A. Adamson

Publication List Details

Period

1965 - 2008

Number

23

Co-Authors

A shallow though extensive H2 2.12 micron imaging survey of Taurus-Auriga-Perseus: I. NGC1333, L1455, L1448 and B1 (2008)

Davis, C. J., Scholz, P., Lucas, P., Smith, M. D., Adamson, A.

We discuss wide-field near-IR imaging of the NGC1333, L1448, L1455 and B1 star forming regions in Perseus. The observations have been extracted from a much larger narrow-band imaging survey of the...

Massive stars exploding in a He-rich circumstellar medium III. SN 2006jc: IR echoes from new and old dust in the progenitor CSM (2008)

Mattila, S., Meikle, W. P. S., Lundqvist, P., Pastorello, A., Kotak, R., Eldridge, J., ...

We present near- and mid-infrared (IR) photometric data of the Type Ibn supernova (SN) 2006jc obtained with the United Kingdom Infrared Telescope (UKIRT), the Gemini North Telescope, and the Spitzer...

The UKIDSS Galactic Plane Survey (2007)

Lucas, P. W., Hoare, M. G., Longmore, A., Schroder, A. C., Davis, C. J., Adamson, A., ...

The UKIDSS Galactic Plane Survey (GPS) is one of the five near infrared Public Legacy Surveys that are being undertaken by the UKIDSS consortium, using the Wide Field Camera on the United Kingdom...

The WFCAM Science Archive (2007)

Hambly, N. C., Collins, R. S., Cross, N. J. G., Mann, R. G., Read, M. A., Sutorius, E. T. W., ...

We describe the WFCAM Science Archive (WSA), which is the primary point of access for users of data from the wide-field infrared camera WFCAM on the United Kingdom Infrared Telescope (UKIRT),...

Computing curves and surfaces from points (2007)

Adamson, A., Encarnação, J.L., Groß, M.

Geometrische Modelle repräsentieren die Form und Struktur von Objekten. Ihre mathematische Beschreibung ist Grundlegend für die Verarbeitung von virtuellen Objekten auf digitalen Computern. Die...

Ray tracing of point models (2007)

Adams, B., Adamson, A.

In this section, the basic ray-surface intersection algorithm based on this surface definition will be discussed. Together, we introduce extensions to handle sharp features such as edges and corners...

Spectropolarimetry of the 3.4 micron absorption feature in NGC 1068 (2006)

Mason, R. E., Wright, G. S., Adamson, A., Pendleton, Y.

In order to test the silicate-core/organic-mantle model of galactic interstellar dust, we have performed spectropolarimetry of the 3.4 micron C-H bond stretch that is characteristic of aliphatic...

Infrared observations of the 2006 outburst of the recurrent nova RS Ophiuchi: the early phase (2006)

Evans, A., Kerr, T., Yang, Bin, Matsuoka, Y., Tsuzuki, Y., Bode, M. F., ...

We present infrared spectroscopy of the recurrent nova RS Ophiuchi, obtained 11.81, 20.75 and 55.71 days following its 2006 eruption. The spectra are dominated by hydrogen recombination lines,...

The UKIRT Infrared Deep Sky Survey (UKIDSS) (2006)

Lawrence, A., Warren, S. J., Almaini, O., Edge, A. C., Hambly, N. C., Jameson, R. F., ...

We describe the goals, design, implementation, and initial progress of the UKIRT Infrared Deep Sky Survey (UKIDSS), a seven year sky survey which began in May 2005, using the UKIRT Wide Field Camera....

Anisotropic point set surfaces (2006)

Adamson, A., Alexa, M.

Point Set Surfaces define smooth surfaces from regular samples based on weighted averaging of the points. Because weighting is done based on a spatial scale parameter, point set surfaces apply...

Point-sampled cell complexes (2006)

Adamson, A., Alexa, M.

A piecewise smooth surface, possibly with boundaries, sharp edges, corners, or other features is defined by a set of samples. The basic idea is to model surface patches, curve segments and points...

Anisotropic point set surfaces (2006)

Adamson, A., Alexa, M.

Point Set Surfaces define smooth surfaces from regular samples based on weighted averaging of the points. Because weighting is done based on a spatial scale parameter, point set surfaces apply...

Adaptive sampling of intersectable models exploiting image and object-space coherence (2005)

Adamson, A., Alexa, M., Nealen, A.

We present a sampling strategy and rendering framework for intersectable models, whose surface is implicitly defined by a black box intersection test that provides the location and normal of the...

Hydrocarbon Dust Absorption in Seyfert Galaxies and ULIRGs (2004)

Mason, R. E., Wright, G., Pendleton, Y., Adamson, A.

We present new spectroscopic observations of the 3.4 micron absorption feature in the Seyfert galaxies, NGC1068 and NGC7674, and the ultraluminous infrared galaxy, IRAS08572+3915. A signature of C-H...

On normals and projection operators for surfaces defined by point sets (2004)

Alexa, M., Adamson, A.

Levin's MLS projection operator allows defining a surface from a set of points and represents a versatile procedure to generate points on this surface. Practical problems of MLS surfaces are a...

Approximating bounded, non-orientable surfaces from points (2004)

Adamson, A., Alexa, M.

We present an approach to surface approximation from points that allows reconstructing surfaces with boundaries, including globally non-orientable surfaces. The surface is defined implicitly using...

Approximating and intersecting surfaces from points (2003)

Adamson, A., Alexa, M.

Point sets become an increasingly popular shape representation. Most shape processing and rendering tasks require the approximation of a continuous surface from the point data. We present a surface...

Ray tracing point set surfaces (2003)

Adamson, A., Alexa, M.

Point set surfaces (PSS) are a smooth manifold surface approximation from a set of sample points. The surface definition is based on a projection operation that constructs local polynomial...

Ray Tracing von Punktmengenflächen (2002)

Adamson, A.

Point set surfaces are a smooth manifold surface approximation from a set of sample points. The surface definition is based on a projection operation that constructs local polynomial approximations....

Spin forbidden bands in Cr III hexamine (1965)

Adamson, A., Dunn, Thomas M.

A large deuterium isotope effect has been found in the spin forbidden bands of the chromium III hexamine complex. The significance of this is discussed.