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... The molecular lines group at Arecibo Observatory consists of Chris Salter, Tapasi Ghosh and Robert Minchin. ... The molecular line group at Arecibo Observatory started in 2006 with a proposal to carry out a spectral census of the star-burst galaxy Arp 220 . ... However, the most interesting discovery came from the observations of the polar ring galaxy, NGC 660. ... Molecular Lines in NGC 660 Arias de Saavedra Benitez et al., ... A cm-Wavelength Search for Pre-Biotic Molecules in Starburst Galaxies. ...

... Bojan Nikolic web pages home . ... I've made a little command-line program that calls the routines for . retrieval of water vapour and phase correction coefficients that I . ... http://www.mrao.cam.ac.uk/~bn204/alma/libaircmdline.html . ... http://www.mrao.cam.ac.uk/~bn204/alma/sweng/libairbuild.html . ... Bojan . Bojan Nikolic Tel: +44 1223 746432 . ... Cavendish Laboratory Fax: +44 1223 354599 . ... Copyright 2012, Bojan Nikolic feedback welcome ...

Updating... 1-st camera description . 2-nd camera description . Astronomical sites Webcams . ... Refresh after s. BTA "in-dome" TV-camera . Archive ) . BTA "outdoor" TV-camera . ... World Observatories Webcams List. ... direct image streaming . ... the only image stream . ... ActiveX module . ... Axis ActiveX module for Microsoft Internet Explorer) . Java Applet . ... Cambozola Java Applet for any browser with Java ) ...

... 2002 Calibration Workshop . Proceedings of the 2002 Calibration Workshop which includes the installation of the ACS and the NICMOS cooling system, was held on October 17-18, 2002, at STScI. Hubble Science Legacy conference . Proceedings of the Hubble Science Legacy conference which was held from April 2-5, 2002, at the University of Chicago. ... CTE Workshop . ... Proceedings from the HST Calibration Workshop that was held at the Space Telescope Science Institute November 15-17, 1993. ...

... User Guide ] Key: line The ``line'' parameter determines the channels that are to be processed from a uv data-set. ... The string part of the line parameter is used to select the spectral or wideband channels. ... The four numbers that accompany the string give: nchan, start, width, step These four numbers specify which channels to select from the input dataset and how to combine them to produce the output channels that the Miriad task will work on. nchan is the number of output channels produced. ...

... An interactive IRAF task for the analysis of Extreme Ultraviolet Explorer ( EUVE ) emission line spectra is presented. The line flux in extracted spectra may be measured by multiple techniques, including fitting individual lines. ... To aid in identifying lines, the positions of known lines may be marked on the spectrum during the fitting process. Also, model EUVE spectra may be constructed and overlaid using plasma emissivities and source emission measures supplied by the user. ...

... Archives . ... tutorial] multispectral imaging, a case study . ... Off from papers for bridging two, allow me to talk about something relevant to the cultural difference between astronomers and statisticians. I hope this could generate a series of comments. ... Comment ( RSS ) | ... Facebook, LinkedIn, hi5, etcтАж in addition to personal blogs. ... Many of signal processing researchers are like the statisticians you describe. ... Comments RSS . ... Entries (RSS) and Comments (RSS) . ...

In order to calculate the line profile of a given absorption line for atomic species Z with a wavelength LAMBDA (in Angstroms) and a microturbulent velocity VT (in km/s). ... mode . ... 1) The input model may contain more than one model (i.e. it may be an entire grid of models). Spectrum will cycle through this grid NMOD times, omitting NSKIP-1 models from the . ... However, the input data following MODE must be repeated NMOD times in order to obtain equivalent results for each model in the grid. ...

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