next up previous contents
Next: node51.html Up: Clusterdetektion in Punktfeldern Previous: Performance

References

Abell1958
ABELL, G.O. (1958). The Distribution of Rich Clusters of Galaxies. Astrophys. J. Suppl. Ser., 3, 211-288.

Abell et al.1989
ABELL, G.O., CORWIN JR., H.G. & OLOWIN, R.P. (1989). A catalogue of rich clusters of galaxies. Astrophys. J. Suppl. Ser., 70, 1-138.

Andernach1991
ANDERNACH, H. (1991). A Catalogue of Measured Redshifts of Abell Clusters of Galaxies. ASP Conf. Ser., 15, 279-284.

Bahcall1988
BAHCALL, N. A. (1988). Large-Scale Structure in the Universe indicated by Galaxy Clusters. Ann. Rev. Astron. Astrophys., 26, 631-686.

Bahcall & Soneira1984
BAHCALL, N. A. & SONEIRA, R. M. (1984). A supercluster catalog. Astrophys. J., 277, 27-37.

Batuski & Burns1985
BATUSKI, D.J. & BURNS, J.D. (1985). Finding lists of candidate superclusters and voids of Abell clusters. Astron. J., 90, 1413-1424.

Binney & Tremaine1987
BINNEY, J. & TREMAINE, S. (1987). Galactic dynamics. Princeton University Press, Princeton.

Blatt et al.1996
BLATT, M., WISEMAN, S. & DOMANY, E. (1996). Superparamagnetic clustering of data. Phys. Rev. Lett., 76, 3251-3254.

Blatt et al.1997
BLATT, M., WISEMAN, S. & DOMANY, E. (1997). Data clustering using a model granular magnet. Unpublished.

Chen et al.1992
CHEN, S., FERRENBERG, A.M. & LANDAU, D.P. (1992). Randomness-induced second-order transitions in the two-dimensional eight-state Potts model: a Monte-Carlo study. Phys. Rev. Lett., 69, 1213-1215.

Doroshkevich et al.1999
DOROSHKEVICH, A.G., M"ULLER, V., RETZLAFF, J. & TUCHANINOV, V. (1999). Large and super-large scale structures from n-body simulations. Mon. Not. R. Astron. Soc., 306, 575-591.

Einasto et al.1994
EINASTO, M., EINASTO, J., TAGO, E., DALTON, G.B. & ANDERNACH, H. (1994). The structure of the Universe traced by rich clusters of galaxies. Mon. Not. R. Astron. Soc., 269, 301-322.

Field1972
FIELD, G.B. (1972). Intergalactic Matter. Ann. Rev. Astron. Astrophys., 10, 227-260.

Fukuda1998
FUKUDA, K. (1998). Frequently Asked Questions in Polyhedral Computation. http://www.ifor.math.ethz.ch/ifor/staff/fukuda/polyfaq/polyfaq.html.

GTOPO301996
GTOPO30 (1996). Global 30 Arc Second Elevation Data Set. http://edcwww.cr.usgs.gov/landdaac/gtopo30/gtopo30.html.

Gutenberg & Richter1956
GUTENBERG, B. & RICHTER, C.F. (1956). Earthquake magnitude, intensity, energy and acceleration. Bull. Seism. Soc. Am., 46, 105-145.

Harwit1988
HARWIT, M. (1988). Astrophysical Concepts. Springer-Verlag, New York Berlin Heidelberg.

Hubble & Humason1931
HUBBLE, E. & HUMASON, M. (1931). The Velocity-Distance Relation among Extra-Galactic Nebulae. Astrophys. J., 74, 43-80.

Kalinkov & Kuneva1995
KALINKOV, M. & KUNEVA, I. (1995). Superclusters of Galaxies. I. The catalog. Astron. Astrophys. Suppl. Ser., 113, 451-457.

Kerscher1998
KERSCHER, M. (1998). Morphologie gro"sr"aumiger Strukturen im Universum, (Dissertationsschrift). Ludwig-Maximilians-Universit"at M"unchen.

Kinzel & Reents1996
KINZEL, W. & REENTS, G. (1996). Physik per Computer. Spektrum Akademischer Verlag, Heidelberg, Berlin, Oxford.

Knebe & M"uller1999
KNEBE, A. & M"ULLER, V. (1999). Formation of groups and clusters of galaxies. Astron. Astrophys., 341, 1-7.

Murray et al.1978
MURRAY, S.S., FORMAN, W., JONES, C. & GIACCONI, R. (1978). Evidence for X-ray emission from superclusters of galaxies determined from UHURU. Astrophys. J. Lett., 219, L89-L93.

NEIC1999
NEIC (1999). Near Real Time Earthquake List. http://wwwneic.cr.usgs.gov/neis/bulletin/bulletin.html. National Earthquake Information Center.

Neumann et al.1989
NEUMANN, W., JACOBS, F. & TITTEL, B. (1989). Erdbeben. BSB B.G. Teubner Verlagsgesellschaft, Leipzig.

Onsager1944
ONSAGER, L. (1944). Phys. Rev., 65, 117.

Oort1983
OORT, J.H. (1983). Superclusters. Ann. Rev. Astron. Astrophys., 21, 373-428.

Petzschmann et al.1999
PETZSCHMANN, O., SCHWARZ, U., SPAHN, F., GREBOGI, C. & KURTHS, J. (1999). Length scales of clustering in granular gases. Phys. Rev. Lett., 82, 4819-4822.

Petzschmann1999
PETZSCHMANN, O. (1999). L"angenskalen granularer Cluster, (Dissertationsschrift). Universität Potsdam.

Postman et al.1992
POSTMAN, M., HUCHRA, J.P. & GELLER, M.J. (1992). The distribution of nearby rich clusters of galaxies. Astrophys. J., 384, 404-422.

Press et al.1992
PRESS, W.H., TEUKOLSKI, S.A., VETTERLING, W.T. & FLANNERY, B.P. (1992). Numerical recipies in C: the art of scientific computing. Cambridge University Press.

Retzlaff et al.1998
RETZLAFF, J., BORGANI, S., GOTTLOBER, S., KLYPIN, A. & M"ULLER, V. (1998). Constraining cosmological models with cluster power spectra. New Astronomy, 3, 631-646.

Ripley1981
RIPLEY, B.D. (1981). Spatial Statistics. Wiley & Sons.

Rood1976
ROOD, H.J. (1976). Nearby groups of galaxy clusters. Astrophys. J., 207, 16-24.

Schmalzing et al.1999
SCHMALZING, J., BUCHERT, T., MELOTT, A.L., SAHNI, V., SATHYAPRAKASH, B.S. & SHANDARIN, S.F. (1999). Disentangling the Cosmic Web. I. Morphology of Isodensity Contours. Astrophys. J., 526, 568-578.

SCSNC1999
SCSNC (1999). Southern California Seismic Network Catalog. http://www.scecdc.scec.org/catalogs.html. Southern California Earthquake Data Center.

Shandarin & Yess1998
SHANDARIN, S.F. & YESS, C. (1998). Detection of Network Structure in the Las Campanas Redshift Survey. Astrophys. J., 505, 12-17.

Shandarin & Zeldovich1989
SHANDARIN, S.F. & ZELDOVICH, YA.B. (1989). The large-scale structure of the universe: Turbulence, intermittency, structures in a self-gravitating medium. Rev. Mod. Phys., 61(2), 185-220.

Shapley1930
SHAPLEY, H. (1930). Harv. Obs. Bull., 874, 9.

Steinhausen & Langer1977
STEINHAUSEN, D. & LANGER, K. (1977). Clusteranalyse. Einführung in Methoden und Verfahren der automatischen Klassifikation. DeGruyter Verlag, Berlin.

Stoyan & Stoyan1992
STOYAN, D. & STOYAN, H. (1992). Fraktale - Formen - Punktfelder. Akademie Verlag, Berlin.

Swendsen & Wang1986
SWENDSEN, R. & WANG, J.-S. (1986). Replica Monte Carlo Simulation of Spin-Glasses. Phys. Rev. Lett., 57, 2607.

Swendsen et al.1992
SWENDSEN, R., WANG, J.-S. & FERRENBERG, A.M. (1992). New Monte Carlo Methods for Improved Efficiency of Computer Simulations in Statistical Mechanics. In The Monte Carlo Method in Condensed Matter Physics, BINDER, K. (Ed.), Springer Verlag, Berlin, Heidelberg, New York. Topics in Applied Physics, 71, 75-91.

The POV-Ray Team1999
THE POV-RAY TEAM (1999). POV-Ray 3.1. http://www.povray.org.

Thuan1980
THUAN, T.X. (1980). The large-scale distribution of galaxies. In Physical Cosmology, 277-289.

Uns"old & Baschek1988
UNS"OLD, A. & BASCHEK, B. (1988). Der neue Kosmos. Springer Verlag, Berlin, New York.

Weinberg1977
WEINBERG, S. (1977). Die ersten drei Minuten. Der Ursprung des Universums. R. Piper & Co. Verlag, M"unchen.

West1989
WEST, M. J. (1989). On the morphology of superclusters. Astrophys. J., 347, 610-626.

White et al.1994
WHITE, M., SCOTT, D. & SILK, J. (1994). Anisotropies in the Cosmic Microwave Background. Ann. Rev. Astron. Astrophys., 32, 319-370.

Wiseman et al.1998
WISEMAN, S., BLATT, M. & DOMANY, E. (1998). Super-paramagnetic clustering of data. Phys. Rev. E, 57, 3767-3783.

Z"oller1999
Z"OLLER, G. (1999). Analyse raumzeitlicher Muster in Erdbebendaten, (Dissertationsschrift). Universit"at Potsdam.

Zucca et al.1993
ZUCCA, E., ZANMORANI, G., SCARAMELLA, R. & VETTOLANI, G. (1993). All-sky catalogs of superclusters of Abell-ACO clusters. Astrophys. J., 407, 470-488.



Udo Schwarz
Thu Mar 1 15:43:04 MET 2001