The Teide Observatory

Bibcode
1991SoPh..133...65P
DOI
10.1007/BF00149825
Palle, P. L.
Bibliographical reference

(IRIS (International Research on the Interior of the Sun) Workshop, 2nd, Tashkent, Uzbek SSR, Sept. 1989, Proceedings. A91-37551 15-92) Solar Physics (ISSN 0038-0938), vol. 133, May 1991, p. 65-67.

Advertised on:
5
1991
Number of authors
1
IAC number of authors
1
Citations
1
Refereed citations
1
Description
The site of the solar spectrometer of the International Research on the Interior of the Sun (IRIS) network, installed in December 1989 in the Teide Observatory (Izana, Tenerife) is described together with the instrumental facilities of the Teide Observatory. The IRIS instrument is housed at the Solar Oscillation Laboratory of the observatory, which also contains the ESA's Multichannel Photometer, the U.S. National Solar Observatory's Pyroheliometer, and the Birmingham University's 4 Solar Spectrophotometer.
Type
Refereed
Helioseismology
Solar observatories
Solar instruments
Telescopes

It may interest you

  • Refereed
    Characterisation at Cryogenic Temperatures of an Attenuator for an Application of Astrophysical Instrumentation with MKIDs
    The use of non-cryogenic certified commercial electronics for cryogenic applications may be attractive due to their cost and availability, but it also carries risks related to reliability, performance and thermal compatibility. The decision to use commercial components that are not certified for cryogenics instead of components specifically
    Rodríguez Ramos L.F. et al.

    Advertised on:

    12
    2024
  • Refereed
    Crimson Behemoth: A massive clumpy structure hosting a dusty AGN at z=4.91
    The current paradigm for the co-evolution of galaxies and their supermassive black holes postulates that dust-obscured active galactic nuclei (AGNs) represent a transitional phase towards a more luminous and unobscured state. However, our understanding of dusty AGNs and their host galaxies at early cosmic times is inadequate due to observational
    Tanaka, Takumi S. et al.

    Advertised on:

    12
    2024
    Bibcode
    2024PASJ...76.1323T
    Citations
    0
  • Refereed
    The Pristine survey: XXIII. Data Release 1 and an all-sky metallicity catalogue based on Gaia DR3 BP/RP spectro-photometry
    We used the spectro-photometric information of ∼219 million stars from Gaia's Data Release 3 (DR3) to calculate synthetic, narrowband, metallicity-sensitive CaHK magnitudes that mimic the observations of the Pristine survey, a survey of photometric metallicities of Milky Way stars that has been mapping more than 6500 deg 2 of the northern sky with
    Martin, Nicolas F. et al.

    Advertised on:

    12
    2024
    Bibcode
    2024A&A...692A.115M
    Citations
    0