The oral sessions will consist of a mixture of 1 hour invited reviews and contributed talks of 30 and 15 min. ... Participants who will not be able to give an oral presentation due to time limitations, will be asked to contribute to the poster session, to stimulate further debate with their results. Please send the *Title* and *Abstract* of your contribution using the form below. ... Contributions received after June 15, 1999 will not be considered in the selection for the oral talks. ... poster . ...

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• Decadal Survey ASTRO 2010 - STScI Participation and Contributions
• Polycyclic Aromatic Hydrocarbon Contribution to the Infrared Output Energy of

NATIONAL ASTRONOMY AND IONOSPHERE CENTER . ... Astronomy . ... Visitor Center . ... Specifications . ... Power Supply . ... Center Frequency: 420 MHz (adjustable from 425 to 435 MHz) . ... Maximum instantaneous bandwidth: 2 MHz . Maximum Peak Power at transmitter output: 2.5 kW . Maximum Avg. Power at transmitter output: 150 kW . ... Power output variation: less than 0.2 dB pulse to pulse after 15 minutes warm up . ... Output power adjustability: continuously adjustable to ~20 dB . ...

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• VLBI at Arecibo Observatory
• Slide 11

I would like to propose two new features for the axes annotation in the GMT. 1st: In astrophysics, we often work with great ranges of values (many orders of magnitude). ... However, GMT 3.2 allows to plot annotations for log10 axes every integer log10 value or even more frequently. The proposed patch allows to specify large steps for the log10 axes, in the form illustrated by an example below. 2nd: 10^0 instead of 1, and 10^1 instead of simply 10 do not look beautiful. ... The patch is here. ...

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• Information for Authors

... One of the major activities going on at my Mira observatory at Sava, Italy, is to record deep sky CCD images for a personal atlas I'm currently working on. ... Images are made using a SpectraSource CCD HPC 1 camera equipped with a Texas Instrument TC215 chip, 1024 square, 12 micron pixels size, at 16 bit. ... After a 40sec exposure, the PC monitor showed a faint glow just above the camera termal noise. ... The image showed clearly a star in the galaxy core, of magnitude 14.5, some 50sec. ...

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• Contributions
• Contributions by amateurs: SN1995ad.
• Contributions by amateurs: SN1996X.

Program: MOMENTS Purpose: Program to calculate moments and other properties of a profile Category: MANIPULATION, CALCULATION, PROFILES File: moments.c Author: M. Vogelaar Keywords: INSET= Give set (, subsets): Maximum number of subsets is 2048. ... 3: Physical coordinate of peak value in profile. ... If there are a certain number of adjacent subsets with amplitudes within the given range, and this number of subsets is greater than or equal to WINDOW, these sub- sets are taken into account. ...

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• Archive of VLBI Observations Majordomo List
• How the rendering is done
• Student Contributions for Wildflowers in the Sky

Proceedings of the XXVIIth Young European Radio Astronomers Conference (YERAC). ... Please Note: e-mail addresses and external links in these contributions were correct when these papers were written in 1995, but may no longer be valid. ... In addition to the hypertext version of each paper, indicated by the link from the title of the paper, there are links to postscript versions of each paper, which are suitable for printing if you want a hardcopy of a given paper. ... Sandor Frey (or postscript ) . ...

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• Astrophysics Group STFC announces бе119 million contribution to The Square
• Contributing to casata Bojan Nikolic web pages (r. 329)
• Abstract

GTK+ 2.0 Tutorial . Prev . Next . This document, like so much other great software out there, was created for free by volunteers. If you are at all knowledgeable about any aspect of GTK that does not already have documentation, please consider contributing to this document. If you do decide to contribute, please mail your text to Tony Gale, gale@gtk.org . Also, be aware that the entirety of this document is free, and any addition by you provide must also be free. ...

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• Contributed Commands
• CCD Image Quality - PixelVision
• Russian-Finnish Symposium, Program

Weaving together Astronomy+Statistics+Computer Science+Engineering+Intrumentation, far beyond the growing borders . ... Archives . ... People . ... To my personal thoughts, the history of astronomy is more interesting than the history of statistics. ... Quintessential Contributions: . ... The contents are only spanned about 100 years and there are great chances that my mind still favors the history of astronomy over the history of statistics. ... Comment ( RSS ) | ... Entries RSS . ... Chandra Blog . ...

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• PAUL J. GREEN - Contributing ConcepTests
• Comments on: Quintessential Contributions By: hlee
• PAUL J. GREEN - Getting Students Involved in Physics & Astronomy!

Next: Armagh Observatory New TSN Up: G. New TSN Action Previous: What We Do . ... The Armagh Observatory seeks to develop this interest by disseminating the results of its scientific research through a programme of public outreach and public understanding of science (PUS). ... partnership with groups and institutions having similar aims and objectives, for example the Astronomical Science Group of Ireland and amateur astronomy organizations; . ...

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• What We Do

. July 14 . November 8 . Previous slide . Next slide . Back to first slide . View graphic version .

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• Description
• CCD gap and bad pixel corrections

... 30, 2006 . ... If you retrieve these files via a Web browser, please note that you need to use the browser's "Save As..." facility. ... Figures must be provided as Encapsulated PostScript files and should be incorporated in your contribution using the standard Latex2e "graphicx" package as demonstrated in the demo file author.tex. ... Please submit the LaTeX source file of your contribution, and PostScript/PDF files of any figures, via email (!!!) to Iris Bronnert ( ibronner@eso.org ). ...

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• ESO - cosmology2002
• AdelePlunkettAstro
• ESO - esaeso-2003

... We have observed and studied critical supercurrents, Ic, in cross-type Nb-Cu/Ni-Nb junctions with Josephson layers prepared from diluted ferromagnetic alloys. For suitable values of the exchange energy in the ferromagnet and the F-layer thickness we have observed Ic(T) oscillation with vanishing Ic for the definite values of T and dF. ... Critical supercurrents, Ic, in Nb-Cu(1-x)Ni(x)-Nb Josephson SFS junctions with F-layers prepared from ferromagnetic Cu(1-x)Ni(x) alloys have been studied. ...

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• Phys. Rev. B 54, 454 (1996): Neminsky et al. - ac susceptibility of Rb

... public class TiffDecoder . ... static int . ... Field Detail public static final int NEW_SUBFILE_TYPE . ... public static final int IMAGE_WIDTH . ... public static final int IMAGE_LENGTH . ... public static final int BITS_PER_SAMPLE . ... public static final int COMPRESSION . ... public static final int PHOTO_INTERP . ... public static final int IMAGE_DESCRIPTION . ... public static final int STRIP_OFFSETS . ... public static final int ORIENTATION . ... public static final int SAMPLES_PER_PIXEL . ...

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• FHT (ImageJ API)
• WISPI Optical Specifications

... Tonight's Sky . ... Sky this Month . ... milky way . ... The Sky This Week: April 1 - 10 . ... Sky this Week . ... Astronomy for Kids . ... Sky Events . Get to Know the Night Sky . ... Is there any way photons could contribute to the mysterious dark matter? ... Get instant access to subscriber content on Astronomy.com! ... If you are already registered on Astronomy.com, please log in below. ... Receive news, sky-event information, observing tips, and more from Astronomy's weekly email newsletter. ...

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Permitted Context: SELECT . ... The OPTION element can only occur within a SELECT element. ... When the form is submitted, the NAME of the enclosing SELECT element is paired with the OPTION's VALUE attribute to contribute a name/value pair for the selection. ... CLASS . ... The string to be used together with the name attribute of the enclosing select element, when submitting the form. ... SELECTED . ... This attribute is used within menus to define shaped hotzones associated with this option's value. ...

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• Acknowledgments
• Ordered Lists

. 1st column is the rest wavelength in Angstroms, 2nd column is the flux, 3rd is the error estimate, 4th the number of spectra contributing at that wavelength, 5th-7th the mean, minimum and maximum redshifts of the contributing spectra. Composite Spectrum of the Blue PHFS sub-sample. Composite Spectrum of the Blue PHFS sub-sample. Composite Spectrum of the LBQS sub-sample. Equivalent widths of the Parkes Quasars. Equivalent widths of the LBQS QSOs. Last updated 13th July 2001. Maintainer: Paul Francis , .

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• Siding Spring Survey

... PGP keys . How it gets done . ... amead@soltec.net - massive editing (many, many corrections), also tried to teach me about the proper use of the apostrophe (when it comes to written language and grammar I am incredibly bad). ... If you wish to contribute written material, edits, or other work to the LASG please email me at seifried@seifried.org . ... So the LASG master copy is stored on my NT Server (which I use as a workstation), and maintained via FrontPage, but how does it get to you? ...

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• LEONARDO TESTI - VIEWGRAPHS/PROCEEDINGS
• Programme - Fractionation of isotopes in space: from the solar system to
• Francesco Fontani's list of publications

ASTROPHYSICS AND COSMOLOGY AFTER GAMOW - THEORY AND OBSERVATIONS . Gamov Memorial International Conference dedicated to 100-th anniversary of George Gamow . ... All contributions should be sent to Prof. S. Silich, e-mail: silich@inaoep.mx using the Macros ( pdf , ps , tex ), the session where your contribution was made. ... The length for the contributions will be:   . ... plenary talks – 12 pages . memorial talks – 6 pages . oral contributions – 4 pages . ... posters – 3 pages . ...

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• Sponsors of Views of the Solar System
• Session in Odessa
• Geomagnetic Indices Kp, ap, Ap, Cp and C9

... Browse on Line . ... To get this to work, add a macro menu item which calls open_include() . ... Oops. ) return } # # We have a filename ; now run through our list of paths see # if we can open the file . # include_path = $g_ include _path path_separator = : bpos = 0 epos = search_string( include_path , path_separator, bpos ) while( epos bpos ) { path_bit = substring( include_path , bpos , epos ) if( open_with_test (path_bit / ...

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• Laboratory for the Stellar Magnetism Study of SAO of the RAS - Magnetic stars -
• Linux I/O port programming mini-HOWTO: Credits
• [NEdit] FAQ: Where to get information

LBO LBO has many unique characteristics that contribute to its wide use as a nonlinear optical crystal. ... LBO Specifications Wavefront Distortion Dimension Tolerance Clear Aperture Scattering Sites Flatness Surface Quality Parallelism Perpendicularity Angle Tolerance Damage Threshold /8 at 633nm (W: +/- 0.1mm ) x (H: +/- 0.1mm ) x (L: + 0.2mm/- 0.1mm ) 80% of central area No visible scattering centers when inspected by a 30 mW green laser /8 at ...

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