Optical surface photometry of radio galaxies. II. Observations and data analysis

Bibcode
2000A&AS..143..369G
DOI
10.1051/aas:2000338
Govoni, F.; Falomo, R.; Fasano, G.; Scarpa, R.
Bibliographical reference

Astronomy and Astrophysics Supplement, v.143, p.369-390

Advertised on:
5
2000
Number of authors
4
IAC number of authors
0
Citations
17
Refereed citations
14
Description
Optical imaging observations for 50 radio galaxies are presented. For each object isophotal contours, photometric profiles, structural parameters (position angle, ellipticity, Fourier coefficients), and total magnitudes are given. These observations, obtained in the Cousins R band, complement the data presented in a previous paper and are part of a larger project aimed at studying the optical properties of low redshift (z<= 0.12) radio galaxies (Govoni et al. 1999). Comments for each individual source are reported.
Type
Refereed
Galaxies
Photometry

It may interest you

  • Refereed
    An ultra-short-period super-Earth with an extremely high density and an outer companion
    We present the discovery and characterization of a new multi-planetary system around the Sun-like star K2-360 (EPIC 201595106). K2-360 was first identified in K2 photometry as the host of an ultra-short-period (USP) planet candidate with a period of 0.88 d. We obtained follow-up transit photometry, confirming the star as the host of the signal
    Livingston, John H. et al.

    Advertised on:

    11
    2024
    Bibcode
    2024NatSR..1427219L
    Citations
    0
  • Refereed
    High-resolution observations of recurrent jets from an arch filament system
    Context. Solar jets are collimated plasma ejections along magnetic field lines observed in hot (extreme-ultraviolet (EUV) jets) and cool (chromospheric surges) temperature diagnostics. Their trigger mechanisms and the relationship between hot and cool jets are still not completely understood. Aims. We aim to investigate the generation of a sequence
    Joshi, Reetika et al.

    Advertised on:

    11
    2024
    Bibcode
    2024A&A...691A.198J
    Citations
    0
  • Refereed
    KISS: Instrument Description and Performance
    Kinetic inductance detectors (KIDs) have been proven as reliable systems for astrophysical observations, especially in the millimeter range. Their compact size enables them to optimally fill the focal plane, thus boosting sensitivity. The KIDs Interferometric Spectral Surveyor (KISS) instrument is a millimeter camera that consists of two KID arrays
    Macías-Pérez, J. F. et al.

    Advertised on:

    11
    2024
    Bibcode
    2024PASP..136k4505M
    Citations
    0