Results 11 to 20 of about 1,047,569 (316)
Extreme Quasars as Distance Indicators in Cosmology [PDF]
Frontiers in Astronomy and Space Sciences, 2020 Quasars accreting matter at very high rates (known as extreme Population A [xA] quasars, possibly associated with super-Eddington accreting massive black holes) may provide a new class of distance indicators covering cosmic epochs from present day up to ...Deborah Dultzin, Paola Marziani, J. A. de Diego, C. A. Negrete, Ascensión Del Olmo, Mary L. Martínez-Aldama, Mary L. Martínez-Aldama, Mauro D'Onofrio, Edi Bon, Natasa Bon, Giovanna M. Stirpe +10 moredoaj +6 more sourcesCosmological distance indicators [PDF]
Space Science Reviews, 2018 We review three distance measurement techniques beyond the local universe:
(1) gravitational lens time delays, (2) baryon acoustic oscillation (BAO), and
(3) HI intensity mapping.A. Agnello, A. Eigenbrod, A. Goobar, A. Hojjati, A. Hojjati, A. More, A. Oscoz, A.G. Riess, A.M. Martin, A.S. Tagore, B.J. Brewer, C. Alcock, C. Grillo, C. Hazard, C. McCully, C. Vanderriest, C. Vuissoz, C. Vuissoz, C.D. Fassnacht, C.D. Fassnacht, C.D. Fassnacht, C.E. Rusu, C.L. Bennett, C.S. Kochanek, C.S. Kochanek, C.W. Morgan, D. Paraficz, D. Sluse, D. Walsh, D.A. Goldstein, D.A. Goldstein, D.H. Weinberg, D.J. Eisenstein, D.J. Eisenstein, E. Eulaers, E. Giannini, E. Jullo, E.E. Falco, E.O. Ofek, E.R. Switzer, F. Courbin, F. Courbin, F. Courbin, F.B. Abdalla, G. Dobler, G. Dobler, G. Efstathiou, G. Golse, G.C.F. Chen, H. Lin, H.J. Seo, H.J. Seo, I. Burud, I. Burud, I. Burud, I. Jee, I. Momcheva, J. Fohlmeister, J. Fohlmeister, J. Hjorth, J. Huchra, J. Lehar, J.R. Shaw, J.R. Shaw, J.W. Nightingale, K. Bandura, K. Liao, K.C. Wong, K.S. Dawson, K.W. Masui, K.W. Masui, L. Amendola, L. Anderson, L. Oldham, L.B. Newburgh, L.J. Hainline, L.L.R. Williams, L.V.E. Koopmans, L.V.E. Koopmans, L.V.E. Koopmans, L.V.E. Koopmans, M. Barnabè, M. Barnabè, M. Cappellari, M. Jauzac, M. Oguri, M. Oguri, M. Oguri, M. Schmidt, M. Sereno, M. Takada, M. Tegmark, M. Tegmark, M. Tewes, M. Tewes, M.A. Zwaan, M.J. Drinkwater, N. Cantale, N. Kaiser, N.A. Grogin, O. Wucknitz, P. Bull, P. Jakobsson, P. Magain, P. Magain, P. Saha, P. Schneider, P. Schneider, P. Schneider, P. Schneider, P. Young, P.A.R. Ade, P.J. Marshall, P.J.E. Peebles, P.L. Kelly, P.L. Kelly, P.L. Kelly, P.L. Schechter, R. Adam, R. Barkana, R. Blandford, R. Blandford, R. Fadely, R. Gavazzi, R. Kawamata, R. Kormann, R.B. Wayth, S. Birrer, S. Cole, S. Dye, S. Hilbert, S. Rathna Kumar, S. Rathna Kumar, S. Refsdal, S. Vegetti, S. Wallington, S. Wyithe, S.A. Rodney, S.H. Suyu, S.H. Suyu, S.H. Suyu, S.H. Suyu, S.H. Suyu, S.H. Suyu, S.H. Suyu, S.H. Suyu, S.J. Warren, S.S. Tie, T. Kundić, T. Matsubara, T. Okumura, T. Okumura, T. Treu, T.C. Chang, T.C. Chang, T.E. Collett, V. Bonvin, V. Bonvin, V.N. Shalyapin, W. Hu, W.L. Freedman, W.N. Colley, X. Fernández, Y. Xu, Y.W. Liao, Z.S. Greene, É. Aubourg +166 morecore +6 more sourcesYoung and Intermediate-age Distance Indicators [PDF]
Space Science Reviews, 2017 Distance measurements beyond geometrical and semi-geometrical methods, rely
mainly on standard candles. As the name suggests, these objects have known
luminosities by virtue of their intrinsic proprieties and play a major role in
our understanding of ...A. Bhardwaj, A. Bhardwaj, A. Bhardwaj, A. Bressan, A. Gallenne, A. García-Varela, A. Nakagawa, A. Nakagawa, A. Nakagawa, A. Siebert, A. Udalski, A. Udalski, A.A. Cole, A.G. Riess, A.G. Riess, A.J. Cuesta, A.J. Monson, A.J. Monson, A.K. Dambis, A.M. Jacyszyn-Dobrzeniecka, B. Aringer, B. Paczyński, B. Schölkopf, B. Sesar, B. Westerlund, B. Zhang, B.F. Madore, B.L. Tatton, C. Alcock, C. Dvorkin, C. Min, C. Ngeow, C. Ngeow, C. Wegg, C.-C. Ngeow, C.-C. Ngeow, C.-C. Ngeow, C.-C. Ngeow, C.A. Haniff, C.D. Laney, C.D. Laney, C.G. Román-Zúñiga, C.W. McAlary, D. Graczyk, D. Huber, D. Minniti, D. Nyu, D. Stello, D. Stello, D.E. Knuth, D.J. Marshall, D.L. Nidever, E. Hubble, E. Kapakos, E. Puzeras, E.F. Schlafly, E.P. Hubble, ESA, F. Caputo, F. Leeuwen van, F. Leeuwen van, F. Leeuwen van, G. Bono, G. Bono, G. Bono, G. Bono, G. Bono, G. Fiorentino, G. Fiorentino, G. Marchi De, G. Pietrzyński, G. Pietrzyński, G. Pietrzyński, G.A. Tammann, G.F. Benedict, G.G. Fazio, G.H. Rieke, G.H. Rieke, G.M. Green, G.P. Benedetto di, G.R. Ricker, H. Kobayashi, H. Nakanishi, H. Rauer, H.-B. Yuan, H.R. Neilson, H.S. Leavitt, I. Soszyński, I. Soszyński, I. Soszyński, J. Bovy, J. Storm, J. Storm, J. Storm, J.-J. Ren, J.A. Cardelli, J.A. Rich, J.F. Koerwer, J.P. Beaulieu, J.P. Gardner, K. Fricke, K. Kusuno, K.A.G. Olsen, K.M. Flaherty, K.Z. Stanek, K.Z. Stanek, Kh.S. Rezaei, L. Girardi, L. Girardi, L. Girardi, L. Girardi, L. Inno, L. Inno, L. Inno, L.D. Matthews, L.D. Matthews, L.M. Macri, M. Marconi, M. Marconi, M. Marengo, M. Marengo, M. Marengo, M. Marengo, M. Romaniello, M. Salaris, M. Shintani, M. Wyman, M.-R.L. Cioni, M.A.C. Perryman, M.E.K. Williams, M.H. Pinsonneault, M.L. McCall, M.M. Phillips, M.S. Xiang, M.W. Feast, M.W. Feast, M.W. Feast, M.W. Werner, N. Kawaguchi, N. Matsunaga, N. Matsunaga, N. Matsunaga, N. Zacharias, N.E. Evans, N.L. Chapman, N.R. Evans, N.R. Simon, O. Bienaymé, O. Pejcha, O.L. Creevey, P. Barmby, P. Fouque, P. Fouqué, P. Kervella, P. Kervella, P. Whitelock, P.R. Wood, Planck Collaboration, R. Grijs de, R. Grijs de, R. Haschke, R. Haschke, R. Indebetouw, R. Kamohara, R.C. Kennicutt Jr., R.D. Cannon, R.E. Luck, R.I. Anderson, R.I. Anderson, R.M. Cutri, R.P. Martin, R.V. Jones, S. Bergh van den, S. Bilir, S. Kanbur, S. Nishiyama, S. Roeser, S. Rubele, S. Subramanian, S. Subramanian, S. Subramanian, S. Subramanian, S. Subramanian, S.C. Keller, S.D. Friedman, S.E. Persson, S.M. Andrievsky, T. Kamezaki, T. Kamezaki, T. Kamezaki, T. Kamezaki, T. Kurayama, T.G. Barnes, V. Ripepi, V. Scowcroft, V. Scowcroft, V. Scowcroft, V.M.R. Muggeo, V.R.M. Muggeo, W. Dehnen, W.H.T. Vlemmings, W.H.T. Vlemmings, W.L. Freedman, W.L. Freedman, W.L. Freedman, W.L. Freedman, W.L. Freedman, X.-W. Liu, Y. Asaki, Y. Huang, Y. Huang, Y. Ita, Y.K. Choi +212 morecore +5 more sourcesLocal Distance Indicators [PDF]
Symposium - International Astronomical Union, 2000 A summary is given of the calibration of the Cepheid scale required in the derivation of distances from observations at V and I, as in the HST work on extragalactic Cepheids. There is some evidence that a small metallicity correction may be necessary in deriving distances in this way.M. W. Feastopenalex +5 more sourcesMattig's relation and dynamical distance indicators [PDF]
Astronomische Nachrichten, 2016 AbstractWe discuss how the redshift (Mattig) method in the Friedmann cosmology relates to dynamical distance indicators based on Newton's gravity (Teerikorpi 2011). It belongs to the class of indicators where the relevant length inside the system is the distance itself (in this case the proper metric distance).P. Teerikorpi, Yu. V. Baryshevopenalex +7 more sourcesCEPHEIDS AS DISTANCE INDICATORS: SOME CURRENT PROBLEMS
Odessa Astronomical Publications, 2017 A general review is given of the calibration of the Cepheid distance scale, with particular reference to its use in the determination of H0. Emphasis is placed on the advantage of using a galactic calibration of the Cepheid scale, rather than relying on ...M. Feastdoaj +1 more source