18 datasets found

Keywords: Markarian galaxies

Filter Results
  • Catalogue of Markarian Galaxies

    Markarian galaxies have a moderate to strong ultraviolet continuum as detected by an objective-prism survey at Byurakan Observatory from 1965 to 1978. The survey was done with a...
  • Survey of 108 E-S0 galaxies

    A survey has been performed of the morphological and photometric properties of 108 E-S0 galaxies out of a complete sample of 112: this sample is built from the Revised...
  • First Byurakan Survey (FBS)

    A Catalogue of galaxies with UV-continuum (Markarian galaxies) detected during the First Byurakan Survey (FBS) is presented. The purpose of the Survey was to search for peculiar...
  • Michigan Emission-Line Objects

    The objects of this catalogue were detected by using the 61-cm aperture Curtis Schmidt telescope in combination with a thin objective prism (1.8{deg}) at the Cerro Tololo...
  • PDS versus Markarian starburst galaxies

    The characteristics of the starburst galaxies from the Pico dos Dias Survey (PDS, Coziol et al., 1998ApJS..119..239C) are compared with those of the nearby ultraviolet (UV)...
  • Optical properties of Markarian galaxies

    A database for the entire Markarian catalog is presented that combines extensive new measurements of their optical parameters with a literature and database search. The...
  • Faint Markarian galaxies of SBS. III.

    We continue our program of spectroscopic observations of objects from the Second Byurakan Survey (SBS). This survey contains more than 3600 objects with m_pg_<19.5mag, half...
  • Markarian galaxies and Zwicky clusters relations

    In the same area covered by Markarian survey and CGCG, there are 1344 Markarian galaxies, of which 597 are positioned inside the contours of Zwicky clusters. Data on these...
  • Sample of starburst nucleus galaxies

    This paper presents optical long-slit spectroscopic observations of 105 barred Markarian IRAS galaxies. These observations are used to determine the spectral type (starburst or...
  • Classification of Markarian galaxies

    Markarian (Mrk) galaxies, revealed due to their ultraviolet excess are very famous; they play a significant role in many astrophysical problems and come in a variety of types:...
  • HST/COS and FUSE UV spectra of Mrk 509

    To elucidate the location, physical conditions, mass outflow rate, and kinetic luminosity of the outflow from the active nucleus of the Seyfert 1 galaxy Mrk 509 we used...
  • Mrk 421 multi-wavelength variability, 2007-2009

    We perform an extensive multi-band variability and correlation study of the TeV blazar Mrk 421 on year time scales, which can bring additional insight on the processes...
  • Mrk421 in March 2010

    A flare from the TeV blazar Mrk 421, occurring in March 2010, was observed for 13 consecutive days from radio to very high energy (VHE; E>100GeV) gamma-rays with MAGIC,...
  • The 2009 multiwavelength campaign on Mrk421

    We perform an extensive characterization of the broadband emission of Mrk 421, as well as its temporal evolution, during the non-flaring (low) state. The high brightness and...
  • Mrk 335 photometry in 1995-2004

    We present results of UBVRI photometry of Mrk 335 in 1995-2004. This object has a large amplitude of variability, reaching about 1.1, 0.9, 0.7mag in the U,B,V and 0.3mag in the...
  • Starbursts in barred spiral galaxies. VI.

    This paper reports a study of the effect of a bar on the neutral hydrogen (HI) content of starburst and Seyfert galaxies. We also make comparisons with a sample of "normal"...
  • Survey of Markarian galaxies

    Results are presented from a multifrequency radio continuum survey of Markarian galaxies (MRKs) and are supplemented by IRAS infrared data from the Faint Source Survey. Radio...
  • F-GAMMA 2.64-43GHz radio data over 2007-2015

    The advent of the Fermi gamma-ray space telescope with its superb sensitivity, energy range, and unprecedented capability to monitor the entire 4{pi} sky within less than 2-3 h,...
You can also access this registry using the API (see API Docs).