Results 11 to 20 of about 983 (58)
The universal shape of the X-ray variability power spectrum of AGN up to z~3 [PDF]
Astronomy & Astrophysics, 2023 We study the ensemble X-ray variability properties of Active Galactic Nuclei (AGN) over a large range of timescales (20 ks $\leq T\leq$ 14 yrs), redshift ($0\leq z \lesssim 3$), luminosities ($10^{40}$ erg s$^{-1}\leq L_X\leq 10^{46}$ erg s$^{-1}$) and ...M. Paolillo, I. Papadakis, W. Brandt, F. Bauer, G. Lanzuisi, V. Allevato, O. Shemmer, X. Zheng, D. D. Cicco, R. Gilli, B. Luo, M. Thomas, P. Tozzi, F. Vito, Y. Q. X. D. D. F. Pancini'', U. Federico, Italy., I. -. Capodimonte, Naples, I. Napoli, D. Physics, Institute of Theoretical, Computational Physics, U. Crete, Heraklion, Greece., Institute of Theoretical Astrophysics, Forth, D. Astronomy, Astrophysics, T. O. S. University, University Park, USA., I. Gravitation, The Cosmos, I. D. Astrof'isica, Centro de Astroingenier'ia, Facultad de F'isica, P. U. C. D. Chile, Santiago, Chile., M. I. O. Astrophysics, Space Telescope Science Institute, Boulder, Colorado., I. Bologna, S. Superiore, Pisa, U. Texas, Denton, L. Observatory, Leiden University, Leiden, The Netherlands., School of Physics Astronomy, S. Science, N. University, China., Key Laboratory of Optical Astronomy, I. Arcetri, Firenze, Cas Key Laboratory for Research in Galaxies, Cosmology, University of Electronic Science, T. China, Hefei, S. Sciences +66 moresemanticscholar +1 more sourceCompleteness of the NASA/IPAC Extragalactic Database (NED) Local Volume Sample [PDF]
Astrophysical Journal Supplement Series, 2023 We introduce the NASA/IPAC Extragalactic Database (NED) Local Volume Sample (NED-LVS), a subset of ∼1.9 million objects with distances out to 1000 Mpc.D. Cook, J. Mazzarella, G. Helou, A. Alcala, T. Chen, R. Ebert, C. Frayer, J. Kim, T. Lo, B. Madore, P. Ogle, M. Schmitz, L. Singer, S. Terek, J. Valladon, X. W. CaltechIPAC, D. O. AstronomyAstrophysics, U. Chicago, Observatories of the Carnegie Institution for Science, Space Telescope Science Institute, NASA's Goddard Space Flight Center, D. Astronomy, San Diego State University, D. PhysicsAstronomy, San Diego State University +24 moresemanticscholar +1 more sourceTransient RFI environment of LOFAR-LBA at 72-75 MHz. Impact on ultra-widefield AARTFAAC Cosmic Explorer observations of the redshifted 21-cm signal [PDF]
Astronomy & Astrophysics, 2023 Measurement of the redshifted 21-cm signal of neutral hydrogen from the Cosmic Dawn (CD) and Epoch of Reionisation (EoR) promises to unveil a wealth of information about the astrophysical processes during the first billion years of evolution of the ...B. Gehlot, L. Koopmans, S. Brackenhoff, E. Ceccotti, S. Ghosh, C.Hofer, Florent Mertens, M. Mevius, S. Munshi, A. Offringa, V. N. Pandey, A. Rowlinson, A. Shulevski, R. Wijers, S. Yatawatta, S. Y. K. A. Institute, U. Groningen, The Netherlands Lerma, Observatoire de Paris, P. university, Cnrs, Sorbonne Universit'e, France, Astron, N. F. F. R. Astronomy, The Netherlands, Anton Pannekoek Institute, U. Amsterdam, D. Sciences, The Open University of Israel, Israel +30 moresemanticscholar +1 more sourceEuclid preparation. XXIX. Water ice in spacecraft. I. The physics of ice formation and contamination [PDF]
Astronomy & Astrophysics, 2023 Molecular contamination is a well-known problem in space flight. Water is the most common contaminant and alters numerous properties of a cryogenic optical system. Too much ice means that Euclid's calibration requirements and science goals cannot be met. Euclid Collaboration M. Schirmer, K. Thurmer, B. Bras, M. Cropper, J. Martín-Fleitas, Y. Goueffon, R. Kohley, A. Mora, M. Portaluppi, G. Racca, A. Short, S. Szmolka, L. Venancio, M. Altmann, Z. Balog, U. Bastian, M. Biermann, D. Busonero, C. Fabricius, F. Grupp, C. Jordi, W. Loffler, A. S. Sell'es, N. Aghanim, A. Amara, L. Amendola, M. Baldi, C. Bodendorf, D. Bonino, E. Branchini, M. Brescia, J. Brinchmann, S. Camera, G. Candini, V. Capobianco, C. Carbone, J. Carretero, M. Castellano, S. Cavuoti, A. Cimatti, R. Clédassou, G. Congedo, C. Conselice, L. Conversi, Y. Copin, L. Corcione, F. Courbin, A. D. Silva, H. Degaudenzi, A. D. Giorgio, J. Dinis, F. Dubath, X. Dupac, S. Dusini, S. Farrens, S. Ferriol, M. Frailis, E. Franceschi, M. Fumana, S. Galeotta, B. Garilli, W. Gillard, B. Gillis, C. Giocoli, S. Haugan, H. Hoekstra, W. Holmes, F. Hormuth, A. Hornstrup, K. Jahnke, S. Kermiche, A. Kiessling, M. Kilbinger, T. Kitching, M. Kunz, H. Kurki-Suonio, S. Ligori, P. Lilje, I. Lloro, E. Maiorano, O. Mansutti, O. Marggraf, K. Markovič, F. Marulli, R. Massey, E. Medinaceli, S. Mei, Y. Mellier, M. Meneghetti, E. Merlin, G. Meylan, Michele Moresco, L. Moscardini, E. Munari, R. Nakajima, S. Niemi, J. Nightingale, T. Nutma, C. Padilla, S. Paltani, F. Pasian, V. Pettorino, S. Pires, G. Polenta, M. Poncet, L. Popa, F. Raison, A. Renzi, J. Rhodes, G. Riccio, E. Romelli, M. Roncarelli, E. Rossetti, R. Saglia, D. Sapone, B. Sartoris, P. Schneider, A. Secroun, G. Seidel, S. Serrano, C. Sirignano, G. Sirri, J. Skottfelt, L. Stanco, P. Tallada-Cresp'i, A. Taylor, I. Tereno, R. Toledo-Moreo, I. Tutusaus, E. Valentijn, L. Valenziano, T. Vassallo, Y. Wang, J. Weller, A. Zacchei, J. Zoubian, S. Andreon, S. Bardelli, P. Battaglia, E. Bozzo, C. Colodro-Conde, M. Farina, J. Graci'a-Carpio, E. Keihanen, V. Lindholm, D. Maino, N. Mauri, N. Morisset, V. Scottez, M. Tenti, E. Zucca, Y. Akrami, C. Baccigalupi, M. Ballardini, A. Biviano, A. Blanchard, A. Borlaff, C. Burigana, R. Cabanac, A. Cappi, C. Carvalho, S. Casas, G. Castignani, T. Castro, K. Chambers, A. Cooray, J. Coupon, H. Courtois, J. Cuby, S. Davini, G. Lucia, G. Desprez, S. Domizio, H. Dole, J. Escartín, S. Escoffier, I. Ferrero, L. Gabarra, K. Ganga, J. García-Bellido, K. George, F. Giacomini, G. Gozaliasl, H. Hildebrandt, J. Kajava, Vanshika Kansal, C. Kirkpatrick, L. Legrand, P. Liebing, A. Loureiro, G. Maggio, M. Magliocchetti, G. Mainetti, R. Maoli, S. Marcin, M. Martinelli, N. Martinet, C. Martins, S. Matthew, M. Maturi, L. Maurin, R. Metcalf, P. Monaco, G. Morgante, S. Nadathur, A. Nucita, L. Patrizii, J. Pollack, V. Popa, D. Potter, M. Pontinen, A. S'anchez, Z. Sakr, A. Schneider, M. Sereno, A. Shulevski, P. Simon, J. Steinwagner, R. Teyssier, J. V. M. F. Astronomie, 17 Konigstuhl, 69117 Heidelberg, Germany, Sandia National Laboratories, Livermore, CA 94550, Usa, European Space AgencyESTEC, 1. Keplerlaan, 2. Noordwijk, The Netherlands., Mullard Space Science Laboratory, U. London, H. Mary, Dorking, Surrey RH5 6NT, Uk, Aurora Technology B.V., 39 Zwarteweg, 2201 AA Noordwijk, Airbus Sas, Toulouse, France, Esacesa, Camino Bajo de Castillo, sn., Urb. Villafranca del Castillo, 28692 Villanueva de la Canada, Madrid, Spain., Aurora Technology for European Space Agency, Camino Bajo de Castillo, sn., Urb. Villafranca del Castillo, Villanueva de la Cañada, 28014 Madrid, A. Rechen-Institut, Zentrum fur Astronomie der Universitat Heidelberg, Monchhofstr. 12--14, 69117 Heidelberg, Syrte, O. Paris, Universit'e Psl, Cnrs, Sorbonne Universit'e, LnE, 6. Paris, I. Torino, 20 viaOsservatorio, 1. P. Torinese, Italy, Institut de Ci'encies del Cosmos, U. Barcelona, 1. Mart'iiFranques, 08193 Barcelona, I. D. E. D. Catalunya, Carrer Gran Capit'a 2-4, 08193 Barcelona, M. F. Physics, 1. Giessenbachstr., 85748 Garching, U. Observatory, F. O. Physics, Ludwig-Maximilians-Universitat, 1. Scheinerstr., 81679 Munich, D. Astrof'isica, E. Barcelona, Universit'e Paris-Saclay, I. D. Spatiale, 91405, Orsay, Institute of Cosmology, Gravitation, U. Portsmouth, PO1 3FX, I. T. Physik, U. Heidelberg, 16 Philosophenweg, D. Bologna, V. G. 932, 40129 Bologna, I. Bologna, V. G. 933, I. Bologna, 62 vialeBertiPichat, 40129 Bologna, D. Fisica, U. Genova, 33 viaDodecaneso, 16146, Genova, I. Genova, Department of PhysicsE. Pancini, U. Federico, 6. ViaCinthia, 80126, Napoli, I. -. Capodimonte, 16 viaMoiariello, 80131 Napoli, I. D. A. E. C. D. Espacco, U. Porto, Caup, Rua das Estrelas, P. Porto, Portugal, U. Torino, 1. ViaP.Giuria, 10125 Torino, I. Torino, Inaf-Iasf Milano, 12 ViaAlfonsoCorti, 20133 Milano, Institut de F'isica d'Altes Energies, T. Z. F. O. Science, Technology, Campus Uab, 08193 Bellaterra, Port d'Informaci'o Cient'ifica, C. Sn, I. Roma, 33 viaFrascati, 00078 Monte Porzio Catone, I. Naples, Centre National d'Etudes Spatiales -- Centre spatial de Toulouse, 14 Avenue Edouard Belin, 9. 31401ToulouseCedex, Institut national de physique nucl'eaire et de physique des particules, 3. R. Michel-Ange, 16 75794ParisC'edex, Institute for Astronomy, U. Edinburgh, R. Observatory, B. Hill, Edinburgh EH9 3HJ, J. B. C. F. Astrophysics, D. Physics, Astronomy, U. Manchester, Oxford Road, M13 9PL, European Space AgencyESRIN, 1. LargoGalileoGalilei, 00044 Frascati, Roma, U. Lyon, 1. UnivClaudeBernardLyon, CNRSIN2p3, I. Lyon, Umr 5822, 69622 Villeurbanne, I. O. Physics, L. O. Astrophysics, E. P. F. Lausanne, Observatoire de Sauverny, 1290 Versoix, Switzerland., D. D. F'isica, F. Ciencias, Universidade de Lisboa, C8 Edif'icio, C. Grande, P. Lisboa, 1049-001 Lisboa, D. O. Astronomy, U. Geneva, 16 ch.d'Ecogia, I. D. A. E. P. Spaziali, V. Cavaliere, 100, 00133 Roma, INFN-Padova, 8. viaMarzolo, 35131 Padova, Universit'e de Paris Cit'e, Cea, Astrophysique, Instrumentation et Mod'elisation Paris-Saclay, 91191 Gif-sur-Yvette, Inaf Trieste, 11 ViaG.B.Tiepolo, 34127 Trieste, A. Universit'e, Cppm, Marseille, Institute of Theoretical Astrophysics, U. Oslo, P. O. B. 1. Blindern, 0315 Oslo, Norway, L. Observatory, Leiden University, 2. NielsBohrweg, 2333 CA Leiden, Jet propulsion Laboratory, C. I. O. Technology., 4800 Oak Grove Drive, Pasadena, Ca, 91109, von Hoerner Sulger GmbH, 8. Schlossplatz, 68723 Schwetzingen, T. Denmark, Elektrovej 327, 2800 Kgs. Lyngby, Denmark, Cosmic Dawn Center, U. Geneve, D'epartement de Physique Th'eorique, Centre for Theoretical Physics, 24 quai Ernest-Ansermet, 4. CH-1211Geneve, 64 P.O.Box, 00014 University of Helsinki, Finland., H. I. O. Physics, 2. GustafHallstrominkatu, U. Helsinki, Helsinki, Nova Optical IR Instrumentation Group at Astron, 4. OudeHoogeveensedijk, 7991PD, Dwingeloo, Argelander Institut fur Astronomie, U. Bonn, 71 AufdemHugel, 53121 Bonn, Institute for Computational Cosmology, D. University, South Road, DH1 3LE, Astroparticule et Cosmologie, 7. Paris, I. Paris, 98 bis boulevard Arago, 75014, París, Umr 7095, 98 bis boulevard Arago, 7. Paris, C. Saclay, Dfrirfu, S. d’Astrophysique, Bat. 709, K. Institute, U. Groningen, PO Box 800, 9700 AV Groningen, Aim, 91191, Gif-sur-Yvette, S. Center, Italian Space Agency, via del Politecnico snc, 00133 Roma, Institute of Space Science, Str. Atomistilor, nr. 409 Muagurele, Ilfov, 077125, România, D. Galilei', U. Padova, D. Astronomia, U. Bologna, V. G. 932, Universitatssternwarte Munchen, F. Physik, Ludwig-Maximilians-Universitat Munchen, 1. Scheinerstrasse, 8. Munchen, Fcfm, U. D. Chile, Blanco Encalada 2008, Santiago, Chile., Institut de Ci'encies de l'Espai, Carrer de Can Magrans +499 moresemanticscholar +1 more sourceX-Ray Detection of the Galaxy’s Missing Baryons in the Circumgalactic Medium of L* Galaxies [PDF]
Astrophysical Journal Letters, 2023 The number of baryons hosted in the disks of galaxies is lower than expected based on the mass of their dark matter halos and the fraction of baryon-to-total matter in the Universe, giving rise to the so-called galaxy missing-baryon problem. The presence F. Nicastro, Y. Krongold, T. Fang, F. Fraternali, S. Mathur, S. Bianchi, A. Rosa, E. Piconcelli, L. Zappacosta, M. Bischetti, C. Feruglio, Anjali Gupta, Zheng Zhou Inaf Osservatorio Astronomico di Roma, Romé, Italy., D. Astronomy, Xiamen University, Xiamen, China., Instituto de Astronomia - Universidad Nacional Autonoma de Mexico, M'exico City, Mexico., K. Institute, University of Gronigen, Gronigen, The Netherlands., A. Department, T. O. S. University, Columbus, Oh, Usa, Center for Cosmology, Astro-particle Physics, D. Fisica, U. Tre, Roma, I. D. A. E. P. Spaziali, I. N. D. A. -. O. A. Trieste, Trieste, D. Fisica, S. Astronomia, Universita di UdineI.N.F.N. Trieste, Columbus State Community College +42 moresemanticscholar +1 more sourceDARWIN – a next-generation liquid xenon observatory for dark matter and neutrino physics [PDF]
International Conference on Rebooting Computing, 2021
The nature of dark matter and properties of neutrinos are among the most pressing issues in contemporary particle physics. The dual-phase xenon time-projection chamber is the leading technology to cover the available parameter space for weakly ...J. Aalbers, K. Abe, V. Aerne, F. Agostini, S. A. Maouloud, D. Akerib, D. Akimov, J. Akshat, A. K. A. Musalhi, F. Alder, S. Alsum, L. Althueser, C. Amarasinghe, F. Amaro, A. Ames, T. Anderson, B. Andrieu, N. Angelides, E. Angelino, J. Angevaare, V. C. Antochi, D. Martin, B. Antunović, E. Aprile, H. Ara'ujo, J. E. Armstrong, F. Arneodo, M. Arthurs, P. Asadi, S. Baek, X. Bai, D. Bajpai, A. Baker, J. Balajthy, S. Balashov, M. Balzer, A. Bandyopadhyay, J. Bang, E. Barberio, J. Bargemann, L. Baudis, D. Bauer, D. Baur, A. Baxter, A. Baxter, M. Bazyk, K. Beattie, J. Behrens, N. Bell, L. Bellagamba, P. Beltrame, M. Benabderrahmane, E. Bernard, G. Bertone, P. Bhattacharjee, A. Bhatti, A. Biekert, T. P. Biesiadzinski, A. R. Binau, R. Biondi, Y. Biondi, H. Birch, F. Bishara, A. Bismark, C. Blanco, G. Blockinger, E. Bodnia, C. Boehm, A. Bolozdynya, P. Bolton, S. Bottaro, C. Bourgeois, B. Boxer, P. Br'as, A. Breskin, P. Breur, C. Brew, J. Brod, E. Brookes, A. Brown, E. Brown, S. Bruenner, G. Bruno, R. Budnik, T. Bui, S. Burdin, S. Buse, J. Busenitz, D. Buttazzo, M. Buuck, A. Buzulutskov, R. Cabrita, C. Cai, D. Cai, C. Capelli, J. Cardoso, M. Carmona-Benitez, M. Cascella, R. Catena, S. Chakraborty, C. Chan, S. Chang, A. Chauvin, A. Chawla, H. Chen, V. Chepel, N. Chott, D. Cichon, A. Chavez, B. Cimmino, M. Clark, R. Co, A. Colijn, J. Conrad, M. Converse, M. Costa, A. Cottle, G. Cox, O. Creaner, J. J. García, J. Cussonneau, J. Cutter, C. Dahl, V. D’Andrea, A. David, M. Decowski, J. Dent, F. Deppisch, L. D. Viveiros, P. Gangi, A. Giovanni, S. D. Pede, J. Dierle, S. Diglio, J. Dobson, M. Doerenkamp, D. Douillet, G. Drexlin, E. Druszkiewicz, D. Dunsky, K. Eitel, A. Elykov, T. Emken, R. Engel, S. R. Eriksen, M. Fairbairn, A. Fan, J. J. Fan, S. Farrell, S. Fayer, N. Fearon, A. Ferella, C. Ferrari, A. Fieguth, S. Fiorucci, H. Fischer, H. Flaecher, M. Flierman, T. Florek, R. Foot, P. J. Fox, R. Franceschini, E. Fraser, C. Frenk, S. Frohlich, T. Fruth, W. Fulgione, C. Fuselli, P. Gaemers, R. Gaior, R. Gaitskell, M. Galloway, F. Gao, I. G. Garcia, J. Genovesi, C. Ghag, S. Ghosh, E. Gibson, W. Gil, D. Giovagnoli, F. Girard, R. Glade-Beucke, F. Gluck, S. Gokhale, A. Gouvea, L. Gr'af, L. Grandi, J. Grigat, B. Grinstein, M. D. Grinten, R. Grossle, H. Guan, M. Guida, R. Gumbsheimer, C. Gwilliam, C. Hall, L. Hall, R. Hammann, K. Han, V. Hannen, S. Hansmann-Menzemer, R. Harata, S. Hardin, E. Hardy, C. Hardy, K. Harigaya, R. Harnik, S. Haselschwardt, M. Hernandez, S. Hertel, A. Higuera, C. Hils, S. Hochrein, L. Hoetzsch, M. Hoferichter, N. Hood, D. Hooper, M. Horn, J. Howlett, D. Huang, Y. Huang, D. Hunt, M. Iacovacci, G. Iaquaniello, R. Ide, C. Ignarra, G. Iloglu, Y. Itow, E. Jacquet, O. Jahangir, J. Jakob, R. James, A. Jansen, W. Ji, X. Ji, F. Joerg, J. Johnson, A. Joy, A. Kaboth, A. Kamaha, K. Kanezaki, K. Kar, M. Kara, N. Kato, P. Kavrigin, S. Kazama, A. Keaveney, J. Kellerer, D. Khaitan, A. Khazov, G. Khundzakishvili, I. Khurana, B. Kilminster, M. Kleifges, P. Ko, M. Kobayashi, D. Kodroff, G. Koltmann, A. Kopec, A. Kopmann, J. Kopp, L. Korley, V. Kornoukhov, E. Korolkova, H. Kraus, L. Krauss, S. Kravitz, L. Kreczko, V. Kudryavtsev, F. Kuger, J. Kumar, B. Paredes, L. LaCascio, Q. Laine, H. Landsman, R. Lang, E. Leason, J. Lee, D. Leonard, K. Lesko, L. Levinson, C. Levy, I. Li, S. C. Li, Tao Li, S. Liang, C. Liebenthal, J. Lin, Q. Lin, S. Lindemann, M. Lindner, A. Lindote, R. Linehan, W. Lippincott, X. Liu, K. Liu, J. Liu, J. Loizeau, F. Lombardi, J. Long, M. Lopes, E. Asamar, W. Lorenzon, C. Lu, S. Luitz, Y. Ma, P. Machado, C. Macolino, T. Maeda, J. Mahlstedt, P. Majewski, A. Manalaysay, A. Mancuso, L. Manenti, A. Manfredini, R. Mannino, N. Marangou, J. March-Russell, F. Marignetti, T. M. Undagoitia, K. Martens, R. Martín, I. Martinez-Soler, J. Masbou, D. Masson, E. Masson, S. Mastroianni, M. Mastronardi, J. Matias-Lopes, M. McCarthy, N. McFadden, E. McGinness, D. Mckinsey, J. Mclaughlin, K. McMichael, P. Meinhardt, J. Men'endez, Y. Meng, M. Messina, R. Midha, D. Milisavljevic, E. Miller, B. Milosevic, S. Milutinović, S. Mitra, K. Miuchi, E. Mizrachi, K. Mizukoshi, A. Molinario, A. Monte, C. Monteiro, M. Monzani, J. S. Moore, K. Morra, J. Morad, J. D. Mendoza, S. Moriyama, E. Morrison, E. Morteau, Y. Mosbacher, B. Mount, J. Müller, A. Murphy, M. Murra, D. Naim, S. Nakamura, E. Nash, N. Navaieelavasani, A. Naylor, C. Nedlik, H. Nelson, F. Neves, J. Newstead, K. Ni, J. Nikoleyczik, V. Niro, U. Oberlack, M. Obradović, K. Odgers, C. O’Hare, P. Oikonomou, I. Olcina, K. Oliver-Mallory, A. Oranday, J. Orpwood, I. Ostrovskiy, K. Ozaki, B. Paetsch, S. Pal, J. Palacio, K. Palladino, J. Palmer, P. Panci, M. Pandurović, A. Parlati, N. Parveen, S. Patton, V. Pvevc, Q. Pellegrini, B. Penning, G. Pereira, R. Peres, Y. Perez-Gonzalez, E. Perry, T. Pershing, R. Petrossian-Byrne, J. Pienaar, A. Piepke, G. Pieramico, M. Pierre, M. Piotter, V. Pizella, G. Plante, T. Pollmann, D. Porzio, J. Qi, Y. Qie, J. Qin, N. Raj, M. R. Silva, K. Ramanathan, D. Garc'ia, J. Ravanis, L. Redard-Jacot, D. Redigolo, S. Reichard, J. Reichenbacher, C. Rhyne, A. Richards, Q. Riffard, G. Rischbieter, A. Rocchetti, S. Rosenfeld, R. Rosero, N. Rupp, T. Rushton, S. Saha, L. Sanchez, P. Sanchez-Lucas, D. Santone, J. Santos, I. Sarnoff, G. Sartorelli, A. Sazzad, M. Scheibelhut, R. Schnee, M. Schrank, J. Schreiner, P. Schulte, D. Schulte, H. Eissing, M. Schumann, T. Schwemberger, A. Schwenk, T. Schwetz, L. Lavina, P. Scovell, H. Sekiya, M. Selvi, E. Semenov, F. Semeria, P. Shagin, S. Shaw, S. Shi, E. Shockley, T. Shutt, R. Si-Ahmed, J. Silk, C. Silva, M. C. Silva, H. Simgen, F. vSimkovic, G. Sinev, R. Singh, W. Skulski, J. Smirnov, R. Smith, M. Solmaz, V. Solovov, P. Sorensen, J. Soria, T. Sparmann, I. Stancu, M. Steidl, A. Stevens, K. Stifter, L. Strigari, D. Subotić, B. Suerfu, A. M. Suliga, T. Sumner, P. Szabó, M. Szydagis, A. Takeda, Y. Takeuchi, P. Tan, C. Taricco, W. Taylor, D. Temples, A. Terliuk +499 moresemanticscholar +1 more sourceThe New Scenario of the Initial Evolution of the Universe [PDF]
, 1996 We propose that the Universe created from ”nothing” with relatively small particles number and quickly relaxed to quasiequilibrium state at the Planck parameters. The classic cosmological solution for this Universe with Λ-term has two branches divided by V.Burdyuzha, O.Lalakulich, Yu.Ponomarev, G. S. O. Sciences, Scientific Research Institute of Physics of Rostov State University +4 moresemanticscholar +1 more sourceThe high energy X-ray probe (HEX-P): the most powerful jets through the lens of a superb X-ray eye [PDF]
Frontiers in Astronomy and Space Sciences, 2023 A fraction of the active supermassive black holes at the centers of galaxies in our Universe are capable of launching extreme kiloparsec-long relativistic jets.L. Marcotulli, M. Ajello, M. Bottcher, P. Coppi, L. Costamante, L. D. Gesu, M. Errando, Javier A. Garc'ia, A. Gokus, I. Liodakis, G. Madejski, K. Madsen, Alberto Moretti, R. Middei, F. McBride, M. Petropoulou, Bindu Rani, T. Sbarrato, D. Stern, G. Vasilopoulos, M. Zacharias, Haocheng Zhang, the HEX-P Collaboration +22 moresemanticscholar +1 more sourceIdentifying the first generation of radio powerful AGN in the Universe with the SKA [PDF]
, 2014 One of the most challenging and exciting subjects in modern astrophysics is that of galaxy formation at the epoch of reionisation. The SKA, with its revolutionary capabilities in terms of frequency range, resolution and sensitivity, will allow to explore J. Afonso, J. Casanellas, I. Prandoni, M. Jarvis, S. Lorenzoni, M. Magliocchetti, Nick Seymour Institute of Astrophysics, S. Sciences, Portugal Faculdade de Ciencias, Universidade de Lisboa Max Planck Institut fur Gravitationsphys Radioastronomia, B. Astrophysics, University of Arizona Astronomy Department, University of the Western Cape INAF-IAPS International Centre Research, Curtin University +13 moresemanticscholar +1 more sourceAssessing the reliability of friends-of-friends groups on the future Javalambre Physics of the Accelerating Universe Astrophysical Survey [PDF]
, 2013 Aims. We have performed a detailed analysis of the ability of the friends-of-friends algorithm to identify real galaxy systems in deep surveys such as the future Javalambre Physics of the Accelerating Universe Astrophysical Survey.A. Zandivarez, E. D'iaz-Gim'enez, C. Oliveira, B. Ascaso, N. Ben'itez, R. Dupke, .. L.Sodr'eJr, J. I. I. Oac, Iag, Csic, U. Michigan, ON Rio de Janeiro, U. Alabama +12 moresemanticscholar +1 more source
