We present new images (ground-based optical and mid-infrared [MIR] from the Spitzer Space Telescope) and spectra (from Spitzer) of the archetypal starburst galaxy M82. The Spitzer data show that the MIR emission extends at least 6 kpc along the minor axis of the galaxy. ... The colors of the MIR emission and the spectra indicate that there is a strong component of aromatic feature emission (the MIR features commonly attributed to polycyclic aromatic hydrocarbons). ... ADS Citation Query . ...

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• Detection of Extended Red Emission in the Diffuse Interstellar Medium
• Spitzer Survey of the Large Magellanic Cloud, Surveying the Agents of a
• Dust Emission Features in NGC 7023 between 0.35 and 2.5 Microns: Extended Red

... Category: CLEAN, MANIPULATION, RADIO, TABLES File: clean.c Author: K.G. Begeman Description: CLEAN finds point source components and subtracts them with their antenna response. ... Keywords: INSET= Set and subset(s) of dirty map(s)/line(s). Maximum number of subset(s) is 2048. ... DEFSET= Set and subset(s) for definition of search area [Search area defined by box]. CLEAN looks for components only where the values in these maps/lines are not equal to BLANK. ... CUTOFF= Cutoff level [0.0]. ...

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• http://www.atnf.csiro.au/pub/people/atzioumi/vsop_ao2/stj_ao2_gps.ps
• casacore: components/ComponentModels/DiskShape.h File Reference
• casacore: components/ComponentModels/PointShape.h File Reference

Extended time series of Solar Activity Indices (ESAI) is database including observational, synthetic and simulated sets to study Solar magnetic field variations and their influence on the Earth. ESAI extend the ordinary lengths of some traditional indices of solar activity: sunspot areas, Wolf numbers (equatorial component of magnetic field of the Sun), polar faculae numbers (polar component), mean latitudes, N-S asymmetry of hemispheres (location of activity). Series . ...

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... Measured Radio Parameters for 116 extended sources without col.10 (T peak) and col.12(Ref.) ... An asterisk in byte 9 indicates that this line refers to the whole source or major parts of it (same as 'c' in byte 38) (1) (2) (3) (4) (5) (6) (7) (8) (9) (11) source Type RA1950 Dec1950 LAS PA Wmaj Wmin PA S_408 cmp h m s +-s d m s +-" (') deg (') (') comp Jy ----+----1----+----2----+----3----+----4----+----5----+----6----+----7- 0002+12 a M2 000208.1 0.3 +123232 9 3.5 105 1.5 ...

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• Sky background definition
• Principal Components Analysis
• The BSA SNRs Survey

... Flux density at 1 GHz (/Jy): 2720 . ... 1991, ApJ, 373, 146. ... ADS . ... VLA at 1.4 GHz and 4.8 GHz (both 1".3), for polarisation studies. ... VLA at 1.4 GHz and 4.8 GHz, for proper motion studies. ... 151 MHz observations for bulk expansion studies. ... Chandra observations, showing outer shock. ... Fesen et al. ... Spitzer observations. ... Chandra observations of rim. ... 2006, ApJ, 636, 848. ... 2006, ApJ, 647, L41. -ray line observations. ... Spitzer and Chandra observations for 3-D structure...

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• Inference of Coefficients for Use in Phase Correction
• Inference of Coefficients for Use in Phase Correction Bojan Nikolic web pages
• OptInt PmWiki : Component Documentation | History

... 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 . ...

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• Comments on: [ArXiv] component separation methods By: hlee By: Sam Leach
• The AstroStat Slog component separation
• Chandra's View of M86

Comment on J2246-1206 . In contrast to the jet pointing to the NE in our image, the 5 GHz VLBI image of Shen et al. (1998) shows no indication of extended emission above the 20 mJy/beam level. Hong et al. (1999) find a jet component to the SE and identify that with a "superluminal" component possibly ejected in 1992. A 15 GHz image from the USNO database, taken nearly at the same epoch as the image of Hong et al. (1999) does not show any component at this position angle. ...

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XMM ­Newton CCF Release Note XMM ­ CCF ­REL­11 RGS CCD Properties C. Erd October 4, 2000 1 CCF components Name of CCF VALDATE List of Blocks changed CAL VERSION XSCS flag RGS1 ADUCONV 0004 2000 ­02­06T16:50:00 ADUCOEFF, OFFSET GAIN --- NO RGS2 ADUCONV 0005 2000 ­01­25T16:27:00 ADUCOEFF, OFFSET GAIN --- NO RGS1 CTI 0001 1998­01­ 01T00 :00:00 CTI , ... The CCD redistribution function is described with a phenomenological model [1, 3], whose parameters are stored in RGS REDIST. ...

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• http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0005-1-0.ps.gz
• http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0159-1-1.ps.gz
• http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0246-1-0.ps.gz

... Class . ... SUMMARY: NESTED | FIELD | ... METHOD . ... java.lang.Object java.awt.Component java.awt.Button ij.gui.TrimmedButton . ... Nested classes/interfaces inherited from class java.awt.Button . ... Nested classes/interfaces inherited from class java.awt.Component . ... Field Summary . Fields inherited from class java.awt.Component . ... Methods inherited from class java.awt.Button . ... Methods inherited from class java.awt.Component . ... Methods inherited from class java.lang.Object . ...

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• MultiLineLabel (ImageJ API)
• ProgressBar (ImageJ API)
• ImageJApplet (ImageJ API)

... Астронет | ... Термин "component" . ... компонента . ... составляющие [компоненты] радиоизлучения Солнца . ... составляющие [компоненты] солнечного радиоизлучения . ... основная компонента (радиоизлучения Солнца) . ... составляющая (радиоизлучения всплесков IV типа) в сантиметровом диапазоне (радиоизлучения Солнца) . ... жесткий компонент (напр. корпускулярного излучения) . ... спорадическая [быстрая] компонента (радиоизлучения Солнца) . ... составляющие [компоненты] радиоизлучения (напр. ...

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• Spacecraft Rosetta Shows Comet has Two Components
• Астронет > Spacecraft Rosetta Shows Comet has Two Components
• Астронет > Страница 33

... Herschel Mission . ... Water along the outflow from a young nearby protostar: a Herschel view . ... Figure 1 shows a detailed view of the IRAS4A outflow through the comparison between the H 2 O emission and the emission from several other molecular tracers of gas with different excitation conditions: H 2 , CO(3-2), CO(14-13), and CO(6-5). The figure nicely reveals where shocks deposit energy into the molecular cloud, lighting up the water emission along the outflow . ...

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• HwB: EISA Connector (Offline)
• Abstract
• Microwave components: few tests

... Currently, there is very little information on comets which are active beyond the orbit of Jupiter. ... Previous observations conducted by our team with the SAO RAS 6-m telescope showed that some of these comets have extended tails dissimilar to the tails of comets forming at close heliocentric distances. ... We for the first time measured the linear polarization of scattered emission for the two distant comets C/2010 S1 (LINEAR) and C/2010 R1 (LINEAR) at heliocentric distances of 5.9-7.0 au. ...

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• Discovery of enrichment of the envelopes of post-AGB stars with heavy metals
• IRAS01005+7910
• Optical component of GRB080319B

CIMA is more than just the observing tool - in fact, the observing tool is just a part of a bigger package called the CIMA software package. ... There is also a another package called the CIMA WAPP software which contains the WAPP software, the special Tcl/Tk interpreter used by CIMA and support libraries. ... All CIMA software components recognize the following general options that are part of the CIMA version selection system: . ... The select_cima script can be used to set up a default version. ...

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• Chapter 5. Listing of Installed Components
• HI Self-Absorption in the Canadian Galactic Plane Survey: First Results
• Some useful data about gains, NFs & compression points of Eddies box components

Last time we saw that flat rotation curves for galaxies, when measured in galaxies with extended gas distributions, provides unambiguous data that shows the mass distribution is dominated by an unseen, spherical halo. ... Perhaps only galaxies with extended dark matter halos are capable of retaining large gaseous extents? . ... Clusters of Galaxies: . ... The case of the Cancer cluster: . ... Below is the velocity distribution of galaxies in the Cancer cluster: . ... What's going on in Cancer? ...

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• The Greenhouse Effect.

... The IRAF 2 display server, XImtool, has been enhanced to allow arbitrary custom components to be dynamically integrated, permitting the functionality of the main display server program to be extended in arbitrary ways with no change to the core program. Components may include both computational and GUI elements; new components are interfaced as named instances of the Widget Server Client class and are fully integrated into the base server using messaging. ...

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• TwoFitlines: An Spectrum and Line Analysis Tool
• Image Reconstruction with Few Strip-Integrated Projections: Enhancements by
• A Spectroscopy Exposure Time Calculator for IRAF

... Keck spectropolarimetry, giving spectral coverage from Ly- to beyond CIII], and HST imaging of a sample of powerful radio galaxies with has been obtained. ... This is a short progress report on a rather extensive programme we are carrying out to study the structure and composition of high redshift radio galaxies (HzRG) -- and, by implication, the host galaxies of radio quasars -- using observations in the optical, IR and mm bands. ... An example of the NICMOS and WFPC 2 imaging is shown in Figure 2 ...

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• ST-ECF IRAF package
• Introduction
• ESLAB 2007

... DpmkSpace (part of SAS) . Cdb server (part of calibDB, in Garching only . Dpserver (part of SA, in Garching only) More about P2PP checks to be performed when installing/configuring it. Go to top of page . More about OT-tcl/tk checks to be performed when installing/configuring it. ... More about Java-OT checks to be performed when installing/configuring it. ...

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• Triple with velocity curves for all components
• Uncorrelated flux component
• DFS Group Home Page

. Search this album . Gallery . :: The First 100 Years . :: Workshops and computer labs . :: Richard Woolley and Jim Banham inspecting optтАж . Sidebar Left . Sidebar Top . No Sidebar . Sidebar Bottom . Sidebar Right . View full size . Title: Richard Woolley and Jim Banham inspecting optical and mechanical components, optical munitions factory, 1944 . File name: OpticalMunita.jpg . Dimensions: 800 x 601 px . Page: 1 2 3 4 5 6 7 8 9 10 24 25 . Powered by Gallery 3.0.9 (Chartres) . Login

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• GSAOI Component Supplier Links Page
• GSAOI Dwarf Galaxies Science Page
• Software Maintenance Manual

... Iron abundance in the atmospheres of components of the binary system 41 Draconis . ... 5B Iron abundances, FeI and FeII lines equivalent widths, and microturbulence velocities were found for the components of a highly eccentric spectroscopic and interferometric binary system 41 Dra from high resolution spectra obtained close to the periastron. Weighted mean values of iron abundances in the atmospheres are lgN(Fe) = 7.66 ± 0.03 and lgN(Fe) = 7.72 ± 0.03 for the component a and b, correspondingly. ...

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• Parameters of the 41 Dra system components
• GRB follow-up team
• Fabry-Perot Interferometer: Gallery Old

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... We present the numerical simulations for an electron-beam-driven and loss-cone-driven electron cyclotron maser (ECM) with different plasma parameters and different magnetic field strengths for a relatively small region and short time-scale in an attempt to interpret the recent discovered intense radio emission from ultracool dwarfs. ... A wide frequency band should therefore be covered by future radio observations. ...

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• Armagh Observatory Preprint No. ???