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
    Massive characterisation of subgiants and red giants with TESS (Kepler and Gaia)
    TESS serves as a formidable tool for investigating stellar variability. Nonetheless, the adaptation of methodologies employed in other space missions, such as Kepler, to deduce long stellar rotation periods or solar-like stellar pulsations has been a challenge. The advent of multiple sectors of data for most stars every two years with the extended
    García, Rafael A. et al.

    Advertised on:

    9
    2024
    Bibcode
    2024tkas.confE.123G
    Citations
    0
  • Non-refereed
    Calibrating the color-redshift relation for an optimum exploitation of Euclid data
    Euclid's three dimensional reconstruction of the matter distribution in the Universe heavily relies on a proper calibration of the color-redshift relation. Getting such calibration was the motivation of the project Complete Calibration of the Color-Redshift Relation (C3R2) survey (Masters et al. 2017), with the goal of mapping the empirical
    Gutierrez, Carlos

    Advertised on:

    8
    2024
    Bibcode
    2024IAUGA..32P2796G
    Citations
    0
  • Non-refereed
    Gas Flows in the Central Region of NGC 4593 with Muse
    Understanding how gas flows into galactic centers, fuels the AGN and in turn is expelled back through feedback processes is of great importance to appreciate the role AGN play in the growth and evolution of galaxies. We use MUSE-AO optical spectra of the inner 7''. 5 × 7''. 5 of the nearby Seyfert 1 galaxy NGC 4593 to understand how gas flows in
    Mulumba, Dorcus et al.

    Advertised on:

    8
    2024
    Bibcode
    2024IAUGA..32P.367M
    Citations
    0