... Gallery . ... Sidebar Left . Sidebar Top . No Sidebar . Sidebar Bottom . Sidebar Right . View full size . Title: Ganymede . Description: A close up view of Ganymede taken with the 24-inch (60cm) telescope at Siding Spring in October 1999. Areas of varying brightness define subtle differences in the surface terrain of the Moon. ... File name: ganymede.jpg . ... Ganymede A close up view of Ganymede taken with the 24-inch (60cm) telescope at Siding Spring in October 1999. ...

... region (region-6.2.2) [xmmsas_20030110_1802-5.4.1] . ... The region task will automatically determine the optimal source and background extraction regions for a detected source in an XMM observation. ... The regions are defined in sky coordinates. region will attempt to maximise the area of the extraction region for each source, whilst ensuring that the extraction regions of neighbouring sources do not overlap, and that the background extraction region for a given source excludes neighbouring...

Go to the previous , next section. ... The plot data may be defined to SM in a number of ways. ... The features of SM are described fully in the next few sections, but let us start with a description of how to produce your first SM plot. Before you start, notice that SM is case sensitive. Keywords may be typed in lower or uppercase (as we do in this manual), but we would recommend using lowercase. ... If you are interested, see the section on "overloading". ...

MRO Delay Line ICD Metrology System to Beam Relay System ICD INT-406-VEN-0013 The Cambridge Delay Line Team rev 0.1 10 August 2007 Cavendish Laboratory JJ Thomson Avenue Cambridge CB3 0HE UK 1 ICD Description Org UoC Owner MF Brief description and preliminary contents Defines space envelope for beam relay pipes above metrology table. One drawing defining beam relay pipe position. ... The full space envelope available for each beam relay pipe is detailed in the diagrams presented in the appendix. ...

... The GHRS has the usual components of an astronomical spectrograph: entrance apertures, a collimator, dispersers, camera mirrors, and detectors. ... The collimator and camera mirrors are unexceptional and need no further description here (see ``The HST Focal Plane and the GHRS Apertures'' on page 73 for details). ... The first two first-order gratings, G140L and G140M, have their spectra imaged by mirror Cam-A onto detector D1, which is optimized for the shortest wavelengths. ...

Next: Order Definition Up: Echelle Reduction Method Previous: Retrieving demonstration and . ... That is the mapping between the space wavelength, spectral order and the space sample x , line y in the raw image. ... Sections and describe the solution of this mapping. The second step in the reduction, described in Section , is to estimate the image background. ... In the rest of this Section the algorithms used in each step of the reduction are described. ...

... Science Users Information > Observing with ESO Telescopes > Phase 3 > Overview . ... Publications with ESO Data . ... Phase 3 FTP Upload . ... Create and upload the release description - 7. ... More about the concepts of data collection and release, see the Phase 3 User Guide , Sect. ... You validate the data before uploading them to ESO using the Phase 3 Release Validator , a java-based tool to be run locally on your system. ... You close the data release using the Phase 3 Release Manage r . ...

This example shows a difference between CSS's table model for HTML and for other document formats. The first, HTML, example is defined by HTML to be illegal, as it would lead to overlapping cells if HTML's rules for layout are followed. ... The diagram depicts how the two examples, the HTML one and the almost identical non-HTML one, might be rendered. ... The rendering of the non-HTML example is on the right, it follows the CSS rules and thus has no overlapping cells. ...

The optical scheme of the instrument is sketched in Figure 1 , it is designed to match the F/20 focal ratio of the TIRGO telescope. We have, following the optical path, the window of the dewar, the order sorting filter (not in figure), a field lens, in Calcium Floride, and the slit, in the focal plane of the telescope. ... The resolving power is (for first order of grating) of about 600 in the center of J band and 950 in the center of the K band, using a slit of two pixel (3.46 arcsec). ...

... StelTexture . StelTextureParams . ... Contains the parameters defining how a texture is created. ... StelTextureParams (bool qgenerateMipmaps=false, GLint afiltering=GL_LINEAR, GLint awrapMode=GL_CLAMP_TO_EDGE) . ... Define the scaling filter to use. Must be one of GL_NEAREST or GL_LINEAR. ... GLint StelTexture::StelTextureParams::filtering . ... Must be one of GL_NEAREST or GL_LINEAR. bool StelTexture::StelTextureParams::generateMipmaps . ... GLint StelTexture::StelTextureParams::wrapMode . ...

lte-codes . Sterne . ... In 2006, Behara and Jeffery introduced a new file format for the model atmospheres produced by STERNE and used by SPECTRUM and SFIT. ... allow depth-dependent descriptions of composition, and . ... model.lambda_ref <lambda ref > . ... abundance < elem > < abund > . ... structure.abundance < elem > : ( needs N depth ) . ab elem,1 , ab elem,2 , ..., ab elem,Ndepth > . ... structure.tau_ref : ( needs N depth ) . ... structure.opac_ref : ( needs N depth ) . ...