Publications [#66705] of Jeffrey L. Krolik

Papers Published

1. Stoughton, C. and Lupton, R.H. and Bernardi, M. and Blanton, M.R. and Burles, S. and Castander, F.J. and Connolly, A.J. and Eisenstein, D.J. and Frieman, J.A. and Hennessy, G.S. and Hindsley, R.B. and Ivezic, E. and Kent, S. and Kunszt, P.Z. and Lee, B.C. and Meiksin, A. and Munn, J.A. and Newberg, H.J. and Nichol, R.C. and Nicinski, T. and Pier, J.R. and Richards, G.T. and Richmond, M.W. and Schlegel, D.J. and Allyn Smith, J. and Strauss, M.A. and SubbaRao, M. and Szalay, A.S. and Thakar, A.R. and Tucker, D.L. and Vanden Berk, D.E. and Yanny, B. and Adelman, J.K. and Anderson, J.E., Jr. and Anderson, S.F. and Annis, J. and Bahcall, N.A. and Bakken, J.A. and Bartelmann, M. and Bastian, S. and Bauer, A. and Berman, E. and Bohringer, H. and Boroski, W.N. and Bracker, S. and Briegel, C. and Briggs, J.W. and Brinkmann, J. and Brunner, R. and Carey, L. and Carr, M.A. and Bing Chen and Christian, D. and Colestock, P.L. and Crocker, J.H. and Csabai, I. and Czarapata, P.C. and Dalcanton, J. and Davidsen, A.F. and Davis, J.E. and Dehnen, W. and Dodelson, S. and Doi, M. and Dombeck, T. and Donahue, M. and Ellman, N. and Elms, B.R. and Evans, M.L. and Eyer, L. and Xiaohui Fan and Federwitz, G.R. and Friedman, S. and Fukugita, M. and Gal, R. and Gillespie, B. and Glazebrook, K. and Gray, J. and Grebel, E.K. and Greenawalt, B. and Greene, G. and Gunn, J.E. and De Haas, E. and Haiman, Z.N. and Haldeman, M. and Hall, P.B. and Hamabe, M. and Hansen, B. and Harris, F.H. and Harris, H. and Harvanek, M. and Hawley, S.L. and Hayes, J.J.E. and Heckman, T.M. and Helmi, A. and Henden, A. and Hogan, C.J. and Hogg, D.W. and Holmgren, D.J. and Holtzman, J. and Chih-Hao Huang and Hull, C. and Ichikawa, S.I. and Ichikawa, T. and Johnston, D.E. and Kauffmann, G. and Kim, R.S.J. and Kimball, T. and Kinney, E. and Klaene, M. and Kleinman, S.J. and Klypin, A. and Knapp, G.R. and Korienek, J. and Krolik, J. and Kron, R.G. and Krzesinski, J. and Lamb, D.Q. and French Leger, R. and Limmongkol, S. and Lindenmeyer, C. and Long, D.C. and Loomis, C. and Loveday, J. and MacKinnon, B. and Mannery, E.J. and Mantsch, P.M. and Margon, B. and McGehee, P. and McKay, T.A. and McLean, B. and Menou, K. and Merelli, A. and Mo, H.J. and Monet, D.G. and Nakamura, O. and Narayanan, V.K. and Nash, T. and Neilsen, E.H., Jr. and Newman, P.R. and Nitta, A. and Odenkirchen, M. and Okada, N. and Okamura, S. and Ostriker, J.P. and Russell, O. and Pauls, A.G. and Peoples, J. and Peterson, R.S. and Petravick, D. and Pope, A. and Pordes, R. and Postman, M. and Prosapio, A. and Quinn, T.R. and Rechenmacher, R. and Rivetta, C.H. and Rix, H.-W. and Rockosi, C.M. and Rosner, R. and Ruthmansdorfer, K. and Sandford, D. and Schneider, D.P. and Scranton, R. and Sekiguchi, M. and Sergey, G. and Sheth, R. and Shimasaku, K. and Smee, S. and Snedden, S.A. and Stebbins, A. and Stubbs, C. and Szapudi, I. and Szkody, P. and Szokoly, G.P. and Tabachnik, S. and Tsvetanov, Z. and Uomoto, A. and Vogeley, M.S. and Voges, W. and Waddell, P. and Walterbos, R. and Shu-I Wang and Watanabe, M. and Weinberg, D.H. and White, R.L. and White, S.D.M. and Wilhite, B. and Wolfe, D. and Yasuda, N. and York, D.G. and Zehavi, I. and Wei Zheng, Sloan Digital Sky Survey: early data release, Astron. J. (USA), vol. 123 no. 1 (2002), pp. 485 - 548 [324741]
   (last updated on 2007/04/16)

   Abstract:
   The Sloan Digital Sky Survey (SDSS) is an imaging and spectroscopic survey that will eventually cover approximately one-quarter of the celestial sphere and collect spectra of ≈10⁶ galaxies, 100000 quasars, 30000 stars, and 30000 serendipity targets. In 2001 June, the SDSS released to the general astronomical community its early data release, roughly 462 deg² of imaging data including almost 14 million detected objects and 54008 follow-up spectra. The imaging data were collected in drift-scan mode in five bandpasses (u, g, r, i, and z); the 95% completeness limits for stars are 22.0, 22.2, 22.2, 21.3, and 20.5, respectively. The photometric calibration is reproducible to 5%, 3%, 3%, 3%, and 5%, respectively. The spectra are flux- and wavelength-calibrated, with 4096 pixels from 3800 to 9200 Å at R≈1800. The authors present the means by which these data are distributed to the astronomical community, descriptions of the hardware used to obtain the data, the software used for processing the data, the measured quantities for each observed object, and an overview of the properties of this data set

   Keywords:
   astronomical catalogues;astronomical photometry;astronomical spectra;galaxies;quasars;stars;stellar photometry;stellar spectra;