Rubin-LSST

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The very flat radio - millimetre spectrum of Cygnus X-1

(1999)

Authors:

RP Fender, GG Pooley, P Durouchoux, RPJ Tilanus, C Brocksopp
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Identification of a Likely Radio Counterpart of the Rapid Burster

(1999)

Authors:

CB Moore, RE Rutledge, DW Fox, RA Guerriero, WHG Lewin, R Fender, J van Paradijs
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A UKST survey of blue objects towards the galactic centre – a search for early-type stars

Astronomy and Astrophysics Supplement Series EDP Sciences 139:2 (1999) 231-244

Authors:

PL Dufton, SJ Smartt, NC Hambly
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Design, performance and status of the CLEO III silicon detector

Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment Elsevier 435:1-2 (1999) 9-15

Authors:

J Fast, MS Alam, J Alexander, A Anastassov, K Arndt, A Bean, C Bebek, R Boyd, G Brandenburg, J Cherwinka, C Darling, J Duboscq, KK Gan, Y Gao, P Hopman, H Kagan, R Kass, D Kim, J Lee, N Menon, D Miller, J Oliver, C Rush, H Severini, I Shipsey, P Skubic, M Spencer, S Timm, E Tourne, C Ward, M Zoeller
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Are recent peculiar velocity surveys consistent?

Cosmic Flows 1999: Towards an Understanding of Large-Scale Structures Astronomical Society of the Pacific (1999)

Authors:

MJ Hudson, RJ Smith, DJ Schlegel, Roger Davies

Abstract:

We compare the bulk flow of the SMAC sample to the predictions of popular cosmological models and to other recent large-scale peculiar velocity surveys. Both analyses account for aliasing of small-scale power due to the sparse and non-uniform sampling of the surveys. We conclude that the SMAC bulk flow is in marginal conflict with flat COBE-normalized Lambda-CDM models which fit the cluster abundance constraint. However, power spectra which are steeper shortward of the peak are consistent with all of the above constraints. When recent large-scale peculiar velocity surveys are compared, we conclude that all measured bulk flows (with the possible exception of that of Lauer & Postman) are consistent with each other given the errors, provided the latter allow for `cosmic covariance'. A rough estimate of the mean bulk flow of all surveys (except Lauer & Postman) is ~400 km/s towards l=270, b=0.
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