Binary 5.7 and 7.5 Filter 634 - U with ND4 filter. Exposure 10 seconds Filter 419 - B with ND4 filter. Exposure 10 seconds Filter 420 - V with ND4 filter. Exposure 10 seconds Filter 421 - R with ND4 filter. Exposure 10 seconds Only ND4 filter. Exposure 10 seconds If possible, a set of exposures on a nearby photometric standard star of about 6th magnitude using the same five settings. A representative flat field for the TEK CCD The exposures should produce maximum pixels with 1000s to 10000s of electrons and so be above the noise but well below saturation. To attempt to apply the physics of blackbody radiation to the two stars, F8 and G4. To attempt to fit the results to the Planck radiation curves and to consider how to make a true colour image. Bright stars have been chosen as there is some scattered moonlight to contend with. The separation of the pair is 16.5 sec, so the centres of the images are about 37 pixels apart. With reasonable seeing, the stellar images should be a few pixels in extent. Manchester, UK 10 November 1996 *************************************************************************** ------- End of Forwarded Message