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Browsing by Author "Centre for Astrophysics Research"

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  • Brassington, Nicola; Fabbiano, G.; Kim, D.-W.; Zezas, A.; Zepf, S.; Kundu, A.; Angelini, L.; Davies, R. L.; Gallagher, J.; Kalogera, V.; Fragos, T.; King, A.R.; Pellegrini, S.; Trinchieri, G. (2008-11-01)
    We present the properties of the discrete X-ray sources detected in our monitoring program of the `typical' elliptical galaxy, NGC 3379, observed with Chandra ACIS-S in five separate pointings, resulting in a co-added ...
  • Brassington, Nicola; Fabbiano, G.; Kim, D.-W.; Zezas, A.; Zepf, S.; Kundu, A.; Angelini, L.; Davies, R. L.; Gallagher, J.; Kalogera, V.; Fragos, T.; King, A.R.; Pellegrini, S.; Trinchieri, G. (2009-04-01)
    We present the properties of the discrete X-ray sources detected in our monitoring program of the globular cluster (GC) rich elliptical galaxy, NGC 4278, observed with Chandra ACIS-S in six separate pointings, resulting ...
  • Hardcastle, M. J.; Lenc, E.; Birkinshaw, M.; Croston, J. H.; Goodger, J. L.; Marshall, H. L.; Perlman, E. S.; Siemiginowska, A.; Stawarz, L.; Worrall, D. M. (2016-02-01)
    We report on deep Chandra observations of the nearby broad-line radio galaxy Pictor A, which we combine with new Australia Telescope Compact Array (ATCA) observations. The new X-ray data have a factor 4 more exposure than ...
  • Ibar, E.; Ivison, R.J.; Best, P.N.; Coppin, Kristen; Pope, A.; Smail, I.; Dunlop, J.S. (2010-01-01)
    We have employed the Giant Metre-wave Radio Telescope and the Very Large Array to map the Lockman Hole. At 610 and 1400 MHz, we reach noise levels of 15 and 6μJy beam , respectively, with well-matched resolutions (~5 ...
  • Mohr-Smith, M.; Drew, Janet; Napiwotzki, Ralf; Simon-Diaz, S.; Wright, N. J.; Barentsen, Geert; Eisloeffel, J.; Farnhill, Hywel; Greimel, R.; Monguio, Maria; Kalari, V.; Parker, Q. A.; Vink, Jorick S. (2017-02-21)
    Massive OB stars are critical to the ecology of galaxies and yet our knowledge of OB stars in the Milky Way, fainter than V ∼ 12, remains patchy. Data from the VST Photometric Hα Survey (VPHAS+) permit the construction of ...
  • Heesen, V.; Rau, U.; Rupen, M. P.; Brinks, E.; Hunter, D. A. (2011-09-20)
    We exploit the vastly increased sensitivity of the Expanded Very Large Array to study the radio continuum and polarization properties of the post-starburst, dwarf irregular galaxy IC 10 at 6 cm, at a linear resolution of ...
  • Brisbin, D.; Harwit, M.; Altieri, B.; Amblard, A.; Arumugam, V.; Aussel, H.; Babbedge, T.; Blain, A.; Bock, J.; Boselli, A.; Buat, V.; Castro-Rodríguez, N.; Cava, A.; Chanial, P.; Clements, D. L.; Conley, A.; Conversi, L.; Cooray, A.; Dowell, C.D.; Dwek, E.; Eales, S.; Elbaz, D.; Fox, M.; Franceschini, A.; Gear, W.; Glenn, J.; Griffin, M.; Halpern, M.; Hatziminaoglou, E.; Ibar, E.; Isaak, K.; Ivison, Rob J.; Lagache, G.; Levenson, L.; Lonsdale, C.J.; Lu, N.; Madden, S.; Maffei, B.; Mainetti, G.; Marchetti, L.; Morrison, G.E.; Nguyen, H.T.; O'Halloran, B.; Oliver, S.J.; Omont, A.; Owen, F.N.; Pannella, M.; Panuzzo, P.; Papageorgiou, A.; Pearson, C.P.; Pérez-Fournon, I.; Pohlen, M.; Rizzo, D.; Roseboom, I.G.; Rowan-Robinson, M.; Portal, M.S.; Schulz, B.; Seymour, N.; Shupe, D. L.; Smith, A.J.; Stevens, Jason; Strazzullo, V.; Symeonidis, M.; Trichas, M.; Tugwell, K.E.; Vaccari, M.; Valtchanov, I.; Vigroux, L.; Wang, L.; Ward, R.; Wright, G.; Xu, C.K.; Zemcov, M. (2010-11-01)
    We present the cross-identification and source photometry techniques used to process Herschel SPIRE imaging taken as part of the Herschel Multi-Tiered Extragalactic Survey (HerMES). Cross-identifications are performed in ...
  • Norris, R.P.; Afonso, J.; Cava, A.; Farrah, D.; Huynh, M.T.; Ivison, R.J.; Jarvis, M.J.; Lacy, M.; Mao, M.; Maraston, C.; Mauduit, J.C.; Middelberg, E.; Oliver, S.; Seymour, N.; Surace, J. (2011)
    Infrared-faint radio sources (IFRSs) are a rare class of objects which are relatively bright at radio wavelengths but very faint at infrared and optical wavelengths. Here we present sensitive near-infrared observations of ...
  • Heywood, I.; Jarvis, M. J.; Baker, A. J.; Bannister, K. W.; Carvalho, C. S.; Hardcastle, M.; Hilton, M.; Moodley, K.; Smirnov, O. M.; Smith, D. J. B.; White, S. V.; Wollack, E. J. (2016-08-21)
    We have used the Karl G. Jansky Very Large Array to image ~100 sq. deg. of SDSS Stripe 82 at 1-2 GHz. The survey consists of 1,026 snapshot observations of 2.5 minutes duration, using the hybrid CnB configuration. The ...
  • Pinfield, D.J.; Gomes, J.; Day-Jones, A. C.; Leggett, S.K.; Gromadzki, M.; Burningham, B.; Ruiz, M. T.; Kurtev, R.; Cattermole, T.; Cardoso, C.; Lodieu, N.; Faherty, J.; Littlefair, S.; Smart, R.; Irwin, M.; Clarke, J. R. A.; Smith, Leigh; Lucas, P.W.; Galvez-Ortiz, M. C.; Jenkins, J. S.; Jones, H.R.A.; Rebolo, R.; Bejar, V. J. S.; Gauza, B. (2014-01)
    A method is defined for identifying late-T and Y dwarfs in WISE down to low values of signal-to-noise. This requires a WISE detection only in the W2-band and uses the statistical properties of the WISE multiframe measurements ...
  • Kopytova, Taisiya G.; Crossfield, Ian J M; Deacon, Niall R.; Brandner, Wolfgang; Buenzli, Esther; Bayo, Amelia; Schlieder, Joshua E.; Manjavacas, Elena; Biller, Beth A.; Kopon, Derek (2014-11-17)
    WISE J085510.83-071442.5 (hereafter, WISE 0855-07) is the coolest Y dwarf known to date and is located at a distance of 2.31 ± 0.08 pc, giving it the fourth largest parallax of any known star or brown dwarf system. We ...
  • Shabala, Stanislav; Deller, Adam; Kaviraj, Sugata; Middelberg, Enno; Turner, Ross; Ting, Yuan-Sen; Allison, James; Davis, Tim (2017-02-01)
    We examine the processes triggering star formation and Active Galactic Nucleus (AGN) activity in a sample of 25 low redshift ($z 10^7$ K) brightness temperature required for an mJIVE-20 detection allows us to unambiguously ...
  • Rubio, Monica; Elmegreen, Bruce G.; Hunter, Deidre A.; Brinks, E.; Cortés, Juan R.; Cigan, Phil (2015-09-10)
    Understanding stellar birth requires observations of the clouds in which they form. These clouds are dense and self-gravitating, and in all existing observations they are molecular, with H2 the dominant species and carbon ...
  • Ginsburg, A.; Henkel, C.; Ao, Y.; Riquelme, D.; Kauffmann, J.; Pillai, T.; Mills, E.~A.~C.; Requena-Torres, M.~A.; Immer, K.; Testi, L.; Ott, J.; Bally, J.; Battersby, C.; Darling, J.; Aalto, S.; Stanke, T.; Kendrew, S.; Kruijssen, J.~M.~D.; Longmore, S.; Guesten, R.; Menten, K.~M.; Dale, James (2016-01-26)
    Context. The Galactic center is the closest region where we can study star formation under extreme physical conditions like those in high-redshift galaxies. Aims. We measure the temperature of the dense gas in the central ...
  • Jeffers, S V; Cameron, A C; Barnes, J R; Aufdenberg, J P; Hussain, G A J (European Space Agency, 2005)
    We have used spectrophotometric data from 9 HST orbits to eclipse-map the primary component of the RS CVn binary SV Cam. From these observations and SV Cam's HIPPARCOS parallax we find that the surface flux in the eclipsed ...
  • Jeffers, S. V.; Cameron, A. Collier; Barnes, J. R.; Aufdenberg, J. P. (2006-08)
    We have used spectrophotometric data from nine Hubble Space Telescope orbits to eclipse-map the primary component of the RS CVn binary SV Cam. From these observations and its HIPPARCOS parallax we find that the surface ...
  • Rauscher, T.; Bieber, R.; Oberhummer, H.; Kratz, K.L.; Dobaczewski, J.; Moller, P.; Sharma, M.M. (1998-04)
    The prediction of cross sections for nuclei far off stability is crucial in the field of nuclear astrophysics. We calculate direct neutron capture on the even-even isotopes Sn124-145 and Pb208-238 with energy levels, masses, ...
  • Smith, Daniel; Hayward, Christopher C. (2015-10-21)
    Panchromatic spectral energy distribution (SED) fitting is a critical tool for determining the physical properties of distant galaxies, such as their stellar mass and star formation rate. One widely used method is the ...
  • Allekotte, I.; Arnaldi, H.; Asorey, H.; Berisso, M.G.; Haro, M.S.; Cillis, A.; Rovero, A.C.; Supanitsky, A.D.; Actis, M.; Antico, F.; Bottani, A.; Ochoa, I.; Ringegni, P.; Vallejo, G.; de la Vega, G.; Etchegoyen, A.; García, B.; Sánchez, F.; Videla, M.; González, F.; Otero, L.; Pallota, J.; Quel, E.; Ristori, P.; Romero, G.E.; Suárez, A.; Akhperjanian, A.; Papyan, G.; Pogosyan, L.; Sahakian, V.; Bissaldi, E.; Egberts, K.; Reimer, A.; Reimer, O.; Shellard, R.C.; Santos, E.M.; de Gouveia Dal Pino, E.M.; Kowal, G.; de Souza, V.; Peixoto, C.J.T.; Maneva, G.; Temnikov, P.; Vankov, H.; Golev, V.; Ovcharov, E.; Bonev, T.; Dimitrov, D.; Hrupec, D.; Nedbal, D.; Rob, L.; Lindfors, E.; Sillanpää, A.; Takalo, L.; Beckmann, V.; Benallou, M.; Boutonnet, C.; Corlier, M.; Courty, B.; Djannati-Ataï, A.; Dufour, C.; Gabici, S.; Guglielmi, L.; Olivetto, C.; Pita, S.; Punch, M.; Selmane, S.; Terrier, R.; Yoffo, B.; Brun, P.; Carton, P.H.; Cazaux, S.; Corpace, O.; Delagnes, E.; Disset, G.; Durand, D.; Glicenstein, J.-F.; Guilloux, F.; Kosack, K.; Medina, C.; Micolon, P.; Mirabel, F.; Moulin, E.; Peyaud, B.; Reymond, J.-M.; Veyssiere, C.; Brau-Nogué, S.; Jean, P.; Knödlseder, J.; Le Padellec, A.; Webb, N.; Cerruti, B.; Dubus, G.; Henri, G.; Petrucci, P.O.; Barbier, C.; Brunetti, L.; Cailles, M.; Deleglise, G.; Elles, S.; Fouque, N.; Gasq, C.; Geffroy, N.; Komin, N.; Kossakowski, R.; Lamanna, G.; Le Flour, T.; Lieunard, B.; Monteiro, I.; Panazol, J.L.; Rosier-Lees, S.; Vialle, J.P.; Becherini, Y.; Clerc, C.; Couturier, S.; de Naurois, M.; Edy, E.; Fillin-Martino, E.; Fontaine, G.; Giebels, B.; Khélifi, B.; Manigot, P.; Moal, B.; Spyrou, S.; Bourgeat, M.; Compin, M.; Feinstein, F.; Gallant, Y.; Lavalley, C.; Renaud, M.; Rivoire, S.; Royer, S.; Vasileiadis, G.; Vorobiov, S.; Boisson, C.; Cerruti, M.; Mottez, F.; Roy, F.; Sol, H.; Venter, L.; Zech, A.; Dournaux, J.-L.; Huet, J.-M.; Laporte, P.; Castarede, H.; Bolmont, J.; Corona, P.; Huppert, J.-F.; Jacholkowska, A.; Naumann, C.; Nayman, P.; Tavernet, J.-P.; Toussenel, F.; Vincent, P.; Carr, J.; Costantini, H.; Ernenwein, J.-P.; Hoffmann, D.; Karkar, S.; Mendes, A.; Artmann, S.; Becker, J.; Schlickeiser, R.; Federici, S.; Pohl, M.; Ruppel, J.; Telezhinsky, I.; Bähr, J.; Behera, B.; Birsin, E.; Decerprit, B.; Heller, R.; Kostka, P.; Kretzschmann, A.; Maier, G.; Melkumyan, D.; Naumann, D.; Arribas, M.P.; Platzer, R.; Prokoph, H.; Schlenstedt, S.; Schmidt, T.; Schultze, J.; Shayduk, M.; Skole, C.; Sternberger, R.; Sulanke, K.H.; Wegner, P.; Welsing, R.; Winde, M.; Wischnewski, R.; Lohse, T.; Oya, I.; Schwanke, U.; Doert, M.; Rhode, W.; Jung, I.; Lopatin, A.; Schulz, A.; Stegmann, C.; Stinzing, F.; Horns, D.; Kneiske, T.; Raue, M.; Tluczykont, M.; Hauser, M.; Quirrenbach, A.; Reimann, C.; Tam, P.H.; Tchernin, C.; Wagner, S.; Walter, P.; Bauer, C.; Bernlöhr, K.; de Oña Wilhelmi, E.; Deil, C.; Domainko, W.; Föhr, C.; Förster, A.; Hahn, J.; Hermann, G.; Hofmann, W.; Hofverberg, P.; Kankanyan, R.; Kihm, T.; Köck, F.; Panter, M.; Rieger, F.; van Eldik, C.; Volpe, F.; de Almeida, U.B.; Colin, P.; Dettlaff, T.; Fink, D.; Fruck, C.; Haefner, D.; Haubold, T.; Jablonski, C.; Jogler, T.; Krause, J.; Lorenz, E.; Mirzoyan, R.; Nowak, N.; Paneque, D.; Reimann, O.; Rodriguez, S.; Saito, K.; Saito, T.; Schweizer, T.; Sun, S.; Takami, H.; Teshima, M.; Wagner, R.M.; Wetteskind, H.; Barnstedt, J.; Bonardi, A.; Dick, J.; Gäbele, W.; Kalkuhl, C.; Kendziorra, E.; Luz, O.; Pühlhofer, G.; Renner, S.; Santangelo, A.; Schanz, T.; Schwarzburg, S.; Tenzer, C.; Spanier, F.; Tibolla, O.; Bais, A.; Balis, D.; Eleftheriadis, C.; Gianakaki, E.; Kokkotas, K.; Liolios, A.; Nikolaidis, A.; Seiradakis, J.; Stergioulas, N.; Vlahos, L.; Mastichiadis, A.; Vlahakis, N.; Aravantinos, A.; Farakos, K.; Fokitis, E.; Maltezos, S.; Aharonian, F.; Drury, L.; Agnetta, G.; Catalano, O.; Cusumano, G.; Giarrusso, S.; La Barbera, N.; La Parola, V.; La Rosa, G.; Maccarone, M.C.; Mangano, A.; Mineo, T.; Romano, P.; Russo, F.; Sacco, B.; Vercellone, S.; Di Pierro, F.; Morello, C.; Vallania, P.; Cavazzani, S.; Zitelli, V.; Basso, S.; Canestrari, R.; Cantu, S.; Casiraghi, M.; Conconi, P.; Covino, S.; Ghigo, M.; Motta, G.; Pareschi, G.; Salini, A.; Spiga, D.; Tagliaferri, G.; Belluso, M.; Billotta, S.; Bonanno, G.; Giro, E.; Lessio, L.; Antonelli, L.A.; Carosi, A.; Di Paolo, A.; Fontana, A.; Testa, V.; Tavani, M.; Ghedina, A.; Molinari, E.; Tosti, G.; Bastieri, D.; Busetto, G.; Buson, S.; Corti, D.; Doro, M.; Giubilato, P.; Lombardi, S.; Mariotti, M.; Mattiazzo, S.; Paiano, S.; Pepato, A.; Pivato, G.; Prandini, E.; Rando, R.; Saggion, A.; Scalzotto, V.; Scarcioffolo, M.; Schultz, C.; Tibaldo, L.; Meucci, M.; Paoletti, R.; Stamerra, A.; Angelis, A.d.; de Lotto, B.; Scapin, V.; Dazzi, F.; Persic, M.; Bamba, A.; Sakaki, N.; Shibata, T.; Yamaoka, K.; Yamazaki, R.; Yoshida, A.; Fukazawa, Y.; Kakuwa, J.; Mizuno, T.; Yonetani, M.; Takahashi, H.; Katagiri, H.; Yanagita, S.; Yoshida, T.; Okumura, A.; Ioka, K.; Kawanaka, N.; Kohri, K.; Nakayama, K.; Ohira, Y.; Tanaka, M.; Chikawa, M.; Muraishi, H.; Yamamoto, T.; Hayashida, M.; Inoue, S.; Totani, T.; Kubo, H.; Tanimori, T.; Nagataki, S.; Mori, K.; Takahashi, K.; Matsumoto, H.; Tajima, H.; Fujita, Y.; Toma, K.; Terada, Y.; Kodani, K.; Kushida, J.; Nishijima, K.; Kabuki, S.; Orito, R.; Sugawara, R.; Asano, K.; Enomoto, R.; Inoue, Y.; Kifune, T.; Murase, K.; Ohishi, M.; Ohka, H.; Yoshikoshi, T.; Nakamori, T.; Gunji, S.; Hagiwara, R.; Tokanai, F.; Hara, S.; Naito, T.; Steenkamp, R.; Vink, J.; Markoff, S.; Bednarek, W.; Niedźwiecki, A.; Sitarek, J.; Sobczyńska, D.; Szanecki, M.; Bogacz, L.; Kozioł, J.; Małkiewicz, P.; Ostrowski, M.; Piechocki, W.; Stawarz, Ł.; Szostek, A.; Wierzcholska, A.; Zagdański, A.; Ziȩtara, K.; Bulik, T.; Cieślar, M.; Gochna, M.; Grudzińska, M.; Kapala, M.; Pojmański, G.; Suchenek, M.; Bajtlik, S.; Barnacka, A.; Borkowski, J.; Dyks, J.; Janiak, M.; Kluźniak, W.; Lubiński, P.; Moderski, R.; Rudak, B.; Sikora, M.; Zajczyk, A.; Zdziarski, A.; Dyrda, M.; Kotuła, J.; Michałowski, J.; Niemiec, J.; Stodulski, M.; Ziółkowski, P.; Zychowski, P.; Katarzyński, K.; Ciesielska, M.; Grygorczuk, J.; Karczewski, M.; Kȩdziora, B.; Płatos, Ł.; Rataj, M.; Seweryn, K.; Tokarz, M.; Wawer, P.; Wawrzaszek, R.; Wiśniewski, Ł.; Kasperek, J.; Rajda, P.; Wolczko, A.; Oziȩbło, A.; Szepieniec, T.; de Jager, O.; van der Walt, J.; Becerra, J.; Berger, K.; López, R.J.G.; Herrero, A.; Conde, M.Á.S.; Berdugo, J.; Carmona, E.; Delgado, C.; Díaz, C.; Mañá, C.; Marín, J.; Martínez, G.; Colomé, J.; de Cea del Pozo, E.; Hadasch, D.; Pedaletti, G.; Torres, D.F.; Rico, J.; Aleksić, J.; Barceló, M.; Blanch, O.; Boix, J.; Cortina, J.; Firpo, R.; Gaweda, J.; Giavitto, G.; González, A.; Grañena, F.; Illa, J.M.; Klepser, S.; López, A.; Martínez, M.; Mazin, D.; Moralejo, A.; Stamatescu, V.; Baixeras, C.; Font, L.; Garrido, D.; Gaug, M.; Munar, P.; Paredes, J.M.; Ribó, M.; Zabalza, V.; Garrido, L.; Gascón, D.; Graciani, R.; Sanuy, A.; Antoranz, P.; Bernardino, T.; Fresnillo, L.; Miranda, J.M.; Vegas, I.; Barrio, J.A.; Contreras, J.L.; Dubois, F.; Hassan, T.; Mirabal, N.; Salazar, E.; Tejedor, L.A.; de la Calle Pérez, I.; Ibarra, A.; Ponz, J.D.; Dravins, D.; Ingjald, J.; Jensen, H.; Conrad, J.; Dickinson, H.; Finley, C.; Hultquist, K.; Ripken, J.; Fransson, C.; Ryde, F.; Botner, O.; Hallgren, A.; Bretz, T.; Ribordy, M.; Biland, A.; Braun, I.; Grimm, O.; Krähenbühl, T.; Roeser, U.; Vogler, P.; von Gunten, H.P.; Weitzel, Q.; Dorner, D.; Farnier, C.; Lenain, J.-P.; Lyard, E.; Walter, R.; Florin, D.; Gadola, A.; Gredig, R.; Huber, B.; Manalaysay, A.; Steiner, S.; Straumann, U.; Vollhardt, A.; Allan, D.; Chadwick, P.M.; Daniel, M.K.; Knappy, A.R.; McComb, T.J.L.; Nolan, S.J.; Rulten, C.B.; Schmoll, J.; Talbot, R.G.; Blake, S.; Parsons, R.D.; Fraser, G.W.; Hinton, J.A.; O'Brien, P.T.; Osborne, J.P.; Starling, R.L.C.; Warwick, R.; White, R.; Wilkinson, M.I.; Greenshaw, T.; Sutcliffe, P.; Green, A.; Ghag, C.; Murphy, A.S.; Kudryavtsev, V.A.; Granot, J.; Hardcastle, M.J.; McCubbin, N.; Preece, R.; Bird, T.; Croston, J.H.; Emmanoulopoulos, D.; Maccarone, T.; McHardy, I.; Cotter, G.; Karastergiou, A.; Mertsch, P.; Potter, W.; Sarkar, S.; Silk, J.; Byrum, K.; Guarino, V.; Wagner, B.; Krennrich, F.; Orr, M.; Weinstein, A.; Konopelko, A.; Smith, N.; Xiong, Q.; Bechtol, K.; Bühler, R.; Cameron, R.; Chiang, J.; Digel, S.W.; Dubois, R.; Funk, S.; Glanzman, T.; Sapozhnikov, L.; Vandenbroucke, J.; Wood, M.; Benbow, W.; Galante, N.; Schroedter, M.; Briggs, M.S.; Connaughton, V.; Arlen, T.; Bobkov, A.A.; Majumdar, P.; Ong, R.A.; Vassiliev, V.V.; Bouvier, A.; Otte, A.N.; Williams, D.A.; Bogdan, M.; Huan, H.; Humensky, T.B.; Wakely, S.P.; Kieda, D.; Beilicke, M.; Buckley, J.H.; Bugaev, V.; Krawczynski, H.; Grube, J.; Gyuk, G.; Falcone, A.D.; Finley, J.P.; Ferenc, D.; Fortson, L.; Karlsson, N.; Aliu, E.; Errando, M.; Mukherjee, R.; Kaaret, P.; Coppi, P.; Szymkowiak, A.; Knapp, J. (2011-12-01)
    Ground-based gamma-ray astronomy has had a major breakthrough with the impressive results obtained using systems of imaging atmospheric Cherenkov telescopes. Ground-based gamma-ray astronomy has a huge potential in ...
  • Schawinski, K.; Lintott, C.J.; Kaviraj, S.; Silk, J.; Zuntz, J.; Bayet, E.; Thomas, D.; Maraston, C.; Viti, S.; Sarzi, M.; Yi, S.K.; Joo, S-J.; Daddi, E.; Bell, T. (2009)
    Residual star formation at late times in early-type galaxies and their progenitors must be suppressed in order to explain the population of red, passively evolving systems we see today. Likewise, residual or newly accreted ...

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