Very low mass stars in Praesepe (Boudreault+, 2010)

Bibcode
2010yCat..35109027B
Boudreault, S.; Bailer-Jones, C. A. L.; Goldman, B.; Henning, T.; Caballero, J. A.
Referencia bibliográfica

VizieR On-line Data Catalog: J/A+A/510/A27. Originally published in: 2010A&A...510A..27B

Fecha de publicación:
7
2010
Número de autores
5
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
The near-infrared (NIR) observations were made on the 3.5m telescope at Calar Alto, Spain (with observation runs of several nights from February 2005 to January 2007). The optical observations were carried out with the Wide Field Imager (WFI) on the MPG/ESO 2.2m telescope at La Silla, Chile during 17-22 March 2007. (2 data files).
Tipo
Sin árbitro
Fotometría

Te puede interesar

  • Sin árbitro
    ANDES, the high resolution spectrograph for the ELT: science goals, project overview, and future developments
    The first generation of ELT instruments includes an optical-infrared high resolution spectrograph, indicated as ELT-HIRES and recently christened ANDES (ArmazoNes high Dispersion Echelle Spectrograph). ANDES consists of three fibre-fed spectrographs ([U]BV, RIZ, YJH) providing a spectral resolution of ∼100,000 with a minimum simultaneous wavelength
    Marconi, A. et al.

    Fecha de publicación:

    7
    2024
    Bibcode
    2024SPIE13096E..13M
    Número de citas
    1
  • Sin árbitro
    An overview of the preliminary optical design of the European Solar Telescope (EST)
    The European Solar Telescope (EST) is a 4-m class-solar telescope that will become part of the next generation of groundbased facilities. Located at the "Observatorio del Roque de los Muchachos" in La Palma (Spain), it will be aimed to study the magnetic connectivity of the solar atmosphere with high spatial and temporal resolution. The EST optical
    Belío-Asin, Marta et al.

    Fecha de publicación:

    8
    2024
    Bibcode
    2024SPIE13094E..2GB
    Número de citas
    0
  • Sin árbitro
    Shape and Mutual Orbit Modeling of Binary Near-Earth Asteroid 2020 BX<SUB>12</SUB>
    Approximately 15% of the near-Earth asteroid (NEA) population are estimated to be binary systems. 54 binaries have Arecibo radar observations; 2020 BX 12 is one of them. Discovered on January 27, 2020, by the Asteroid Terrestrial-impact Last Alert System (ATLAS) survey at Mauna Loa Observatory, 2020 BX 12 has an absolute magnitude of 20.6 and an
    Zambrano-Marin, Luisa Fernanda et al.

    Fecha de publicación:

    10
    2024
    Bibcode
    2024DPS....5631203Z
    Número de citas
    0