Results 31 to 40 of about 66,413 (243)
Hydra — Centaurus: A Redshift Survey [PDF]
Symposium - International Astronomical Union, 1988 The survey consists of 2 samples : SAMPLE A, 85% complete to B(T) = 14.0 in the region between 10 and 14 Hours in R.A. and between −20 and −50 degrees in DEC., SAMPLE B, complete to B(0) = 14.5 in two regions one between R.A. 13 and 14 hours, DEC between −25 and −33, the other between 11 and 12 hours, DEC from −33 to −27.G Chincarini, L da Costa, A.P. Fairall, P Pellegrini, G Vettolani, C Willmer +5 moreopenaire +1 more sourceThe SSA22 H i Tomography Survey (SSA22-HIT). I. Data Set and Compiled Redshift Catalog
The Astronomical Journal, 2023 We conducted a deep spectroscopic survey, named SSA22-HIT, in the SSA22 field with the DEep Imaging MultiObject Spectrograph (DEIMOS) on the Keck telescope, designed to tomographically map high- z H i gas through analysis of Ly α absorption in background Ken Mawatari, Akio K. Inoue, Toru Yamada, Tomoki Hayashino, J. Xavier Prochaska, Khee-Gan Lee, Nicolas Tejos, Nobunari Kashikawa, Takuya Otsuka, Satoshi Yamanaka, David J. Schlegel, Yuichi Matsuda, Joseph F. Hennawi, Ikuru Iwata, Hideki Umehata, Shiro Mukae, Masami Ouchi, Yuma Sugahara, Yoichi Tamura +18 moredoaj +1 more sourceThe 2Mass Redshift Survey [PDF]
Highlights of Astronomy, 1998 With the current convergence of determinations of the Hubble Constant (e.g. The Extragalactic Distance Scale, 1997, Livio, Donahue and Panagia, eds.) to values within ±25% rather than a factor of two, and the clear possibility of determining q0 using high redshift supernovae (Garnavich et al.J. Huchra, E. Tollestrup, S. Schneider, M. Skrutski, T. Jarrett, T. Chester, R. Cutri +6 moreopenaire +1 more sourceSpectral Templates from Multicolor Redshift Surveys [PDF]
, 1999 Understanding how the physical properties of galaxies (e.g. their spectral
type or age) evolve as a function of redshift relies on having an accurate
representation of galaxy spectral energy distributions.Alexander S. Szalay, Andrew J. Connolly, Baum W. A., Everson R., Hogg D. W., István Csabai, Karhunen H., Koo D. C., Mark Dickinson, Tamás Budavári +9 morecore +4 more sourcesThe effects of spatial resolution on Integral Field Spectrograph surveys
at different redshifts. The CALIFA perspective [PDF]
, 2013 Over the past decade, 3D optical spectroscopy has become the preferred tool
for understanding the properties of galaxies and is now increasingly used to
carry out galaxy surveys. Low redshift surveys include SAURON, DiskMass,
ATLAS3D, PINGS and VENGA. At Aguerri, J. A. L., Bekeraite, S., Bland-Hawthorn, J., Bomans, D. J., de Lorenzo-Caceres, A., del Olmo, A., Falcon-Barroso, J., Galbany, L., García-Lorenzo, B., Husemann, B., Iglesias-Paramo, J., Kehrig, C., Kennicutt, R. C., Lopez-Sanchez, A. R., Marino, R. A., Marmol-Queralto, E., Marquez, I., Mast, D., Mendez-Abreu, J., Monreal-Ibero, A., Papaderos, P., Relano, M., Rosales-Ortega, F. F., Sanchez, S. F., van de Ven, G., Vílchez, J. M., Walcher, C. J., Wild, V., Wisotzki, L., Ziegler, B. +29 morecore +4 more sourcesPhotometric redshifts in the SWIRE Survey [PDF]
Monthly Notices of the Royal Astronomical Society, 2008 22 pages, 23 figures. Accepted for publication in MNRAS. Revised 28/2/08.Rowan-Robinson, Michael, Babbedge, Tom, Oliver, Seb, Trichas, Markos, Berta, Stefano, Lonsdale, Carol, Smith, Gene, Shupe, David, Surace, Jason, Arnouts, Stephane, Ilbert, Olivier, Le Févre, Olivier, Afonso-Luis, Alejandro, Perez-Fournon, Ismael, Hatziminaoglou, Evanthia, Polletta, Mari, Farrah, Duncan, Vaccari, Mattia +17 moreopenaire +6 more sourcesA Redshift Survey of IRAS Galaxies [PDF]
Symposium - International Astronomical Union, 1988 We have completed a redshift survey of approximately 2200 IRAS galaxies, flux limited at 60μ. The survey covers 76% of the sky and has a characteristic depth of ≈ 6000 km s−1, making it ideal for large scale structure studies requiring whole sky coverage.Michael A. Strauss, Marc Davisopenaire +1 more sourceOptical Redshift Surveys [PDF]
Highlights of Astronomy, 1992 Redshift surveys of galaxies have been over the past decade the major source of information for studies of the large-scale structure of the Universe. Following the completion of the original CfA Redshift Survey, several groups have joined the endeavor, probing different regions of the sky to different depths in a remarkable long-term effort to study ...openaire +1 more sourceThe density and peculiar velocity fields of nearby galaxies [PDF]
, 1995 We review the quantitative science that can be and has been done with
redshift and peculiar velocity surveys of galaxies in the nearby universe.
After a brief background setting the cosmological context for this work, the
first part of this review ...Aaronson, Aaronson, Aaronson, Aaronson, Aaronson, Abell, Abell, Adams, Alimi, Andrews, Arnett, Babul, Babul, Babul, Babul, Bagla, Bahcall, Bahcall, Bahcall, Bahcall, Bahcall, Bahcall, Balian, Balkowski, Bardeen, Bardeen, Bartlett, Baugh, Baum, Baumgart, Bean, Bennett, Bernardeau, Bernardeau, Bernardeau, Bernardeau, Bernardeau, Bernstein, Bernstein, Bertschinger, Bertschinger, Bertschinger, Bertschinger, Bertschinger, Bertschinger, Bicay, Bicay, Binggeli, Binney, Blumenthal, Blumenthal, Bond, Bonometto, Borgani, Bothun, Bothun, Bothun, Bothun, Bothun, Bothun, Bothun, Bottinelli, Bottinelli, Bottinelli, Bouchet, Bouchet, Bouchet, Bouchet, Bouchet, Bower, Brainerd, Brainerd, Brainerd, Branchini, Briggs, Broadhurst, Broadhurst, Bunn, Burstein, Burstein, Burstein, Burstein, Bushouse, Börner, Carlberg, Carroll, Carruthers, Cen, Cen, Cen, Cen, Cen, Chaboyer, Charlier, Choloniewski, Choloniewski, Ciardullo, Ciardullo, Ciardullo, Ciardullo, Cole, Cole, Cole, Coleman, Coles, Coles, Coles, Coles, Colless, Colless, Colless, Collins, Colombi, Colombi, Connolly, Corwin, Courteau, Courteau, Cowie, Cowie, da Costa, da Costa, da Costa, Dalcanton, Dalton, Davies, Davis, Davis, Davis, Davis, Davis, Davis, Davis, Davis, Davis, Davis, Davis, Davis, Davis, de Carvalho, de Lapparent, de Lapparent, de Lapparent, de Lapparent, de Lapparent, de Vaucouleurs, de Vaucouleurs, de Vaucouleurs, de Vaucouleurs, Dekel, Dekel, Dekel, Dekel, Dekel, Dekel, Dekel, Deul, Dey, Di Nella, Disney, Djorgovski, Doroshkevich, Doroshkevich, Dressler, Dressler, Dressler, Dressler, Dressler, Dressler, Dressler, Dressler, Dressler, Dressler, Dressler, Dressler, Eder, Efstathiou, Efstathiou, Efstathiou, Efstathiou, Efstathiou, Efstathiou, Einasto, Einasto, Ellis, Fabbri, Faber, Faber, Faber, Faber, Faber, Faber, Faber, Federspiel, Feiten, Feldman, Feldman, Fisher, Fisher, Fisher, Fisher, Fisher, Fisher, Fisher, Fisher, Fisher, Freedman, Freeman, Freudling, Frieman, Fry, Fry, Fry, Fry, Fry, Fry, Fry, Fry, Fukugita, Gaztañaga, Gaztañaga, Gaztañaga, Gaztañaga, Gelb, Gelb, Geller, Geller, Geller, Giavalisco, Giovanelli, Giovanelli, Giovanelli, Giovanelli, Giovanelli, Giovanelli, Gott, Gott, Gould, Gramann, Gramann, Gramann, Gray, Gregg, Gregory, Gregory, Gregory, Groth, Groth, Gudehus, Gunn, Gunn, Gunn, Gunn, Guzmàn, Guzmàn, Guzmàn, Guzzo, Guzzo, Górski, Górski, Górski, Hamilton, Hamilton, Hamilton, Hamilton, Hamilton, Hamilton, Hamuy, Han, Han, Han, Han, Harmon, Harrison, Harrison, Hart, Heavens, Helou, Hinshaw, Hoessel, Hoffman, Hoffman, Hubble, Huchra, Huchra, Huchra, Huchra, Hudson, Hudson, Hudson, Hudson, Hudson, Hudson, Hutchings, Ichikawa, Ikeuchi, Jacoby, Jacoby, Jacoby, Jacoby, Jaffe, Jain, Jeffrey A. Willick, Juszkiewicz, Juszkiewicz, Juszkiewicz, Juszkiewicz, Juszkiewicz, Kahn, Kaiser, Kaiser, Kaiser, Kaiser, Kaiser, Kaiser, Kaiser, Kaiser, Kaiser, Kamionkowski, Kamionkowski, Kashlinsky, Katz, Kerr, Kirshner, Kirshner, Kirshner, Kirshner, Kleinmann, Klypin, Kogut, Kolatt, Kolatt, Kolb, Kormendy, Kraan-Korteweg, Kraan-Korteweg, Kraan-Korteweg, Lahav, Lahav, Lahav, Lahav, Lahav, Lahav, Lahav, Lahav, Lahav, Landy, Landy, Lauberts, Lauberts, Lauer, Lauer, Liddle, Lidsey, Lightman, Lilje, Limber, Lin, Ling, Little, Lonsdale, Loveday, Loveday, Loveday, Lu, Lucchin, Lucey, Lucey, Luppino, Lynden-Bell, Lynden-Bell, Lynden-Bell, Lynden-Bell, Lynden-Bell, Maddox, Maddox, Maddox, Maddox, Makino, Malmquist, Malmquist, Mancinelli, Martel, Marzke, Matarrese, Mathewson, Mathewson, Mathewson, Matsubara, Matsubara, Maurogordato, McGaugh, Meiksin, Meiksin, Michael A. Strauss, Mo, Mo, Mo, Mo, Mo, Moore, Moore, Moscardini, Mould, Mould, Muciaccia, Nicoll, Nilson, Nusser, Nusser, Nusser, Nusser, Oemler, Oort, Osterbrock, Osterbrock, Ostriker, Paczyñski, Padmanabhan, Padmanabhan, Park, Park, Partridge, Paturel, Peacock, Peacock, Peacock, Peacock, Peacock, Peebles, Peebles, Peebles, Peebles, Peebles, Peebles, Peebles, Peebles, Peebles, Peebles, Peebles, Peebles, Peebles, Peebles, Peebles, Peebles, Peebles, Peebles, Peletier, Pellegrini, Pen, Perlmutter, Phillips, Picard, Pierce, Pierce, Pierce, Pierce, Plionis, Postman, Postman, Postman, Postman, Press, Primack, Pskovskii, Pskovskii, Ramella, Regös, Reiss, Renzini, Roth, Roth, Rowan-Robinson, Rowan-Robinson, Rubin, Rubin, Rubin, Rubin, Rubin, Rubin, Rubin, Ryden, Sachs, Saha, Salzer, Salzer, Sandage, Sandage, Sandage, Sandage, Sandage, Sandage, Sandage, Sanders, Santiago, Santiago, Santiago, Santiago, Santiago, Sargent, Sargent, Saslaw, Saunders, Saunders, Saunders, Schaefer, Schaefer, Schaeffer, Scharf, Scharf, Schechter, Schechter, Schechter, Schlegel, Schmidt, Schmidt, Schmidt, Schneider, Schombert, Schombert, Schommer, Scott, Segal, Seldner, Seljak, Shandarin, Shane, Shanks, Shaver, Shaya, Shaya, Shaya, Shectman, Shu, Silk, Silk, Silk, Silk, Simmons, Smoot, Sodré, Soifer, Soifer, Spinoglio, Spinrad, Spinrad, Stebbins, Strauss, Strauss, Strauss, Strauss, Strauss, Strauss, Strauss, Strauss, Strauss, Suto, Suto, Suto, Szalay, Szapudi, Szapudi, Szomoru, Szomoru, Tammann, Taylor, Taylor, Teerikorpi, Teerikorpi, Teerikorpi, Tegmark, Thuan, Toller, Tonry, Tonry, Tonry, Tonry, Tonry, Tonry, Tonry, Tonry, Tonry, Tormen, Tormen, Torres, Triay, Trimble, Tucker, Tully, Tully, Tully, Tully, Tully, Tully, Tully, Tully, Tully, Turner, Turner, Tyson, Valls-Gabaud, Villumsen, Villumsen, Vittorio, Vogeley, Vogeley, Vogeley, Weinberg, Weinberg, Weinberg, Weinberg, Weinberg, Weinberg, Weinberg, Weinberg, Wheeler, White, White, White, White, White, White, White, White, Whitmore, Willick, Willick, Willick, Willick, Wright, Yahil, Yahil, Yahil, Yahil, Yahil, Yamada, Zabludoff, Zaroubi, Zaroubi, Zel'dovich, Zel'dovich, Zurek, Zwicky, Łokas +643 morecore +2 more sources
