14.2k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Centre National de la Recherche ScientifiqueFR1.2k papers
- California Institute of TechnologyUS1k papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR744 papers
- University of CambridgeGB676 papers
- University College LondonGB641 papers
- University of TorontoCA603 papers
- National Institute for AstrophysicsIT595 papers
- Sapienza University of RomeIT578 papers
- Stanford UniversityUS550 papers
- European Southern ObservatoryCL540 papers
- Jet Propulsion LaboratoryUS533 papers
- University of ManchesterGB523 papers
19 papers · 2 filters
Environmental Effects on the Faint End of the Luminosity Function
S. Phillipps, J. B. Jones, R. M. Smith +2
Recent studies have demonstrated that many galaxy clusters have luminosity functions (LFs) which are steep at the faint end. However, it is equally clear that not all clusters have…
Modelling ISO Galaxy Counts with Luminosity and Merger Rate Evolution
Nathan Roche, Steve Eales
We model galaxy evolution in the 6.75 and 15 micron passbands of the ISO satellite, by combining models of galaxy evolution at optical wavelengths (which are consistent with the op…
Deep optical imaging of the field of PC1643+4631A&B, I: Spatial distributions and the counts of faint galaxies
Toby Haynes, Garret Cotter, Joanne C. Baker +4
We present deep optical images of the PC1643+4631 field obtained at the WHT. This field contains two quasars at redshifts z=3.79 & 3.83 and a cosmic microwave background (CMB) decr…
15um ISO observations of a CFRS field: the cosmic SFR as derived from UV, optical, mid-IR and radio photometry
H. Flores, F. Hammer, T. Thuan +7
The CFRS 1452+52 field has been deeply imaged with the Infrared Space Observatory (ISO) using ISOCAM through the LW3 filter (12-18um). Careful data analysis and comparison to deep…
Deep Galaxy survey at 6.75 micron with the ISO satellite
H. Flores, F. Hammer, F. X. Désert +8
Deep 6.75um mid-IR ISOCAM observations were obtained of the Canada-France Redshift Survey (CFRS) 1415+52 field with the Infrared Space Observatory. The identification of the source…
Found: High Surface Brightness Compact Galaxies
M. J. Drinkwater, S. Phillipps, J. B. Jones +5
We are using the 2dF spectrograph to make a survey of all objects (`stars' and `galaxies') in a 12 sq.deg region towards the Fornax cluster. We have discovered a population of comp…
Cosmological Evolution of the Submillimetre Luminosity of High-Redshift Radio Galaxies
D. H. Hughes, J. S. Dunlop, E. N. Archibald +2
A systematic survey measuring the submillimetre continuum luminosity in radio galaxies between redshifts z ~ 0.1 - 5 is currently in progress. The first results from observations w…
The Angular Correlation Function of K=19.5 Galaxies and the Detection of a Cluster at z=0.775
Nathan Roche, Steve Eales, Hans Hippelein +1
On five K-band Omega camera images, covering a total of 162.2 sq. arcmin to K=19.5, we investigate (i) the clustering environment of 5 radio galaxies at 0.7<z<0.8 and (ii) the gala…
Spiral Structure in IP Peg: Confronting Theory and Observations
Takuya Matsuda, Makoto Makita, Hiroshi Yukawa +1
The first convincing piece of evidence of spiral structure in the accretion disc in IP Pegasi was found by Steeghs et al. (1997). We performed two kinds of 2D hydrodynamic simulati…
The Canada-UK Deep Submillimetre Survey: First Submillimetre Images, the Source Counts, and Resolution of the Background
Stephen Eales, Simon Lilly, Walter Gear +5
We present the first results of a deep unbiased submillimetre survey carried out at 450 and 850 microns. We detected 12 sources at 850 microns, giving a surface density of sources…
SCUBA imaging of NGC 7331 dust ring
S. Bianchi, P. B. Alton, J. I. Davies +1
We present observations of the spiral galaxy NGC 7331 using the Sub-millimetre Common User Bolometer Array (SCUBA) on the James Clark Maxwell Telescope. We have detected a dust rin…
Numerical Computation of Two Dimensional Wind Accretion of Isothermal Gas
Eiji Shima, Takuya Matsuda, Ulrich Anzer +2
A new numerical algorithm for calculating isothermal wind accretion flows has been developed and is applied here to the analysis of the hydrodynamics of two-dimensional plane symme…
Morphology of Clusters and Superclusters in N-body simulations of Cosmological Gravitational Clustering
B. S. Sathyaprakash, Varun Sahni, Sergei F. Shandarin
We analyse shapes of overdense regions (clusters and superclusters) in controlled N-body simulations of gravitational clustering with power law initial spectra P(k) \propto k^n, n…
Filaments and Pancakes in the IRAS 1.2 Jy Redshift Catalogue
B. S. Sathyaprakash, Varun Sahni, Sergei F. Shandarin +1
We explore shapes of clusters and superclusters in the IRAS 1.2 Jy redshift survey with three reconstructions spanning the range β= 0.1, 0.5, 1.0, where β= Ω^{0.6}/b, b is the bias…
The Luminosity Distribution in Galaxy Clusters: A Dwarf Population - Density Relation?
S. Phillipps, S. P. Driver, W. J. Couch +1
Recent work suggests that rich clusters of galaxies commonly have large populations of dwarf (i.e. low luminosity) members, that is their luminosity function (LF) turns up to a ste…
The Discovery of the Smallest Blue Compact Dwarf Galaxies
M. J. Drinkwater, M. D. Gregg, R. M. Smith
In a spectroscopic survey of the Fornax cluster to Bj=17.5 using the FLAIR spectrograph on the UK Schmidt Telescope we have discovered seven new compact dwarf cluster members. Thes…
The Angular Correlation Function and Hierarchical Moments of 70000 Faint Galaxies to R=23.5
Nathan Roche, Steve Eales
We investigate the angular correlation function, omega(theta), and third and fourth-order hierarchical moments of a survey with approx. 70000 faint galaxies detected on a total are…
A Complete 2dF Survey of Fornax
M. J. Drinkwater, E. M. Sadler, J. I. Davies +5
We are using the 2dF spectrograph on the Anglo-Australian Telescope to obtain spectra for a complete sample of all 14000 objects with 16.5<B<19.7 in a 12 square degree area centred…
Shapefinders: A new shape diagnostic for large scale structure
Varun Sahni, B. S. Sathyaprakash, Sergei F. Shandarin
We construct a set of shape-finders which determine shapes of compact surfaces (iso-density surfaces in galaxy surveys or N-body simulations) without fitting them to ellipsoidal co…