Zobrazeno 1 - 10
of 124
pro vyhledávání: '"Stuhlinger M"'
Autor:
Fuerst, F., Tomsick, J. A., Yamaoka, K., Dauser, T., Miller, J. M., Clavel, M., Corbel, S., Fabian, A. C., Garcia, J., Harrison, F. A., Loh, A., Kaaret, P., Kalemci, E., Migliari, S., Miller-Jones, J. C. A., Pottschmidt, K., Rahoui, F., Rodriguez, J., Stern, D., Stuhlinger, M., Walton, D. J., Wilms, J.
We present a detailed spectral analysis of XMM-Newton and NuSTAR observations of the accreting transient black hole GRS 1739-278 during a very faint low hard state at ~0.02% of the Eddington luminosity (for a distance of 8.5 kpc and a mass of 10 M_su
Externí odkaz:
http://arxiv.org/abs/1609.07530
Autor:
Arévalo, P., Bauer, F. E., Puccetti, S., Walton, D. J., Koss, M., Boggs, S. E., Brandt, W. N., Brightman, M., Christensen, F. E., Comastri, A., Craig, W. W., Fuerst, F., Gandhi, P., Grefenstette, B. W., Hailey, C. J., Harrison, F. A., Luo, B., Madejski, G., Madsen, K. K., Marinucci, A., Matt, G., Saez, C., Stern, D., Stuhlinger, M., Treister, E., Urry, C. M., Zhang, W. W.
The Circinus galaxy is one of the nearest obscured AGN, making it an ideal target for detailed study. Combining archival Chandra and XMM-Newton data with new NuSTAR observations, we model the 2-79 keV spectrum to constrain the primary AGN continuum a
Externí odkaz:
http://arxiv.org/abs/1406.3345
Autor:
Martin-Carrillo, A., Kirsch, M. G. F., Caballero, I., Freyberg, M. J., Ibarra, A., Kendziorra, E., Lammers, U., Mukerjee, K., Schönherr, G., Stuhlinger, M., Saxton, R. D., Staubert, R., Suchy, S., Wellbrock, A., Webb, N., Guainazzi, M.
Reliable timing calibration is essential for the accurate comparison of XMM-Newton light curves with those from other observatories, to ultimately use them to derive precise physical quantities. The XMM-Newton timing calibration is based on pulsar an
Externí odkaz:
http://arxiv.org/abs/1204.0978
Autor:
Chernyakova, M., Neronov, A., Courvoisier, T. J. -L., Turler, M., Soldi, S., Beckmann, V., Lubinski, P., Walter, R., Page, K. L., Stuhlinger, M., Staubert, R., McHardy, I. M.
The aim of this paper is to study the evolution of the broadband spectrum of one of the brightest and nearest quasars 3C 273. We analyze the data obtained during quasi-simultaneous INTEGRAL and XMM monitoring of the blazar 3C 273 in 2003--2005 in the
Externí odkaz:
http://arxiv.org/abs/astro-ph/0701825
Autor:
Stuhlinger, M., Altieri, B., Baskill, D., Dennerl, K., Esquej, M. P., Freyberg, M., Haberl, F., Herder, J. W. den, Kaastra, J., Kirsch, M. G. F., Metcalfe, L., Pollock, A. M. T., Read, A. M., Saxton, R. D., Sembay, S., Smith, M. J. S., Talavera, A., Vink, J., de Vries, C.
Further achievements of the XMM-Newton cross-calibration - XMM internal as well as with other X-ray missions - are presented. We explain the major changes in the new version SASv6.5 of the XMM-Newton science analysis system. The current status of the
Externí odkaz:
http://arxiv.org/abs/astro-ph/0511395
Autor:
Page, K. L., Turner, M. J. L., Done, C., O'Brien, P. T., Reeves, J. N., Sembay, S., Stuhlinger, M.
Publikováno v:
Mon.Not.Roy.Astron.Soc.349:57,2004
A series of nine XMM-Newton observations of the radio-loud quasar 3C 273 are presented, concentrating mainly on the soft excess. Although most of the individual observations do not show evidence for iron emission, co-adding them reveals a weak, broad
Externí odkaz:
http://arxiv.org/abs/astro-ph/0312148
Autor:
Courvoisier, T. J. -L., Beckmann, V., Bourban, G., Chenevez, J., Chernyakova, M., Deluit, S., Favre, P., Grindlay, J. E., Lund, N., O'Brien, P., Page, K., Produit, N., Türler, M., Turner, M. J. L., Staubert, R., Stuhlinger, M., Walter, R., Zdziarski, A. A.
Publikováno v:
Astron.Astrophys.411:L343-L356,2003
INTEGRAL has observed the bright quasar 3C 273 on 3 epochs in January 2003 as one of the first observations of the open programme. The observation on January 5 was simultaneous with RXTE and XMM-Newton observations. We present here a first analysis o
Externí odkaz:
http://arxiv.org/abs/astro-ph/0308212
Publikováno v:
In Advances in Space Research 2006 38(7):1393-1397
Autor:
Stabile, G., Trines, S.A., Arbelo, E., Dagres, N., Brugada, J., Kautzner, J., Pokushalov, E., Maggioni, A.P., Laroche, C., Anselmino, M., Beinart, R., Traykov, V., Lundqvist, C.B., Steinwender, C., Chasnoits, A., Mairesse, G., Balabanski, T., Riahi, S., Nawar, M., Maaty, M.A. el, Raatikainen, P., Anselme, F., Lewalter, T., Brodherr, T., Efremidis, M., Geller, L., Glover, ben, Glikson, M., Gaita, F., Rekvava, R., Kalejs, O., Trines, S., Kalarus, Z., Oliveira, M.M., Adra-Gao, P., Ciudin, R., Mikhaylov, E., Sinkovec, M., Villacastin, J.P., Blomstrom-Lundqvist, C., Sychov, O., Roberts, P., Scherr, G.D.D., Manninger, M., Mastnak, B., Pachinger, O., Hintringer, F., Stuhlinger, M., Steinwender, L.C., Xhaet, Y.O., Shalganov, S.T., Stoyanov, M., Protich, M., Traykov, S.V., Marchov, D., Kaninski, G., Chasnoits, M.A., Cihak, R., Haman, K.L., Schmidt, B., Chun, K.R.J., Perrotta, L., Bordignon, S., Tilz, R., Willems, S., Hindricks, G., Koutsouraki, I.S., Sorensen, B.G., Galal, C.W., AbdelWahab, A., Mokhtar, C.S.S., Ortega, I.G., Martinez, J.G.M., Calatrava, M.D., Sabate, R.V., Girbau, L.M., Arcocha, M.F., Gaztanaga, L., Zamarreno, E., Alvarez, M., Macias, R., Villalobos, F.S., Perez, J.C.R., Castellano, N.P., Canadas, V., Ferrer, J.J.G., Filgueiras, D., Campal, J.M.R., Sanchez-Borque, P., Benezet-Mazuecos, J., Ramos, J.T., Lozano, F., Urda, V.C., Cordero, A.B., Palomo, C.M., Ruiz-Salas, A., Alzueta, J., Peinado, R., Filqueiras-Rama, D., Gallanti, A.G., Garofalo, D., Calvo, N., Antolin, J.J.O., Pedrote, A., Arana-Rueda, E., Garcia-Riesco, L., Lund, J., Defaye, P., Jacon, P., Venier, S., Dugenet, F., Piot, O., Copie, X., Paziaud, O., Lepillier, A., Costa, A. da, Romeyer-Bouchard, C., Boveda, S., Albenque, J.P., Combes, N., Combes, S., Ferracci, A., Pisapia, A., Katritsis, D., Letsas, K., Vlachos, K., Lioni, L., Vassilikos, V.P., Szegedi, N., Szeplaki, G., Tahin, T., Csanadi, Z., Sandorfi, G., Kiss, A., Nagy-Balo, E., Saghy, L., Glover, B.M., Galvin, J., Keelan, E., Nof, E., Grimaldi, M., Quadrini, F., Monaco, A. di, Troisi, F., Tritto, M., Renzullo, E., Sanzo, A., Zagari, D., Pappone, C., Agricola, P.M.G., Bella, P. della, Iuliano, A., Bongiorni, M.G., Calo, L., Ruvo, E. de, Sciarra, L., Ferraris, F., Ponti, R. de, Marazzi, R., Doni, L.A., Kim, A., Molhoek, S., Gelder, I. van, Rienstra, M., Compier, M.G., Pison, L., Crijns, H.J., Vernooy, K., Luermans, J., Jordaens, L., Groot, N. de, Szili-Torok, T., Bhagwandien, R., Elvan, Z.A., Buist, T., Gal, P., Lubinski, A., Krolak, T., Nowak, S., Mizia-Stec, K., Wnuk-Wojnar, A.M., Lelakowski, J., Kazmierczak, J., Kulakowski, P., Baran, J., Opolski, G., Kiliszek, M., Lodzinski, P., Borodzicz, S., Balsam, P., Blaszyk, K., Pytkowski, M., Kuteszko, R., Ciszewski, J., Fuglewicz, A., Wozniak, A., Adamczyk, K., Adragao, P., Cunha, P., Grecu, I.M., Tinica, G., Muresan, L., Rosu, R., Khomenko, E., Romanov, A., Bayramova, S., Mikhaylov, E.N., Lebedev, D.S., Patsouk, A.V., Yashin, S., Kryzhanovskiy, D., Bazayev, S.V., Morgunov, D., Silin, I., Popov, S., Kuznetsov, V., Jonsson, A., Platonov, P., Holmqvist, F., Kongstad, O., Yuan, S., Hoglund, N., Malmborg, H., Mortsell, D., Pernat, A., Morgan, J., Greenwood, E.F., Fletcher, L.L., Kravchenko, D.T., Doronin, A., Meshkova, M., Karpenko, I., Goryatchiy, A., Abramova, A., ESC-EHRA Atrial Fibrillation Abla
Publikováno v:
Pacing and Clinical Electrophysiology, 42(3), 313-320. WILEY
Background Atrial fibrillation (AF) promotes atrial remodeling that in turn promotes AF perpetuation. The aim of our study is to investigate the impact of AF history length on 1-year outcome of AF catheter ablation in a cohort of patients enrolled in
Autor:
Furst, F, Tomsick, JA, Yamaoka, K, Dauser, T, Miller, JM, Clavel, M, Corbel, S, Fabian, A, Garcia, J, Harrison, FA, Loh, A, Kaaret, P, Kalemci, E, Migliari, S, Miller-Jones, JCA, Pottschmidt, K, Rahoui, F, Rodriguez, J, Stern, D, Stuhlinger, M, Walton, DJ, Wilms, J
We present a detailed spectral analysis of $\small \textit{XMM-Newton}$ and $\small \textit{NuSTAR}$ observations of the accreting transient black hole GRS 1739−278 during a very faint low hard state at ~0.02% of the Eddington luminosity (for a dis
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9aa6dd81922a5c70d443c120e06d4b76