Skip to main content Accessibility help
×
Hostname: page-component-586b7cd67f-tf8b9 Total loading time: 0 Render date: 2024-11-28T16:05:51.575Z Has data issue: false hasContentIssue false

8 - Priority Disputes and the Timeline of Publications

Published online by Cambridge University Press:  02 December 2020

Laird A. Thompson
Affiliation:
University of Illinois, Urbana-Champaign
Get access

Summary

Two challenges have been made regarding the Gregory and Thompson 1978 discovery priority of cosmic voids and the extended structure (called “bridges”) that connect one rich cluster with its nearest neighbor(s). The primary challenge is by the Center for Astrophysics group called CfA2 headed by Geller and her late collaborator Huchra. A less significant challenge is by Chincarini, one of the Arizona redshift survey members. These issues are discussed point by point starting with the CfA2 challenge. Table 8.1 summarizes the Arizona work as of 1984–1985 (just before the CfA2 survey began). This table as well as the extensive “timeline” table (Table 8.2) demonstrate that the CfA2 survey was a latecomer in the pioneering period and represents nothing more than an incremental step forward. The Chincarini challenge is based on data that belonged to our Arizona consortium (a subgroup headed by Tarenghi) and was published by Chincarini without permission.

Type
Chapter
Information
Publisher: Cambridge University Press
Print publication year: 2020

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

CMB precursor references:

McKellar, A. (1941). Molecular Lines from the Lowest States of the Atomic Molecules Composed of Atoms Probably Present in Interstellar Space. Pub. Dominion Astrophys. Observatory (Victoria), 7, pp. 25172.Google Scholar
Alpher, R. and Herman, R. (1948). Evolution of the Universe. Nature, vol. 162, pp.7745.Google Scholar
Shmaonov, T. (1957). Ph.D. Thesis. Also reported in Pribori i Tekhniika Experimenta (in Russian), 1, p. 83.Google Scholar
Doroshkevich, A. and Novikov, I. (1964). Mean Density of Radiation in the Metagalaxy and Certain Problems in Relativistic Cosmology. Soviet Physics Doklady, 9, pp. 1114.Google Scholar
Dicke, R., Peebles, P., Roll, P., and Wilkinson, D. (1965). Cosmic Black-Body Radiation. Astrophys. J., 142, pp. 4149.Google Scholar

CMB detection references:

Penzias, A. and Wilson, R. (1965). A Measurement of Excess Antenna Temperature at 4080 MHz Astrophys. J., 142, 419–21.Google Scholar
Roll, P. and Wilkinson, D. (1966). Cosmic Background Radiation at 3.2 cm – Support for Cosmic Black-Body Radiation. Phys. Rev. Lett., 16, pp. 4057.Google Scholar
Conklin, E. (1969). Velocity of the Earth with Respect to the Cosmic Background Radiation. Nature, 222, pp. 9712.Google Scholar
Uson, J. and Wilkinson, D. (1984). Small-Scale Isotropy of the Cosmic Microwave Background at 19.5 GHz. Astrophys. J., 283, pp. 4718.Google Scholar
Mather, J. et al. (1990). A Preliminary Measurement of the Cosmic Microwave Background Spectrum by the Cosmic Background Explorer (COBE) Satellite. Astrophys. J., 354, pp. L37L40.Google Scholar
Smoot, G. et al. (1992). Structure in the COBE Differential Microwave Radiometer First-Year Maps. Astrophys. J., 396, pp. L1L5.Google Scholar
Spergel, D. et al. (2003). First-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters. Astrophys. J., 148, pp. 17594.Google Scholar

LSS precursor references:

Herschel, W. (1784). Account of Some Observations Tending to Investigate the Construction of the Heavens. Phil. Trans., 74, Section XIII, pp. 43751.Google Scholar
Herschel, W. (1811). Astronomical Observations Relating to the Construction of the Heavens, Arranged for the Purpose of a Critical Examination, the Result of which Appears to Throw Some New Light upon the Organization of the Celestial Bodies. Phil. Trans., Section LXIII, pp. 43751.Google Scholar
Shapley, H. and Ames, A. (1932a). Annals of the Astronomical Observatory of Harvard College, 88, No. 2, pp. 4375 (Shapley-Ames Catalogue); 1932b, Harvard College Observatory, Bulletin No. 887, pp. 16.Google Scholar
Humason, M., Mayall, N., and Sandage, A. (1956). Redshifts and Magnitudes of Extragalactic Nebulae. Astron. J., 61, pp. 97162.Google Scholar
Mayall, N. (1960). Advantages of Electronic Photography for Extragalactic Spectroscopy. Ann. Astrophys., 23, pp. 34459.Google Scholar
de Vaucouleurs, G. (1965). Nearby Groups of Galaxies. Ch. 14, pp. 557–600 in Galaxies and the Universe. eds. Sandage, A., Sandage, M., Kristian, J., and Tamman, G. University of Chicago Press (Chicago, Illinois). The Compendium Series was published in 1975 but a note in the article gives 1965 as the date of submission.Google Scholar
Chincarini, G. and Martins, D. (1975). On the “Seyfert Sextet,” VV 115. Astrophys. J., 196, pp. 3357.Google Scholar
Chincarini, G. and Rood, H. (1975). Size of the Coma Cluster. Nature, 257, pp. 2945.Google Scholar
Tifft, W. and Gregory, S. (1976). Direct Observations of the Large-Scale Distribution of Galaxies. Astrophys. J., 205, pp. 696708.Google Scholar
Chincarini, G. and Rood, H. (1976). The Coma Supercluster – Analysis of Zwicky-Herzog Cluster 16 in Field 158. Astrophys. J., 206, pp. 307.Google Scholar

LSS detection references:

Gregory, S. and Thompson, L. (1978). The Coma/A1367 Supercluster and Its Environs. Astrophys. J., 222, pp. 78499.Google Scholar
Chincarini, G. (1978). Clumpy Structure of the Universe and General Field. Nature, 272, pp. 5156. (The “rogue” paper.)Google Scholar
Joeveer, M., Einasto, J., and Tago, E. (1978). Spatial Distribution of Galaxies and Clusters of Galaxies in the Southern Galactic Hemisphere. Mon. Not. Royal Astron. Soc.,185, pp. 35770.Google Scholar
Tarenghi, M., Tifft, W., Chincarini, G., Rood, H., and Thompson, L. (1979). The Hercules Supercluster. I. Basic Data. Astrophys. J., 234, pp. 793801.Google Scholar
Tarenghi, M., Chincarini, G., Rood, H., and Thompson, L. (1980). The Hercules Supercluster. II. Analysis. Astrophys. J., 235, pp. 72442.Google Scholar
Einasto, J., Joeveer, M., and Saar, E. (1980). Structure of Superclusters and Supercluster Formation. Mon. Not. Royal Astron. Soc., 193, pp. 35375.Google Scholar
Gregory, S., Thompson, L., and Tifft, W. (1981). The Perseus Supercluster. Astrophys. J., 243, pp. 41126.Google Scholar
Kirshner, R., Oemler, A., Jr., Schechter, P., and Shectman, S. (1981). A Million Cubic Megaparsec Void in Boötes. Astrophys. J. Lett., 248, L57L60.Google Scholar
Chincarini, G., Thompson, L., and Rood, H. (1981). Supercluster Bridge between Groups of Galaxy Clusters. Astrophys. J. Lett., 249, L47L50.Google Scholar
Davis, M., Huchra, J., Latham, D., and Tonry, J. (1982). A Survey of Galaxy Redshifts. II. The Large Scale Spatial Distribution. Astrophys. J., 253, pp. 42345. (CfA1)Google Scholar
Zeldovich, Y., Einasto, J., and Shandarin, S. (1982). Giant Voids in the Universe. Nature, 300, pp. 40713.Google Scholar
Chincarini, G., Giovanelli, R., and Haynes, M. (1983). 21 Centimeter Observations of Supercluster Galaxies – The Bridge between Coma and A1367. Astrophys. J., 269, pp. 1328.Google Scholar
Gregory, S. and Thompson, L. (1984). The A2197 and A2197 Galaxy Clusters. Astrophys. J., 286, pp. 42236.Google Scholar
Giovanelli, R. and Haynes, M. (1985). A 21 cm Survey of the Pisces-Perseus Supercluster. I – The Declination Zone +27.5 to +33.5 degrees. Astron. J., 90, pp. 244573.Google Scholar
Giovanelli, R., Haynes, M., and Chincarini, G. (1986). Morphological Segregation in the Pisces-Perseus Supercluster. Astrophys. J., 300, pp. 7792.Google Scholar
de Lapparent, V., Geller, M., and Huchra, J. (1986). A Slice of the Universe. Astrophys. J. Lett., 302, pp. L1-L5. (CfA2)Google Scholar
Gott, J.,III, Melott, A., and Dickinson, M. (1986). The Sponge-like Topology of Large-Scale Structure in the Universe. Astrophys. J., 306, pp. 34157.Google Scholar
Geller, M. & Huchra, J. (1989). Mapping the Universe. Science, 246, pp. 897903.Google Scholar
Wegner, G., Haynes, M., and Giovanelli, R. (1993). A Survey of the Pisces-Perseus Supercluster. V – The Declination Strip +33.5 deg to +39.5 deg and the Main Supercluster Ridge. Astron. J., 105, pp. 125170.Google Scholar
Shectman, S., Landy, S., Oemler, A., Jr., Tucker, D., Lin, H., Kirshner, R., and Schechter, P. (1996). The Las Campanas Redshift Survey. Astrophys. J., 470, pp. 17288.Google Scholar
Falco, E., Kurtz, M., Geller, M., Huchra, J., Peters, J., Berlind, P., Mink, D., Tokarz, S., and Elwell, B. (1999). The Updated Zwicky Catalog (UZC). Pub. Astron. Soc. Pacific, 111, pp. 43852.Google Scholar
Colless, M., Dalton, G., Maddox, S., Sutherland, W., and 25 coauthors (2001). The 2dF Galaxy Redshift Survey: Spectra and Redshifts. Mon. Not. Royal Astron. Soc., 238, pp. 103963.Google Scholar
Strauss, M., Weinberg, D., Lupton, R., Narayanan, V., and 32 coauthors (2002). Spectroscopic Target Selection in the Sloan Digital Sky Survey: The Main Galaxy Sample. Astron. J., 124, pp. 181024.Google Scholar

LSS theory references:

Holmberg, E. (1937). A Study of Double and Multiple Galaxies together with Inquiries into Some General Metagalactic Problems with an Appendix Containing a Catalogue of 827 Double and Multiple Galaxies. Medd. Lund Obs., No. 6, pp. 3173.Google Scholar
Peebles, P. and Dicke, R. (1968). Origin of the Globular Clusters. Astrophys. J., 154, pp. 891908.Google Scholar
Harrison, E. (1970). Fluctuations at the Threshold of Classical Cosmology. Phys. Rev. D, 1, pp. 272630.Google Scholar
Zeldovich, Y. (1970). Gravitational Instability: An Approximate Theory for Large Density Perturbations. Astron. and Astrophys., 5, pp. 849.Google Scholar
Peebles, P. and Yu, J. (1970). Primeval Adiabatic Perturbation in an Expanding Universe. Astrophys. J., 162, pp. 81536.Google Scholar
Zeldovich, Y. (1972). A Hypothesis, Unifying the Structure and the Entropy of the Universe. Mon. Not. Royal Astron. Soc., 160, pp. 1P–3P.Google Scholar
Sunyaev, R. and Zeldovich, Y. (1972). Formation of Clusters of Galaxies; Protocluster Fragmentation and Intergalactic Gas Heating. Astron. and Astrophys., 20, pp. 189200.Google Scholar
Shandarin, S. 1975 (private communication: hand-to-hand transfer of the computer plot).Google Scholar
Doroshkevich, A., Zeldovich, Y., and Sunyaev, R. (1976). “Adiabatic Theory of Formation of Galaxies. In Origin and Evolution of Galaxies and Stars.” OEGS Conference, pp. 65104. (in Russian).Google Scholar
Gibbons, G. and Hawking, S. (1977) Cosmological Event Horizons, Thermodynamics, and Particle Creation. Phys. Rev. D, 15, pp. 273851.Google Scholar
Doroshkevich, A. and Shandarin, S. (1978). A Statistical Approach to the Theory of Galaxy Formation. Soviet Astron., 22, pp. 65360.Google Scholar
Soneira, R. and Peebles, P. (1978). A Computer Model Universe – Simulation of the Nature of the Galaxy Distribution in the Lick Catalog. Astron. J., 83, pp. 84560.Google Scholar
White, S. and Rees, M. (1978). Core Condensation in Heavy Halos – A Two-Stage Theory for Galaxy Formation and Clustering. Mon. Not. Royal Astron. Soc., 183, pp. 341–58.Google Scholar
Aarseth, S., Gott, J., III and Turner, E. (1979). N-Body Simulation of Galaxy Clustering. I. Initial Conditions and Galaxy Collapse Times. Astrophys. J., 228, pp. 66483.Google Scholar
Peebles, P. (1980). Large Scale Structure of the Universe (Princeton, NJ: Princeton University Press).Google Scholar
Bond, J., Szalay, A., and Turner, M. (1982). Formation of Galaxies in a Gravitino-Dominated Universe. Phys. Rev. Lett., 48, pp. 16369.Google Scholar
Blumenthal, G, Pagels, H, and Primack, J (1982). Galaxy Formation by Dissipationless Particles Heavier than Neutrinos, Nature, 299, pp. 378.Google Scholar
Peebles, P. (1982). Large-Scale Background Temperature and Mass Fluctuations Due to Scale-Invariant Primeval Perturbations. Astrophys. J., 263, pp. L1L5.Google Scholar
Centrella, J. and Melott, A. 1983 Three-Dimensional Simulation of Large-Scale Structure in the Universe. Nature, vol. 305, pp. 1968.Google Scholar
Klypin, A. and Shandarin, S. (1983). Three-Dimensional Numerical Model of the Formation of Large-Scale Structure in the Universe. Mon. Not. Royal Astron. Soc., 204, pp. 891907.Google Scholar
Melott, A., Einasto, J., Saar, E., Suisalu, I., Klypin, A., and Shandarin, S. (1983). Cluster Analysis of the Non-Linear Evolution of Large-Scale Structure in an Axion/Gravitino/Photino Dominated Universe. Phys. Rev. Lett., 51, pp. 9358.Google Scholar
Kaiser, N (1984). On the Spatial Correlations of Abell Clusters. Astrophys. J., 284, pp. L9L12.Google Scholar
Blumenthal, G., Faber, S., Primack, J., and Rees, M. (1984). Formation of Galaxies and Large-Scale Structure with Cold Dark Matter. Nature, 311, pp. 51725.Google Scholar
Davis, M., Efstathiou, G., Frenk, C., and White, S. (1985). The Evolution of Large-Scale Structure in a Universe Dominated by Cold Dark Matter. Astrophys. J., 292, pp. 37194.Google Scholar
White, S., Frenk, C., Davis, M., and Efstathiou, G. (1987). Clusters, Filaments, and Voids in a Universe Dominated by Cold Dark Matter. Astrophys. J., 313, pp. 50516.Google Scholar
Beacom, J., Dominik, K., Melott, A., Perkins, S., and Shandarin, S. (1991). Gravitational Clustering in the Expanding Universe: Controlled High-Resolution Studies in Two Dimensions. Astrophys. J., 372, pp. 351363.Google Scholar
Bond, J., Kofman, L., and Pogosyan, D. (1996). How Filaments are Woven into the Cosmic Web. Nature, 380, pp. 6036.Google Scholar

Save book to Kindle

To save this book to your Kindle, first ensure [email protected] is added to your Approved Personal Document E-mail List under your Personal Document Settings on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part of your Kindle email address below. Find out more about saving to your Kindle.

Note you can select to save to either the @free.kindle.com or @kindle.com variations. ‘@free.kindle.com’ emails are free but can only be saved to your device when it is connected to wi-fi. ‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.

Find out more about the Kindle Personal Document Service.

Available formats
×

Save book to Dropbox

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Dropbox.

Available formats
×

Save book to Google Drive

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Google Drive.

Available formats
×