229 datasets found

Keywords: seyfert galaxies

Filter Results
  • Narrow-band imaging of 5 Seyfert-1 galaxies

    Spatially resolved emission-line spectroscopy is a powerful tool to determine the physical conditions in the narrow-line region (NLR) of active galactic nuclei (AGNs). We...
  • Narrow-band imaging of 6 Seyfert-2 galaxies

    While [OIII] narrow-band imaging is commonly used to measure the size of the narrow-line regions (NLRs) in active galactic nuclei (AGNs), it can be contaminated by emission from...
  • Radio Sources in Low-Luminosity AGNs. IV

    We present the completed results of a high resolution radio imaging survey of all (~200) low-luminosity active galactic nuclei (LLAGNs) and AGNs in the Palomar Spectroscopic...
  • VLBI and VLA obs. of Seyfert galaxies

    We have obtained mas-scale resolution very long baseline interferometry (VLBI) images of a sample of Seyfert 1 and Seyfert 2 galaxies at 5GHz (wavelength, {lambda}=6cm). The...
  • AGNs from RXTE 3-20keV All-Sky Survey

    We compiled a sample of 95 AGNs serendipitously detected in the 3-20keV band at Galactic latitude |b|>10deg during the RXTE slew survey (XSS, Revnivtsev et al., Cat. ), and...
  • Mid-infrared and hard X-ray emission in AGN

    We use mid-infrared spectral decomposition to separate the 6{mu}m mid-infrared AGN continuum from the host emission in the ISO low resolution spectra of 71 active galaxies and...
  • Radio Emission from VLA FIRST Survey AGN

    Using the most recent (April 2003) version of the VLA FIRST survey radio catalog (Cat. ), we have searched for radio emission from >2800 AGN taken from the most recent (2001)...
  • Core dominance in extragalactic radio sources

    In this paper, based on a paper by Liu and Zhang (2002, Cat. ), we have chosen a sample of 542 extragalactic sources (27 BL Lac objects, 300 galaxies (radio galaxies and Seyfert...
  • QSOs in the M3 field

    We present results from a variability and proper motion (VPM) search for QSOs in the field around M3. The VPM search is demonstrated to be powerful technique for efficiently...
  • The Hamburg/SAO Survey for ELGs. V.

    We present the fifth list with results of the Hamburg/SAO Survey for Emission-Line Galaxies (HSS therein, SAO - Special Astrophysical Observatory, Russia). The list is a result...
  • NGC 5548 UBVRI phot. and Halpha, Hbeta fluxes

    Results of a ground-based optical monitoring campaign on NGC 5548 in June 1998 are presented. The broad-band fluxes (U, B, V), and the spectrophotometric optical continuum flux...
  • Monitoring Mkn 279 in BVRI and H{beta} fluxes

    Mid-infrared images of the Seyfert 1 galaxy Mrk 279 obtained with the ISO satellite are presented together with the results of a one-year monitoring campaign of the...
  • Soft X-ray properties of Seyfert galaxies

    We present a catalogue of ROSAT detected sources in the sample of spectroscopically selected Seyfert 1 and Seyfert 2 galaxies of Rafanelli et al. (1995AJ....109.1546R). The...
  • The Hamburg/SAO Survey for ELGs. IV

    We present the fourth list with results of the Hamburg/SAO Survey for Emission-Line Galaxies (HSS hereafter, SAO -- Special Astrophysical Observatory, Russia). The main goal of...
  • Hamburg/ESO survey for bright QSOs. III.

    Appendix to the above paper, containing the two large tables A.1 and B.1 described in the paper. Table A.1 gives the basic properties of the 207 survey fields used to construct...
  • Seyferts in galaxy pairs and groups

    The occurrence of Seyfert galaxies in 6 samples representative of different cosmological environments (i.e. isolated pairs, compact and loose groups) is analysed. To avoid...
  • NGC 4151 line-continuum diagram sequences

    We present the first results of an 8-year spectroscopic monitoring of the Seyfert 1.5 galaxy NGC 4151 carried out with a CCD spectrograph at the 2.6-m Shajn Telescope of the...
  • NGC 5548 continuum light curve

    The variations of the [OIII]{lambda}5007 line profile in NGC 5548 are examine d from CCD spectra obtained at the Ohio State University and Crimean Astrophysic al Observatory in...
  • NGC 5548 Profile variability

    Optical emission line intensities of the variable Seyfert 1 galaxy NGC 5548 are presented.
  • Identification of X-ray sources around Seyferts

    Excess numbers of X-ray sources around bright Seyfert galaxies have been demonstrated with significances of association up to 7.4-sigma (Radecke, 1997A&A...319...18R). The...
You can also access this registry using the API (see API Docs).