Stellar integrated fluxes for 216 stars in the wavelength range 380 nm-900 NM

Bibcode
1988A&A...203..341P
Selby, M. J.; Arribas, S.; Mountain, C. M.; Leggett, S. K.; Haddock, D. J.; Booth, A. J.; Blackwell, D. E.; Petford, A. D.
Bibliographical reference

Astronomy and Astrophysics (ISSN 0004-6361), vol. 203, no. 2, Sept. 1988, p. 341-347.

Advertised on:
9
1988
Number of authors
8
IAC number of authors
1
Citations
11
Refereed citations
10
Description
The paper reports measurements of the integrated fluxes over the wavelength range 380 nm - 900 nm for 216 stars using a Reticon spectrometer in conjunction with the 1 m Kapteyn telescope of the Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias. Methods are proposed for deriving visible integrated fluxes from 13-colour photometry, UBVRI and BV photometry. Such fluxes are useful for deriving stellar effective temperatures and angular diameters.
Type
Refereed
Binary stars
Interstellar extinction

It may interest you

  • Refereed
    A Perspective on the Milky Way Bulge Bar as Seen from the Neutron-capture Elements Cerium and Neodymium with APOGEE

    This study probes the chemical abundances of the neutron-capture elements cerium and neodymium in the inner Milky Way from an analysis of a sample of ∼2000 stars in the Galactic bulge bar spatially contained within ∣X Gal∣ < 5 kpc, ∣Y Gal∣ < 3.5 kpc, and ∣Z Gal∣ < 1 kpc, and spanning metallicities between ‑2.0 ≲ [Fe/H] ≲ +0.5. We classify the

    Sales-Silva, J. V. et al.

    Advertised on:

    4
    2024
    Bibcode
    2024ApJ...965..119S
  • Refereed
    The variability patterns of the TeV blazar PG 1553 + 113 from a decade of MAGIC and multiband observations

    PG 1553 + 113 is one of the few blazars with a convincing quasi-periodic emission in the gamma-ray band. The source is also a very high energy (VHE; >100 GeV) gamma-ray emitter. To better understand its properties and identify the underlying physical processes driving its variability, the MAGIC Collaboration initiated a multiyear, multiwavelength

    MAGIC Collaboration et al.

    Advertised on:

    4
    2024
    Bibcode
    2024MNRAS.529.3894M
    Citations
    0
  • Refereed
    A Very-High-Energy Gamma-Ray View of the Transient Sky

    The development of the latest generation of Imaging Atmospheric Cherenkov Telescopes (IACTs) over recent decades has led to the discovery of new extreme astrophysical phenomena in the very-high-energy (VHE, E > 100 GeV) gamma-ray regime. Time-domain and multi-messenger astronomy are inevitably connected to the physics of transient VHE emitters

    Carosi, Alessandro et al.

    Advertised on:

    3
    2024
    Bibcode
    2024Univ...10..163C
    Citations
    0