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Browsing by Author "Coe, M. J."

Browsing by Author "Coe, M. J."

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  • Be/X-ray binary SXP6.85 undergoes large Type II outburst in the Small Magellanic Cloud 
    Townsend, L. J.; Coe, M. J.; McBride, V. A.; Bird, A. J.; Schurch, M. P. E.; Corbet, R. H. D.; Haberl, F.; Galache, J. L.; Udalski, A. (2010)
    ABSTRACT The Small Magellanic Cloud (SMC) Be/X-ray binary pulsar SXP6.85 = XTE J0103-728 underwent a large Type II outburst beginning on 2008 August 10. The source was consistently seen for the following 20 weeks (MJD = ...
  • The Chandra Small Magellanic Cloud Wing Survey - the search for X-ray binaries 
    McGowan, K. E.; Coe, M. J.; Schurch, M. P. E.; McBride, V. A.; Galache, J. L.; Edge, W. R. T.; Corbet, R. H. D.; Laycock, S.; Buckley, D. A. H. (2008)
    We have detected 523 sources in a survey of the Small Magellanic Cloud (SMC) Wing with Chandra. By cross-correlating the X-ray data with optical and near-infrared catalogues, we have found 300 matches. Using a technique ...
  • A Comprehensive Library of X-Ray Pulsars in the Small Magellanic Cloud: Time Evolution of Their Luminosities and Spin Periods 
    Yang, J.; Laycock, S. G. T.; Christodoulou, D. M.; Fingerman, S.; Coe, M. J.; Drake, Jeremy J. (2017)
    We have collected and analyzed the complete archive of XMM-Newton (116), Chandra (151), and RXTE (952) observations of the Small Magellanic Cloud (SMC), spanning 1997–2014. The resulting observational library provides a ...
  • D'Arros and St. Joseph, Amirante Islands 
    Stoddart, David R.; Coe, M. J.; Fosberg, F. Raymond (1979)
  • High-mass X-ray binary SXP18.3 undergoes the longest type II outburst ever seen in the Small Magellanic Cloud 
    Schurch, M. P. E.; Coe, M. J.; Galache, J. L.; Corbet, R. H. D.; McGowan, K. E.; McBride, V. A.; Townsend, L. J.; Udalski, A.; Haberl, F. (2009)
  • INTEGRAL deep observations of the Small Magellanic Cloud 
    Coe, M. J.; Bird, A. J.; Buckley, D. A. H.; Corbet, R. H. D.; Dean, A. J.; Finger, M.; Galache, J. L.; Haberl, F.; McBride, V. A.; Negueruela, I.; Schurch, M.; Townsend, L. J.; Udalski, A.; Wilms, J.; Zezas, Andreas (2010)
  • The Large Observatory for X-ray Timing (LOFT) 
    Feroci, M.; Stella, L.; van, der Klis; Courvoisier, T. J. -L; Hernanz, M.; Hudec, R.; Santangelo, A.; Walton, D.; Zdziarski, A.; Barret, D.; Belloni, T.; Braga, J.; Brandt, S.; Budtz-Jørgensen, C.; Campana, S.; den Herder, J. -W; Huovelin, J.; Israel, G. L.; Pohl, M.; Ray, P.; Vacchi, A.; Zane, S.; Argan, A.; Attinà, P.; Bertuccio, G.; Bozzo, E.; Campana, R.; Chakrabarty, D.; Costa, E.; De Rosa, A.; Del Monte, E.; Di Cosimo, S.; Donnarumma, I.; Evangelista, Y.; Haas, D.; Jonker, P.; Korpela, S.; Labanti, C.; Malcovati, P.; Mignani, R.; Muleri, F.; Rapisarda, M.; Rashevsky, A.; Rea, N.; Rubini, A.; Tenzer, C.; Wilson-Hodge, C.; Winter, B.; Wood, K.; Zampa, G.; Zampa, N.; Abramowicz, M. A.; Alpar, M. A.; Altamirano, D.; Alvarez, J. M.; Amati, L.; Amoros, C.; Antonelli, L. A.; Artigue, R.; Azzarello, P.; Bachetti, M.; Baldazzi, G.; Barbera, M.; Barbieri, C.; Basa, S.; Baykal, A.; Belmont, R.; Boirin, L.; Bonvicini, V.; Burderi, L.; Bursa, M.; Cabanac, C.; Cackett, E.; Caliandro, G. A.; Casella, P.; Chaty, S.; Chenevez, J.; Coe, M. J.; Collura, A.; Corongiu, A.; Covino, S.; Cusumano, G.; D'Amico, F.; Dall'Osso, S.; De Martino, D.; De Paris, G.; Di Persio, G.; Di Salvo, T.; Done, C.; Dovciak, M.; Drago, A.; Ertan, U.; Fabiani, S.; Falanga, M.; Fender, R.; Ferrando, P.; Della, Monica Ferreira; Fraser, G.; Frontera, F.; Fuschino, F.; Galvez, J. L.; Gandhi, P.; Giommi, P.; Godet, O.; Gögüs, E.; Goldwurm, A.; Götz, D.; Grassi, M.; Guttridge, P.; Hakala, P.; Henri, G.; Hermsen, W.; Horak, J.; Hornstrup, A.; in't Zand, J. J. M.; Isern, J.; Kalemci, E.; Kanbach, G.; Karas, V.; Kataria, D.; Kennedy, T.; Klochkov, D.; Kluzniak, W.; Kokkotas, K.; Kreykenbohm, I.; Krolik, J.; Kuiper, L.; Kuvvetli, I.; Kylafis, N.; Lattimer, J. M.; Lazzarotto, F.; Leahy, D.; Lebrun, F.; Lin, D.; Lund, N.; Maccarone, T.; Malzac, J.; Marisaldi, M.; Martindale, A.; Mastropietro, M.; McClintock, J.; McHardy, I.; Mendez, M.; Mereghetti, S.; Miller, M. C.; Mineo, T.; Morelli, E.; Morsink, S.; Motch, C.; Motta, S.; Muñoz-Darias, T.; Naletto, G.; Neustroev, V.; Nevalainen, J.; Olive, J. F.; Orio, M.; Orlandini, M.; Orleanski, P.; Ozel, F.; Pacciani, L.; Paltani, S.; Papadakis, I.; Papitto, A.; Patruno, A.; Pellizzoni, A.; Petrácek, V.; Petri, J.; Petrucci, P. O.; Phlips, B.; Picolli, L.; Possenti, A.; Psaltis, D.; Rambaud, D.; Reig, P.; Remillard, R.; Rodriguez, J.; Romano, P.; Romanova, M.; Schanz, T.; Schmid, C.; Segreto, A.; Shearer, A.; Smith, A.; Smith, P. J.; Soffitta, P.; Stergioulas, N.; Stolarski, M.; Stuchlik, Z.; Tiengo, A.; Torres, D.; Török, G.; Turolla, R.; Uttley, P.; Vaughan, S.; Vercellone, S.; Waters, R.; Watts, A.; Wawrzaszek, R.; Webb, N.; Wilms, J.; Zampieri, L.; Zezas, Andreas; Ziolkowski, J. (2012)
    High-time-resolution X-ray observations of compact objects provide direct access to strong-field gravity, to the equation of state of ultradense matter and to black hole masses and spins. A 10 m<SUP>2</SUP>-class instrument ...
  • Long-term optical variability of high-mass X-ray binaries. II. Spectroscopy 
    Reig, P.; Nersesian, A.; Zezas, Andreas; Gkouvelis, L.; Coe, M. J. (2016)
    Context. High-mass X-ray binaries are bright X-ray sources. The high-energy emission is caused by the accretion of matter from the massive companion onto a neutron star. The accreting material comes from either the strong ...
  • On the Geometry of the X-ray emission from pulsars a consistent inclination and beaming solution for the Be/X-ray pulsar SXP 1062 
    Cappallo, R. C.; Laycock, S. G. T.; Christodoulou, D. M.; Roy, A.; Bhattacharya, S.; Coe, M. J.; Zezas, Andreas (2020)
    SXP 1062 is a long-period X-ray pulsar (XRP) with a Be optical companion located in the Small Magellanic Cloud. First discovered in 2010 from XMM-Newton data, it has been the target of multiple observational campaigns due ...
  • On the geometry of the X-ray emission from pulsars: the changing aspect of the Be/X-ray pulsar SXP348 
    Cappallo, R.; Laycock, S. G. T.; Christodoulou, D. M.; Coe, M. J.; Zezas, Andreas (2019)
    The X-ray source SXP348 is a high-mass X-ray binary system in the Small Magellanic Cloud. Since its 1998 discovery by BeppoSAX, this pulsar has exhibited a spin period of ~340-350 s. In an effort to determine the orientation ...
  • An optical and X-ray study of the counterpart to the Small Magellanic Cloud X-ray binary pulsar system SXP327 
    Coe, M. J.; Schurch, M.; Corbet, R. H. D.; Galache, J.; McBride, V. A.; Townsend, L. J.; Udalski, A. (2008)
  • Optical and X-ray variability of two Small Magellanic Cloud X-ray binary pulsars - SXP46.6 and SXP6.85 
    McGowan, K. E.; Coe, M. J.; Schurch, M. P. E.; Corbet, R. H. D.; Galache, J. L.; Udalski, A. (2008)
  • Optical follow-up of new Small Magellanic Cloud wing Be/X-ray binaries 
    Schurch, M. P. E.; Coe, M. J.; McGowan, K. E.; McBride, V. A.; Buckley, D. A. H.; Galache, J. L.; Corbet, R. H. D.; Still, M.; Vaisanen, P.; Kniazev, A.; Nordsieck, K. (2007)

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