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Marco Scodeggio - Publications

Affiliations: 
1997 Cornell University, Ithaca, NY, United States 
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6 high-probability publications. We are testing a new system for linking publications to authors. You can help! If you notice any inaccuracies, please sign in and mark papers as correct or incorrect matches. If you identify any major omissions or other inaccuracies in the publication list, please let us know.

Year Citation  Score
2008 Guzzo L, Pierleoni M, Meneux B, Branchini E, Le Fèvre O, Marinoni C, Garilli B, Blaizot J, De Lucia G, Pollo A, McCracken HJ, Bottini D, Le Brun V, Maccagni D, Picat JP, ... ... Scodeggio M, et al. A test of the nature of cosmic acceleration using galaxy redshift distortions. Nature. 451: 541-4. PMID 18235494 DOI: 10.1038/Nature06555  0.351
2005 Le Fèvre O, Paltani S, Arnouts S, Charlot S, Foucaud S, Ilbert O, McCracken HJ, Zamorani G, Bottini D, Garilli B, Le Brun V, Maccagni D, Picat JP, Scaramella R, Scodeggio M, et al. A large population of galaxies 9 to 12 billion years back in the history of the Universe. Nature. 437: 519-21. PMID 16177783 DOI: 10.1038/Nature03979  0.366
2001 Scodeggio M. Astronomy. Toward resolving the mystery of galaxy formation. Science (New York, N.Y.). 294: 537-8. PMID 11641488 DOI: 10.1126/science.1065709  0.356
1998 Scodeggio M, Giovanelli R, Haynes MP. The universality of the fundamental plane of E and S0 galaxies: Sample definition and I-band photometric data Astronomical Journal. 116: 2728-2737. DOI: 10.1086/300639  0.568
1998 Dale DA, Giovanelli R, Haynes MP, Scodeggio M, Hardy E, Campusano LE. Seeking the local convergence depth. II. Tully-Fisher observations of the clusters A114, A119, A194, A2295, A2457, A2806, A3193, A3381, and A3744 Astronomical Journal. 115: 418-435. DOI: 10.1086/300229  0.573
1997 Dale DA, Giovanelli R, Haynes MP, Scodeggio M, Hardy E, Campusano LE. Seeking the local convergence depth. I. Tully-Fisher observations of the clusters A168, A397, A569, A1139, A1228, and A1983 Astronomical Journal. 114: 455-473. DOI: 10.1086/118486  0.599
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