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  • Mainieri, V.; Bongiorno, A.; Merloni, A.; Aller, M.; Carollo, M.; Iwasawa, K.; Koekemoer, A. M.; Mignoli, M.; Silverman, J. D.; Bolzonella, M.; Brusa, M.; Comastri, A.; Gilli, R.; Halliday, C.; Ilbert, O.; Lusso, E.; Salvato, M.; Vignali, C.; Zamorani, G.; Contini, T.; Kneib, J. P.; Le Fèvre, O.; Lilly, S.; Renzini, A.; Scodeggio, M.; Balestra, I.; Bardelli, S.; Caputi, K.; Coppa, G.; Cucciati, O.; de la Torre, S.; de Ravel, L.; Franzetti, P.; Garilli, B.; Iovino, A.; Kampczyk, P.; Knobel, C.; Kova, K.; Lamareille, F.; Le Borgne, J. F.; Le Brun, V.; Maier, C.; Nair, P.; Pello, R.; Peng, Y.; Perez Montero, E.; Pozzetti, L.; Ricciardelli, E.; Tanaka, M.; Tasca, L.; Tresse, L.; Vergani, D.; Zucca, E.; Aussel, H.; Capak, P.; Cappelluti, N.; Elvis, M.; Fiore, F.; Hasinger, G.; Impey, C.; Le Floc'h, E.; Scoville, N.; Taniguchi, Y.; Trump, J. (2011)
    <br/> Aims: We explore the connection between black hole growth at the center of obscured quasars selected from the XMM-COSMOS survey and the physical properties of their host galaxies. We study a bolometric regime ( ? ...
  • van, der Werf; Isaak, K. G.; Meijerink, R.; Spaans, M.; Rykala, A.; Fulton, T.; Loenen, A. F.; Walter, F.; Weiß, A.; Armus, Lee; Fischer, J.; Israel, F. P.; Harris, A. I.; Veilleux, S.; Henkel, C.; Savini, G.; Lord, S.; Smith, Howard A.; González-Alfonso, E.; Naylor, D.; Aalto, Susanne; Charmandaris, Vassilis; Dasyra, K. M.; Evans, A.; Gao, Y.; Greve, T. R.; Güsten, R.; Kramer, C.; Martín-Pintado, J.; Mazzarella, J.; Papadopoulos, P. P.; Sanders, D. B.; Spinoglio, L.; Stacey, G.; Vlahakis, C.; Wiedner, M. C.; Xilouris, E. M. (2010)
    We present a full high resolution SPIRE FTS spectrum of the nearby ultraluminous infrared galaxy Mrk 231. In total 25 lines are detected, including CO J = 5-4 through J = 13-12, 7 rotational lines of H<SUB>2</SUB>O, 3 of ...
  • Balakrishnan, Mayura; Draghis, Paul A.; Miller, Jon M.; Bright, Joe; Fender, Robert; Ng, Mason; Cackett, Edward; Fabian, Andrew; Kuntz, Kip; Miller-Jones, James C. A.; Proga, Daniel; Ray, Paul S.; Raymond, John; Reynolds, Mark; Zoghbi, Abderahmen (2023)
    A number of neutron stars have been observed within the remnants of the core-collapse supernova explosions that created them. In contrast, black holes are not yet clearly associated with supernova remnants (SNRs). Indeed, ...
  • Nardini, E.; Reeves, J. N.; Gofford, J.; Harrison, F. A.; Risaliti, G.; Braito, V.; Costa, M. T.; Matzeu, G. A.; Walton, D. J.; Behar, E.; Boggs, S. E.; Christensen, F. E.; Craig, W. W.; Hailey, C. J.; Matt, G.; Miller, J. M.; O'Brien, P. T.; Stern, D.; Turner, T. J.; Ward, M. J. (2015)
    The evolution of galaxies is connected to the growth of supermassive black holes in their centers. During the quasar phase, a huge luminosity is released as matter falls onto the black hole, and radiation-driven winds can ...
  • Ripperda, B.; Liska, Matthew; Chatterjee, K.; Musoke, G.; Philippov, A. A.; Markoff, S. B.; Tchekhovskoy, A.; Younsi, Z. (2022)
    Magnetic reconnection can power bright, rapid flares originating from the inner magnetosphere of accreting black holes. We conduct extremely high-resolution (5376 Ã- 2304 Ã- 2304 cells) general-relativistic magnetohydrodynamics ...
  • Brusa, Marcella; Fiore, F.; Santini, P.; Grazian, A.; Comastri, Andrea; Zamorani, G.; Hasinger, G.; Merloni, A.; Civano, Francesca; Fontana, A.; Mainieri, V. (2009)
  • Ricarte, Angelo; Qiu, Richard; Narayan, Ramesh (2021)
    The circular polarization of black hole accretion flows can encode properties of the underlying magnetic field structure. Using general relativistic magnetohydrodynamic (GRMHD) simulations, we study the imprint of magnetic ...
  • Bower, Geoffrey C.; Dexter, Jason; Markoff, Sera; Gurwell, Mark A.; Rao, Ramprasad; McHardy, Ian (2015)
    We analyze the light curves of 413 radio sources at submillimeter wavelengths using data from the Submillimeter Array calibrator database. The database includes more than 20,000 observations at 1.3 and 0.8 mm that span 13 ...
  • Schild, R. E.; Leiter, Darryl J. (2010)
    Not Available
  • Roelofs, Freek; Fromm, Christian M.; Mizuno, Yosuke; Davelaar, Jordy; Janssen, Michael; Younsi, Ziri; Rezzolla, Luciano; Falcke, Heino (2021)
    Context. The Event Horizon Telescope (EHT) has imaged the shadow of the supermassive black hole in M 87. A library of general relativistic magnetohydrodynamics (GMRHD) models was fit to the observational data, providing ...
  • Agís-González, B.; Miniutti, G.; Kara, E.; Fabian, A. C.; Sanfrutos, M.; Risaliti, G.; Bianchi, S.; Strotjohann, N. L.; Saxton, R. D.; Parker, M. L. (2014)
    We report results from multi-epoch X-ray observations of the Seyfert 1.5 galaxy ESO 362-G18 performed between 2005 November and 2010 June. ESO 362-G18 generally exhibits the typical X-ray spectrum of type 1 active galactic ...
  • Lohfink, Anne M.; Reynolds, Christopher S.; Miller, Jon M.; Brenneman, Laura W.; Mushotzky, Richard F.; Nowak, Michael A.; Fabian, Andrew C. (2012)
    We present an analysis of all XMM-Newton and Suzaku X-ray spectra of the nearby luminous Seyfert galaxy Fairall 9. Confirming previous analyses, we find robust evidence for a broad iron line associated with X-ray reflection ...
  • McClintock, Jeffrey E.; Narayan, Ramesh; Steiner, James F. (2014)
    The spins of ten stellar black holes have been measured using the continuum-fitting method. These black holes are located in two distinct classes of X-ray binary systems, one that is persistently X-ray bright and another ...
  • Gottlieb, Ore; Lalakos, Aretaios; Bromberg, Omer; Liska, Matthew; Tchekhovskoy, Alexander (2022)
    We present a suite of the first 3D GRMHD collapsar simulations, which extend from the self-consistent jet launching by an accreting Kerr black hole (BH) to the breakout from the star. We identify three types of outflows, ...
  • Gottlieb, Ore; Liska, Matthew; Tchekhovskoy, Alexander; Bromberg, Omer; Lalakos, Aretaios; Giannios, Dimitrios; Mösta, Philipp (2022)
    Long-duration ?-ray bursts (GRBs) accompany the collapse of massive stars and carry information about the central engine. However, no 3D models have been able to follow these jets from their birth via black hole (BH) to ...
  • Vulic, N.; Hornschemeier, A. E.; Wik, D. R.; Yukita, M.; Zezas, A.; Ptak, A. F.; Lehmer, B. D.; Antoniou, V.; Maccarone, T. J.; Williams, B. F.; Fornasini, F. M. (2018)
    Nearby galaxy surveys have long classified X-ray binaries (XRBs) by the mass category of their donor stars (high-mass and low-mass). The NuSTAR observatory, which provides imaging data at E &gt; 10 keV, has enabled the ...
  • Smith, Lisa F.; Arcand, Kimberly Kowal; Smith, Benjamin K.; Smith, Randall K.; Bookbinder, Jay; Smith, Jeffrey K. (2017)
    This study extended research on the development of explanatory labels for astronomical images for the nonexpert lay public. The research questions addressed how labels with leading questions/metaphors and relevance to ...
  • Narayan, Ramesh; Quataert, Eliot (2023)
    Recent developments have ushered in a new era in the field of black-hole astrophysics, providing a direct view of the remarkable environment near black-hole event horizons. These observations have enabled astronomers to ...
  • Southwick, Charles H. (1955)

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