Results 1 to 10 of about 5,019,889 (353)
Cosmological 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 +8 more sourcesExtreme 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 +7 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 sourcesGamma-Ray Bursts as Distance Indicators by a Statistical Learning Approach [PDF]
The Astrophysical Journal LettersGamma-ray bursts (GRBs) can be probes of the early Universe, but currently, only 26% of GRBs observed by the Neil Gehrels Swift Observatory have known redshifts ( z ) due to observational limitations.Maria Giovanna Dainotti, Aditya Narendra, Agnieszka Pollo, Vahé Petrosian, Malgorzata Bogdan, Kazunari Iwasaki, Jason Xavier Prochaska, Enrico Rinaldi, David Zhou +8 moredoaj +2 more sourcesK-band versus I-band Surface Brightness Fluctuations as distance
indicators [PDF]
, 2001 We evaluate the method of optical and infrared Surface Brightness
Fluctuations (SBF) as a distance indicator and its application on 8-m class
telescopes, such as the Very Large Telescope (VLT).Ajhar, Bertin, Blakeslee, Blakeslee, Bruzual, Buzzoni, Charlot, Cowie, D. R. Silva, Elston, Feast, Ferrarese, Fluks, Freedman, Freedman, Grillmair, Gunn, Harris, Jensen, Jensen, Jensen, Kauffmann, Lauer, Lejeune, Liu, Luppino, Mei, Mei, P. J. Quinn, Pahre, Pahre, Persson, S. Mei, Silva, Smail, Sodemann, Sodemann, Thomsen, Tonry, Tonry, Tonry, Tonry, Tonry, Worthey, Worthey +44 morecore +4 more sourcesSALT2: using distant supernovae to improve the use of type Ia supernovae as distance indicators [PDF]
, 2007 We present an empirical model of Type Ia supernovae spectro-photometric evolution with time. The model is built using a large data set including light-curves and spectra of both nearby and distant supernovae, the latter being observed by the SNLS ...J. Guy, P. Astier, S. Baumont, D. Hardin, R. Pain, N. Regnault, S. Basa, R. G. Carlberg, A. Conley, S. Fabbro, D. Fouchez, I. M. Hook, D. A. Howell, K. Perrett, C. J. Pritchet, J. Rich, M. Sullivan, P. Antilogus, E. Aubourg, G. Bazin, J. Bronder, M. Filiol, N. Palanque-Delabrouille, P. Ripoche, V. Ruhlmann-Kleider +24 moreopenalex +3 more sourcesAstronomical Distance Determination in the Space Age: Secondary Distance Indicators [PDF]
, 2018 The formal division of the distance indicators into primary and secondary leads to difficulties in description of methods which can actually be used in two ways: with, and without the support of the other methods for scaling.A. Cavaliere, A. Conley, A. Conley, A. Cucchiara, A. Dressler, A. Einstein, A. Einstein, A. Einstein, A. Gal-Yam, A. Goobar, A. Goobar, A. Heger, A. Królak, A. Sternberg, A.D. Code, A.G. Riess, A.G. Riess, A.G. Riess, A.G. Riess, A.G. Riess, A.G. Riess, A.G. Riess, A.G. Riess, A.G. Riess, A.G. Riess, A.G. Riess, A.G. Riess, A.J. Barth, A.J. Monson, A.J. Ruiter, A.L. Argon, A.L. King, A.L. King, A.M. Cherepashchuk, A.M. Hopkins, A.M. Ritchey, A.P.S. Crotts, A.P.S. Crotts, A.T. Steffen, A.V. Filippenko, A.V. Filippenko, A.V. Tutukov, B. Czerny, B. Czerny, B. Paczynski, B. Sathyaprakash, B. Wang, B. Wang, B.E. Schaefer, B.E. Schaefer, B.F. Schutz, B.F. Schutz, B.F. Schutz, B.J. Shappee, B.J. Shappee, B.J. Shappee, B.M. Peterson, B.M. Peterson, B.M. Peterson, B.M. Peterson, B.P. Abbott, B.P. Abbott, B.P. Abbott, B.P. Abbott, B.P. Abbott, B.P. Abbott, B.P. Abbott, B.P. Abbott, B.P. Abbott, B.P. Schmidt, B.P. Schmidt, Bożena Czerny, C. Barbarino, C. Gea, C.B. D’Andrea, C.L. MacLeod, C.M. Gaskell, C.P. Ma, C.R. Burns, C.R. Burns, D. Chelouche, D. Chelouche, D. García-Senz, D. Grupe, D. Ilić, D. Jack, D. Kasen, D. Kasen, D. Kasen, D. Kea, D. Maoz, D. Maoz, D. Maoz, D. Poznanski, D. Rubin, D. Watson, D.A. Coulter, D.A. Howell, D.A. Starkey, D.C. Leonard, D.C. Leonard, D.E. Holz, D.J. Schlegel, D.M. Scolnic, D.O. Jones, D.O. Jones, D.W. Just, E. Baron, E. Berger, E. Cappellaro, E. da Cunha, E. De Filippis, E. Lusso, E. Lusso, E.D. Reese, E.E.E. Gall, E.F. Olivares, E.F. Schlafly, E.K. Grassberg, E.L. Fitzpatrick, E.M. Cackett, E.M.L. Humphreys, Edward Cackett, Elisabeta Lusso, F. Acernese, F. Hoyle, F. La Franca, F. Patat, F. Patat, F. Thim, F. Vagnetti, F. van Leeuwen, F.A.E. Pirani, F.K. Röpke, F.Y. Wang, F.Y. Wang, G. Fiorentino, G. Folatelli, G. Hosseinzadeh, G. Miknaitis, G. Nelemans, G. Pietrzyński, G. Risaliti, G. Weigelt, G. Zamorani, Guido Risaliti, H. Bondi, H. Shapley, H. Tananbaum, I. Hachisu, I. Hachisu, I. Hachisu, I. Robinson, I. Steer, I. Wanders, I.I. Litvinova, I.M. Hook, I.M. McHardy, I.M.H. Etherington, I.P. Pskovskii, I.S. Jang, J. Aasi, J. Braatz, J. Gao, J. Guy, J. Guy, J. Hjorth, J. Modzelewska, J. Parrent, J. Polshaw, J. Polshaw, J. Tonry, J. Whelan, J.A. Cardelli, J.A. Frieman, J.B. Jensen, J.C. Wheeler, J.E. Carlstrom, J.E. O’Donnell, J.J. Walmswell, J.L. Tonry, J.M. Wang, J.P. Anderson, J.P. Blakeslee, J.P. Blakeslee, J.P. Uzan, J.R. Herrnstein, J.S.W. Claeys, J.W. Sulentic, Joseph B. Jensen, K. Hryniewicz, K. Ichikawa, K. Krisciunas, K. Krisciunas, K. Lepo, K. Maeda, K. Maeda, K. Maguire, K. Nomoto, K.J. Shen, K.S. Kawabata, K.S. Mandel, K.T. Korista, K.Y. Lo, L. Bildsten, L. Chomiuk, L. Cortese, L. Piersanti, L. Wang, L.C. Ho, L.P. Singer, M. Bartelmann, M. Betoule, M. Birkinshaw, M. Bonamente, M. Chevallier, M. Dall’Ora, M. della Valle, M. Elitzur, M. Elvis, M. Foley, M. Gierliński, M. Gilfanov, M. Haas, M. Hamuy, M. Hamuy, M. Hamuy, M. Hamuy, M. Hicken, M. Kishimoto, M. Miyoshi, M. Nikolajuk, M. Rigault, M. Rigault, M. Sasdelli, M. Sereno, M. Stritzinger, M. Sullivan, M. Sullivan, M. Young, M.A. Abramowicz, M.C. Bentz, M.C. Bentz, M.C. Bentz, M.C. Bentz, M.C.P. Bours, M.G. Dainotti, M.L. Graham, M.L. Pumo, M.M. Fausnaugh, M.M. Fausnaugh, M.M. Phillips, M.M. Phillips, M.M. Phillips, M.M. Phillips, M.T.B. Nielsen, M.T.B. Nielsen, Massimo Dall’Ora, Maurizio Salaris, Michał Bejger, N. Chotard, N. Dalal, N. Elias-Rosa, N. Elias-Rosa, N. Itoh, N. Ivanova, N. Suzuki, N.I. Shakura, N.R. Tanvir, O. Yaron, O.C. Wilson, P. Du, P. Du, P. Du, P. Galianni, P. Lesaffre, P. Lira, P. Massey, P. Massey, P. Nugent, P. Ruiz-Lapuente, P.A.R. Ade, P.J. Brown, P.J. Brown, P.M. Dos Santos, R. Amanullah, R. Amanullah, R. Antonucci, R. Barvainis, R. Di Stefano, R. Di Stefano, R. Edelson, R. F. L. Holanda, R. Minkowski, R. Nair, R. Pakmor, R. Pakmor, R. Tripp, R.A. Edelson, R.A. Sunyaev, R.B. Tully, R.C. Mitchell, R.D. Blandford, R.F.L. Holanda, R.F.L. Holanda, R.F.L. Holanda, R.F.L. Holanda, R.F.L. Holanda, R.F.L. Holanda, R.J. Foley, R.J. Foley, R.J. Foley, R.J. Foley, R.J. Foley, R.N. Lang, R.P. Kirshner, Rachael Beaton, S. Blondin, S. Bose, S. Collier, S. Collier, S. Hilbert, S. Jha, S. Jha, S. Justham, S. Kaspi, S. Kaspi, S. Koshida, S. Koshida, S. Mateos, S. Mei, S. Nissanke, S. Perlmutter, S. Perlmutter, S. Perlmutter, S. Perlmutter, S. Perlmutter, S.E. Woosley, S.E. Woosley, S.F. Hönig, S.G. Sergeev, S.I. Blinnikov, S.J. Collier, S.J. Smartt, S.J. Smartt, S.M. Faber, Saurabh W. Jha, Silvia Toonen, T. de Jaeger, T. de Jaeger, T. Matheson, T.A. Davis, T.A. Weaver, T.E. Woods, T.W.S. Holoien, T.W.S. Holoien, T.W.S. Holoien, Takeo Minezaki, V.L. Oknyanskij, V.P. Utrobin, W. Baade, W. Li, W. Li, W.E. Kerzendorf, W.L. Freedman, W.L. Freedman, W.L. Freedman, W.L. Freedman, W.L. Freedman, W.M. Wood-Vasey, X. Wang, X. Wang, X. Yang, Y. Andrillat, Y. Aso, Y. Avni, Y. Kobayashi, Y. Shen, Y. Yang, Y. Yoshii, Y. Yoshii, Yuzuru Yoshii, Z. Li +382 morecore +6 more sourcesType II supernovae as distance indicators at near-IR wavelengths [PDF]
Monthly notices of the Royal Astronomical Society, 2018 Motivated by the advantages of observing at near-IR wavelengths, we investigate Type II supernovae (SNe II) as distance indicators at those wavelengths through the Photospheric Magnitude Method (PMM).Ósmar Rodríguez, G. Pignata, M. Hamuy, A. Clocchiatti, M. M. Phillips, K. Krisciunas, N. Morrell, G. Folatelli, M. Roth, S. Castellón, In Sung Jang, Y. Apostolovski, P. López, S. Marchi, Ricardo Ramírez, P. Sanchéz-Sáez +15 moreopenalex +3 more sources
