A. More

Publication List Details

Period

2005 - 2009

Number

14

Co-Authors

The mass distribution of a moderate redshift galaxy group and brightest group galaxy from gravitational lensing and kinematics (2009)

McKean, J. P., Auger, M. W., Koopmans, L. V. E., Vegetti, S., Czoske, O., Fassnacht, C. D., ...

The gravitational lens system CLASS B2108+213 has two radio-loud lensed images separated by 4.56 arcsec. The relatively large image separation implies that the lensing is caused by a group of...

A new window of exploration in the mass spectrum: strong lensing by galaxy groups in the SL2S (2009)

Limousin, M., Cabanac, R., Gavazzi, R., Motta, V., Richard, J., ...

The existence of strong lensing systems with Einstein radii covering the full mass spectrum, from ~1-2" (produced by galaxy scale dark matter haloes) to > 10" (produced by galaxy cluster scale...

The role of luminous substructure in the gravitational lens system MG 2016+112 (2009)

More, A., McKean, John P., More, Surhud, Porcas, Richard W., Koopmans, Leon V. E., Garrett, M. A.

MG 2016+112 is a quadruply imaged lens system with two complete images A and B and a pair of merging partial images in region C as seen in the radio. The merging images are found to violate the...

The role of luminous substructure in the gravitational lens system MG 2016+112 (2009)

More, A., McKean, John P., More, Surhud, Porcas, Richard W., Koopmans, Leon V. E., Garrett, M. A.

MG 2016+112 is a quadruply imaged lens system with two complete images A and B and a pair of merging partial images in region C as seen in the radio. The merging images are found to violate the...

A New Window of Exploration in the Mass Spectrum: Strong Lensing by Galaxy Groups in the SL2S (2008)

Limousin, M., Cabanac, R., Gavazzi, R., Motta, V., Richard, J., ...

The existence of strong lensing systems with Einstein radii (Re) covering the full mass spectrum, from ~1-2" (produced by galaxy scale dark matter haloes) to >10" (produced by galaxy cluster scale...

The role of luminous substructure in the gravitational lens system MG 2016+112 (2008)

More, A., McKean, J. P., More, S., Porcas, R. W., Koopmans, L. V. E., Garrett, M. A.

MG 2016+112 is a quadruply imaged lens system with two complete images A and B and a pair of merging partial images in region C as seen in the radio. The merging images are found to violate the...

Edinburgh Virtual Environment Centre (2008)

Ann Marie Shillito, Silvia Scali, Dr. Mark Wright, Haptics For, A More, Experiential Quality In, ...

jewellery and metal, CAD and rapid prototyping. Project manager and principal investigator (ECA) for ‘Tacitus ’ project. Silvia Scali: Research Assistant at Edinburgh College of Art, MA...

"Interval Rational = Algebraic " Revisited: (2008)

A More, Computer Realistic Result, Anatoly V. Lakeyev, Vladik Kreinovich

1 Reminder: Main Result From [1] In [1], the following question is analyzed: what will happen if we add the "inter-val computations " operation to the list of basic arithmetic...

Probing a massive radio galaxy with gravitational lensing (2007)

More, A., McKean, J. P., Muxlow, T. W. B., Porcas, R. W., Fassnacht, C. D., Koopmans, L. V. E.

The gravitational lens system CLASS B2108+213 has two lensed images separated by 4.56 arcsec. Such a wide image separation suggests that the lens is either a massive galaxy, or is composed of a group...

Course Objectives (2007)

Students Will, B. Groups, A. More, Vector Spaces, E. Norm, Schwartz Inequalities, ...

34.98> n (9.0 hours) A. Linear Transformations B. Equivalence of Norms C. General Rules and Definitions for Differentiation D. Revisit Minimum Functional Theorem with Calculus E. Gradients,...

Multi-Frequency VLBI Observations of the Gravitational Lens B2016+112 (2007)

More, A., Porcas, R. W.

We present Global VLBI and HSA images of the gravitational lens B2016+112 at 18, 6 and 3.6 cm. Previous VLBI observations showed that images A and B (which are clearly lensed images of a single...

Harvesting Resources with OAI-PMH (2005)

De Sompel, Xiaoming Liu, Michael L. Nelson, Carl Lagoze, Simeon Warner, Terry Harrison, ...

The problem is not that the WWW doesn’t work; it clearly does. The problem is that our expectations have been lowered. more on DL/WWW, from the NSF Post-DL Workshop: