Faint NIR Polarimetric Standards

Bibcode
2008eic..work..511B
DOI
10.1007/978-3-540-76963-7_69
Barrena, R.; Acosta-Pulido, J. A.; Manchado, A.
Referencia bibliográfica

The 2007 ESO Instrument Calibration Workshop, ESO Astrophysics Symposia European Southern Observatory. ISBN 978-3-540-76962-0. Springer-Verlag Berlin Heidelberg, 2008, p. 511

Fecha de publicación:
0
2008
Número de autores
3
Número de autores del IAC
3
Número de citas
1
Número de citas referidas
1
Descripción
We report on the preparation of a catalog of faint polarizedstandards for near infrared bands. The catalog will onlycontain faint targets (below J ≃ 14) which should be areference list for observations in 10 m class telescopes. Weexpect to have a list with more than 50 targets contained inseveral fields distributed in a wide right ascension range.The data are being collected using the polarization mode of LIRISinstrument (mounted at the Cassegrain focus of the WHTtelescope). Here we show some examples of the use of LIRISpolarimetry and a first sample of the catalog.
Tipo
Sin árbitro

Te puede interesar

  • Sin árbitro
    Study of basaltic asteroids through their phase curves
    Introduction Classified as type-V, the basaltic asteroids of the Main Belt (MB), for the most part, are connected to Vesta's dynamic family. However, since the discovery of the V-type asteroid (1459) Magnya in the outer MB, several new asteroids have been found in different regions, including V-types from inner regions not belonging to the Vesta
    Arcoverde, Plicida et al.

    Fecha de publicación:

    9
    2024
    Bibcode
    2024EPSC...17..999A
    Número de citas
    0
  • Sin árbitro
    ANDES, the high-resolution spectrograph for the ELT: design of the adaptive optics system
    ANDES,the high resolution spectrograph for the ELT, will work both in seeing limited mode and with Adaptive Optics (AO) correction. ANDES-SCAO is a single conjugated AO system working with natural guide stars, feeding the IFU coupled to the YJH spectrograph. The main science goal of the ANDES AO mode is the characterization of the exo-planet
    Pinna, Enrico et al.

    Fecha de publicación:

    8
    2024
    Bibcode
    2024SPIE13097E..4WP
    Número de citas
    0