... User Guide ] Task: uvlin Purpose: Separate continuum and lines in a spectral data-set. ... No default. ... The output can be either the line, continuum, or fitted line shape, as specified by the options keyword. ... This is the default. fit The output data-set is the fitted line shape data. ... The "nowindow" option causes uvlin to do a single fit over all windows. lpropc The line shape is constant throughout the data-set, and the intensity is proportional to the continuum strength. ...

... Archives . ... The PCA and ICA is used for separating mixed components with some assumptions. ... The need of source separation methods in astronomy has led various adaptations of decomposition methods available. ... I rarely come up with a paper which gathered and summarized component separation methods applicable to astronomical data. In that regards, the following paper seems useful to overview methods of reducing dimensionality for astronomers. [arxiv:0805.0269] . ... Chandra Blog . ...

... 314, 2004 F. Ochsenbein, M. Al len, and D. Egret, eds. BDB - a database for all typ es of double stars Edouard Oblak, Bernard Debray Besanёon Observatory, F-25010 Besanёon Cedex, UMR CNRS 6091 c c Tomasz Kundera Cracow Observatory, PL-30244 Cracow Abstract. We present the general characteristics of a database for binary and multiple stars from all observational categories, specifically designed to address the awkward topics of the identification of stellar components. ...

. Some commands accept multiple options. These can be grouped together after a single hyphen: command -abc argument . A small number of commands require each option to be given separately. Check the command synopsis for a command to see how a command requires its options to be given. An option that takes an argument, such as the name of a printer or a filename is given separately. Examples .

... A MIDAS command line is structured as command/qualifier par1 par2 ... par8 !comments . ... In case you omit the qualifier, the default qualifier of that command is used by MIDAS. The default qualifier of a MIDAS command may be displayed via SHOW/COMMAND command . ... If the command procedure which is activated by a MIDAS command uses the CROSSREF command, it is also possible to execute that command via: command/qualifier label4=par4 label1=par1 label7=par7 ... !comments . ... command/qualifier ? ...

... The analysis of NICMOS polarization images is aimed at determining the Stokes' Parameters, and from those the polarization angle and degree for each pixel. NICMOS Camera 1 and Camera 2 each contain three polarizers, whose principal axes of transmission are separated by 120 degrees. ... The images in the three filters need to be compared, in order to produce the Stokes' parameters. ... The Stokes parameters can then be combined to yield the polarized intensity, I p: . ...

A1634 2002-Feb-01 20:19:52 Technical Page Proposal Type: Regular General Category: Astronomy Sub-Category: Spectroscopy Observation Category: Extragalactic Total Time Requested: 36 Hours Proposal Title: The LGS 3 Field: Resolving a Possible HVC-Dwarf Spheroidal Interaction ABSTRACT: We have used Arecibo (A1340) to observe a previously unresolved HI cloud near LGS 3 and determined it is actually a high-velocity cloud (HVC) separate from the dwarf galaxy. ... X Maybe Part of the observing run. ...

... Meta Index / Home Page / Description / Generation of the Calibration / Using the CCF constituents . Normally a valid CCF constituent will have the CATEGORY attribute set to XMMCCF . However, it is possible to instruct cifbuild to accept constituents with a different category via the parameter category . ... If the parameter append is true, then cifbuild appends to the CIF set pointed to by calindexset any other CCF constituent that is not already in that CIF. ...

... Cross-shaped galaxy ZGC 2315+03 (Fig.1) has been described by Zwicky (1971) as ``post-eruptive or the result of the crossing of a compact galaxy through an edge-on spiral'' . This object was included in the Polar-Ring Catalog (C-71) by Whitmore et al. (1990) as a possible candidate for Polar-Ring Galaxies (PRG). ... One of them is galaxy 'disk' and the other is 'polar-ring'. ... The facts against the polar-ring nature of ZGC 2315+03 can be summarized as follows: . ...

The nasa.gov site requires that JavaScripts be enabled in your browser. ... Contact NASA . ... The following are astronauts who are employed at NASA. Astronaut assignments and category definitions (e.g., "active" astronauts, "management" astronauts) are contained in a separate Flight Operations Directorate (FOD) policy letter. Astronaut . ... Acaba, Joseph M. 2004 . ... Aunon, Serena M. 2009 . ... Barratt, Michael R. 2000 . ... Burbank, Daniel C. 1996 . ... Cassada, Josh A. 2013 . ... 1998 . ...

. B0101ћ8-3012 . Redshift = 0.89, Separation = 16 arcsec. Projected separation is 71/h kpc. The difference in the measured velocities is 300?850 km/s. From the flux ratios, it is clear that the continuum shapes are also remarkably similar. | Front page | . | << - QSO close pairs | . Robert J. Smith, ">rsmith@mso.anu.edu.au Last modified: Fri Sep 24 11:39:02 EST 1999 .

See also: Name-based Virtual Hosts Support . As the term IP-based indicates, the server must have a different IP address for each IP-based virtual host . ... There are two ways of configuring apache to support multiple hosts. ... For each installation, use the Listen directive in the configuration file to select which IP address (or virtual host) that daemon services. e.g. Listen www.smallco.com:80 I