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. ...

Еще в разделе: (Показать все результаты (>4749) - www.naic.edu/ )

• Heiles Symposium Presentations
• Cold Hydrogen Clouds in the Milky Way: An Evolutionary Missing Link?
• Spectral-Line Observing

We present results of new Monte Carlo calculations made with the DIRTY code of radiative transfer of stellar and scattered radiation for a dusty giant late-type galaxy like the Milky Way, which illustrate the effect of the attenuation of stellar light by internal dust on the integrated photometry of the individual bulge and disk components. ... In addition, we find that the structure of the dusty ISM affects more sensitively the observed magnitudes than the observed colors of both bulge and disk. ...

Еще в разделе: (Показать все результаты (>12461) - www.stsci.edu/ )

• Technique
• Fine Guidance Sensor Instrument Handbook
• HST Primer for Cycle 22

Geomagnetic disturbances can be monitored by ground-based magnetic observatories recording the three magnetic field components. The global Kp index is obtained as the mean value of the disturbance levels in the two horizontal field components, observed at 13 selected, subauroral stations . ... Geomagnetic activity is the occurrence of K variations. ... But K still remains a local index, describing disturbances in the vicinity of each observatory. ...

Еще в разделе: (Показать все результаты (>663) - www.iki.rssi.ru/ )

• TCV [Oulu]
• Examples of the raw magnetic field information, obtained with the MIF-M
• Solar wind and IMF [Oulu]

... Bojan Nikolic web pages (r. 329) . ... We present a Bayesian approach to calculating the coefficients that convert the outputs of ALMA 183 GHz water-vapour radiometers into estimates of path fluctuations that can be used to correct the observed interferometric visibilities. ... Inference of Coefficients for Use in Phase Correction . ... Simulating Atmospheric Phase Errors, Phase Correction and the Impact on ALMA Science . ... Copyright 2005 -- 2016, Bojan Nikolic feedback welcome ...

Еще в разделе: (Показать все результаты (>999) - www.mrao.cam.ac.uk/ )

• Inference of Coefficients for Use in Phase Correction
• Data Format Session at 2001 IAU WG Meeting
• 1803+78: A Helical Core Jet

... ATNF Home . About ATNF . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Australia Telescope User Committee . ... Astrophysics graduate student programs . ... Australian Square Kilometre Array Pathfinder . Murchison Radio-astronomy Observatory . ... Parkes radio telescope . Australia Telescope Compact Array . Mopra radio telescope . ... Visiting Parkes radio telescope . Visiting Australia Telescope Compact Array . ... Parkes radio telescope webcam . ...

Еще в разделе: (Показать все результаты (>25802) - www.atnf.csiro.au/ )

• ATNF Daily Astronomy Picture
• Red synchrotron jets in Parkes quasars
• PhD Thesis Abstract

... 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 . ...

Еще в разделе: (Показать все результаты (>1447) - hea-www.harvard.edu/ )

• The AstroStat Slog component separation
• Chandra Images for SNR J0519.5-6902
• The AstroStat Slog maximum entropy

... Initial mass function and binary stars . ... The principal goal of this study is to show that the real shape of the initial mass function for low- and intermediate-mass stars differs from the observed one. In particular, comparison of radii of eclipsing binary components and single stars shows a noticeable difference for B0V-G0V components of eclipsing binaries and single stars of the corresponding spectral type. ...

Еще в разделе: (Показать все результаты (>395) - xray.sai.msu.ru/ )

• Structure of the Galaxy
• Initial Distributions of Binary Parameters
• Number of accreting X-ray binaries of selected types

... Galaxies 99 Cosmic background with model of cloudy interstellar medium Yu. ... Figure 1: Averaged spectrum of the cosmic background I f in frequency range 0.25 200 MHz for the Galactic poles. ... First interpretation of the cosmic noise background spectrum at broad band frequency range 0.25 200 MHz with a model of the cloudy interstellar medium ISM is presented here. ... Synthesized background spectra I f for regions of the Galactic poles at the frequency range 0.25 200 MHz is presented in Fig. ...

Еще в разделе: (Показать все результаты (>275) - www.gao.spb.ru/ )

• http://www.gao.spb.ru/english/as/j2014/presentations/perepelkin.pdf
• Phase light curves of young binary systems

... Contacts . 2012: . ... We refined the fundamental parameters of the components, the orbital periods, and the conditions of photospheric heating of the secondary component by the ultraviolet radiation of the hot component. ... The observations of the star clusters associated with ultra-luminous x-ray sources (ULXs) in four galaxies on the 6-meter and VLT telescopes have shown that all the ULXs are located within 200pc of very young star clusters (younger than 5 million years). ... Archive . ...

Еще в разделе: (Показать все результаты (>226) - mavr.sao.ru/ )

• CH Cyg
• HD965
• Galaxy sector, archive 2008

... Institute of Solid-State Physics, Russian Academy of Sciences, 142432 Chernogolovka, Moscow Region, Russia . In an investigation of the resistivity anisotropy of YBa 2 Cu 3 O 7 - x single crystals with suboptimal oxygen content it is observed that the superconducting transition for the component c of the resistivity tensor is shifted to lower temperatures with respect to the transition for the component a b . ... 1998 American Institute of Physics. PACS: 74.72.Bk, 74.25.Fy, 74.62.Bf ...

Еще в разделе: (Показать все результаты (>1124) - www.issp.ac.ru/ )

• LPCBC: Abstract 2_11
• III International Astronomy Olympiad, Problems to solve

Abstract -- Calculations are performed for the linear polarization of starlight due to extinction by aligned dust grains when the starlight traverses a medium with irregular magnetic fields. This medium is intended to represent the optically thick components of interstellar clouds which are observed to make little, if any, contribution to the polarization of starlight. ...

Еще в разделе: (Показать все результаты (>36) - www.inasan.rssi.ru/ )

• Project: PAHs
• Circular Polarization

... Here some data observed on the 6m telescope with IFP installed in the OLD focal reducer are presented. ... Mkn 3: velocity field . ... NGC 5252: [OIII] image . ... NGC 5252 was observed 23 Feb. 1998 in the [OIII]5007 emission line with CCD TK1024 as detector. ... We observed the ionized gas velocity fields of the spiral galaxies with two purpose. ... Restored velocity field of NGC 157 in the reference frame rotating with the pattern speed overlaid on the Ha image of the galaxy . ... NGC 4100 . ...

Еще в разделе: (Показать все результаты (>644) - jet.sao.ru/ )

• INASAN preprint: A method of the reconstruction of 3D velocity field of gas in
• These galaxies were observed (Project: vortex)
• Parameters of the 41 Dra system components

... Up: Software Systems and Tools . ... This case study examines the use of the latest software techniques for merging independent Java applets and applications. STScI's new Java interface to the archive, StarView II, will make use of the ST-ECF stand-alone FITS image viewer JIPA. We discuss how state-of-the-art software techniques like Remote Method Invocation (RMI), multithreading, and the Reflection API influence the design of a common interface between StarView II and JIPA. ...

Еще в разделе: (Показать все результаты (>1280) - www.adass.org/ )

• A Computer-Based Technique for Automatic Description and Classification of
• Calculating the Position and Velocity Components of HST
• Developing a Wavelet CLEAN Algorithm for Radio-Interferometer Imaging

SPECTRUM ANALYZER OF MAGNETIC PHENOMENA SAMW . Spectrum analyzer allows onboard computation of electromagnetic waves spectra registered (observed) in the ionosphere and magnetosphere in the ELF/VLF frequency band. ... It consists of magnetic antenna, preamplifier, 16 bit sigma delta AD converter, DSP processor and telemetry interface. ... The channels of lower frequencies are averaged and transmitted with lower repetition rate so the telemetry volume is reduced. ... Dynamic range: 90 dB . ...

Еще в разделе: (Показать все результаты (>58) - space.univ.kiev.ua/ )

• SET OF MAGNETIC AND ELECTRIC FIELD DETECTORS EXO-EM

... A concrete application is displayed step by step by the command: TUTORIAL/CLOUD . The data used for this example are CaII absorption features observed in the spectrum of SN 1986g in NGC 5128 (observer: S. d'Odorico, instrument: CASPEC). ... Sampling is 0.05? per pixel and the measured instrumental resolution, 17km/s. The final cloud model consists of 12 absorption doublets. The corresponding image includes both components K and H and has been convolved by a gaussian PSF of 0.22? (17km/s) FWHM. ...

Еще в разделе: (Показать все результаты (>1068) - www.sao.ru/ )

• MIT-GB catalog
• Format of the table for atomic parameters (ABSP.TBL).
• A fast-scan extragalactic source survey at 4.755 GHz

... SB, Porb = 55.9212d. V0745 Cas| ... Component B of the double system observed brighter than in the Hipparcos Input Catalogue. ... The variability may be due to the fainter component. ... Type ELL: is also possible. pi Cas| ... Variability type and spectral type (F2/F3Ib/II) do not agree. ... Variability type and spectral type (F3/F5II) do not agree. ... Variability may be due to component B. VZ Pic| ... Variability may be due to component B. V1377 Ori| ... SB, Porb = 9.073d. V0421 Cep|105091| ...

Еще в разделе: (Показать все результаты (>12) - www.sai.msu.ru/ )

DFS Trouble Shooting . ... According to symptoms usually observed by users, the most probable causes are described, and corresponding solutions proposed. First symptom as it can be observed by a user . Optional) Second symptom as it can be observed by a user First possible cause . Optional) Second possible cause First proposed solution: Describe step by step the procedure to fix the problem. ... Optional) Second proposed solution: Describe step by step the procedure to fix the problem. ...

Еще в разделе: (Показать все результаты (>13173) - www.eso.org/ )

• OYSTER Lab
• ESO - Thesis Topic: Magnetic fields in massive stars
• ESO - Thesis Topic: Properties of kinematically decoupled structures in

. An example of ULF electromagnetic fields detection by the IESP-2M instrument. The figure presented is the dynamic spectrogram. E and B components are measured in satellite coordinates. Observations were made in the auroral region. Electromagnetic turbulence, which was observed mostly in electric components, is typical for this phenomenon. Fig.1 .

Еще в разделе: (Показать все результаты (>1346) - www.cosmos.ru/ )

• Examples of the raw magnetic field information, obtained with the MIF-M
• Space Research Institute (IKI) Seminar
• Multipoint correlations of the solar wind parameters observed by several

Marc White . ... Turbulent entrainment processes may play an important role in the outflows from young stellar objects at all stages of their evolution. In particular, lateral entrainment of ambient material by high-velocity, well-collimated protostellar jets may be the cause of the multiple emission-line velocity components observed in the microjet-scale outflows driven by classical T Tauri stars. ... University of Amsterdam; STARPLAN, Copenhagen, Jul 2013 . ... E marc.white@anu.edu.au . ...

Еще в разделе: (Показать все результаты (>475) - www.mso.anu.edu.au/ )

• Richard Woolley and Jim Banham inspecting optical and mechanical components,
• Software Maintenance Manual
• GSAOI Component Supplier Links Page

... astro-ph . ... Whitespace-separated words are treated as AND ed. Show 10 50 100 articles per page in Full Compact mode . ... Quasar Variability in the Framework of Poissonian Models . ... It is shown that in this very general framework the well established anti-correlation between variability amplitude and wavelength can only be understood as an effect of an underlying spectral component which remains stable on long time-scales, and is redder than the variable component. ...

Еще в разделе: (Показать все результаты (>62) - vo.astronet.ru/ )