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In about half of Seyfert galaxies, the X-ray emission is absorbed by an optically thin, ionized medium, the so-called "Warm Absorber", whose origin and location is still a matter of debate. The aims o...
F00183-7111 is one of the most extreme Ultra-Luminous Infrared Galaxies known. Here we present a VLBI image which shows that F00183-7111 is powered by a combination of a radio-loud Active Galactic Nuc...
We report far-infrared (FIR) imaging of the Seyfert 2 galaxy NGC 3081 in the range 70-500 micron, obtained with an unprecedented angular resolution, using the Herschel Space Observatory instruments PA...
VII Zw 403: HI Structure in a Blue Compact Dwarf Galaxy     Structure  Compact Dwarf Galaxy       font style='font-size:12px;'> 2011/9/30
We present optical (UBVJ), ultraviolet (FUV, NUV), and high resolution atomic hydrogen (HI) observations of the nearby blue compact dwarf (BCD), VII Zw 403. We find that VII Zw 403 has a relatively hi...
We report Fermi/LAT observations and broad-band spectral modeling of the radio-loud active galaxy 4C +55.17 (z=0.896), formally classified as a flat-spectrum radio quasar. Using 19 months of all-sky s...
We have assembled the largest sample of ultra hard X-ray selected (14-195 keV) AGN with host galaxy optical data to date, with 185 nearby (z<0.05), moderate luminosity AGN from the Swift BAT sample. T...
This paper continues our development of non-parametric tests for analysing the completeness in apparent magnitude of magnitude-redshift surveys. The purpose of this third and final paper in our comple...
We present new GMRT observations of HDF 130, an inverse-Compton (IC) ghost of a giant radio source that is no longer being powered by jets. We compare the properties of HDF 130 with the new and import...
Optical and near IR galaxy number counts in the GOYA survey. The ages of ellipticals。
Mid-infrared sub-arcsecond spectroscopy of active galaxy nuclei     Mid-infrared  spectroscopy  active galaxy n       font style='font-size:12px;'> 2009/6/30
Mid-infrared sub-arcsecond spectroscopy of active galaxy nuclei。
Hot gas and the gaseous structure of the galaxy     HYDRODYNAMICS  SUPERNOVAREMNANTS  X-RAYS  GALAXIES       font style='font-size:12px;'> 2009/6/4
A parochial review is presented concerning the status of our understandingof hot gas regions in the Galaxy and their implications for the overall distributionsof the Galaxy gaseous components. We hav...
Hot gas in the galaxy:what do we know for sure?      GENERAL GALAXY  BUBBLES ISM  GENERAL X-RAYS       font style='font-size:12px;'> 2009/6/4
Major advances have been made in the past decade in our knowledge of the hotinterstellar gas of our Milky Way galaxy. The Di.use X-ray Spectrometer obtainedspectra in the 0.15?.28 keV range from the G...
In this work, based on the analytical model with delayed production approximation developed by Pagel & Tautvaiˇsien˙e (1995) for the Galaxy, the analytic solutions of the distribution of neutron expos...

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