نتایج جستجو برای: radio

تعداد نتایج: 100901  

2009
Isabella Prandoni Raffaella Morganti Arturo Mignano

We are currently exploiting the deep radio/optical/IR information available for the extra-galactic component of the Spitzer First Look Survey (FLS) to investigate the physical properties of faint radio-selected AGNs, with the aim of studying the AGN component of sub–mJy radio fields. One of the key unresolved issues is whether, as a function of cosmic epoch, low-power AGNs are more related to e...

2003
P. N. Best J. N. Arts H. J. A. Röttgering

A new sample of radio sources, with the designated name CENSORS (A Combined EISNVSS Survey Of Radio Sources), has been defined by combining the NRAO VLA Sky Survey (NVSS) at 1.4 GHz with the ESO Imaging Survey (EIS) Patch D, a 3 by 2 degree region of sky centred at 09 51 36.0, −21 00 00 (J2000). New radio observations of 199 NVSS radio sources with NVSS flux densities S1.4 GHz > 7.8 mJy are pre...

2008
E. J. Murphy J. D. P. Kenney G. Helou A. Chung J. H. Howell

We present a study on the effects of the intracluster medium (ICM) on the interstellar medium (ISM) of 10 Virgo cluster galaxies using Spitzer far-infrared (FIR) and VLA radio continuum imaging. Relying on the FIR-radio correlation within normal galaxies, we use our infrared data to create model radio maps which we compare to the observed radio images. For 6 of our sample galaxies we find regio...

I. O Badiru K. M Sunday O. T Yekinni,

There is disparity in access to Information and Communication Technologies between male and female especially in developing countries. This study did a gender analysis of access and use of ICTs in Ekiti state, Nigeria. Multistage sampling procedure was used to select 178 respondents. Data collected were analysed using descriptive statistics and t-test at α0.05. Radio (198.7), mobile phones (186...

Guangbin Luo Zhenghong Lee

Positron emission tomography (PET) imaging using 2-deoxy-2-[F-18]fluoro-D-glucose (FDG) has proven valuable in the diagnosis, staging and restaging for many cancers. However, its application for liver cancer has remained limited owing in part to the relatively high background uptake of the tracer in the liver plus the significant variability of the tumor specific uptake in liver cancer among pa...

1997
L. FERETTI

The Coma cluster is peculiar in the radio domain owing to the presence of cluster-wide diffuse sources: the radio halo Coma C, the relic source 1253+275, and the bridge between them. Diffuse radio sources in clusters are a rare and poorly understood phenomenon. We summarize here the properties of the diffuse radio sources in Coma and their relation to other cluster properties. 1 Radio emission ...

2007
William Sherwood Alok R. Patnaik

We have performed quasi-simultaneous radio ux density measurements at 2.7 and 10 GHz for all PG quasars with radio ux densities between 4-200 mJy. We nd that a large fraction of these sources are variable, at-spectrum quasars. This brings the total fraction of at-spectrum quasars with a ratio between radio and optical ux of R > 10 | a value previously used to deene a radio-loud quasar | to 40% ...

2001
K. Igarashi N. A. Armand A. G. Pavelyev Ch. Reigber J. Wickert K. Hocke G. Beyerle

The radio holography methodology may be applied in the scientific programs for future small satellite that will use radio signals emitted by radio navigation, radio communication satellites for precise measuring effects of radio waves propagation at low elevation angles and for global monitoring of radio communication channels passed through the atmosphere and ionosphere. Another task consists ...

1994
Heino Falcke Matthew A. Malkan Peter L. Biermann

We investigate the correlation between the accretion disk (UV) luminosity and the radio core emission of a quasar sample, containing all PG quasars, also deriving empirical conversion factors from emission line luminosities to disk luminosities. This method allows us to investigate the radio properties of AGN on the absolute scale set by the accretion power. In a radio vs. Ldisk plot we find th...

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