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All Outputs (5)

A Million Element Integral Field Unit (MEIFU) (2002)
Conference Proceeding
Morris, S., Content, R., Sharples, R., Bower, R., Davies, R., & Baugh, C. (2002). A Million Element Integral Field Unit (MEIFU). In Scientific Drivers for ESO Future VLT/VLTI Instrumentation: Proceedings of the ESO Workshop Held in Garching, Germany, 11-15 June 2001 (99-107). https://doi.org/10.1007/10857019_16

We describe an instrument concept that will provide simultaneous spectra for a million spatial samples on the sky. With the proposed field of view and spectral resolution, it will be able to measure redshifts and line strengths for around 2-4000 z∼∼3... Read More about A Million Element Integral Field Unit (MEIFU).

The 2dF Galaxy Redshift Survey: the environmental dependence of galaxy star formation rates near clusters (2002)
Journal Article
Lewis, I., Balogh, M., De Propris, R., Couch, W., Bower, R., Offer, A., …Taylor, K. (2002). The 2dF Galaxy Redshift Survey: the environmental dependence of galaxy star formation rates near clusters. Monthly Notices of the Royal Astronomical Society, 334(3), 673-683. https://doi.org/10.1046/j.1365-8711.2002.05558.x

We have measured the equivalent width of the Hα emission line for 11 006 galaxies brighter than Mb=−19 (ΩΛ= 0.7, Ωm= 0.3, H0= 70 km s−1 Mpc−1) at 0.05 < z < 0.1 in the 2dF Galaxy Redshift Survey (2dFGRS), in the fields of 17 known galaxy clusters. Th... Read More about The 2dF Galaxy Redshift Survey: the environmental dependence of galaxy star formation rates near clusters.

Distinguishing Local and Global Influences on Galaxy Morphology: A Hubble Space Telescope Comparison of High and Low X-Ray Luminosity Clusters. (2002)
Journal Article
Balogh, M. L., Smail, I., Bower, R., Ziegler, B., Smith, G., Davies, R. L., …Ebeling, H. (2002). Distinguishing Local and Global Influences on Galaxy Morphology: A Hubble Space Telescope Comparison of High and Low X-Ray Luminosity Clusters. Astrophysical Journal, 566(1), 123-136. https://doi.org/10.1086/338056

We present a morphological analysis of 17 X-ray-selected clusters at z ~ 0.25, imaged uniformly with the Hubble Space Telescope Wide Field Planetary Camera 2 (WFPC2). Eight of these clusters comprise a subsample selected for their low X-ray luminosit... Read More about Distinguishing Local and Global Influences on Galaxy Morphology: A Hubble Space Telescope Comparison of High and Low X-Ray Luminosity Clusters..