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  1. No Access

    Chapter and Conference Paper

    Galactic Bulge from TMGS Star Counts

    The bulge of the Galaxy is analysed by inverting K-band star counts from the Two-Micron Galactic Survey in a number of off-plane regions. Assuming a non-variable luminosity function within the bulge, we derive th...

    M. López-Corredoira, F. Garzón… in The Impact of Near-Infrared Sky Surveys on… (1998)

  2. No Access

    Chapter and Conference Paper

    Galactic Structure and Morphology of the Milky Way from the TMGS

    We discuss the Two Micron Galactic Survey, a project which has been running since 1989 at the IAC map** extended areas of the Galactic plane and bulge with a dedicated IR camera. With the analysis made so fa...

    F. Garzón, P. L. Hammersley, X. Calbet… in New Extragalactic Perspectives in the New … (1996)

  3. No Access

    Chapter and Conference Paper

    Sampling the Bar Population

    The Two Micron Galactic Survey (TMGS, Garzón et al. 1993), has detected a large amount of bright sources on the Galactic plane at l = 27° (Fig. 1 left). This has been attributed to a star formation region at the ...

    X. Calbet, M. Lopez-Corredoira… in New Extragalactic Perspectives in the New … (1996)

  4. No Access

    Chapter and Conference Paper

    Chasing Shadows in the TMGS

    Dust clouds in the Two Micron Galactic Survey (TMGS) show up as areas of lower than expected star counts. However, the increased penetration of the infrared wavelengths means that only major dust clouds produc...

    P. L. Hammersley, T. Mahoney, F. Garzón… in New Extragalactic Perspectives in the New … (1996)

  5. No Access

    Chapter and Conference Paper

    Extinction in the Direction of the End-of-Bar Star Formation Region

    V RI CCD photometry of selected Two Micron Galactic Survey fields towards the end-of-bar star formation region between l = 18°, b = 0° and l = 27°, b = 0° has been carried out at the 1.0–m Jakobu...

    T. J. Mahoney, P. L. Hammersley… in New Extragalactic Perspectives in the New … (1996)

  6. No Access

    Article

    Galactic structure from the Two Micron Galactic Survey

    The Two Micron Galactic Survey (TMGS) is the most sensitive large scale point source near infrared survey of the Galactic Plane yet attempted. The Galactic plane has been drift-scanned in several regions over ...

    F. Garzón, P. L. Hammersley, T. Mahoney, X. Calbet… in Astrophysics and Space Science (1994)

  7. No Access

    Chapter and Conference Paper

    Galactic Structure from the Two Micron Galactic Survey

    The Two Micron Galactic Survey (TMGS) is the most sensitive large scale point source near infrared survey of the Galactic Plane yet attempted. The Galactic plane has been drift-scanned in several regions over ...

    F. Garzón, P. L. Hammersley, T. Mahoney… in Science with Astronomical Near-Infrared Sk… (1994)

  8. No Access

    Chapter and Conference Paper

    Preliminary results of the Two Micron Galactic Survey

    We present the first results of the Two-Micron Galactic Survey (TMGS). The sources are concentrated on the Galactic plane, the width of the distribution increasing between 0° and 30° longitude. Several. obscur...

    X. Calbet, T. Mahoney, P. Hammersley, F. Garzón, M. Selby in Galactic Bulges (1993)

  9. No Access

    Chapter and Conference Paper

    Cross-Correlation of the Two Micron Galactic Survey with IRAS

    The Two Micron Galactic Survey (TMGS) is described by Calbet et al. (this symposium) and Mahoney et al. (1990). It has been cross-correlated with the IRAS point source catalogue (IRPS) using a 15-arcsec search ra...

    T. Mahoney, F. Garzón, X. Calbet, P. Hammersley, M. J. Selby in Galactic Bulges (1993)