... For historical reasons, it is useful to offer comparisons between the current WFPC2, and its predecessor WF/PC-1, which was returned to Earth in December 1993. Field format: WF/PC-1 contained 8 cameras and CCDs, each CCD having 800 x 800 pixels. ... Many differences derive from the fact that the WF/PC-1 CCDs were thinned, backside illuminated devices whereas the WFPC2 CCDs are thick, frontside illuminated devices. WF/PC-1 CCDs were thinned and backside illuminated. ...

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• Ionization and Thermal Structures of the Absorption-Line Systems of Quasars
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. Next: Table File System Up: No Title Previous: MIDAS User Levels . љ . This chapter will contain information on the data structures used in MIDAS such as keys ( keywords ), descriptors , frames ( bulk data frames ), catalogs , and tables . At the present moment we refer the reader to the previous chapter which gives a basic description of data structures used. Rein Warmels . Mon Jan 22 12:06:29 MET 1996

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• Structure of Tables
• Structure of the Book
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. Update is coming soon.

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• Examples of editing previous command lines
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... We describe a parallel code for 3-D structure detection and morphological analysis. The method is based on a multiscale technique, the wavelet transform and on segmentation analysis. ... This paper presents a new parallel code, that allows a rapid structure detection and morphological analysis in a 3-D set of data points. ... Segmentation analysis. ... Our code is based on the programming paradigm MASTER/SLAVE . ... Finally, the morphological analysis is executed by the master. ...

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• A New PROS Task for Calculating HRI Source Intensities or Upper Limits

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... In this section, we develop a physical model of the secondary as a disk that is centrifugally supported in the radial direction and hydrostatically supported in the vertical direction. We assume that the disk is vertically isothermal and well mixed. ... where is the mean molecular mass of the gas, is the orbital period at the outer edge of the disk in years, and all of the mass of the secondary has been assumed to be concentrated near its center, so the Keplerian approximation is valid. ...

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• Structure of the Spectral Package
• *qpspec* - Extraction of Photon Distributions from QPOE files
• The Chandra Multiwavelength Project (ChaMP)

Next: Sample Properties Up: Sample Identification Previous: Comments on Individual Sources . Previously known serendipitous sources were selected by cross-correlating WGACAT with a variety of optical and radio catalogs, including the Ver?n-Cetty & Ver?n (1996) and Hewitt & Burbidge (1993) quasar catalogs, the 1 Jy (Stickel et al. 1994) and S4 (Stickel & K?hr 1994) radio catalogs, and the BL Lac catalog of Padovani & Giommi (1995b). ... Details of these 97 objects are given in Table 6. ...

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• COBRA file structure
• CHAMELEON file structure
• Organization of data

Next: Contents Up: Description Previous: Description Index . ASAP data handling works on objects called scantables. ... Each row contains just one spectrum for each beam, IF and polarisation. ... A collection of cycles for one source is termed a scan (and each scan has a unique numeric identifier, the SCANNO). ... If you have scan-averaged your data in time, i.e. you have averaged all cycles within a scan, then each scan would hold just one (averaged) integration. ...

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• The structure of neutron stars
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• The SM Tutorial - Where do I go from here?

Next: Armagh Planetarium Up: Introduction Previous: Vision Contents . The Armagh Observatory and the Armagh Planetarium are distinctive organizations, part of a single corporate entity ``The Governors of the Armagh Observatory and Planetarium '' described in The Armagh Observatory and Planetarium ( Northern Ireland ) Order 1995, which superseded the original 1791 Act of the Irish Parliament entitled ``An Act for Settling and Preserving a Public ... Armagh Planetarium . ...

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• Robert Hill | International Year of Astronomy in Ireland | Astronomy 2009
• Armagh Planetarium
• EXTREME HELIUM STARS

Next: RGS_HKPARMINT Up: RGS_EXAFS Previous: References Contents . CCDID = 1 / CCD Identifier . ENERGY (eV) . MABSLEN (cm) . ... Next: RGS_HKPARMINT Up: RGS_EXAFS Previous: References Contents Michael Smith 2011-09-20 ...

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• ODF Structure
• Previous RGS source list.

Next: Transparency of the Stochastic Up: Model of the Galaxy Previous: Frequency distribution of galactic . ... The parameters of the model resulted from a numerical fitting of various data, such as the observed distribution of the young star population and neutral hydrogen, the density of population II stars in the vicinity of the Sun, the galactic rotation curve and the dynamics and distribution of globular clusters   and dwarf irregular satellites of the Galaxy. ...

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• The Transmission Gratings
• Frequency distribution of galactic binaries
• Transparency of the Stochastic Background

Main Program Travel Where to go in Moscow Information . ... The 2014 year marks the 100th anniversary of Yakov Zeldovich . ... John Carlstrom (University of Chicago) . ... Lyman Page (Princeton University) . ... The conference will be held at the Space Research Institute (IKI) in Moscow, Russia, on June 16-20, 2014 . ... International Conference: Cosmology and High Energy Astrophysics (Zeldovich-90) 20-24 Dec 2004, Moscow, Russia . ... 2014 Space Research Institute, Moscow Русская версия ...

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• Second Spectrum-RG/eROSITA Conference
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2007 Jan 08) Bright comet C/2006 P1 (McNaught) . 2005 Jan 20) Tornado near Coonabarabran . 2005 Jan 16) Major upgrade in progress . 2005 Jan 16) Near Earth Comet 162P/Siding Spring . 2004 Apr) 2004 CB identified as a comet . 2004 Apr) Systematic surveying commenced 2004 March 16 . 2004 Apr) Media Releases on commencement of survey . 2004 Jan) 'Accidental' discovery of 2003 XB22 . ... Siding Spring Survey Main Page . ... Previous News Items . ...

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• Emma Kirby - Outreach
• Research Interests
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. AO Home AO Astronomy Schedule Receivers CIMA AO IDL . Approved projects for 2015B . Approved projects for 2015A . Approved projects for 2014B . Approved projects for 2014A . Approved projects for 2013B . Approved projects for 2013A . Last updated: Sunday, 24-Jan-2016 08:26:24 AST . R. Minchin

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• The SMUDGES Survey
• Searching the Environment around LyAlpha Absorbers
• Simulations of 3 ALFA Surveys

... General information . ... Staff . Research staff . Technical, administrative & librarian staff . ... Staff in alphabetic order . Research . ... Technical reports . Projects . ... General interest seminars . ... IT Services . ... Information . Resources and catalogs . ... Historical highlights . Historical research . Historical archive . ... Projects and events . Online resources . ...

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Next: Amorphous magnesium silicate Up: Examples of data contained Previous: Examples of data contained . ... We have used the infrared optical constants of forsterite contained in the database for calculating the absorption cross sections of spherical and non-spherical particles in the Rayleigh limit (see Fig. The spectra are obtained by averaging the cross sections calculated for the three different crystallographic directions. ...

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• Examples of data contained in the JPDOC
• Wavelength dependence
• Model realization and some results

... Bojan Nikolic web pages (r. 329) . ALMA . ... AATM is a re-packaging of the version of ATM as used by the ALMA online calibration software ?TelCal?. ... The main reason for AATM is to bring the version of ATM used by ALMA to an as wide an audience as possible. ... This version of AATM therefore corresponds exactly to version on ATM-0_3_0 branch of the CVS, and will (I believe) be the same as what is used in ALMA 7.1. ... Computing dispersive atmospheric delay with AATM . ... ATM and AATM . ...

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• ALMA WVR phase correction algorithms and software Bojan Nikolic web pages (r.
• Atmospheric Modelling for ALMA
• OOF Reduction Software

. Album : asv-album :: Travels to distant places and countries :: 1997/08 Kyoto, Nara (Japan) :: 20/08 Nijo castle (ancient shogun palace). Assembly opening. Maiko . Up . << Prev . This shot is slightly better than previous. Next >> . Album created by album tool a Marginal Hack by David Ljung on Tue Jun 23 14:46:12 2015 .

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• Image: Harvard Medical School, view from the previous building
• Image: Same shot. Slightly worse than previous.
• RELATED WORK

... Aloisi, A. The Old Stellar Population . Alonso-Herrero, A. HST /NICMOS Observations of the . ... Balcells, M. HST-NICMOS Observations of Galactic . ... Baum, S.A. Investigating the Evolution of . ... Becklin, E.E. A Coronagraphic Search for . ... Clampin, M. The Old Stellar Population . ... Close, L. HST NICMOS Observations of . ... The Stellar Population in . Geballe, T.R. HST NICMOS Observations of . ... Greggio, L. The Old Stellar Population . ... Leitherer, C. The Old Stellar Population . ...

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• The Structure and Composition of High Redshift Radio Galaxies
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• NICMOS Science

. F IGURE . 6. Reconstruction of the distribution of Z for four groups of stars at the Solar Galactocentric distance within a column with a 80 pc 2 square base. See the caption for Fig.2 for a description of the plots for the four groups (a-d). The solid curve and Z 0 values have the same meaning as in Fig.5c . discussion in the text | previous figure .

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