Gamma-ray line features from the Crab Nebula in the energy range 50-2000 keV
(1983)
Journal Article
Ayre, C., Myers, R., Thompson, M., Bhat, P., Ma, ,., & Q., Y. (1983). Gamma-ray line features from the Crab Nebula in the energy range 50-2000 keV. Monthly Notices of the Royal Astronomical Society, 205, 285-295. https://doi.org/10.1093/mnras/205.2.285
Outputs (1101)
The velocity fields and radio structures of the active galaxies NGC 5643 and NGC 7582 (1985)
Journal Article
Morris, S., Ward, M., Whittle, M., Wilson, A., & Taylor, K. (1985). The velocity fields and radio structures of the active galaxies NGC 5643 and NGC 7582. Monthly Notices of the Royal Astronomical Society, 216, 193-217. https://doi.org/10.1093/mnras/216.2.193
Laser beacon wave-front sensing without focal anisoplanatism (2002)
Journal Article
Buscher, D., Love, G., & Myers, R. (2002). Laser beacon wave-front sensing without focal anisoplanatism. Optics Letters, 27(3), 149-151. https://doi.org/10.1364/ol.27.000149Wave-front sensing from artificial beacons is normally performed by formation of a focused spot in the atmosphere and sensing of the wave-front distortions produced during the beam's return passage. We propose an alternative method that senses the di... Read More about Laser beacon wave-front sensing without focal anisoplanatism.
Testing stellar population models with star clusters in the Large Magellanic Cloud (2002)
Journal Article
Beasley, M., Hoyle, F., & Sharples, R. (2002). Testing stellar population models with star clusters in the Large Magellanic Cloud. Monthly Notices of the Royal Astronomical Society, 336(1), 168-188. https://doi.org/10.1046/j.1365-8711.2002.05714.xWe present high signal-to-noise ratio integrated spectra of 24 star clusters in the Large Magellanic Cloud (LMC), obtained using the FLAIR spectrograph at the UK Schmidt telescope. The spectra have been placed on to the Lick/IDS system in order to te... Read More about Testing stellar population models with star clusters in the Large Magellanic Cloud.
A wide-field K-band survey - I. Galaxy counts in B, V, I and K (1996)
Journal Article
Gardner, J., Sharples, R., Carrasco, B., & Frenk, C. (1996). A wide-field K-band survey - I. Galaxy counts in B, V, I and K. Monthly Notices of the Royal Astronomical Society, 282, L1-L6. https://doi.org/10.1093/mnras/282.1.l1
Quantitative Study of Galaxy Morphology (2003)
Journal Article
Džanović, D., Sharples, R., Benson, A., & Frenk, C. (2003). Quantitative Study of Galaxy Morphology. Astrophysics and Space Science, 285, 73-77
A 12.6-ms pulsar in Cygnus X-3 (1985)
Journal Article
Chadwick, P., Dipper, N., Dowthwaite, J., Gibson, A., & Harrison, A. (1985). A 12.6-ms pulsar in Cygnus X-3. Nature, 318, 642-644. https://doi.org/10.1038/318642a0
Adaptive Modally Addressed Liquid Crystal Lenses (2004)
Journal Article
Hands, P., Kirby, A., & Love, G. (2004). Adaptive Modally Addressed Liquid Crystal Lenses. Proceedings of SPIE, 5518, 136-143
A wide-field K-band survey - II. Galaxy clustering (1996)
Journal Article
Baugh, C., Gardner, J., Frenk, C., & Sharples, R. (1996). A wide-field K-band survey - II. Galaxy clustering. Monthly Notices of the Royal Astronomical Society, 283, L15-L19. https://doi.org/10.1093/mnras/283.1.l15
The abundance of Lyα emitters in hierarchical models (2005)
Journal Article
Le Delliou, M., Lacey, C., Baugh, C., Guiderdoni, B., Bacon, R., Courtois, H., …Morris, S. (2005). The abundance of Lyα emitters in hierarchical models. Monthly Notices of the Royal Astronomical Society, 357(1), L11-L15. https://doi.org/10.1111/j.1745-3933.2005.00007.xWe present predictions for the abundance of Lyα emitters in hierarchical structure formation models. We use the GALFORM semi-analytical model of galaxy formation to explore the impact on the predicted counts of varying assumptions about the escape fr... Read More about The abundance of Lyα emitters in hierarchical models.
The MARTINI adaptive optics instrument (2000)
Journal Article
Doel, A., Dunlop, C., Buscher, D., Myers, R., Sharples, R., & Major, J. (2000). The MARTINI adaptive optics instrument. New Astronomy, 5, 223-233
New measurements of the 12.6 millisecond pulsar in Cygnus X-3 (1990)
Journal Article
Brazier, K., Carraminana, A., Chadwick, P., Dipper, N., Lincoln, E., Mackie, P., …Turver, K. (1990). New measurements of the 12.6 millisecond pulsar in Cygnus X-3. Astrophysical Journal, 350, 745-753. https://doi.org/10.1086/168425
Enhancement of the gamma ray signal in atmospheric Cerenkov light measurements using the University of Durham VHE gamma ray telescopes (1990)
Journal Article
Brazier, K., Carraminaña, A., Chadwick, P., Dipper, N., Lincoln, E., Mannings, V., …Turver, K. (1990). Enhancement of the gamma ray signal in atmospheric Cerenkov light measurements using the University of Durham VHE gamma ray telescopes. Nuclear Physics B - Proceedings Supplements, 14, 250-255
Stereoscopic Measurements of the Cerenkov Radiation Produced by TeV Gamma-Rays (1996)
Journal Article
Chadwick, P., Dickinson, J., Dickinson, M., Dipper, N., Holder, J., McComb, T., …Turver, K. (1996). Stereoscopic Measurements of the Cerenkov Radiation Produced by TeV Gamma-Rays. Space Science Reviews, 75, 153-167
The effect of the geomagnetic field on TeV gamma -ray detection (1992)
Journal Article
Bowden, C., Bradbury, S., Chadwick, P., Dickinson, J., Dipper, N., Edwards, P., …Turver, K. (1992). The effect of the geomagnetic field on TeV gamma -ray detection. Journal of Physics G: Nuclear and Particle Physics, 18, L55-L60. https://doi.org/10.1088/0954-3899/18/2/007
Centaurus X-3: A Source of High-Energy Gamma Rays (1998)
Journal Article
Chadwick, P., Dickinson, M., Dipper, N., Kendall, T., McComb, T., Orford, K., …Turver, K. (1998). Centaurus X-3: A Source of High-Energy Gamma Rays. Astrophysical Journal, 503, 391-
Constraints on the dark energy equation of state from the imprint of baryons on the power spectrum of clusters (2005)
Journal Article
Angulo, R., Baugh, C., Frenk, C., Bower, R., Jenkins, A., & Morris, S. (2005). Constraints on the dark energy equation of state from the imprint of baryons on the power spectrum of clusters. Monthly Notices of the Royal Astronomical Society, 362(1), L25-L29. https://doi.org/10.1111/j.1745-3933.2005.00067.xAcoustic oscillations in the baryon–photon fluid leave a signature in the matter power spectrum. The overall shape of the spectrum and the wavelength of the oscillations depend upon the sound horizon scale at recombination. Using the Λ cold dark matt... Read More about Constraints on the dark energy equation of state from the imprint of baryons on the power spectrum of clusters.
Low light level CCDs and visibility parameter estimation (2004)
Journal Article
Basden, A., & Haniff, C. (2004). Low light level CCDs and visibility parameter estimation. Monthly Notices of the Royal Astronomical Society, 347, 1187-1197. https://doi.org/10.1111/j.1365-2966.2004.07283.x
Dual-conjugate wavefront generation for adaptive optics (2000)
Journal Article
Kelly, T., Buscher, D., Clark, P., Dunlop, C., Love, G., Myers, R., …Zadrozny, A. (2000). Dual-conjugate wavefront generation for adaptive optics. Optics Express, 7(11), 368-374. https://doi.org/10.1364/oe.7.000368We present results of the isoplanatic performance of an astronomical adaptive optics system in the laboratory, by using a dual layer turbulence simulator. We describe how the performance of adaptive correction degrades with off-axis angle. These expe... Read More about Dual-conjugate wavefront generation for adaptive optics.
Adaptive optics for astronomy: theoretical performance and limitations (1996)
Journal Article
Wilson, R., & Jenkins, C. (1996). Adaptive optics for astronomy: theoretical performance and limitations. Monthly Notices of the Royal Astronomical Society, 278, 39-61