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The 2dF Galaxy Redshift Survey: The blue galaxy fraction and implications for the Butcher-Oemler effect

(2004)

Authors:

Roberto De Propris, Matthew Colless, John Peacock, Warrick Couch, Simon Driver, Michael Balogh, Ivan Baldry, Carlton Baugh, Joss Bland-Hawthorn, Terry Bridges, Russell Cannon, Shaun Cole, Chris Collins, Nicholas Cross, Gavin Dalton, George Efstathiou, Richard Ellis, Carlos Frenk, Karl Glazebrook, Edward Hawkins, Carole Jackson, Ofer Lahav, Ian Lewis, Stuart Lumsden, Steve Maddox, Darren Madgwick, Peder Norberg, Will Percival, Bruce Peterson, Will Sutherland, Keith Taylor
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The 2dF Galaxy Redshift Survey: The clustering of galaxy groups

(2004)

Authors:

Nelson D Padilla, CM Baugh, VR Eke, P Norberg, S Cole, CS Frenk, DJ Croton, IK Baldry, J Bland-Hawthorn, T Bridges, R Cannon, M Colless, C Collins, W Couch, G Dalton, R De Propris, SP Driver, G Efstathiou, RS Ellis, K Glazebrook, C Jackson, O Lahav, I Lewis, S Lumsden, S Maddox, D Madgwick, JA Peacock, BA Peterson, W Sutherland, K Taylor.
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Galaxy groups in the 2dFGRS: the luminous content of the groups

(2004)

Authors:

VR Eke, CS Frenk, CM Baugh, S Cole, P Norberg, JA Peacock, IK Baldry, J Bland-Hawthorn, T Bridges, R Cannon, M Colless, C Collins, W Couch, G Dalton, R De Propris, SP Driver, G Efstathiou, RS Ellis, K Glazebrook, C Jackson, O Lahav, I Lewis, S Lumsden, S Maddox, D Madgwick, BA Peterson, W Sutherland, K Taylor
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Galaxy groups in the 2dFGRS: the group-finding algorithm and the 2PIGG catalogue

(2004)

Authors:

VR Eke, CM Baugh, S Cole, CS Frenk, P Norberg, JA Peacock, IK Baldry, J Bland-Hawthorn, T Bridges, R Cannon, M Colless, C Collins, W Couch, G Dalton, R De Propris, SP Driver, G Efstathiou, RS Ellis, K Glazebrook, C Jackson, O Lahav, I Lewis, S Lumsden, S Maddox, D Madgwick, BA Peterson, W Sutherland, K Taylor
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Mid-infrared polarimetry and magnetic fields: An observing strategy

Monthly Notices of the Royal Astronomical Society 348:1 (2004) 279-284

Authors:

DK Aitken, JH Hough, PF Roche, CH Smith, CM Wright

Abstract:

Linear polarimetry in the mid-infrared can be used to obtain magnetic field directions in astronomical sources. However, since the polarization can arise from emission and/or absorption from aligned grains, care is needed to plan observations so that enough information is obtained to identify and separate the components of polarization. Procedures for doing this from spectropolarimetry, and from polarimetric imaging at a minimum of two wavebands and making an appropriate filter choice, are presented here, together with an example.
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