ELAIS optical ident. at 15um & 1.4GHz (Gonzalez-Solares+, 2005)

Bibcode
2006yCat..73580333G
Gonzalez-Solares, E. A.; Perez-Fournon, I.; Rowan-Robinson, M.; Oliver, S.; Vaccari, M.; Lari, C.; Irwin, M.; McMahon, R. G.; Hodgkin, S.; Ciliegi, P.; Serjeant, S.; Willott, C. J.
Bibliographical reference

VizieR On-line Data Catalog: J/MNRAS/358/333. Originally published in: 2005MNRAS.358..333G

Advertised on:
2
2006
Number of authors
12
IAC number of authors
0
Citations
0
Refereed citations
0
Description
To identify the mid-IR sources with optical objects we use the data from the Wide Field Survey (WFS, McMahon et al., 2001NewAR..45...97M). This survey has been carried out using the Wide Field Camera (WFC) on the 2.5-m Isaac Newton Telescope (INT) on the Observatorio del Roque de Los Muchachos (La Palma). (2 data files).
Type
Non-refereed
Infrared sources
Radio sources

It may interest you

  • Non-refereed
    HARMONI at ELT: HIPOTEC electronics and control system
    HARMONI is the first light visible and near-IR integral field spectrograph for the ELT. It covers a large spectral range from 470nm to 2450nm with resolving powers from 3300 to 18000 and spatial sampling from 60 mas to 4 mas. It can operate in two Adaptive Optics modes - SCAO (including a High Contrast capability) and LTAO - or with NOAO. The
    Menéndez Mendoza, Saúl et al.

    Advertised on:

    7
    2024
    Bibcode
    2024SPIE13096E..4ZM
    Citations
    0
  • Non-refereed
    GTCAO low-frequency tip-tilt offload to M2
    GTCAO is the instrument that implements Adaptive Optics on GTC. For atmospheric turbulence correction, GTCAO uses a deformable mirror. Unlike other AO systems, GTCAO does not include a dedicated mirror for low-frequency tip-tilt (TT) correction. In the absence of dedicated correction, the TT components of atmospheric turbulence are corrected by the
    Marco de la Rosa, J. et al.

    Advertised on:

    8
    2024
    Bibcode
    2024SPIE13097E..7SM
    Citations
    0