... These data were originally part of a PhD-thesis at Leiden Observatory by M.H. Wieringa (1991). 1 name Name of source (char8, example : '76W0771*') 2 freq MHz Frequency of source detection in MHz (int, example : 327 or 608 ) 3 ra_1950 radians B1950 Right Ascension (in radians) ( real , example : 2.328327) 4 ra_1950_deg degrees B1950 Right Ascension (in degrees) ( real , example : 133.403290) 5 ra_err seconds Error in RA ( ... 70W : Umi, 327 MHz only, one field. ... Columns 21 Rows 5850...

Еще в разделе: (Показать все результаты (>1844) - www.sao.ru/ )

• Principal Components Analysis
• A 10-GHz Radio Continuum Survey
• A 20 cm VLA survey of Abell clusters of galaxies

... We have been using it to analyze PC images of known gravitational lenses and QSOs which are candidates for lensing (Falco 1993). ... Fig. 1 plots the higher contours of the PC image of 0142 in the upper left, and its power spectrum in the upper right. ... If we fit the envelope of the power spectrum with a binary model, we find that best fit gives a separation of the two components of 1.3 PC pixels or about 58 mas. ... The lower two curves are cuts through the 0142 power spectrum. ...

Еще в разделе: (Показать все результаты (>19291) - www.stsci.edu/ )

• Fine Guidance Sensor Instrument Handbook
• Absorption line spectra of the UV bright z=2.4 QSO HE 1122-1649
• Power Spectral Analysis

On March 29, 2003, an exceptionally bright Gamma-Ray Burst (GRB) was discovered by the HETE-2 satellite (Vanderspek et al. ... 2003, GCN, 2020, 1), GRB 030329 is the nearest cosmological burst detected to date, and its extreme brightness can be attributed to its proximity. ... In the fourth epoch, 51 days after the burst, GRB 030329 appeared resolved at 15 GHz with a component appearing to the north east at 0.28 +/- 0.05 mas from the main component (Fig. a). ... days after the burst. ...

Еще в разделе: (Показать все результаты (>4028) - www.naic.edu/ )

• NGC7674.html

Detected Supernovae . The search have produced till now the detections of 4 SNe. ... This result highlights the power of infrared monitoring in detecting Obscured SNe and indicates that optical surveys are probably missing a significant fraction of SNe, especially in obscured systems such as starburst galaxies. ... In Fig. we show the archival SOFI image of NGC3256 (left) and the first image obtained in 2001 (right) where SN2001db has been detected. ...

Еще в разделе: (Показать все результаты (>8301) - www.arcetri.astro.it/ )

• IBIS: Technical Description
• G35.20-1.74 (Abstract)
• S155 (Abstract)

Comment on J0627-3529 . We have detected the core of an FR-I object and early-type galaxy (Venturi et al. 1995). The core is 0.54 Jy at 2.3 GHz on the Parkes-Tidbinbilla baseline (Morganti et al. 1997) and 0.6 Jy at 5 GHz (VLA data, Ekers et al. (1989) and Morganti, Killeen & Tadhunter (1993)). The VLBA image at 2.3 GHz with the resolution of 15x9 mas shows a "core-jet" structure, with the core brightness of 494 mJy/beam (Venturi et al. ...

Еще в разделе: (Показать все результаты (>428) - www.vsop.isas.ac.jp/ )

Multiґfrequency VLBI observations of the GPS source 1934 ґ 638 A. K. Tzioumis, E. A. King, J. E. Reynolds, D. L. Jauncey R. G. Gough Australia Telescope National Facility, Australia R. A. Preston, D. W. Murphy, S. J. Tingay, D. L. Meier D. L. Jones Jet Propulsion Laboratory, Pasadena, CA, USA J. E. J. Lovell PKS 1934ґ638 is an archetypal GPS source, peaking at 1.4 GHz and exhibits almost no flux density variability. ... RHS: VLBI image of PKS 1934ґ638 at 4.8 GHz. ...

Еще в разделе: (Показать все результаты (>10940) - www.atnf.csiro.au/ )

• http://www.atnf.csiro.au/research/masermeeting/web_papers/309_Goss.pdf
• http://www.atnf.csiro.au/research/WALLABY/Wallaby2010/RJurek-Wallaby2010.pdf
• PPTA Wiki | Projects / Tnoise

... Meta Index / Home Page This section documents warnings and errors generated by this task (if any). ... error . odffix could not find any dataset resembling an ODF component. ... odffix could find a wayt to extract the pointing information from the ODF. corrective action: Use a default pointing. ... odffix has detected a pre-existing attitude history file. corrective action: Because the pre-existing file could have been generated by scisim, a new attitude history file will not be created. ...

Еще в разделе: (Показать все результаты (>33042) - xmm.vilspa.esa.es/ )

• Cross References to In-Flight Calibration Targets

... Posts tagged ?principle component analysis? ... From SINGS (Spitzer Infrared Nearby Galaxies Survey): Isn?t it a beautiful Hubble tuning fork? ... Tags: Classification , clustering , factor analysis , Hubble , multivariate analysis , principle component analysis , SING , Spitzer , tuning fork . ... Comment . ... Entries RSS . Comments RSS . ... General comments . ... vlk on [MADS] Parallel Coordinates . upvc windows on [MADS] Parallel Coordinates . ... Entries (RSS) and Comments (RSS) . ...

Еще в разделе: (Показать все результаты (>3216) - hea-www.harvard.edu/ )

• The AstroStat Slog ICA
• The AstroStat Slog component separation
• The AstroStat Slog 2009 September

... The hot component shows very spectacular activity: irregular outbursts accompanied by fast, massive outflows and jets. ... Diffraction-limited images for both components of CH Cyg binary system were reconstructed using visible speckle interferometry at BTA 6-m telescope (Fig.1). The orbital period 15.6 years and masses: 2.0 Msun and 0.7 Msun for red giant and white dwarf, respectively were derived from angular distance (0.042") and magnitude difference (2 m ) of the components. ... Fig.1. ...

Еще в разделе: (Показать все результаты (>643) - mavr.sao.ru/ )

• Galaxy sector, archive 1994
• Solar system sector, archive 1994
• Galaxy sector, archive 2012

Kholtygin A.F., Burlakova T.E., Fabrika S.N., Valyavin G.G., Yushkin M.V. Microvariability of Line Profiles in the Spectra of OB Stars: delta Ori A . ... We have studied variability of the spectral lines of the OB star delta Ori A -the brightest component of the delta Ori triple system. ... However, some of the variable features go outside the band, presumably due to either imhomogeneities in the stellar wind from .Ori Aa1 or non-radial pulsations of the weaker components of the system, Aa 2 or Ab. ...

Еще в разделе: (Показать все результаты (>227) - www.astro.spbu.ru/ )

• Kholtygin et al., Astron. Astroph. Trans., (2003)
• Kholtygin et al., Magn. Field Conf., August 2003 (2004)

To appear in "Fourth Workshop on Robotic Autonomous Observatories (2015)"RevMexAA(SC) METEOR OBSERVATIONS WITH MINI-MEGATORTORA WIDE-FIELD MONITORING SYSTEM S. Karpov, 1, 3 N. Orekhova2 G. Beskin, 1, 3 A. Biryukov3,4 S. Bondar,2 E. Ivanov,2 E. Katkova,2 A. Perkov, and V. Sasyuk3 RESUMEN 2 Favor de prop orcionar un resumen en espanol. ... The faintest detected meteors has the peak brightness about 10 mag, while the ma jority - from 4 to 8 mag. ... 2010; Karpov et al. 2013; Beskin et al. ...

Еще в разделе: (Показать все результаты (>121) - vo.astronet.ru/ )

• astro-ph

... The remote planet Pluto and its moon Charon orbit the Sun at a mean distance of almost 6,000 million kilometres, or nearly fourty times farther out than the Earth. During a recent investigation by an international group of astronomers [1], the best picture ever of Pluto and Charon [2] was secured with the European Space Agency's Faint Object Camera at the Hubble Space Telescope (HST). ... The new HST image was taken when Charon was near its maximum elongation from Pluto (0.9 arcseconds). ...

Еще в разделе: (Показать все результаты (>15578) - www.eso.org/ )

• Rapid Changes in the Inner Coma of Comet Hyakutake
• The Brightness of the Night Sky
• DFOS Installation: continue

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... This is the first in a series of papers in which we describe and report the analysis of a large survey of Herbig Ae/Be stars in circular spectropolarimetry. Using the ESPaDOnS and Narval high-resolution spectropolarimeters at the Canada-France-Hawaii and Bernard Lyot Telescopes, respectively, we have acquired 132 circularly-polarised spectra of 70 Herbig Ae/Be stars and Herbig candidates. ...

Еще в разделе: (Показать все результаты (>2442) - star.arm.ac.uk/ )

• Explosive Events
• Observations with the Faulkes Telescopes
• Bright Point Studies

In this gallery are many images of Low Surface Brightness Galaxies which have recently been discovered and analyzed. ... The central surface brightness of this galaxy is 24.28 . Malin 2 This galaxy is another huge disk galaxy with a scale length of 15 kpc and a redshift of 15000 km/a. The high surface brightness knot in one of its spiral arms actually has the same color, luminosity and H-alpha equivalent width as the entire Large Magellanic Cloud . ... Truly it is a Low Surface Brightness Galaxy. ...

Еще в разделе: (Показать все результаты (>350) - zebu.uoregon.edu/ )

• Galaxy Gallery Page II

Role in the Universe IAU Symposium 209, 2002 M. Dopita, S. Kwok and R.S. Sutherland, eds. Near-infrared monitoring of the carbon star IRC +10 216 : A high spatial-resolution time sequence of dust -shell evolution G. Weigelt , T. Blocker, K.-H. Hofmann, A. Men'shchikov, J.M. Winters Max{Planck{Institut fur Radioastronomie, 53121 Bonn, Germany Y. Balega Special Astrophysical Observatory, Nizhnij Arkhyz, 35147, Russia The carbon star IRC +10 ... 2000, Tuthill et al. 2000). ...

Еще в разделе: (Показать все результаты (>804) - jet.sao.ru/ )

• NES NES
• Results scientific researchs LRS
• GRB follow-up team

Peremennye Zvezdy ( Variable Stars ) 33 , No. ... I present the discovery of an eclipsing component in light variations of the known High-Amplitude Delta Scuti star GSC 1374-01131 based on the Catalina Surveys publicly available data. ... From a single night of their observations, the variable was classified as a HADS (High-Amplitude Delta Scuti) star, with the light elements: . ... The light curves of GSC 1374-01131 based on Catalina data, folded with periods of pulsations and eclipses. ...

Еще в разделе: (Показать все результаты (>108113) - www.astronet.ru/ )

• XWare > APOD

... Previous: ESO C Library for an Image Processing Software Environment (eclipse) . ... A new CLEAN-type algorithm searches for model components not in the dirty image but in the multi-resolution wavelet transform of the dirty image based on the dirty beam. ... The improvement of this prototype Wavelet CLEAN, which does convolve with the dirty beam, can be attributed to a suppression of noise and aliasing in the dirty image by use of information in the sidelobes of the whole image domain. ...

Еще в разделе: (Показать все результаты (>1994) - www.adass.org/ )

• GIM2D: An IRAF package for the Quantitative Morphology Analysis of Distant
• Simulated AXAF Observations with MARX
• Data Modeling and Analysis

This WWW form allows the user to list selected portions of the NRAO/VLA Sky Survey (NVSS) radio source catalog. ... Until the completion of the survey the source catalog will NOT cover the entire region of the survey and care must be exercised in interpreting the results of a catalog search. ... The second parameter in the "Search radius" box or one of the optional items in a position list can be used to specify a region in which to look for other sources. ... An example of a position list entry is: . ...

Еще в разделе: (Показать все результаты (>1962) - www.mrao.cam.ac.uk/ )

• G327.6+14.6
• Bojan Nikolic -- 90 GHz Continuum Observations of Messier 66
• Inference of Coefficients for Use in Phase Correction

NMW survey overview . Access image archive . ... The New Milky Way survey aims to detect bright (V<13.5) optical transients near the Galactic plane using an automated wide-field (8x6 deg.) system capable of surveying the whole Milky Way area visible from the observing site in one night. ... All images obtained during the transient search survey are available online (please use the image archive access form ). ... Images per field: . ... Images per night: . ... Milky Way imaging time: . ...

Еще в разделе: (Показать все результаты (>3) - scan.sai.msu.ru/ )

... 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 (>281) - www.gao.spb.ru/ )

• http://www.gao.spb.ru/english/as/publ/miller_malkin_ivsgm-2008.pdf
• Conferences
• Articles