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Cited article:

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Outer structure of the Galactic warp and flare: explaining the Canis Major over-density

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Distances to Anomalous X‐Ray Pulsars Using Red Clump Stars

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The thick disc component of the Galaxy from near infrared colour–magnitude diagrams

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Absolute Proper Motion of the Canis Major Dwarf Galaxy Candidate

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The Wavelength Dependence of Interstellar Extinction from 1.25 to 8.0 μm Using GLIMPSE Data

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Probing the Canis Major stellar over-density as due to the Galactic warp

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Detection of the Canis Major galaxy at (l;b) = (244°; −8°) and in the background of Galactic open clusters

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Stellar density distribution in the NIR on the Galactic plane at longitudes 15–27 deg. Clues for the Galactic bar?

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