... Neutral Hydrogen 21cm line emission is widely used to chart the warm and cool diffuse components of the interstellar medium. ... The ongoing Canadian Galactic Plane Survey (CGPS) meets these criteria to an unprecedented degree, permitting the comparison of HI, CO, and dust features at arcminute scales over hundreds of square of degrees of the Milky Way. We will present the first results of an investigation of neutral Hydrogen self-absorption features in the CGPS dataset. ...

Еще в разделе: (Показать все результаты (>4104) - www.naic.edu/ )

This source is hiding behind our Galaxy at a distance of ~18 Mpc, located at a galactic latitide of 0 degrees. ... As we look towards longer wavelengths, 60 micron, to try and penetrate the Galactic Plane, we still see confusion from galactic sources. ... If the image seems some what confusing that is because the MOST is a continuum radio telescope and when it looks in the direction of our Galaxy it detects radiation from sources within our Galaxy and from sources that may lie behind our Galaxy. ...

Еще в разделе: (Показать все результаты (>17246) - www.atnf.csiro.au/ )

• Results
• The optical emission from gamma-ray quasars
• Multifrequency Observations of the Gamma-Ray Blazar 3C 279 in Low-State during

... 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 (>17153) - www.stsci.edu/ )

• Spitzer Survey of the Large Magellanic Cloud, Surveying the Agents of a
• Power Spectral Analysis
• Fine Guidance Sensor Instrument Handbook

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/ )

... 88, Jan. 1983, p. 1-15. l. A survey of extragalactic radio sources made using driven declination scans is reported covering an area of about 0.07 sr to a limiting flux density of 35 mJy. The fast-scan survey was carried out at a galactic latitude greater than 17 deg with the NRAO 91-m telescope operating at 4.755 GHz, and the 480 sources detected were reobserved at 1.4 GHz with the National Astronomy and Ionosphere Center 305-m telescope at Arecibo. ...

Еще в разделе: (Показать все результаты (>2096) - www.sao.ru/ )

• Radio patrol survey by Gregory and Taylor
• Results and conclusions
• Principal Components Analysis

The SCUBA Local Universe Galaxy Survey Dust along the Hubble sequence Catherine Vlahakis University of Bonn Collaborators: Steve Eales (Cardiff University) Loretta Dunne (University of Nottingham) Overview What is SLUGS? Results from the survey Recent work using SLUGS results ­ the FIR-radio relation Introduction: SLUGS SLUGS ­ a submm survey of galaxies in the local Universe ­ at 850m and 450m Survey of ~200 nearby galaxies: 104 60m-selected ("IRS") (Dunne et al. ...

Еще в разделе: (Показать все результаты (>6977) - www.arcetri.astro.it/ )

• K-band Arcetri Obscured Supernova Search - Detected Supernovae
• K-band Arcetri Obscured Supernova Search - What is the KAOSS Projrect?
• A homogeneous chemical analysis of the inner Galactic disk from the first data

... 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 (>342) - www.gao.spb.ru/ )

• http://www.gao.spb.ru/english/as/publ/miller_malkin_ivsgm-2008.pdf
• http://www.gao.spb.ru/english/personal/malkin/publ/zm135.pdf
• http://www.gao.spb.ru/english/as/j2014/presentations/perepelkin.pdf

EVIDENCE FOR 1809 keV GAMMA-RAY EMISSION FROM 26Al DECAYS IN THE VELA REGION WITH INTEGRAL/ SPI StИphane Schanne(1,*), Patrick Sizun(1), David Maurin(1), Bertrand Cordier(1), Andreas von Kienlin(2), Clarisse Hamadache (1) (2 ... -Institut fЭr extraterrestrische Physik, D-85740 Garching, Germany (*) corresponding author: schanne{at}hep.saclay.cea.fr ABSTRACT The Vela ... SPI background in the 26Al signal region. ... 1995, A&A 298, L25, 1.809 MeV gammarays from the VELA region. ...

Еще в разделе: (Показать все результаты (>815) - hea.iki.rssi.ru/ )

• http://hea.iki.rssi.ru/integral06/papers/B32_Cordier01-26Feb07_18:49:16.pdf
• http://hea.iki.rssi.ru/integral06/papers/D34_Bottacini01-12Mar07_13:28:35.pdf
• http://hea.iki.rssi.ru/conf/hea2007/presentations/26.12.2007/02-cherepashchuk.pdf

... Director of the RAS ISR . RAS Academician . ... Astrophysics module Kvant of the orbital complex Mir launched in 1987 contains the largest on the station complex of the scientific equipment named the orbital observatory Roentgen. Observatory Roentgen consists of 4 X-ray telescopes, jointly exceeding the range of energies from 2 to 800 keV. ... Among the most significant results that were received in the observatory Roentgen are: . ... measurement of the periods of 9 X-ray pulsars; . ...

Еще в разделе: (Показать все результаты (>120) - www.cosmoworld.ru/ )

... Primordial theory review : Dick Bond . Defects and the CMB review : Andy Albrecht . ... Gravitational wave contribution to CMB anisotropies : V.B. Lukash and E.V. Mikheeva . C_l from cosmic strings : Lloyd Knox . Some aspects of CMB anisotropies induced from topological defects : Mairi Sakellariadou . ... CMB anisotropies from scaling sources : Ruth Durrer . ... SZ observations I : Sarah Church . ... Holes in the microwave sky? ... Detecting cosmic strings in the CMB : James Robinson . ...

Еще в разделе: (Показать все результаты (>2356) - www.mrao.cam.ac.uk/ )

• OptInt PmWiki : MROIFastTipTilt / Tech Meet 4
• Astrophysics Group COAST Astronomical Results
• Measurements of anisotropies in the Cosmic Microwave Background Radiation on

... Estimation of the residual Soft Proton flare contamination . ... The script can be run on any EPIC event files (MOS1, MOS2 and/or pn), to estimate the amount of *residual* Soft Proton (SP) flare contamination, i.e. it should only be used *after* attempts have been made to clean the event files for SPs using GTI filtering. ... The higher the in-FOV to out-of-FOV ratio, the more the file is contaminated by SPs: . ... File is not contaminated by SPs. ... File is slightly contaminated by SPs. ...

Еще в разделе: (Показать все результаты (>30387) - xmm.vilspa.esa.es/ )

• XMM-Newton Trainee Project 2004
• Smoothing of mosaics

Find Similar Abstracts . ... The velocity of clusters of galaxies relative to the microwave background - The possibility of its measurement . ... 02/1980 . ... BACKGROUND RADIATION, GALACTIC CLUSTERS, MICROWAVE EMISSION, POLARIZED RADIATION, VELOCITY MEASUREMENT, BACKGROUND NOISE, COSMIC GASES, COSMOLOGY . ... Use: Authors Title Abstract Text Text Query with Keywords Return: Query Results Query Form Database: Astronomy Instrumentation Physics and Geophysics ABSTRACT QUERY USER FEEDBACK HELP ...

Еще в разделе: (Показать все результаты (>653) - xray.sai.msu.ru/ )

• Number of accreting X-ray binaries of selected types
• Results of calculations
• Structure of the Galaxy

... Space Research Institute . Main . ... Main results of the experimental and theoretical research completed in 2010 . ... Moon's topography is shown based on LOLA laser altimeter data, white contour shows a permanently shadowed region and a white rhomb indicates LCROSS spacecraft impact location. ... Ultra deep survey of the sky in hard X-rays, performed by INTEGRAL observatory . INTEGRAL observatory has completed the first and the most sensitive survey of the sky in hard X-ray energy band. ...

Еще в разделе: (Показать все результаты (>1574) - www.cosmos.ru/ )

• SKA-3 Results Page
• Main results of the experimental and theoretical research completed in 2009
• IESP-2M Results Page

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 (>94441) - www.astronet.ru/ )

• Астронет > Англо-Русский Словарь

Properties of the interstellar gas clouds . ... The angular resolution of this Survey was 2.4' x 130', velocity resolution was 6.3 km/s, r.m.s. fluctuations of antenna temperature (T a ) was 0.25 K. All clouds with kinematical distances r a Some selection effects were discovered and our statistic results were corrected for them. Figure 1. ... In the very high mass range the number of neutral gas clouds may be decreased because of gravitational instability or/and molecularization. ...

Еще в разделе: (Показать все результаты (>943) - jet.sao.ru/ )

• Results scientific researchs LRS
• GRB follow-up team
• Results scientific researchs 5

Next: A New IRAF Catalog Access Tool for Astrometry . Up: Iraf Packages . ... Twofitlines is a tool developed within IRAF, optimized to be used with data containing multiple spectra along the spatial axis of the detector. A given spectral feature can be decomposed in one or several Gaussian components. ... A given spectral feature can be modeled using one or more components (currently only Gaussian profiles are available), . ... Close spectral features could be modeled simultaneously. ...

Еще в разделе: (Показать все результаты (>1993) - www.adass.org/ )

• A Spectroscopy Exposure Time Calculator for IRAF
• GIM2D: An IRAF package for the Quantitative Morphology Analysis of Distant
• The ROSAT RESULTS ARCHIVE: Tools and Methods

... Introduction (in Russian) . Chapter 2 (in Russian) . ... Detection of non-Gaussianity in observational CMB data . Methods of phase-analysis for component separation and CMB restoration . New pixelization scheme for the sky CMB maps and the package GLESP to CMB study in this pixelization scheme . New estimates of cosmological parameters using ages of FRII radio galaxies . ... New methods of creation of astrophysical data bases and their implementation in the databases of CATS and SEDs . ...

Еще в разделе: (Показать все результаты (>72) - sed.sao.ru/ )

• Methods and results of radio cosmology. Plan.
• Methods and results of radio cosmology

... 1994: . As a result of comparing the spectra of active solar regions from the observations with high spatial resolution in the microwave range at the RATAN-600 (the S-component) with a flare component observed at meter wavelengths on the VLA (USA) we revealed the presence of a strong and prolonged noise storm exactly where a weak decaying active region (with the presence of powerful active regions in the disk) is located. ... Archive . ...

Еще в разделе: (Показать все результаты (>366) - mavr.sao.ru/ )

• Solar system sector, archive 1997
• Galaxy sector, archive 2012
• Discovery of enrichment of the envelopes of post-AGB stars with heavy metals

... We detect three main diffuse components: the Virgo ICM at ~2.4 keV, the extended halo of M86 at ~1.2 keV, and the cooler central and stripped gas of M86 at ~0.8 keV. The most striking feature is a long tail of emission, which consists of a plume ~ 4' north of M86 and two main extensions emanating from the plume. ... Ram pressure stripping from an aspherical potential can also explain the split "double tails" seen in M86 and in other Virgo cluster galaxies in the field. ...

Еще в разделе: (Показать все результаты (>4528) - hea-www.harvard.edu/ )

• Magnetospheric Emission From Isolated Pulsars
• The AstroStat Slog Blog Archive [ArXiv] component separation methods
• The AstroStat Slog principle component analysis

.

Еще в разделе: (Показать все результаты (>392) - zebu.uoregon.edu/ )

• Thermal History of the Universe
• Risk Management And Perception
• U of O High Energy Physics Seminars