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1. Implications For The Origin Of GRB 051103 From LIGO Observations

Author: The LIGO Scientific Collaboration, Abadie, J., Abbott, B. P., Abbott, T. D., Abbott, R., Abernathy, M., Adams, C., Adhikari, R., Affeldt, C., Ajith, P., Allen, B., Allen, G. S., Ceron, E. Amador, Amariutei, D., Amin, R. S., Anderson, S. B., Anderson, W. G., Arai, K., Arain, M. A., Araya, M. C., Aston, S. M., Atkinson, D., Aufmuth, P., Aulbert, C., Aylott, B. E., Babak, S., Baker, P., Ballmer, S., Barker, D., Barnum, S., Barr, B., Barriga, P., Barsotti, L., Barton, M. A., Bartos, I., Bassiri, R., Bastarrika, M., Bauchrowitz, J., Behnke, B., Bell, A. S., Belopolski, I., Benacquista, M., Bertolini, A., Betzwieser, J., Beveridge, N., Beyersdorf, P. T., Bilenko, I. A., Billingsley, G., Birch, J., Biswas, R., Black, E., Blackburn, J. K., Blackburn, L., Blair, D., Bland, B., Bock, O., Bodiya, T. P., Bogan, C., Bondarescu, R., Bork, R., Born, M., Bose, S., Boyle, M., Brady, P. R., Braginsky, V. B., Brau, J. E., Breyer, J., Bridges, D. O., Brinkmann, M., Britzger, M., Brooks, A. F., Brown, D. A., Brummitt, A., Buonanno, A., Burguet-Castell, J., Burmeister, O., Byer, R. L., Cadonati, L., Camp, J. B., Campsie, P., Cannizzo, J., Cannon, K., Cao, J., Capano, C., Caride, S., Caudill, S., Cavaglia, M., Cepeda, C., Chalermsongsak, T., Chalkley, E., Charlton, P., Chelkowski, S., Chen, Y., Christensen, N., Chua, S. S. Y., Chung, S., Chung, C. T. Y., Clara, F., Clark, D., Clark, J., Clayton, J. H., Conte, R., Cook, D., Corbitt, T. R. C., Cornish, N., Costa, C. A., Coughlin, M., Coward, D. M., Coyne, D. C., Creighton, J. D. E., Creighton, T. D., Cruise, A. M., Cumming, A., Cunningham, L., Culter, R. M., Dahl, K., Danilishin, S. L., Dannenberg, R., Danzmann, K., Das, K., Daudert, B., Daveloza, H., Davies, G., Daw, E. J., Dayanga, T., DeBra, D., Degallaix, J., Dent, T., Dergachev, V., DeRosa, R., DeSalvo, R., Dhurandhar, S., Di Palma, I., Diaz, M., Donovan, F., Dooley, K. L., Dorsher, S., Douglas, E. S. D., Drever, R. W. P., Driggers, J. C., Dumas, J. -C., Dwyer, S., Eberle, T., Edgar, M., Edwards, M., Effler, A., Ehrens, P., Engel, R., Etzel, T., Evans, M., Evans, T., Factourovich, M., Fairhurst, S., Fan, Y., Farr, B. F., Fazi, D., Fehrmann, H., Feldbaum, D., Finn, L. S., Flanigan, M., Foley, S., Forsi, E., Fotopoulos, N., Frede, M., Frei, M., Frei, Z., Freise, A., Frey, R., Fricke, T. T., Friedrich, D., Fritschel, P., Frolov, V. V., Fulda, P., Fyffe, M., Garcia, J., Garofoli, J. A., Gholami, I., Ghosh, S., Giaime, J. A., Giampanis, S., Giardina, K. D., Gill, C., Goetz, E., Goggin, L. M., Gonzalez, G., Gorodetsky, M. L., Gossler, S., Graef, C., Grant, A., Gras, S., Gray, C., Greenhalgh, R. J. S., Gretarsson, A. M., Grosso, R., Grote, H., Grunewald, S., Guido, C., Gupta, R., Gustafson, E. K., Gustafson, R., Hage, B., Hallam, J. M., Hammer, D., Hammond, G., Hanks, J., Hanna, C., Hanson, J., Harms, J., Harry, G. M., Harry, I. W., Harstad, E. D., Hartman, M. T., Haughian, K., Hayama, K., Heefner, J., Hendry, M. A., Heng, I. S., Heptonstall, A. W., Herrera, V., Hewitson, M., Hild, S., Hoak, D., Hodge, K. A., Holt, K., Hong, T., Hooper, S., Hosken, D. J., Hough, J., Howell, E. J., Hughey, B., Husa, S., Huttner, S. H., Ingram, D. R., Inta, R., Isogai, T., Ivanov, A., Johnson, W. W., Jones, D. I., Jones, G., Jones, R., Ju, L., Kalmus, P., Kalogera, V., Kandhasamy, S., Kanner, J. B., Katsavounidis, E., Katzman, W., Kawabe, K., Kawamura, S., Kawazoe, F., Kells, W., Kelner, M., Keppel, D. G., Khalaidovski, A., Khalili, F. Y., Khazanov, E. A., Kim, N., Kim, H., King, P. J., Kinzel, D. L., Kissel, J. S., Klimenko, S., Kondrashov, V., Kopparapu, R., Koranda, S., Korth, W. Z., Kozak, D., Kringel, V., Krishnamurthy, S., Krishnan, B., Kuehn, G., Kumar, R., Kwee, P., Landry, M., Lantz, B., Lastzka, N., Lazzarini, A., Leaci, P., Leong, J., Leonor, I., Li, J., Lindquist, P. E., Lockerbie, N. A., Lodhia, D., Lormand, M., Lu, P., Luan, J., Lubinski, M., Luck, H., Lundgren, A. P., Macdonald, E., Machenschalk, B., MacInnis, M., Mageswaran, M., Mailand, K., Mandel, I., Mandic, V., Marandi, A., Marka, S., Marka, Z., Maros, E., Martin, I. W., Martin, R. M., Marx, J. N., Mason, K., Matichard, F., Matone, L., Matzner, R. A., Mavalvala, N., McCarthy, R., McClelland, D. E., McGuire, S. C., McIntyre, G., McIver, J., McKechan, D. J. A., Meadors, G., Mehmet, M., Meier, T., Melatos, A., Melissinos, A. C., Mendell, G., Mercer, R. A., Meshkov, S., Messenger, C., Meyer, M. S., Miao, H., Miller, J., Mino, Y., Mitrofanov, V. P., Mitselmakher, G., Mittleman, R., Miyakawa, O., Moe, B., Moesta, P., Mohanty, S. D., Moraru, D., Moreno, G., Mossavi, K., Mow-Lowry, C. M., Mueller, G., Mukherjee, S., Mullavey, A., Muller-Ebhardt, H., Munch, J., Murphy, D., Murray, P. G., Nash, T., Nawrodt, R., Nelson, J., Newton, G., Nishizawa, A., Nolting, D., Nuttall, L., O'Reilly, B., O'Shaughnessy, R., Ochsner, E., O'Dell, J., Ogin, G. H., Oldenburg, R. G., Osthelder, C., Ott, C. D., Ottaway, D. J., Ottens, R. S., Overmier, H., Owen, B. J., Page, A., Pan, Y., Pankow, C., Papa, M. A., Patel, P., Pedraza, M., Pekowsky, L., Penn, S., Peralta, C., Perreca, A., Phelps, M., Pickenpack, M., Pinto, I. M., Pitkin, M., Pletsch, H. J., Plissi, M. V., Podkaminer, J., Pold, J., Postiglione, F., Predoi, V., Price, L. R., Prijatelj, M., Principe, M., Privitera, S., Prix, R., Prokhorov, L., Puncken, O., Quetschke, V., Raab, F. J., Radkins, H., Raffai, P., Rakhmanov, M., Ramet, C. R., Rankins, B., Mohapatra, S. R. P., Raymond, V., Redwine, K., Reed, C. M., Reed, T., Reid, S., Reitze, D. H., Riesen, R., Riles, K., Roberts, P., Robertson, N. A., Robinson, C., Robinson, E. L., Roddy, S., Rollins, J., Romano, J. D., Romie, J. H., Rover, C., Rowan, S., Rudiger, A., Ryan, K., Sakata, S., Sakosky, M., Salemi, F., Salit, M., Sammut, L., de la Jordana, L. Sancho, Sandberg, V., Sannibale, V., SantamarÌa, L., Santiago-Prieto, I., Santostasi, G., Saraf, S., Sathyaprakash, B. S., Sato, S., Saulson, P. R., Savage, R., Schilling, R., Schlamminger, S., Schnabel, R., Schofield, R. M. S., Schulz, B., Schutz, B. F., Schwinberg, P., Scott, J., Scott, S. M., Searle, A. C., Seifert, F., Sellers, D., Sengupta, A. S., Sergeev, A., Shaddock, D. A., Shaltev, M., Shapiro, B., Shawhan, P., Weerathunga, T. Shihan, Shoemaker, D. H., Sibley, A., Siemens, X., Sigg, D., Singer, A., Singer, L., Sintes, A. M., Skelton, G., Slagmolen, B. J. J., Slutsky, J., Smith, R., Smith, J. R., Smith, M. R., Smith, N. D., Somiya, K., Sorazu, B., Soto, J., Speirits, F. C., Stein, A. J., Steinlechner, J., Steinlechner, S., Steplewski, S., Stefszky, M., Stochino, A., Stone, R., Strain, K. A., Strigin, S., Stroeer, A. S., Stuver, A. L., Summerscales, T. Z., Sung, M., Susmithan, S., Sutton, P. J., Szokoly, G. P., Talukder, D., Tanner, D. B., Tarabrin, S. P., Taylor, J. R., Taylor, R., Thomas, P., Thorne, K. A., Thorne, K. S., Thrane, E., Thuring, A., Tokmakov, K. V., Torres, C., Torrie, C. I., Traylor, G., Trias, M., Tseng, K., Ugolini, D., Urbanek, K., Vahlbruch, H., Vaishnav, B., Vallisneri, M., Broeck, C. Van Den, van der Sluys, M. V., van Veggel, A. A., Vass, S., Vaulin, R., Vecchio, A., Veitch, J., Veitch, P. J., Veltkamp, C., Villar, A. E., Vorvick, C., Vyachanin, S. P., Waldman, S. J., Wallace, L., Wanner, A., Ward, R. L., Wei, P., Weinert, M., Weinstein, A. J., Weiss, R., Wen, L., Wen, S., Wessels, P., West, M., Westphal, T., Wette, K., Whelan, J. T., Whitcomb, S. E., White, D., Whiting, B. F., Wilkinson, C., Willems, P. A., Williams, H. R., Williams, L., Willke, B., Winkelmann, L., Winkler, W., Wipf, C. C., Wiseman, A. G., Woan, G., Wooley, R., Worden, J., Yablon, J., Yakushin, I., Yamamoto, K., Yamamoto, H., Yang, H., Yeaton-Massey, D., Yoshida, S., Yu, P., Zanolin, M., Zhang, L., Zhang, Z., Zhao, C., Zotov, N., Zucker, M. E., Zweizig, J., Bizouard, M. A., Dietz, A., Guidi, G. M., and Was, M.
Subjects: Astrophysics - High Energy Astrophysical Phenomena, General Relativity and Quantum Cosmology
Abstract: We present the results of a LIGO search for gravitational waves (GWs) associated with GRB 051103, a short-duration hard-spectrum gamma-ray burst (GRB) whose electromagnetically determined sky position is coincident with the spiral galaxy M81, which is 3.6 Mpc from Earth. Possible progenitors for short-hard GRBs include compact object mergers and soft gamma repeater (SGR) giant flares. A merger progenitor would produce a characteristic GW signal that should be detectable at the distance of M81, while GW emission from an SGR is not expected to be detectable at that distance. We found no evidence of a GW signal associated with GRB 051103. Assuming weakly beamed gamma-ray emission with a jet semi-angle of 30 deg we exclude a binary neutron star merger in M81 as the progenitor with a confidence of 98%. Neutron star-black hole mergers are excluded with > 99% confidence. If the event occurred in M81 our findings support the the hypothesis that GRB 051103 was due to an SGR giant flare, making it the most distant extragalactic magnetar observed to date., Comment: 8 pages, 3 figures. For a repository of data used in the publication, go to: https://dcc.ligo.org/cgi-bin/DocDB/ShowDocument?docid=15166 . Also see the announcement for this paper on ligo.org at: http://www.ligo.org/science/Publication-GRB051103/index.php
Published: 2012
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2. Beating the spin-down limit on gravitational wave emission from the Vela pulsar

Author: The LIGO Scientific Collaboration, the Virgo Collaboration, Abadie, J., Abbott, B. P., Abbott, R., Abernathy, M., Accadia, T., Acernese, F., Adams, C., Adhikari, R., Affeldt, C., Allen, B., Allen, G. S., Ceron, E. Amador, Amariutei, D., Amin, R. S., Anderson, S. B., Anderson, W. G., Antonucci, F., Arai, K., Arain, M. A., Araya, M. C., Aston, S. M., Astone, P., Atkinson, D., Aufmuth, P., Aulbert, C., Aylott, B. E., Babak, S., Baker, P., Ballardin, G., Ballmer, S., Barker, D., Barnum, S., Barone, F., Barr, B., Barriga, P., Barsotti, L., Barsuglia, M., Barton, M. A., Bartos, I., Bassiri, R., Bastarrika, M., Basti, A., Bauchrowitz, J., Bauer, Th. S., Behnke, B., Bejger, M., Beker, M. G., Bell, A. S., Belletoile, A., Belopolski, I., Benacquista, M., Bertolini, A., Betzwieser, J., Beveridge, N., Beyersdorf, P. T., Bilenko, I. A., Billingsley, G., Birch, J., Birindelli, S., Biswas, R., Bitossi, M., Bizouard, M. A., Black, E., Blackburn, J. K., Blackburn, L., Blair, D., Bland, B., Blom, M., Bock, O., Bodiya, T. P., Bogan, C., Bondarescu, R., Bondu, F., Bonelli, L., Bonnand, R., Bork, R., Born, M., Boschi, V., Bose, S., Bosi, L., Bouhou, B., Boyle, M., Braccini, S., Bradaschia, C., Brady, P. R., Braginsky, V. B., Brau, J. E., Breyer, J., Bridges, D. O., Brillet, A., Brinkmann, M., Brisson, V., Britzger, M., Brooks, A. F., Brown, D. A., Brummit, A., Budzyński, R., Bulik, T., Bulten, H. J., Buonanno, A., Burguet--Castell, J., Burmeister, O., Buskulic, D., Buy, C., Byer, R. L., Cadonati, L., Cagnoli, G., Cain, J., Calloni, E., Camp, J. B., Campagna, E., Campsie, P., Cannizzo, J., Cannon, K., Canuel, B., Cao, J., Capano, C., Carbognani, F., Caride, S., Caudill, S., Cavaglià, M., Cavalier, F., Cavalieri, R., Cella, G., Cepeda, C., Cesarini, E., Chaibi, O., Chalermsongsak, T., Chalkley, E., Charlton, P., Chassande-Mottin, E., Chelkowski, S., Chen, Y., Chincarini, A., Christensen, N., Chua, S. S. Y., Chung, C. T. Y., Chung, S., Clara, F., Clark, D., Clark, J., Clayton, J. H., Cleva, F., Coccia, E., Colacino, C. N., Colas, J., Colla, A., Colombini, M., Conte, R., Cook, D., Corbitt, T. R., Cornish, N., Corsi, A., Costa, C. A., Coughlin, M., Coulon, J. -P., Coward, D. M., Coyne, D. C., Creighton, J. D. E., Creighton, T. D., Cruise, A. M., Culter, R. M., Cumming, A., Cunningham, L., Cuoco, E., Dahl, K., Danilishin, S. L., Dannenberg, R., D'Antonio, S., Danzmann, K., Das, K., Dattilo, V., Daudert, B., Daveloza, H., Davier, M., Davies, G., Daw, E. J., Day, R., Dayanga, T., De Rosa, R., DeBra, D., Debreczeni, G., Degallaix, J., del Prete, M., Dent, T., Dergachev, V., DeRosa, R., DeSalvo, R., Dhurandhar, S., Di Fiore, L., Di Lieto, A., Di Palma, I., Emilio, M. Di Paolo, Di Virgilio, A., Díaz, M., Dietz, A., Donovan, F., Dooley, K. L., Dorsher, S., Douglas, E. S. D., Drago, M., Drever, R. W. P., Driggers, J. C., Dumas, J. -C., Dwyer, S., Eberle, T., Edgar, M., Edwards, M., Effler, A., Ehrens, P., Engel, R., Etzel, T., Evans, M., Evans, T., Factourovich, M., Fafone, V., Fairhurst, S., Fan, Y., Farr, B. F., Fazi, D., Fehrmann, H., Feldbaum, D., Ferrante, I., Fidecaro, F., Finn, L. S., Fiori, I., Flaminio, R., Flanigan, M., Foley, S., Forsi, E., Forte, L. A., Fotopoulos, N., Fournier, J. -D., Franc, J., Frasca, S., Frasconi, F., Frede, M., Frei, M., Frei, Z., Freise, A., Frey, R., Fricke, T. T., Friedrich, D., Fritschel, P., Frolov, V. V., Fulda, P., Fyffe, M., Galimberti, M., Gammaitoni, L., Garcia, J., Garofoli, J. A., Garufi, F., Gáspár, M. E., Gemme, G., Genin, E., Gennai, A., Ghosh, S., Giaime, J. A., Giampanis, S., Giardina, K. D., Giazotto, A., Gill, C., Goetz, E., Goggin, L. M., González, G., Gorodetsky, M. L., Goßler, S., Gouaty, R., Graef, C., Granata, M., Grant, A., Gras, S., Gray, C., Greenhalgh, R. J. S., Gretarsson, A. M., Greverie, C., Grosso, R., Grote, H., Grunewald, S., Guidi, G. M., Guido, C., Gupta, R., Gustafson, E. K., Gustafson, R., Hage, B., Hallam, J. M., Hammer, D., Hammond, G., Hanks, J., Hanna, C., Hanson, J., Harms, J., Harry, G. M., Harry, I. W., Harstad, E. D., Hartman, M. T., Haughian, K., Hayama, K., Hayau, J. -F., Hayler, T., Heefner, J., Heitmann, H., Hello, P., Hendry, M. A., Heng, I. S., Heptonstall, A. W., Herrera, V., Hewitson, M., Hild, S., Hoak, D., Hodge, K. A., Holt, K., Hong, T., Hooper, S., Hosken, D. J., Hough, J., Howell, E. J., Huet, D., Hughey, B., Husa, S., Huttner, S. H., Ingram, D. R., Inta, R., Isogai, T., Ivanov, A., Jaranowski, P., Johnson, W. W., Jones, D. I., Jones, G., Jones, R., Ju, L., Kalmus, P., Kalogera, V., Kandhasamy, S., Kanner, J. B., Katsavounidis, E., Katzman, W., Kawabe, K., Kawamura, S., Kawazoe, F., Kells, W., Kelner, M., Keppel, D. G., Khalaidovski, A., Khalili, F. Y., Khazanov, E. A., Kim, H., Kim, N., King, P. J., Kinzel, D. L., Kissel, J. S., Klimenko, S., Kondrashov, V., Kopparapu, R., Koranda, S., Korth, W. Z., Kowalska, I., Kozak, D., Kringel, V., Krishnamurthy, S., Krishnan, B., Królak, A., Kuehn, G., Kumar, R., Kwee, P., Landry, M., Lantz, B., Lastzka, N., Lazzarini, A., Leaci, P., Leong, J., Leonor, I., Leroy, N., Letendre, N., Li, J., Li, T. G. F., Liguori, N., Lindquist, P. E., Lockerbie, N. A., Lodhia, D., Lorenzini, M., Loriette, V., Lormand, M., Losurdo, G., Lu, P., Luan, J., Lubinski, M., Lück, H., Lundgren, A. P., Macdonald, E., Machenschalk, B., MacInnis, M., Mageswaran, M., Mailand, K., Majorana, E., Maksimovic, I., Man, N., Mandel, I., Mandic, V., Mantovani, M., Marandi, A., Marchesoni, F., Marion, F., Márka, S., Márka, Z., Maros, E., Marque, J., Martelli, F., Martin, I. W., Martin, R. M., Marx, J. N., Mason, K., Masserot, A., Matichard, F., Matone, L., Matzner, R. A., Mavalvala, N., McCarthy, R., McClelland, D. E., McGuire, S. C., McIntyre, G., McKechan, D. J. A., Meadors, G., Mehmet, M., Meier, T., Melatos, A., Melissinos, A. C., Mendell, G., Mercer, R. A., Merill, L., Meshkov, S., Messenger, C., Meyer, M. S., Miao, H., Michel, C., Milano, L., Miller, J., Minenkov, Y., Mino, Y., Mitrofanov, V. P., Mitselmakher, G., Mittleman, R., Miyakawa, O., Moe, B., Moesta, P., Mohan, M., Mohanty, S. D., Mohapatra, S. R. P., Moraru, D., Moreno, G., Morgado, N., Morgia, A., Mosca, S., Moscatelli, V., Mossavi, K., Mours, B., Mow--Lowry, C. M., Mueller, G., Mukherjee, S., Mullavey, A., Müller-Ebhardt, H., Munch, J., Murray, P. G., Nash, T., Nawrodt, R., Nelson, J., Neri, I., Newton, G., Nishida, E., Nishizawa, A., Nocera, F., Nolting, D., Ochsner, E., O'Dell, J., Ogin, G. H., Oldenburg, R. G., O'Reilly, B., O'Shaughnessy, R., Osthelder, C., Ott, C. D., Ottaway, D. J., Ottens, R. S., Overmier, H., Owen, B. J., Page, A., Pagliaroli, G., Palladino, L., Palomba, C., Pan, Y., Pankow, C., Paoletti, F., Papa, M. A., Parameswaran, A., Pardi, S., Parisi, M., Pasqualetti, A., Passaquieti, R., Passuello, D., Patel, P., Pathak, D., Pedraza, M., Pekowsky, L., Penn, S., Peralta, C., Perreca, A., Persichetti, G., Phelps, M., Pichot, M., Pickenpack, M., Piergiovanni, F., Pietka, M., Pinard, L., Pinto, I. M., Pitkin, M., Pletsch, H. J., Plissi, M. V., Podkaminer, J., Poggiani, R., Pöld, J., Postiglione, F., Prato, M., Predoi, V., Price, L. R., Prijatelj, M., Principe, M., Privitera, S., Prix, R., Prodi, G. A., Prokhorov, L., Puncken, O., Punturo, M., Puppo, P., Quetschke, V., Raab, F. J., Rabeling, D. S., Rácz, I., Radkins, H., Raffai, P., Rakhmanov, M., Ramet, C. R., Rankins, B., Rapagnani, P., Raymond, V., Re, V., Redwine, K., Reed, C. M., Reed, T., Regimbau, T., Reid, S., Reitze, D. H., Ricci, F., Riesen, R., Riles, K., Roberts, P., Robertson, N. A., Robinet, F., Robinson, C., Robinson, E. L., Rocchi, A., Roddy, S., Rolland, L., Rollins, J., Romano, J. D., Romano, R., Romie, J. H., Rosińska, D., Röver, C., Rowan, S., Rüdiger, A., Ruggi, P., Ryan, K., Sakata, S., Sakosky, M., Salemi, F., Salit, M., Sammut, L., de la Jordana, L. Sancho, Sandberg, V., Sannibale, V., Santamaría, L., Santiago-Prieto, I., Santostasi, G., Saraf, S., Sassolas, B., Sathyaprakash, B. S., Sato, S., Satterthwaite, M., Saulson, P. R., Savage, R., Schilling, R., Schlamminger, S., Schnabel, R., Schofield, R. M. S., Schulz, B., Schutz, B. F., Schwinberg, P., Scott, J., Scott, S. M., Searle, A. C., Seifert, F., Sellers, D., Sengupta, A. S., Sentenac, D., Sergeev, A., Shaddock, D. A., Shaltev, M., Shapiro, B., Shawhan, P., Weerathunga, T. Shihan, Shoemaker, D. H., Sibley, A., Siemens, X., Sigg, D., Singer, A., Singer, L., Sintes, A. M., Skelton, G., Slagmolen, B. J. J., Slutsky, J., Smith, J. R., Smith, M. R., Smith, N. D., Smith, R., Somiya, K., Sorazu, B., Soto, J., Speirits, F. C., Sperandio, L., Stefszky, M., Stein, A. J., Steinlechner, J., Steinlechner, S., Steplewski, S., Stochino, A., Stone, R., Strain, K. A., Strigin, S., Stroeer, A. S., Sturani, R., Stuver, A. L., Summerscales, T. Z., Sung, M., Susmithan, S., Sutton, P. J., Swinkels, B., Szokoly, G. P., Tacca, M., Talukder, D., Tanner, D. B., Tarabrin, S. P., Taylor, J. R., Taylor, R., Thomas, P., Thorne, K. A., Thorne, K. S., Thrane, E., Thüring, A., Titsler, C., Tokmakov, K. V., Toncelli, A., Tonelli, M., Torre, O., Torres, C., Torrie, C. I., Tournefier, E., Travasso, F., Traylor, G., Trias, M., Tseng, K., Turner, L., Ugolini, D., Urbanek, K., Vahlbruch, H., Vaishnav, B., Vajente, G., Vallisneri, M., Brand, J. F. J. van den, Broeck, C. Van Den, van der Putten, S., van der Sluys, M. V., van Veggel, A. A., Vass, S., Vasuth, M., Vaulin, R., Vavoulidis, M., Vecchio, A., Vedovato, G., Veitch, J., Veitch, P. J., Veltkamp, C., Verkindt, D., Vetrano, F., Viceré, A., Villar, A. E., Vinet, J. -Y., Vocca, H., Vorvick, C., Vyachanin, S. P., Waldman, S. J., Wallace, L., Wanner, A., Ward, R. L., Was, M., Wei, P., Weinert, M., Weinstein, A. J., Weiss, R., Wen, L., Wen, S., Wessels, P., West, M., Westphal, T., Wette, K., Whelan, J. T., Whitcomb, S. E., White, D., Whiting, B. F., Wilkinson, C., Willems, P. A., Williams, H. R., Williams, L., Willke, B., Winkelmann, L., Winkler, W., Wipf, C. C., Wiseman, A. G., Woan, G., Wooley, R., Worden, J., Yablon, J., Yakushin, I., Yamamoto, H., Yamamoto, K., Yang, H., Yeaton-Massey, D., Yoshida, S., Yu, P., Yvert, M., Zanolin, M., Zhang, L., Zhang, Z., Zhao, C., Zotov, N., Zucker, M. E., Zweizig, J., Buchner, S., Hotan, A., and Palfreyman, J.
Subjects: Astrophysics - High Energy Astrophysical Phenomena, General Relativity and Quantum Cosmology
Abstract: We present direct upper limits on continuous gravitational wave emission from the Vela pulsar using data from the Virgo detector's second science run. These upper limits have been obtained using three independent methods that assume the gravitational wave emission follows the radio timing. Two of the methods produce frequentist upper limits for an assumed known orientation of the star's spin axis and value of the wave polarization angle of, respectively, $1.9\ee{-24}$ and $2.2\ee{-24}$, with 95% confidence. The third method, under the same hypothesis, produces a Bayesian upper limit of $2.1\ee{-24}$, with 95% degree of belief. These limits are below the indirect {\it spin-down limit} of $3.3\ee{-24}$ for the Vela pulsar, defined by the energy loss rate inferred from observed decrease in Vela's spin frequency, and correspond to a limit on the star ellipticity of $\sim 10^{-3}$. Slightly less stringent results, but still well below the spin-down limit, are obtained assuming the star's spin axis inclination and the wave polarization angles are unknown., Comment: 37 pages, 6 figures corrected typo in the Authors field
Published: 2011
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3. Search for Gravitational Wave Bursts from Six Magnetars

Author: Abadie, J., Abbott, B. P., Abbott, R., Abernathy, M., Accadia, T., Acerneseac, F., Adams, C., Adhikari, R., Affeldt, C., Allen, B., Allen, G. S., Ceron, E. Amador, Amariutei, D., Amin, R. S., Anderson, S. B., Anderson, W. G., Antonuccia, F., Arai, K., Arain, M. A., Araya, M. C., Aston, S. M., Astonea, P., Atkinson, D., Aufmuth, P., Aulbert, C., Aylott, B. E., Babak, S., Baker, P., Ballardin, G., Ballmer, S., Barker, D., Barnum, S., Baroneac, F., Barr, B., Barriga, P., Barsotti, L., Barsuglia, M., Barton, M. A., Bartos, I., Bassiri, R., Bastarrika, M., Bastiab, A., Bauchrowitz, J., Bauera, Th. S., Behnke, B., Bekera, M. G., Bell, A. S., Belletoile, A., Belopolski, I., Benacquista, M., Bertolini, A., Betzwieser, J., Beveridge, N., Beyersdorf, P. T., Bilenko, I. A., Billingsley, G., Birch, J., Birindellia, S., Biswas, R., Bitossia, M., Bizouarda, M. A., Black, E., Blackburn, J. K., Blackburn, L., Blair, D., Bland, B., Bloma, M., Bock, O., Bodiya, T. P., Bogan, C., Bondarescu, R., Bondub, F., Bonelliab, L., Bonnand, R., Bork, R., Born, M., Boschia, V., Bose, S., Bosia, L., Bouhou, B., Boyle, M., Braccinia, S., Bradaschiaa, C., Brady, P. R., Braginsky, V. B., Brau, J. E., Breyer, J., Bridges, D. O., Brilleta, A., Brinkmann, M., Brissona, V., Britzger, M., Brooks, A. F., Brown, D. A., Brummit, A., Budzyńskib, R., Bulikbc, T., Bultenab, H. J., Buonanno, A., Burguet--Castell, J., Burmeister, O., Buskulic, D., Buy, C., Byer, R. L., Cadonati, L., Cagnolia, G., Cain, J., Calloniab, E., Camp, J. B., Campagnaab, E., Campsie, P., Cannizzo, J., Cannon, K., Canuel, B., Cao, J., Capano, C., Carbognani, F., Caride, S., Caudill, S., Cavaglià, M., Cavaliera, F., Cavalieri, R., Cellaa, G., Cepeda, C., Cesarinib, E., Chaibia, O., Chalermsongsak, T., Chalkley, E., Charlton, P., Chassande-Mottin, E., Chelkowski, S., Chen, Y., Chincarini, A., Christensen, N., Chua, S. S. Y., Chung, C. T. Y., Chung, S., Clara, F., Clark, D., Clark, J., Clayton, J. H., Clevaa, F., Cocciaab, E., Colacinoab, C. N., Colas, J., Collaab, A., Colombinib, M., Conte, R., Cook, D., Corbitt, T. R., Cornish, N., Corsia, A., Costa, C. A., Coughlin, M., Coulona, J. -P., Coward, D. M., Coyne, D. C., Creighton, J. D. E., Creighton, T. D., Cruise, A. M., Culter, R. M., Cumming, A., Cunningham, L., Cuoco, E., Dahl, K., Danilishin, S. L., Dannenberg, R., D'Antonioa, S., Danzmann, K., Das, K., Dattilo, V., Daudert, B., Daveloza, H., Daviera, M., Davies, G., Daw, E. J., Day, R., Dayanga, T., De Rosaab, R., DeBra, D., Debreczeni, G., Degallaix, J., del Preteac, M., Dent, T., Dergachev, V., DeRosa, R., DeSalvo, R., Dhurandhar, S., Di Fiorea, L., Di Lietoab, A., Di Palma, I., Emilioac, M. Di Paolo, Di Virgilioa, A., Díaz, M., Dietz, A., Donovan, F., Dooley, K. L., Dorsher, S., Douglas, E. S. D., Dragocd, M., Drever, R. W. P., Driggers, J. C., Dumas, J. -C., Dwyer, S., Eberle, T., Edgar, M., Edwards, M., Effler, A., Ehrens, P., Engel, R., Etzel, T., Evans, M., Evans, T., Factourovich, M., Fafoneab, V., Fairhurst, S., Fan, Y., Farr, B. F., Fazi, D., Fehrmann, H., Feldbaum, D., Ferranteab, I., Fidecaroab, F., Finn, L. S., Fiori, I., Flaminio, R., Flanigan, M., Foley, S., Forsi, E., Fortea, L. A., Fotopoulos, N., Fourniera, J. -D., Franc, J., Frascaab, S., Frasconia, F., Frede, M., Frei, M., Frei, Z., Freise, A., Frey, R., Fricke, T. T., Friedrich, D., Fritschel, P., Frolov, V. V., Fulda, P., Fyffe, M., Galimberti, M., Gammaitoniab, L., Garcia, J., Garofoli, J. A., Garufiab, F., Gáspár, M. E., Gemme, G., Genin, E., Gennaia, A., Ghosh, S., Giaime, J. A., Giampanis, S., Giardina, K. D., Giazottoa, A., Gill, C., Goetz, E., Goggin, L. M., González, G., Gorodetsky, M. L., Goßler, S., Gouaty, R., Graef, C., Granata, M., Grant, A., Gras, S., Gray, C., Greenhalgh, R. J. S., Gretarsson, A. M., Greveriea, C., Grosso, R., Grote, H., Grunewald, S., Guidiab, G. M., Guido, C., Gupta, R., Gustafson, E. K., Gustafson, R., Hage, B., Hallam, J. M., Hammer, D., Hammond, G., Hanks, J., Hanna, C., Hanson, J., Harms, J., Harry, G. M., Harry, I. W., Harstad, E. D., Hartman, M. T., Haughian, K., Hayama, K., Hayaub, J. -F., Hayler, T., Heefner, J., Heitmann, H., Helloa, P., Hendry, M. A., Heng, I. S., Heptonstall, A. W., Herrera, V., Hewitson, M., Hild, S., Hoak, D., Hodge, K. A., Holt, K., Hong, T., Hooper, S., Hosken, D. J., Hough, J., Howell, E. J., Huet, D., Hughey, B., Husa, S., Huttner, S. H., Ingram, D. R., Inta, R., Isogai, T., Ivanov, A., Jaranowskid, P., Johnson, W. W., Jones, D. I., Jones, G., Jones, R., Ju, L., Kalmus, P., Kalogera, V., Kandhasamy, S., Kanner, J. B., Katsavounidis, E., Katzman, W., Kawabe, K., Kawamura, S., Kawazoe, F., Kells, W., Kelner, M., Keppel, D. G., Khalaidovski, A., Khalili, F. Y., Khazanov, E. A., Kim, H., Kim, N., King, P. J., Kinzel, D. L., Kissel, J. S., Klimenko, S., Kondrashov, V., Kopparapu, R., Koranda, S., Korth, W. Z., Kowalskab, I., Kozak, D., Kringel, V., Krishnamurthy, S., Krishnan, B., Królakae, A., Kuehn, G., Kumar, R., Kwee, P., Landry, M., Lantz, B., Lastzka, N., Lazzarini, A., Leaci, P., Leong, J., Leonor, I., Leroya, N., Letendre, N., Li, J., Lia, T. G. F., Liguoriab, N., Lindquist, P. E., Lockerbie, N. A., Lodhia, D., Lorenzinia, M., Lorietteb, V., Lormand, M., Losurdoa, G., Lu, P., Luan, J., Lubinski, M., Lück, H., Lundgren, A. P., Macdonald, E., Machenschalk, B., MacInnis, M., Mageswaran, M., Mailand, K., Majoranaa, E., Maksimovicb, I., Mana, N., Mandel, I., Mandic, V., Mantovaniac, M., Marandi, A., Marchesonia, F., Marion, F., Márka, S., Márka, Z., Maros, E., Marque, J., Martelliab, F., Martin, I. W., Martin, R. M., Marx, J. N., Mason, K., Masserot, A., Matichard, F., Matone, L., Matzner, R. A., Mavalvala, N., McCarthy, R., McClelland, D. E., McGuire, S. C., McIntyre, G., McKechan, D. J. A., Meadors, G., Mehmet, M., Meier, T., Melatos, A., Melissinos, A. C., Mendell, G., Mercer, R. A., Merill, L., Meshkov, S., Messenger, C., Meyer, M. S., Miao, H., Michel, C., Milanoab, L., Miller, J., Minenkova, Y., Mino, Y., Mitrofanov, V. P., Mitselmakher, G., Mittleman, R., Miyakawa, O., Moe, B., Moesta, P., Mohan, M., Mohanty, S. D., Mohapatra, S. R. P., Moraru, D., Moreno, G., Morgado, N., Morgiaab, A., Moscaab, S., Moscatellia, V., Mossavi, K., Mours, B., Mow--Lowry, C. M., Mueller, G., Mukherjee, S., Mullavey, A., Müller-Ebhardt, H., Munch, J., Murray, P. G., Nash, T., Nawrodt, R., Nelson, J., Neriab, I., Newton, G., Nishida, E., Nishizawa, A., Nocera, F., Nolting, D., Ochsner, E., O'Dell, J., Ogin, G. H., Oldenburg, R. G., O'Reilly, B., O'Shaughnessy, R., Osthelder, C., Ott, C. D., Ottaway, D. J., Ottens, R. S., Overmier, H., Owen, B. J., Page, A., Pagliaroliac, G., Palladinoac, L., Palombaa, C., Pan, Y., Pankow, C., Paolettia, F., Papa, M. A., Parameswaran, A., Pardiab, S., Parisiab, M., Pasqualetti, A., Passaquietiab, R., Passuelloa, D., Patel, P., Pathak, D., Pedraza, M., Pekowsky, L., Penn, S., Peralta, C., Perreca, A., Persichettiab, G., Phelps, M., Pichota, M., Pickenpack, M., Piergiovanniab, F., Pietkad, M., Pinard, L., Pinto, I. M., Pitkin, M., Pletsch, H. J., Plissi, M. V., Podkaminer, J., Poggianiab, R., Pöld, J., Postiglione, F., Prato, M., Predoi, V., Price, L. R., Prijatelj, M., Principe, M., Privitera, S., Prix, R., Prodiab, G. A., Prokhorov, L., Puncken, O., Punturoa, M., Puppoa, P., Quetschke, V., Raab, F. J., Rabelingab, D. S., Rácz, I., Radkins, H., Raffai, P., Rakhmanov, M., Ramet, C. R., Rankins, B., Rapagnaniab, P., Raymond, V., Reab, V., Redwine, K., Reed, C. M., Reed, T., Regimbaua, T., Reid, S., Reitze, D. H., Ricciab, F., Riesen, R., Riles, K., Roberts, P., Robertson, N. A., Robineta, F., Robinson, C., Robinson, E. L., Rocchia, A., Roddy, S., Rolland, L., Rollins, J., Romano, J. D., Romanoac, R., Romie, J. H., Rosińskacf, D., Röver, C., Rowan, S., Rüdiger, A., Ruggi, P., Ryan, K., Sakata, S., Sakosky, M., Salemi, F., Salit, M., Sammut, L., de la Jordana, L. Sancho, Sandberg, V., Sannibale, V., Santamaría, L., Santiago-Prieto, I., Santostasi, G., Saraf, S., Sassolas, B., Sathyaprakash, B. S., Sato, S., Satterthwaite, M., Saulson, P. R., Savage, R., Schilling, R., Schlamminger, S., Schnabel, R., Schofield, R. M. S., Schulz, B., Schutz, B. F., Schwinberg, P., Scott, J., Scott, S. M., Searle, A. C., Seifert, F., Sellers, D., Sengupta, A. S., Sentenac, D., Sergeev, A., Shaddock, D. A., Shaltev, M., Shapiro, B., Shawhan, P., Weerathunga, T. Shihan, Shoemaker, D. H., Sibley, A., Siemens, X., Sigg, D., Singer, A., Singer, L., Sintes, A. M., Skelton, G., Slagmolen, B. J. J., Slutsky, J., Smith, J. R., Smith, M. R., Smith, N. D., Smith, R., Somiya, K., Sorazu, B., Soto, J., Speirits, F. C., Sperandioab, L., Stefszky, M., Stein, A. J., Steinlechner, J., Steinlechner, S., Steplewski, S., Stochino, A., Stone, R., Strain, K. A., Strigin, S., Stroeer, A. S., Sturaniab, R., Stuver, A. L., Summerscales, T. Z., Sung, M., Susmithan, S., Sutton, P. J., Swinkels, B., Szokoly, G. P., Tacca, M., Talukder, D., Tanner, D. B., Tarabrin, S. P., Taylor, J. R., Taylor, R., Thomas, P., Thorne, K. A., Thorne, K. S., Thrane, E., Thüring, A., Titsler, C., Tokmakov, K. V., Toncelliab, A., Tonelliab, M., Torreac, O., Torres, C., Torrie, C. I., Tournefier, E., Travassoab, F., Traylor, G., Trias, M., Tseng, K., Turner, L., Ugolini, D., Urbanek, K., Vahlbruch, H., Vaishnav, B., Vajenteab, G., Vallisneri, M., Brandab, J. F. J. van den, Broeck, C. Van Den, van der Puttena, S., van der Sluys, M. V., van Veggel, A. A., Vass, S., Vasuth, M., Vaulin, R., Vavoulidisa, M., Vecchio, A., Vedovatoc, G., Veitch, J., Veitch, P. J., Veltkamp, C., Verkindt, D., Vetranoab, F., Viceréab, A., Villar, A. E., Vineta, J. -Y., Voccaa, H., Vorvick, C., Vyachanin, S. P., Waldman, S. J., Wallace, L., Wanner, A., Ward, R. L., Wasa, M., Wei, P., Weinert, M., Weinstein, A. J., Weiss, R., Wen, L., Wen, S., Wessels, P., West, M., Westphal, T., Wette, K., Whelan, J. T., Whitcomb, S. E., White, D., Whiting, B. F., Wilkinson, C., Willems, P. A., Williams, H. R., Williams, L., Willke, B., Winkelmann, L., Winkler, W., Wipf, C. C., Wiseman, A. G., Woan, G., Wooley, R., Worden, J., Yablon, J., Yakushin, I., Yamamoto, H., Yamamoto, K., Yang, H., Yeaton-Massey, D., Yoshida, S., Yu, P., Yvert, M., Zanolin, M., Zhang, L., Zhang, Z., Zhao, C., Zotov, N., Zucker, M. E., Zweizig, J., Aptekar, R. L., Boynton, W. V., Briggs, M. S., Cline, T. L., Connaughton, V., Frederiks, D. D., Gehrels, N., Goldsten, J. O, Golovin, D., van der Horst, A. J., Hurley, K. C., Kaneko, Y., von Kienlin, A., Kouveliotou, C., Krimm, H. A., Lin, L., Mitrofanov, I., Ohno, M., Palshin, V. D., Rau, A., Sanin, A., Tashiro, M. S., Terada, Y., and Yamaoka, K.
Subjects: Astrophysics - High Energy Astrophysical Phenomena, General Relativity and Quantum Cosmology
Abstract: Soft gamma repeaters (SGRs) and anomalous X-ray pulsars (AXPs) are thought to be magnetars: neutron stars powered by extreme magnetic fields. These rare objects are characterized by repeated and sometimes spectacular gamma-ray bursts. The burst mechanism might involve crustal fractures and excitation of non-radial modes which would emit gravitational waves (GWs). We present the results of a search for GW bursts from six galactic magnetars that is sensitive to neutron star f-modes, thought to be the most efficient GW emitting oscillatory modes in compact stars. One of them, SGR 0501+4516, is likely ~1 kpc from Earth, an order of magnitude closer than magnetars targeted in previous GW searches. A second, AXP 1E 1547.0-5408, gave a burst with an estimated isotropic energy >10^{44} erg which is comparable to the giant flares. We find no evidence of GWs associated with a sample of 1279 electromagnetic triggers from six magnetars occurring between November 2006 and June 2009, in GW data from the LIGO, Virgo, and GEO600 detectors. Our lowest model-dependent GW emission energy upper limits for band- and time-limited white noise bursts in the detector sensitive band, and for f-mode ringdowns (at 1090 Hz), are 3.0x10^{44} d_1^2 erg and 1.4x10^{47} d_1^2 erg respectively, where d_1 = d_{0501} / 1 kpc and d_{0501} is the distance to SGR 0501+4516. These limits on GW emission from f-modes are an order of magnitude lower than any previous, and approach the range of electromagnetic energies seen in SGR giant flares for the first time., Comment: 9 pages, 3 figures; v2 minor clarifications and new references
Published: 2010
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4. Characterization of cellular accumulation and toxicity of illudin S in sensitive and nonsensitive tumor cells

Author: Kelner, M. J., McMorris, Trevor C., Montoya, Mark A., Estes, Leita, Rutherford, Mary, Samson, Kyra M., and Taetle, Raymond
Published: 1997
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5. Acylfulvenes, a new class of potent antitumor agents

Author: McMorris, T. C., Kelner, M. J., Wang, W., Diaz, M. A., Estes, L. A., and Taetle, R.
Published: 1996
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6. Search For Gravitational Wave Bursts From Six Magnetars

Author: Abadie, J., Abbott, B. P., Abbott, R., Abernathy, M., Accadia, T., Acernese, F., Adams, C., Adhikari, R., Affeldt, C., Allen, B., Allen, G. S., Ceron, E. A., Amariutei, D., Amin, R. S., Anderson, S. B., Anderson, W. G., Antonucci, F., Arai, K., Arain, M. A., Araya, M. C., Aston, S. M., Astone, P., Atkinson, D., Aufmuth, P., Aulbert, C., Aylott, B. E., Babak, S., Baker, P., Ballardin, G., Ballmer, S., Barker, D., Barnum, S., Barone, F., Barr, B., Barriga, P., Barsotti, L., Barsuglia, M., Barton, M. A., Bartos, I., Bassiri, R., Bastarrika, M., Basti, A., Bauchrowitz, J., Bauer, T. S., Behnke, B., Beker, M. G., Bell, A. S., Belletoile, A., Belopolski, I., Benacquista, M., Bertolini, A., Betzwieser, J., Beveridge, N., Beyersdorf, P. T., Bilenko, I. A., Billingsley, G., Birch, J., Birindelli, S., Biswas, R., Bitossi, M., Bizouard, M. A., Black, E., Blackburn, J. K., Blackburn, L., Blair, D., Bland, B., Blom, M., Bock, O., Bodiya, T. P., Bogan, C., Bondarescu, R., Bondu, F., Bonelli, L., Bonnand, R., Bork, R., Born, M., Boschi, V., Bose, S., Bosi, L., Bouhou, B., Boyle, M., Braccini, S., Bradaschia, C., Brady, P. R., Braginsky, V. B., Brau, J. E., Breyer, J., Bridges, D. O., Brillet, A., Brinkmann, M., Brisson, V., Britzger, M., Brooks, A. F., Brown, D. A., Brummit, A., Budzynski, R., Bulik, T., Bulten, H. J., Buonanno, A., Burguet-Castell, J., Burmeister, O., Buskulic, D., Buy, C., Byer, R. L., Cadonati, L., Cagnoli, G., Cain, J., Calloni, E., Camp, J. B., Campagna, E., Campsie, P., Cannizzo, J., Cannon, K., Canuel, B., Cao, J., Capano, C., Carbognani, F., Caride, S., Caudill, S., Cavaglia, M., Cavalier, F., Cavalieri, R., Cella, G., Cepeda, C., Cesarini, E., Chaibi, O., Chalermsongsak, T., Chalkley, E., Charlton, P., Chassande-Mottin, E., Chelkowski, S., Chen, Y., Chincarini, A., Christensen, N., S. S. Y., C. T. Y., Chung, S., Clara, F., Clark, D., Clark, J., Clayton, J. H., Cleva, F., Coccia, E., Colacino, C. N., Colas, J., Colla, A., Colombini, M., Conte, R., Cook, D., Corbitt, T. R., Cornish, N., Corsi, A., Costa, C. A., Coughlin, M., Coulon, J. P., Coward, D. M., Coyne, D. C., J. D. E., Creighton, T. D., Cruise, A. M., Culter, R. M., Cumming, A., Cunningham, L., Cuoco, E., Dahl, K., Danilishin, S. L., Dannenberg, R., Antonio, S. D., Danzmann, K., Das, K., Dattilo, V., Daudert, B., Daveloza, H., Davier, M., Davies, G., Daw, E. J., Day, R., Dayanga, T., Rosa, R. D., Debra, D., Debreczeni, G., Degallaix, J., Prete, M. D., Dent, T., Dergachev, V., Derosa, R., Desalvo, R., Dhurandhar, S., Fiore, L. D., Lieto, A. D., Palma, I. D., Paolo, M. D., Virgilio, A. D., Diaz, M., Dietz, A., Donovan, F., Dooley, K. L., Dorsher, S., E. S. D., Drago, M., R. W. P., Driggers, J. C., Dumas, J. C., Dwyer, S., Eberle, T., Edgar, M., Edwards, M., Effler, A., Ehrens, P., Engel, R., Etzel, T., Evans, M., Evans, T., Factourovich, M., Fafone, V., Fairhurst, S., Fan, Y., Farr, B. F., Fazi, D., Fehrmann, H., Feldbaum, D., Ferrante, I., Fidecaro, F., Finn, L. S., Fiori, I., Flaminio, R., Flanigan, M., Foley, S., Forsi, E., Forte, L. A., Fotopoulos, N., Fournier, J. D., Franc, J., Frasca, S., Frasconi, F., Frede, M., Frei, M., Frei, Z., Freise, A., Frey, R., Fricke, T. T., Friedrich, D., Fritschel, P., Frolov, V. V., Fulda, P., Fyffe, M., Galimberti, M., Gammaitoni, L., Garcia, J., Garofoli, J. A., Garufi, F., Gaspar, M. E., Gemme, G., Genin, E., Gennai, A., Ghosh, S., Giaime, J. A., Giampanis, S., Giardina, K. D., Giazotto, A., Gill, C., Goetz, E., Goggin, L. M., Gonzalez, G., Gorodetsky, M. L., Gossler, S., Gouaty, R., Graef, C., Granata, M., Grant, A., Gras, S., Gray, C., R. J. S., Gretarsson, A. M., Greverie, C., Grosso, R., Grote, H., Grunewald, S., Guidi, G. M., Guido, C., Gupta, R., Gustafson, E. K., Gustafson, R., Hage, B., Hallam, J. M., Hammer, D., Hammond, G., Hanks, J., Hanna, C., Hanson, J., Harms, J., Harry, G. M., Harry, I. W., Harstad, E. D., Hartman, M. T., Haughian, K., Hayama, K., Hayau, J. F., Hayler, T., Heefner, J., Heitmann, H., Hello, P., Hendry, M. A., Heng, I. S., Heptonstall, A. W., Herrera, V., Hewitson, M., Hild, S., Hoak, D., Hodge, K. A., Holt, K., Hong, T., Hooper, S., Hosken, D. J., Hough, J., Howell, E. J., Huet, D., Hughey, B., Husa, S., Huttner, S. H., Ingram, D. R., Inta, R., Isogai, T., Ivanov, A., Jaranowski, P., Johnson, W. W., Jones, D. I., Jones, G., Jones, R., Ju, L., Kalmus, P., Kalogera, V., Kandhasamy, S., Kanner, J. B., Katsavounidis, E., Katzman, W., Kawabe, K., Kawamura, S., Kawazoe, F., Kells, W., Kelner, M., Keppel, D. G., Khalaidovski, A., Khalili, F. Y., Khazanov, E. A., Kim, H., Kim, N., King, P. J., Kinzel, D. L., Kissel, J. S., Klimenko, S., Kondrashov, V., Kopparapu, R., Koranda, S., Korth, W. Z., Kowalska, I., Kozak, D., Kringel, V., Krishnamurthy, S., Krishnan, B., Krolak, A., Kuehn, G., Kumar, R., Kwee, P., Landry, M., Lantz, B., Lastzka, N., Lazzarini, A., Leaci, P., Leong, J., Leonor, I., Leroy, N., Letendre, N., Li, J., T. G. F., Liguori, N., Lindquist, P. E., Lockerbie, N. A., Lodhia, D., Lorenzini, M., Loriette, V., Lormand, M., Losurdo, G., Lu, P., Luan, J., Lubinski, M., Lueck, H., Lundgren, A. P., Macdonald, E., Machenschalk, B., Macinnis, M., Mageswaran, M., Mailand, K., Majorana, E., Maksimovic, I., Man, N., Mandel, I., Mandic, V., Mantovani, M., Marandi, A., Marchesoni, F., Marion, F., Marka, S., Marka, Z., Maros, E., Marque, J., Martelli, F., Martin, I. W., Martin, R. M., Marx, J. N., Mason, K., Masserot, A., Matichard, F., Matone, L., Matzner, R. A., Mavalvala, N., Mccarthy, R., Mcclelland, D. E., Mcguire, S. C., Mcintyre, G., D. J. A., Meadors, G., Mehmet, M., Meier, T., Melatos, A., Melissinos, A. C., Mendell, G., Mercer, R. A., Merill, L., Meshkov, S., Messenger, C., Meyer, M. S., Miao, H., Michel, C., Milano, L., Miller, J., Minenkov, Y., Mino, Y., Mitrofanov, V. P., Mitselmakher, G., Mittleman, R., Miyakawa, O., Moe, B., Moesta, P., Mohan, M., Mohanty, S. D., S. R. P., Moraru, D., Moreno, G., Morgado, N., Morgia, A., Mosca, S., Moscatelli, V., Mossavi, K., Mours, B., Mow-Lowry, C. M., Mueller, G., Mukherjee, S., Mullavey, A., Mueller-Ebhardt, H., Munch, J., Murray, P. G., Nash, T., Nawrodt, R., Nelson, J., Neri, I., Newton, G., Nishida, E., Nishizawa, A., Nocera, F., Nolting, D., Ochsner, E., J. O'Dell, Ogin, G. H., Oldenburg, R. G., Reilly, B. O., Shaughnessy, R. O., Osthelder, C., Ott, C. D., Ottaway, D. J., Ottens, R. S., Overmier, H., Owen, B. J., Page, A., Pagliaroli, G., Palladino, L., Palomba, C., Pan, Y., Pankow, C., Paoletti, F., Papa, M. A., Parameswaran, A., Pardi, S., Parisi, M., Pasqualetti, A., Passaquieti, R., Passuello, D., Patel, P., Pathak, D., Pedraza, M., Pekowsky, L., Penn, S., Peralta, C., Perreca, A., Persichetti, G., Phelps, M., Pichot, M., Pickenpack, M., Piergiovanni, F., Pietka, M., Pinard, L., Pinto, I. M., Pitkin, M., Pletsch, H. J., Plissi, M. V., Podkaminer, J., Poggiani, R., Poeld, J., Postiglione, F., Prato, M., Predoi, V., Price, L. R., Prijatelj, M., Principe, M., Privitera, S., Prix, R., Prodi, G. A., Prokhorov, L., Puncken, O., Punturo, M., Puppo, P., Quetschke, V., Raab, F. J., Rabeling, D. S., Racz, I., Radkins, H., Raffai, P., Rakhmanov, M., Ramet, C. R., Rankins, B., Rapagnani, P., Raymond, V., Re, V., Redwine, K., Reed, C. M., Reed, T., Regimbau, T., Reid, S., Reitze, D. H., Ricci, F., Riesen, R., Riles, K., Roberts, P., Robertson, N. A., Robinet, F., Robinson, C., Robinson, E. L., Rocchi, A., Roddy, S., Rolland, L., Rollins, J., Romano, J. D., Romano, R., Romie, J. H., Rosinska, D., Roever, C., Rowan, S., Udiger, A. R., Ruggi, P., Ryan, K., Sakata, S., Sakosky, M., Salemi, F., Salit, M., Sammut, L., L. S. de, Sandberg, V., Sannibale, V., Santamaria, L., Santiago-Prieto, I., Santostasi, G., Saraf, S., Sassolas, B., Sathyaprakash, B. S., Sato, S., Satterthwaite, M., Saulson, P. R., Savage, R., Schilling, R., Schlamminger, S., Schnabel, R., R. M. S., Schulz, B., Schutz, B. F., Schwinberg, P., Scott, J., Scott, S. M., Searle, A. C., Seifert, F., Sellers, D., Sengupta, A. S., Sentenac, D., Sergeev, A., Shaddock, D. A., Shaltev, M., Shapiro, B., Shawhan, P., Weerathunga, T. S., Shoemaker, D. H., Sibley, A., Siemens, X., Sigg, D., Singer, A., Singer, L., Sintes, A. M., Skelton, G., B. J. J., Slutsky, J., Smith, J. R., Smith, M. R., Smith, N. D., Smith, R., Somiya, K., Sorazu, B., Soto, J., Speirits, F. C., Sperandio, L., Stefszky, M., Stein, A. J., Steinlechner, J., Steinlechner, S., Steplewski, S., Stochino, A., Stone, R., Strain, K. A., Strigin, S., Stroeer, A. S., Sturani, R., Stuver, A. L., Summerscales, T. Z., Sung, M., Susmithan, S., Sutton, P. J., Swinkels, B., Szokoly, G. P., Tacca, M., Talukder, D., Tanner, D. B., Tarabrin, S. P., Taylor, J. R., Taylor, R., Thomas, P., Thorne, K. A., Thorne, K. S., Thrane, E., Thuering, A., Titsler, C., Tokmakov, K. V., Toncelli, A., Tonelli, M., Torre, O., Torres, C., Torrie, C. I., Tournefier, E., Travasso, F., Traylor, G., Trias, M., Tseng, K., Turner, L., Ugolini, D., Urbanek, K., Vahlbruch, H., Vaishnav, B., Vajente, G., Vallisneri, M., J. F. J., Den, C. V., S. v. der, M. V. van, A. A. van, Vass, S., Vasuth, M., Vaulin, R., Vavoulidis, M., Vecchio, A., Vedovato, G., Veitch, J., Veitch, P. J., Veltkamp, C., Verkindt, D., Vetrano, F., Vicere, A., Villar, A. E., Vinet, J. Y., Vocca, H., Vorvick, C., Vyachanin, S. P., Waldman, S. J., Wallace, L., Wanner, A., Ward, R. L., Was, M., Wei, P., Weinert, M., Weinstein, A. J., Weiss, R., Wen, L., Wen, S., Wessels, P., West, M., Westphal, T., Wette, K., Whelan, J. T., Whitcomb, S. E., White, D., Whiting, B. F., Wilkinson, C., Willems, P. A., Williams, H. R., Williams, L., Willke, B., Winkelmann, L., Winkler, W., Wipf, C. C., Wiseman, A. G., Woan, G., Wooley, R., Worden, J., Yablon, J., Yakushin, I., Yamamoto, H., Yamamoto, K., Yang, H., Yeaton-Massey, D., Yoshida, S., Yu, P., Yvert, M., Zanolin, M., Zhang, L., Zhang, Z., Zhao, C., Zotov, N., Zucker, M. E., Zweizig, J., Aptekar, R. L., Boynton, W. V., Briggs, M. S., Cline, T. L., Connaughton, V., Frederiks, D. D., Gehrels, N., Goldsten, J. O., Golovin, D., A. J. van, Hurley, K. C., Kaneko, Y., Kienlin, A. V., Kouveliotou, C., Krimm, H. A., Lin, L., Mitrofanov, I., Ohno, M., Pal Shin, V. D., Rau, A., Sanin, A., Tashiro, M. S., Terada, Y., Yamaoka, K., Collaboration, L. S., Collaboration, V., Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), APC - Cosmologie, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Observatoire de la Côte d'Azur (OCA), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut de Physique de Rennes (IPR), Université de Rennes (UR)-Centre National de la Recherche Scientifique (CNRS), Laboratoire des matériaux avancés (LMA), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), APC - Gravitation (APC-Gravitation), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Max-Planck-Gesellschaft-Max-Planck-Gesellschaft, Ecole Superieure de Physique et de Chimie Industrielles de la Ville de Paris (ESPCI Paris), Université Paris sciences et lettres (PSL), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Université de Rennes 1 (UR1), Université de Rennes (UNIV-RENNES)-Université de Rennes (UNIV-RENNES)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), (Astro)-Particles Physics, Student Lab and Education, Laboratoire d'Annecy de Physique des Particules (LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules), Physique Corpusculaire et Cosmologie - Collège de France (PCC), Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-AstroParticule et Cosmologie (APC (UMR_7164)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Centre National de la Recherche Scientifique (CNRS), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Ecole Supérieure de Physique et de Chimie Industrielles (ESPCI), Mairie de Paris, Laboratoire d'Annecy de Physique des Particules ( LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules ), Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Savoie Mont Blanc ( USMB [Université de Savoie] [Université de Chambéry] ) -Centre National de la Recherche Scientifique ( CNRS ), Physique Corpusculaire et Cosmologie - Collège de France ( PCC ), Collège de France ( CdF ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Paris Diderot - Paris 7 ( UPD7 ) -Centre National de la Recherche Scientifique ( CNRS ) -Collège de France ( CdF ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Paris Diderot - Paris 7 ( UPD7 ) -Centre National de la Recherche Scientifique ( CNRS ) -AstroParticule et Cosmologie ( APC - UMR 7164 ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Centre National de la Recherche Scientifique ( CNRS ) -Observatoire de Paris-Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ), Observatoire de la Côte d'Azur ( OCA ), Centre National de la Recherche Scientifique ( CNRS ), Laboratoire de l'Accélérateur Linéaire ( LAL ), Université Paris-Sud - Paris 11 ( UP11 ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ), Institut de Physique de Rennes ( IPR ), Université de Rennes 1 ( UR1 ), Université de Rennes ( UNIV-RENNES ) -Université de Rennes ( UNIV-RENNES ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire des matériaux avancés ( LMA ), Université Claude Bernard Lyon 1 ( UCBL ), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ) -Centre National de la Recherche Scientifique ( CNRS ), AstroParticule et Cosmologie ( APC - UMR 7164 ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ), APC - Gravitation ( APC-Gravitation ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut), Max-Planck-Institut-Max-Planck-Institut, Ecole Supérieure de Physique et de Chimie Industrielles ( ESPCI ), The LIGO Scientific Collaboration, The Virgo Collaboration, F., Acernese, F., Barone, Calloni, Enrico, DE ROSA, Rosario, L., Di Fiore, Garufi, Fabio, Milano, Leopoldo, S., Mosca, M., Parisi, G., Persichetti, R., Romano, and Pinto, Innocenzo
Subjects: Astrophysics::High Energy Astrophysical Phenomena, SGR 1900+14, FOS: Physical sciences, Astrophysics, General Relativity and Quantum Cosmology (gr-qc), Astrophysics::Cosmology and Extragalactic Astrophysics, Magnetar, 01 natural sciences, General Relativity and Quantum Cosmology, [ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], stars: magnetars, Settore FIS/05 - Astronomia e Astrofisica, Pulsar, X-RAY PULSAR, gravitational waves, 0103 physical sciences, QC176, Gravitational waves, Stars, Magnetars, OSCILLATIONS, 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), 010308 nuclear & particles physics, Gravitational wave, ORIGIN, MAGNETIZED NEUTRON-STARS, Settore FIS/01 - Fisica Sperimentale, SOFT-GAMMA-REPEATER, Astronomy and Astrophysics, LOCALIZATION, GEO600, LIGO, Magnetic field, Neutron star, 13. Climate action, Space and Planetary Science, DISCOVERY, DISTANCE, [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], Astrophysics - High Energy Astrophysical Phenomena, GIANT FLARE
Abstract: Soft gamma repeaters (SGRs) and anomalous X-ray pulsars (AXPs) are thought to be magnetars: neutron stars powered by extreme magnetic fields. These rare objects are characterized by repeated and sometimes spectacular gamma-ray bursts. The burst mechanism might involve crustal fractures and excitation of non-radial modes which would emit gravitational waves (GWs). We present the results of a search for GW bursts from six galactic magnetars that is sensitive to neutron star f-modes, thought to be the most efficient GW emitting oscillatory modes in compact stars. One of them, SGR 0501+4516, is likely ~1 kpc from Earth, an order of magnitude closer than magnetars targeted in previous GW searches. A second, AXP 1E 1547.0-5408, gave a burst with an estimated isotropic energy >10^{44} erg which is comparable to the giant flares. We find no evidence of GWs associated with a sample of 1279 electromagnetic triggers from six magnetars occurring between November 2006 and June 2009, in GW data from the LIGO, Virgo, and GEO600 detectors. Our lowest model-dependent GW emission energy upper limits for band- and time-limited white noise bursts in the detector sensitive band, and for f-mode ringdowns (at 1090 Hz), are 3.0x10^{44} d_1^2 erg and 1.4x10^{47} d_1^2 erg respectively, where d_1 = d_{0501} / 1 kpc and d_{0501} is the distance to SGR 0501+4516. These limits on GW emission from f-modes are an order of magnitude lower than any previous, and approach the range of electromagnetic energies seen in SGR giant flares for the first time., 9 pages, 3 figures; v2 minor clarifications and new references
Published: 2011

7. GHB: EFFECT ON SERUM OSMOLALITY

Author: Ingels, M, Kelner, M, Ly, B, and Clark, RF
Subjects: Gamma-hydroxybutyrate -- Adverse and side effects, Poisoning, Accidental -- Care and treatment, Environmental issues, Health, Pharmaceuticals and cosmetics industries
Abstract: Background: Physicians are often called upon to treat patients with coma of unclear etiology. Gamma hydroxybutyrate (GHB) is one possible cause. Although GHB levels can be obtained, the lab turnaround time is usually several days. GHB has a relatively small molecular weight (MW = 104). The purpose of this study was to determine 1) whether GHB's measured contribution to serum osmolality correlates with the expected calculated value and 2) whether this is significant at clinically relevant serum concentrations. Methods: The sodium salt of GHB was dissolved in pooled human serum to make GHB concentrations of 3000 mcg/mL, 2000 mcg/mL, and 1000 mcg/mL. These samples and a control were analyzed on an osmometer to determine serum osmolality by freezing point depression, and were compared to the calculated expected osmolality. To determine clinical relevance, reference levels for GHB-associated coma were obtained from a national laboratory and local poison center records. Results: The expected changes in osmolality due to GHB at these concentrations are 28.8, 19.2, and 9.6 mOsm/L, respectively. The measured change in osmolality from GHB in this study were 28.5, 18, and 10.5 mOsm/L. Reference laboratory materials state that levels greater than 260 mcg/mL produce deep sleep/coma. The highest blood GHB level seen by this poison center in a comatose patient was 645 mcg/mL. The calculated contributions to an osmol gap of these levels are 2.5 and 6.2 mOsm/L, respectively. Conclusion: The measured contribution of GHB to serum osmolality can be predicted by calculations based on GHB's molecular weight. Patients may be comatose due to GHB and have only minimal elevation in serum osmolality. While the contribution of GHB must be considered when evaluating an osmol gap, GHB alone is unlikely to cause significant elevations at clinically encountered serum concentrations., Ingels M, Kelner M, Ly B, Clark RF. University of California at San Diego, Medical Center, San Diego, [...]
Published: 2000

8. Detailed quantification of delta subsidence, compaction and interaction with man-made structures: the case of the NCA airport, France

Author: Cavalié, O., primary, Sladen, A., additional, and Kelner, M., additional
Published: 2015
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9. Very low latency search for low mass compact binary coalescences in the LIGO S6 and Virgo VSR2 data

Author: Buskulic, D., Abadie, J., Abbott, B.P., Abbott, R., Abernathy, M., Adams, C., Adhikari, R., Affeldt, C., Allen, B., Allen, G.S., Amador Ceron, E., Amariutei, D., Amin, R.S., Anderson, S.B., Anderson, W.G., Arai, K., Arain, M.A., Araya, M.C., Aston, S.M., Atkinson, D., Aufmuth, P., Aulbert, C., Aylott, B.E., Babak, S., Baker, P., Ballmer, S., Barker, D., Barnum, S., Barr, B., Barriga, P., Barsotti, L., Barton, M.A., Bartos, I., Bassiri, R., Bastarrika, M., Bauchrowitz, J., Behnke, B., Bell, A.S., Belopolski, I., Benacquista, M., Bertolini, A., Betzwieser, J., Beveridge, N., Beyersdorf, P.T., a Bilenko, I., Billingsley, G., Birch, J., Biswas, R., Black, E., K Blackburn, J., Blackburn, L., Blair, D., Bland, B., Bock, O., P Bodiya, T., Bogan, C., Bondarescu, R., Bork, R., Born, M., Bose, S., Boyle, M., R Brady, P., B Braginsky, V., E Brau, J., Breyer, J., O Bridges, D., Brinkmann, M., Britzger, M., F Brooks, A., Brown, D.A, Brummitt, A., Buonanno, A., Burguet-Castell, J., Burmeister, O., L Byer, R., Cadonati, L., B Camp, J., Campsie, P., Cannizzo, J., Cannon, K., Cao, J., Capano, C., Caride, S., Caudill, S., Cavaglia, M., Cepeda, C., Chalermsongsak, T., Chalkley, E., Charlton, P., Chelkowski, S., Chen, Y., Christensen, N., S y Chua, S., Chung, S., T y Chung, C., Clara, F., Clark, D., Clark, J., H Clayton, J., Conte, R., Cook, D., R C Corbitt, T., Cornish, N., Costa, C.A, Coughlin, M., M Coward, D., C Coyne, D., D E Creighton, J., D Creighton, T., M Cruise, A., Cumming, A., Cunningham, L., M Culter, R., Dahl, K., L Danilishin, S., Dannenberg, R., Danzmann, K., Das, K., Daudert, B., Daveloza, H., Davies, G., J Daw, E., Dayanga, T., Debra, D., Degallaix, J., Dent, T., Dergachev, V., Derosa, R., Desalvo, R., Dhurandhar, S., Di Palma, I., d'Iaz, M., Donovan, F., L Dooley, K., Dorsher, S., S D Douglas, E., W P Drever, R., C Driggers, J., Dumas, J.-C, Dwyer, S., Eberle, T., Edgar, M., Edwards, M., Effler, A., Ehrens, P., Engel, R., Etzel, T., Evans, M., Evans, T., Factourovich, M., Fairhurst, S., Fan, Y., F Farr, B., Fazi, D., Fehrmann, H., Feldbaum, D., S Finn, L., Flanigan, M., Flasch, K., Foley, S., Forsi, E., Fotopoulos, N., Frede, M., Frei, M., Frei, Z., Freise, A., Frey, R., Fricke, T.T., Friedrich, D., Fritschel, P., V Frolov, V., Fulda, P., Fyffe, M., Garcia, J., Garofoli, J.A, Gholami, I., Ghosh, S., Giaime, J.A, Giampanis, S., D Giardina, K., Gill, C., Goetz, E., M Goggin, L., Gonz'Alez, G., L Gorodetsky, M., Gossler, S., Graef, C., Grant, A., Gras, S., Gray, C., J S Greenhalgh, R., M Gretarsson, A., Grosso, R., Grote, H., Grunewald, S., Guido, C., Gupta, Rajiv, K Gustafson, E., Gustafson, R., Hage, B., M Hallam, J., Hammond, G., Hanks, J., Hanna, C., Hanson, J., Harms, J., M Harry, G., W Harry, I., D Harstad, E., T Hartman, M., Haughian, K., Hayama, K., Heefner, J., S Heng, I., W Heptonstall, A., Herrera, V., Hild, S., Hoak, D., a Hodge, K., Holt, K., Hong, T., Hooper, S., J Hosken, D., Hough, J., J Howell, E., Hughey, B., Husa, 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Mavalvala, N., Mccarthy, R., E Mcclelland, D., C Mcguire, S., Mcintyre, G., Mciver, J., J a Mckechan, D., Meadors, G., Mehmet, M., Meier, T., Melatos, A., C Melissinos, A., Mendell, G., a Mercer, R., Meshkov, S., Messenger, C., S Meyer, M., Miao, H., Miller, J., Mino, Y., P Mitrofanov, V., Mitselmakher, G., Mittleman, R., Miyakawa, O., Moe, B., Moesta, P., D Mohanty, S., Moraru, D., Moreno, G., Mossavi, K., M Mow-Lowry, C., Mueller, G., Mukherjee, S., Mullavey, A., M¨ Uller-Ebhardt, H., Munch, J., Murphy, D., G Murray, P., Nash, T., Nawrodt, R., Nelson, J., Newton, G., Nishizawa, A., Nolting, D., O'Reilly, B., O'Shaughnessy, R., Ochsner, E., O'Dell, J., H Ogin, G., G Oldenburg, R., Osthelder, C., D Ott, C., J Ottaway, D., S Ottens, R., Overmier, H., J Owen, B., Page, A., Pan, Y., Pankow, C., Papa, M.A, Pareja, M., Parameswaran, A., Patel, P., Pedraza, M., Pekowsky, L., Penn, S., Peralta, C., Perreca, A., Phelps, M., Pickenpack, M., M Pinto, I., Pitkin, M., J Pletsch, H., V Plissi, M., 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Ward, R., Wei, P., Weinert, M., J Weinstein, A., Weiss, R., Wen, L., Wen, S., Wessels, P., West, M., Westphal, T., Wette, K., T Whelan, J., E Whitcomb, S., White, D., F Whiting, B., Wilkinson, C., a Willems, P., R Williams, H., Williams, L., Willke, B., Winkelmann, L., Winkler, W., G Wiseman, A., Woan, G., Wooley, R., Worden, J., Yablon, J., Yakushin, I., Yamamoto, K., Yamamoto, H., Yang, H., Yeaton-Massey, D., Yoshida, S., Yu, P., Zanolin, M., Zhang, L., Zhang, Zhen, Zhao, C., Zotov, N., E Zucker, M., Zweizig, J., Accadia, T., Acernese, F., Antonucci, F., Astone, P., Ballardin, G., Barone, F., Barsuglia, M., Bauer, T.S., Beker, M.G., Belletoile, A., Birindelli, S., Bitossi, M., Bizouard, M.A., Blom, M., Bondu, François, Bonelli, L., Bonnand, R., Boschi, V., Bosi, L., Bouhou, B., Braccini, S., Bradaschia, C., Brillet, A., Brisson, V., Budzynski, R., Bulik, T., Bulten, H.J., Lesvigne-Buy, Christelle, Cagnoli, G., Calloni, E., Campagna, E., Canuel, B., Carbognani, F., Cavalier, F., Cavalieri, R., Cella, G., Cesarini, E., Chaibi, O., Chassande-Mottin, E., Chincarini, A., Cleva, F., Coccia, E., Colacino, C.N., Colas, J., Colla, A., Colombini, M., Corsi, A., Coulon, J.-P., Cuoco, E., d'Antonio, S., Dattilo, V., Davier, M., Day, R., de Rosa, R., Debreczeni, G., del Prete, M., Di Fiorea, L., Di Lieto, A., Di Paolo Emilio, M., Di Virgilio, A., Dietz, A., Drago, M., Fafone, V., Ferrante, I., Fidecaro, F., Fiori, I., Flaminio, R., Forte, L.A., Fournier, J.-D., Franc, J., Frasca, S., Frasconi, F., Galimberti, M., Gammaitoni, L., Garufi, F., Gaspar, M.E., Gemme, G., Genin, E., Gennai, A., Giazotto, A., Gouaty, R., Granata, M., Greverie, C., Guidi, G.M., Hayau, J.-F., Heitmann, H., Hello, P., Huet, D., Jaranowski, P., Kowalskac, I., Krolak, A., Leroy, N., Letendre, N., Li, T.G.F., Liguori, N., Lorenzini, M., Loriette, V., Losurdo, G., Majorana, E., Maksimovic, I., Man, N., Mantovani, M., Marchesoni, F., Marion, F., Marque, J., Martelli, F., Masserot, A., Michel, Christine, Milano, L., Minenkov, Y., Mohan, M., Morgado, N., Morgia, A., Mosca, S., Moscatelli, V., Mours, B., Neri, I., Nocera, F., Pagliaroli, G., Palladino, L., Palomba, C., Paoletti, F., Pardi, S., Parisi, M., Pasqualetti, A., Passaquieti, R., Passuello, D., Persichetti, G., Pichot, M., Piergiovanni, F., Pietka, M., Pinard, L., Poggiani, R., Prato, M., Prodi, G.A., Punturo, M., Puppo, P., Rabeling, D.S., Racz, I., Rapagnani, P., Re, V., Regimbau, T., Ricci, F., Robinet, F., Rocchi, A., Rolland, L., Romano, R., Rosinska, D., Ruggi, P., Sassolas, B., Sentenac, D., Sperandio, L., Sturani, R., Swinkels, B., Toncelli, A., Tonelli, M., Torre, O., Tournefier, E., Travasso, F., Vajente, G., van den Brand, J.F.J., van Der Putten, S., Vasuth, M., Vavoulidis, M., Vedovato, G., Verkindt, D., Vetrano, F., Vicere, A., Vinet, J.-Y., Vocca, H., Ward, R.L., Was, M., Yvert, M., Laboratoire d'Annecy de Physique des Particules ( LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules ), Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Savoie Mont Blanc ( USMB [Université de Savoie] [Université de Chambéry] ) -Centre National de la Recherche Scientifique ( CNRS ), APC - Cosmologie, Physique Corpusculaire et Cosmologie - Collège de France ( PCC ), Collège de France ( CdF ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Paris Diderot - Paris 7 ( UPD7 ) -Centre National de la Recherche Scientifique ( CNRS ) -Collège de France ( CdF ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Paris Diderot - Paris 7 ( UPD7 ) -Centre National de la Recherche Scientifique ( CNRS ) -AstroParticule et Cosmologie ( APC - UMR 7164 ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Centre National de la Recherche Scientifique ( CNRS ) -Observatoire de Paris-Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ), Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux ( ARTEMIS ), Université Nice Sophia Antipolis ( UNS ), Université Côte d'Azur ( UCA ) -Université Côte d'Azur ( UCA ) -Institut national des sciences de l'Univers ( INSU - CNRS ) -Observatoire de la Côte d'Azur, Université Côte d'Azur ( UCA ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire de l'Accélérateur Linéaire ( LAL ), Université Paris-Sud - Paris 11 ( UP11 ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ), Institut de Physique de Rennes ( IPR ), Université de Rennes 1 ( UR1 ), Université de Rennes ( UNIV-RENNES ) -Université de Rennes ( UNIV-RENNES ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire des matériaux avancés ( LMA ), Université Claude Bernard Lyon 1 ( UCBL ), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ) -Centre National de la Recherche Scientifique ( CNRS ), AstroParticule et Cosmologie ( APC - UMR 7164 ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ), APC - Gravitation ( APC-Gravitation ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut), Max-Planck-Institut-Max-Planck-Institut, ESPCI ParisTech, LIGO, VIRGO, Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux (ARTEMIS), Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Institut de Physique de Rennes (IPR), Université de Rennes 1 (UR1), Université de Rennes (UNIV-RENNES)-Université de Rennes (UNIV-RENNES)-Centre National de la Recherche Scientifique (CNRS), Laboratoire des matériaux avancés (LMA), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon, APC - Gravitation (APC-Gravitation), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Max-Planck-Gesellschaft-Max-Planck-Gesellschaft, Ecole Superieure de Physique et de Chimie Industrielles de la Ville de Paris (ESPCI Paris), Université Paris sciences et lettres (PSL), The LIGO Scientific, Collaboration, the VIRGO, Collaboration, Calloni, Enrico, DE ROSA, Rosario, Forte, LUCA ANTONIO, Garufi, Fabio, Milano, Leopoldo, Mosca, Simona, Pardi, Silvio, Parisi, Maria, G., Persichetti, Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université de Rennes (UR)-Centre National de la Recherche Scientifique (CNRS), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Laboratoire d'Annecy de Physique des Particules (LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules), Physique Corpusculaire et Cosmologie - Collège de France (PCC), Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-AstroParticule et Cosmologie (APC (UMR_7164)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, and PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI)
Subjects: Physics, Solar mass, Physics and Astronomy (miscellaneous), 010308 nuclear & particles physics, Gravitational wave, Detector, Real-time computing, Astronomy, Binary number, 01 natural sciences, LIGO, [ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], Computer Science::Hardware Architecture, Coincident, 0103 physical sciences, [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], Low Mass, 010303 astronomy & astrophysics
Abstract: International audience; A very low latency search pipeline has been developed for the LIGO S6 and Virgo VSR2 science runs, targeting signals from coalescing compact binary systems with total mass from 2 to 35 solar masses. The goal of this search is to provide both single-detector triggers and multi-detector coincident triggers with a latency of a few minutes, the former for online detector monitoring and the latter to allow searching for electromagnetic counterparts to possible gravitational wave candidates. The features and current performance of this low latency search pipeline are presented.
Published: 2010

10. Search for Gravitational Waves from Compact Binary Coalescence in LIGO and Virgo Data from S5 and VSR1

Author: Abadie, J., Abbott, B., Abbott, R., Abernathy, M., Accadia, T., Acerneseac, F., Adams, C., Adhikari, R., Affeldt, C., Allen, B., Allen, G., Ceron, E., Amariutei, D., Amin, R., Anderson, S., Anderson, W., Antonuccia, F., Arai, K., Arain, M., Araya, M., Aston, S., Astonea, P., Atkinson, D., Aufmuth, P., Aulbert, C., Aylott, B., Babak, S., Baker, P., Ballardin, G., Ballmer, S., Barker, D., Barnum, S., Baroneac, F., Barr, B., Barriga, P., Barsotti, L., Barsuglia, M., Barton, M., Bartos, I., Bassiri, R., Bastarrika, M., Bastiab, A., Bauchrowitz, J., Bauera, T., Behnke, B., Bekera, M., Bell, A., Belletoile, A., Belopolski, I., Benacquista, M., Bertolini, A., Betzwieser, J., Beveridge, N., Beyersdorf, P., Bilenko, I., Billingsley, G., Birch, J., Birindellia, S., Biswas, R., Bitossia, M., Bizouarda, M., Black, E., Blackburn, J., Blackburn, L., Blair, D., Bland, B., Bloma, M., Bock, O., Bodiya, T., Bogan, C., Bondarescu, R., Bondub, F., Bonelliab, L., Bonnand, R., Bork, R., Born, M., Boschia, V., Bose, S., Bosia, L., Bouhou, B., Boyle, M., Braccinia, S., Bradaschiaa, C., Brady, P., Braginsky, V., Brau, J., Breyer, J., Bridges, D., Brilleta, A., Brinkmann, M., Brissona, V., Britzger, M., Brooks, A., Brown, D., Brummit, A., Budzyńskib, R., Bulikbc, T., Bultenab, H., Buonanno, A., Burguet--Castell, J., Burmeister, O., Buskulic, D., Buy, C., Byer, R., Cadonati, L., Cagnolia, G., Cain, J., Calloniab, E., Camp, J., Campagnaab, E., Campsie, P., Cannizzo, J., Cannon, K., Canuel, B., Cao, J., Capano, C., Carbognani, F., Caride, S., Caudill, S., Cavaglià, M., Cavaliera, F., Cavalieri, R., Cellaa, G., Cepeda, C., Cesarinib, E., Chaibia, O., Chalermsongsak, T., Chalkley, E., Charlton, P., Chassande-Mottin, E., Chelkowski, S., Chen, Y., Chincarini, A., Christensen, N., Chua, S., Chung, C., Chung, S., Clara, F., Clark, D., Clark, J., Clayton, J., Clevaa, F., Cocciaab, E., Colacinoab, C., Colas, J., Collaab, A., Colombinib, M., Conte, R., Cook, D., Corbitt, T., Cornish, N., Corsia, A., Costa, C., Coughlin, M., Coulona, J., Coward, D., Coyne, D., Creighton, J., Creighton, T., Cruise, A., Culter, R., Cumming, A., Cunningham, L., Cuoco, E., Dahl, K., Danilishin, S., Dannenberg, R., D'Antonioa, S., Danzmann, K., Das, K., Dattilo, V., Daudert, B., Daveloza, H., Daviera, M., Davies, G., Daw, E., Day, R., Dayanga, T., Rosaab, R., DeBra, D., Debreczeni, G., Degallaix, J., Preteac, M., Dent, T., Dergachev, V., DeRosa, R., DeSalvo, R., Dhurandhar, S., Fiorea, L., Lietoab, A., Palma, I., Emilioac, M., Virgilioa, A., Díaz, M., Dietz, A., Donovan, F., Dooley, K., Dorsher, S., Douglas, E., Dragocd, M., Drever, R., Driggers, J., Dumas, J., Dwyer, S., Eberle, T., Edgar, M., Edwards, M., Effler, A., Ehrens, P., Engel, R., Etzel, T., Evans, M., Evans, T., Factourovich, M., Fafoneab, V., Fairhurst, S., Fan, Y., Farr, B., Fazi, D., Fehrmann, H., Feldbaum, D., Ferranteab, I., Fidecaroab, F., Finn, L., Fiori, I., Flaminio, R., Flanigan, M., Foley, S., Forsi, E., Fortea, L., Fotopoulos, N., Fourniera, J., Franc, J., Frascaab, S., Frasconia, F., Frede, M., Frei, M., Frei, Z., Freise, A., Frey, R., Fricke, T., Friedrich, D., Fritschel, P., Frolov, V., Fulda, P., Fyffe, M., Galimberti, M., Gammaitoniab, L., Garcia, J., Garofoli, J., Garufiab, F., Gáspár, M., Gemme, G., Genin, E., Gennaia, A., Ghosh, S., Giaime, J., Giampanis, S., Giardina, K., Giazottoa, A., Gill, C., Goetz, E., Goggin, L., González, G., Gorodetsky, M., Goßler, S., Gouaty, R., Graef, C., Granata, M., Grant, A., Gras, S., Gray, C., Greenhalgh, R., Gretarsson, A., Greveriea, C., Grosso, R., Grote, H., Grunewald, S., Guidiab, G., Guido, C., Gupta, R., Gustafson, E., Gustafson, R., Hage, B., Hallam, J., Hammer, D., Hammond, G., Hanks, J., Hanna, C., Hanson, J., Harms, J., Harry, G., Harry, I., Harstad, E., Hartman, M., Haughian, K., Hayama, K., Hayaub, J., Hayler, T., Heefner, J., Heitmann, H., Helloa, P., Hendry, M., Heng, I., Heptonstall, A., Herrera, V., Hewitson, M., Hild, S., Hoak, D., Hodge, K., Holt, K., Hong, T., Hooper, S., Hosken, D., Hough, J., Howell, E., Huet, D., Hughey, B., Husa, S., Huttner, S., Ingram, D., Inta, R., Isogai, T., Ivanov, A., Jaranowskid, P., Johnson, W., Jones, D., Jones, G., Jones, R., Ju, L., Kalmus, P., Kalogera, V., Kandhasamy, S., Kanner, J., Katsavounidis, E., Katzman, W., Kawabe, K., Kawamura, S., Kawazoe, F., Kells, W., Kelner, M., Keppel, D., Khalaidovski, A., Khalili, F., Khazanov, E., Kim, H., Kim, N., King, P., Kinzel, D., Kissel, J., Klimenko, S., Kondrashov, V., Kopparapu, R., Koranda, S., Korth, W., Kowalskab, I., Kozak, D., Kringel, V., Krishnamurthy, S., Krishnan, B., Królakae, A., Kuehn, G., Kumar, R., Kwee, P., Landry, M., Lantz, B., Lastzka, N., Lazzarini, A., Leaci, P., Leong, J., Leonor, I., Leroya, N., Letendre, N., Li, J., Lia, T., Liguoriab, N., Lindquist, P., Lockerbie, N., Lodhia, D., Lorenzinia, M., Lorietteb, V., Lormand, M., Losurdoa, G., Lu, P., Luan, J., Lubinski, M., Lück, H., Lundgren, A., Macdonald, E., Machenschalk, B., MacInnis, M., Mageswaran, M., Mailand, K., Majoranaa, E., Maksimovicb, I., Mana, N., Mandel, I., Mandic, V., Mantovaniac, M., Marandi, A., Marchesonia, F., Marion, F., Márka, S., Márka, Z., Maros, E., Marque, J., Martelliab, F., Martin, I., Martin, R., Marx, J., Mason, K., Masserot, A., Matichard, F., Matone, L., Matzner, R., Mavalvala, N., McCarthy, R., McClelland, D., McGuire, S., McIntyre, G., McKechan, D., Meadors, G., Mehmet, M., Meier, T., Melatos, A., Melissinos, A., Mendell, G., Mercer, R., Merill, L., Meshkov, S., Messenger, C., Meyer, M., Miao, H., Michel, C., Milanoab, L., Miller, J., Minenkova, Y., Mino, Y., Mitrofanov, V., Mitselmakher, G., Mittleman, R., Miyakawa, O., Moe, B., Moesta, P., Mohan, M., Mohanty, S., Mohapatra, S., Moraru, D., Moreno, G., Morgado, N., Morgiaab, A., Moscaab, S., Moscatellia, V., Mossavi, K., Mours, B., Mow--Lowry, C., Mueller, G., Mukherjee, S., Mullavey, A., Müller-Ebhardt, H., Munch, J., Murray, P., Nash, T., Nawrodt, R., Nelson, J., Neriab, I., Newton, G., Nishida, E., Nishizawa, A., Nocera, F., Nolting, D., Ochsner, E., O'Dell, J., Ogin, G., Oldenburg, R., O'Reilly, B., O'Shaughnessy, R., Osthelder, C., Ott, C., Ottaway, D., Ottens, R., Overmier, H., Owen, B., Page, A., Pagliaroliac, G., Palladinoac, L., Palombaa, C., Pan, Y., Pankow, C., Paolettia, F., Papa, M., Parameswaran, A., Pardiab, S., Parisiab, M., Pasqualetti, A., Passaquietiab, R., Passuelloa, D., Patel, P., Pathak, D., Pedraza, M., Pekowsky, L., Penn, S., Peralta, C., Perreca, A., Persichettiab, G., Phelps, M., Pichota, M., Pickenpack, M., Piergiovanniab, F., Pietkad, M., Pinard, L., Pinto, I., Pitkin, M., Pletsch, H., Plissi, M., Podkaminer, J., Poggianiab, R., Pöld, J., Postiglione, F., Prato, M., Predoi, V., Price, L., Prijatelj, M., Principe, M., Privitera, S., Prix, R., Prodiab, G., Prokhorov, L., Puncken, O., Punturoa, M., Puppoa, P., Quetschke, V., Raab, F., Rabelingab, D., Rácz, I., Radkins, H., Raffai, P., Rakhmanov, M., Ramet, C., Rankins, B., Rapagnaniab, P., Raymond, V., Reab, V., Redwine, K., Reed, C., Reed, T., Regimbaua, T., Reid, S., Reitze, D., Ricciab, F., Riesen, R., Riles, K., Roberts, P., Robertson, N., Robineta, F., Robinson, C., Robinson, E., Rocchia, A., Roddy, S., Rolland, L., Rollins, J., Romano, J., Romanoac, R., Romie, J., Rosińskacf, D., Röver, C., Rowan, S., Rüdiger, A., Ruggi, P., Ryan, K., Sakata, S., Sakosky, M., Salemi, F., Salit, M., Sammut, L., Sancho de la Jordana, L., Sandberg, V., Sannibale, V., Santamaría, L., Santiago-Prieto, I., Santostasi, G., Saraf, S., Sassolas, B., Sathyaprakash, B., Sato, S., Satterthwaite, M., Saulson, P., Savage, R., Schilling, R., Schlamminger, S., Schnabel, R., Schofield, R., Schulz, B., Schutz, B., Schwinberg, P., Scott, J., Scott, S., Searle, A., Seifert, F., Sellers, D., Sengupta, A., Sentenac, D., Sergeev, A., Shaddock, D., Shaltev, M., Shapiro, B., Shawhan, P., Weerathunga, T., Shoemaker, D., Sibley, A., Siemens, X., Sigg, D., Singer, A., Singer, L., Sintes, A., Skelton, G., Slagmolen, B., Slutsky, J., Smith, J., Smith, M., Smith, N., Smith, R., Somiya, K., Sorazu, B., Soto, J., Speirits, F., Sperandioab, L., Stefszky, M., Stein, A., Steinlechner, J., Steinlechner, S., Steplewski, S., Stochino, A., Stone, R., Strain, K., Strigin, S., Stroeer, A., Sturaniab, R., Stuver, A., Summerscales, T., Sung, M., Susmithan, S., Sutton, P., Swinkels, B., Szokoly, G., Tacca, M., Talukder, D., Tanner, D., Tarabrin, S., Taylor, J., Taylor, R., Thomas, P., Thorne, K., Thrane, E., Thüring, A., Titsler, C., Tokmakov, K., Toncelliab, A., Tonelliab, M., Torreac, O., Torres, C., Torrie, C., Tournefier, E., Travassoab, F., Traylor, G., Trias, M., Tseng, K., Turner, L., Ugolini, D., Urbanek, K., Vahlbruch, H., Vaishnav, B., Vajenteab, G., Vallisneri, M., van den Brandab, J., Broeck, C., van der Puttena, S., van der Sluys, M., van Veggel, A., Vass, S., Vasuth, M., Vaulin, R., Vavoulidisa, M., Vecchio, A., Vedovatoc, G., Veitch, J., Veitch, P., Veltkamp, C., Verkindt, D., Vetranoab, F., Viceréab, A., Villar, A., Vineta, J., Voccaa, H., Vorvick, C., Vyachanin, S., Waldman, S., Wallace, L., Wanner, A., Ward, R., Wasa, M., Wei, P., Weinert, M., Weinstein, A., Weiss, R., Wen, L., Wen, S., Wessels, P., West, M., Westphal, T., Wette, K., Whelan, J., Whitcomb, S., White, D., Whiting, B., Wilkinson, C., Willems, P., Williams, H., Williams, L., Willke, B., Winkelmann, L., Winkler, W., Wipf, C., Wiseman, A., Woan, G., Wooley, R., Worden, J., Yablon, J., Yakushin, I., Yamamoto, H., Yamamoto, K., Yang, H., Yeaton-Massey, D., Yoshida, S., Yu, P., Yvert, M., Zanolin, M., Zhang, L., Zhang, Z., Zhao, C., Zotov, N., Zucker, M., Zweizig, J., The Ligo Scientific, Collaboration, Virgo, Collaboration, Calloni, Enrico, DE ROSA, Rosario, Garufi, Fabio, Milano, Leopoldo, Mosca, Simona, Pardi, Silvio, Parisi, Maria, G., Persichetti, Pinto, Innocenzo, Laboratoire d'Annecy de Physique des Particules ( LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules ), Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Savoie Mont Blanc ( USMB [Université de Savoie] [Université de Chambéry] ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire de l'Accélérateur Linéaire ( LAL ), Université Paris-Sud - Paris 11 ( UP11 ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ), ESPCI ParisTech, APC - Cosmologie, Physique Corpusculaire et Cosmologie - Collège de France ( PCC ), Collège de France ( CdF ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Paris Diderot - Paris 7 ( UPD7 ) -Centre National de la Recherche Scientifique ( CNRS ) -Collège de France ( CdF ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Paris Diderot - Paris 7 ( UPD7 ) -Centre National de la Recherche Scientifique ( CNRS ) -AstroParticule et Cosmologie ( APC - UMR 7164 ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Centre National de la Recherche Scientifique ( CNRS ) -Observatoire de Paris-Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ), Observatoire de la Côte d'Azur ( OCA ), Centre National de la Recherche Scientifique ( CNRS ), Institut de Physique de Rennes ( IPR ), Université de Rennes 1 ( UR1 ), Université de Rennes ( UNIV-RENNES ) -Université de Rennes ( UNIV-RENNES ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire des matériaux avancés ( LMA ), Université Claude Bernard Lyon 1 ( UCBL ), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ) -Centre National de la Recherche Scientifique ( CNRS ), AstroParticule et Cosmologie ( APC - UMR 7164 ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ), APC - Gravitation ( APC-Gravitation ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut), Max-Planck-Institut-Max-Planck-Institut, Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Ecole Superieure de Physique et de Chimie Industrielles de la Ville de Paris (ESPCI Paris), Université Paris sciences et lettres (PSL), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Observatoire de la Côte d'Azur (OCA), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Institut de Physique de Rennes (IPR), Université de Rennes (UR)-Centre National de la Recherche Scientifique (CNRS), Laboratoire des matériaux avancés (LMA), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), APC - Gravitation (APC-Gravitation), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Max-Planck-Gesellschaft-Max-Planck-Gesellschaft, Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Université de Rennes 1 (UR1), Université de Rennes (UNIV-RENNES)-Université de Rennes (UNIV-RENNES)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), (Astro)-Particles Physics, Laboratoire d'Annecy de Physique des Particules (LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules), Physique Corpusculaire et Cosmologie - Collège de France (PCC), Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-AstroParticule et Cosmologie (APC (UMR_7164)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Centre National de la Recherche Scientifique (CNRS), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), The LIGO Scientific Collaboration, and The Virgo Collaboration
Subjects: Nuclear and High Energy Physics, Stellar mass, Astrophysics::High Energy Astrophysical Phenomena, X-ray binary, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, FORMS, 7. Clean energy, 01 natural sciences, Gravitational-wave astronomy, General Relativity and Quantum Cosmology, [ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], Binary black hole, 0103 physical sciences, Binary star, Laser interferometry, Gravitational wave interferometers, BLACK HOLES, 010306 general physics, QC, Astrophysics::Galaxy Astrophysics, QB, Physics, GRAVITATIONAL WAVES, NEUTRON STARS, 010308 nuclear & particles physics, Gravitational wave, Settore FIS/01 - Fisica Sperimentale, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy, LIGO, Neutron star, [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]
Abstract: LIGO Sci Collaboration; Virgo Collaboration; International audience; We report the results of the first search for gravitational waves from compact binary coalescence using data from the Laser Interferometer Gravitational-Wave Observatory and Virgo detectors. Five months of data were collected during the Laser Interferometer Gravitational-Wave Observatory's S5 and Virgo's VSR1 science runs. The search focused on signals from binary mergers with a total mass between 2 and 35M(circle dot). No gravitational waves are identified. The cumulative 90%-confidence upper limits on the rate of compact binary coalescence are calculated for nonspinning binary neutron stars, black hole-neutron star systems, and binary black holes to be 8: 7 X 10(-3) yr(-1) L-10(-1), 2.2 X 10(-3) yr(-1) L-10(-1), and 4.4 X 10(-4) yr(-1) L-10(-1), respectively, where L-10 is 10(10) times the blue solar luminosity. These upper limits are compared with astrophysical expectations.
Published: 2010

11. Mice with a homozygous null mutation for the most abundant glutathione peroxidase, Gpx1, show increased susceptibility to the oxidative stress- inducing agents paraquat and hydrogen peroxide.

Author: Zheng S.S., Kola I., Hertzog P.J., De Haan J.B., Beart P.M., Bladier C., Griffiths P., Kelner M., O'Shea R.D., Cheung N.S., Bronson R.T., Silvestro M.J., Wild S., Zheng S.S., Kola I., Hertzog P.J., De Haan J.B., Beart P.M., Bladier C., Griffiths P., Kelner M., O'Shea R.D., Cheung N.S., Bronson R.T., Silvestro M.J., and Wild S.
Abstract: Glutathione peroxidases have been thought to function in cellular antioxidant defense. However, some recent studies on Gpx1 knockout (-/-) mice have failed to show a role for Gpx1 under conditions of oxidative stress such as hyperbaric oxygen and the exposure of eye lenses to high levels of H2O2. These findings have, unexpectedly, raised the issue of the role of Gpx1, especially under conditions of oxidative stress. Here we demonstrate a role for Gpx1 in protection against oxidative stress by showing that Gpx1 (-/-) mice are highly sensitive to the oxidant paraquat. Lethality was already detected within 24 h in mice exposed to paraquat at 10 mg . kg-1 (approximately 1/7 the LD50 of wild-type controls). The effects of paraquat were dose-related. In the 30 mg . kg-1-treated group, 100% of mice died within 5 h, whereas the controls showed no evidence of toxicity. We further demonstrate that paraquat transcriptionally upregulates Gpx1 in normal cells, reinforcing a role for Gpx1 in protection against paraquat toxicity. Finally, we show that cortical neurons from Gpx1 (-/-) mice are more susceptible to H2O2; 30% of neurons from Gpx1 (-/-) mice were killed when exposed to 65 muM H2O2, whereas the wild-type controls were unaffected. These data establish a function for Gpx1 in protection against some oxidative stressors and in protection of neurons against H2O2. Further, they emphasize the need to elucidate the role of Gpx1 in protection against different oxidative stressors and in different disease states and suggest that Gpx1 (-/-) mice may be valuable for studying the role of H2O2 in neurodegenerative disorders.
Published: 2012

12. The emerging role of the physician in genetic counselling and testing for heritable breast, ovarian and colon cancer

Author: Taylor, K M and Kelner, M J
Subjects: Moral Obligations, Ovarian Neoplasms, Genetic Research, Health Knowledge, Attitudes, Practice, Genetic Services, Information Dissemination, Uncertainty, Breast Neoplasms, Genetic Counseling, Disclosure, Empirical Research, Colorectal Neoplasms, Hereditary Nonpolyposis, Neoplastic Syndromes, Hereditary, Predictive Value of Tests, Risk Factors, Humans, Family, Female, Interdisciplinary Communication, Genetic Testing, Physician's Role, Research Article, Forecasting
Abstract: As a genetic testing for susceptibility to breast, ovarian and colon cancer becomes more readily available, physicians are faced with an increasing demand for information about inherited cancer risk. Because advances in treatment have not kept pace with advances in predictive testing, the provision of genetic counselling and testing marks a departure from the traditional role of the physician. A systematic framework is needed within which the physician's emerging role in predictive testing for heritable cancer can be delineated. The development of such a framework will require collaboration among professionals in a range of scientific disciplines, as well as the suspension of traditional assumptions about the physicians role.
Published: 1996

13. ChemInform Abstract: Total Synthesis of Hydroxymethylacylfulvene (XIII), an Antitumor Derivative of Illudin S.

Author: MCMORRIS, T. C., primary, HU, Y., additional, YU, J., additional, and KELNER, M. J., additional
Published: 2010
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14. ChemInform Abstract: Design and Synthesis of Antitumor Acylfulvenes.

Author: MCMORRIS, T. C., primary, YU, J., additional, HU, Y., additional, ESTES, L. A., additional, and KELNER, M. J., additional
Published: 2010
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15. ChemInform Abstract: Reaction of Antitumor Hydroxymethylacylfulvene (HMAF) with Thiols.

Author: MCMORRIS, T. C., primary, YU, J., additional, ESTES, L. A., additional, and KELNER, M. J., additional
Published: 2010
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16. Opinions of health policy makers on integration of complementary and conventional medicine

Author: Kelly, M, primary, Hardwick, K, additional, Moritz, S, additional, Kelner, M, additional, Rickhi, B, additional, and Quan, H, additional
Published: 2010
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17. The need to demonstrate efficacy and safety: the views of complementary/alternative medicine leaders

Author: Kelner, M J, primary and Wellman, B, additional
Published: 2010
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18. Dosing of troxacitabine (Troxatyl [T], SGX-145) based on renal function

Author: Kelner, M. J., primary, Giles, F. J., additional, Feldman, E. J., additional, Roboz, G. J., additional, Deangelo, D. J., additional, and Burley, S. K., additional
Published: 2006
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19. Troxacitabine administered by continuous infusion (CI) is well tolerated and effective in adults with relapsed or refractory acute myeloid leukemia (AML)

Author: Roboz, G., primary, Jolivet, J., additional, Kelner, M., additional, Allen-Bard, S., additional, Park, L., additional, Lokker, N. A., additional, Giese, N. A., additional, and Feldman, E. J., additional
Published: 2005
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20. Quality end-of-life care: patients' perspectives.

Author: Singer PA, Martin DK, Kelner M, Singer, P A, Martin, D K, and Kelner, M
Abstract: Context: Quality end-of-life care is increasingly recognized as an ethical obligation of health care providers, both clinicians and organizations. However, this concept has not been examined from the perspective of patients.Objective: To identify and describe elements of quality end-of-life care from the patient's perspective.Design: Qualitative study using in-depth, open-ended, face-to-face interviews and content analysis.Setting: Toronto, Ontario.Participants: A total of 126 participants from 3 patient groups: dialysis patients (n = 48), people with human immunodeficiency virus infection (n = 40), and residents of a long-term care facility (n = 38).Outcome Measures: Participants' views on end-of-life issues.Results: Participants identified 5 domains of quality end-of-life care: receiving adequate pain and symptom management, avoiding inappropriate prolongation of dying, achieving a sense of control, relieving burden, and strengthening relationships with loved ones.Conclusion: These domains, which characterize patients' perspectives on end-of-life care, can serve as focal points for improving the quality of end-of-life care. [ABSTRACT FROM AUTHOR]
Published: 1999
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21. ChemInform Abstract: An Acetal Derivative of Illudin S with Improved Antitumor Activity.

Author: MCMORRIS, T. C., primary, YU, J., additional, GANTZEL, P. K., additional, ESTES, L. A., additional, and KELNER, M. J., additional
Published: 1997
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22. Strengthening medical research through an integrated approach

Author: Kelner, M J, primary and Taylor, K M, additional
Published: 1995
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23. HPLC Analysis of Novel Anti-Cancer Agents-Illudins and Their Analogs

Author: Brandšteterová, E., primary, Kelner, M. J., additional, Mc Morris, T. C., additional, Wang, W., additional, and Bangell, R, additional
Published: 1993
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24. High-power electron beam controlled discharge N2O laser.

Author: Frolov, K., Ionin, Andrei A., Kelner, M., Sinitsyn, Dmitrii V., Suchkov, A. F., and Zhivukcin, I.
Published: 1991
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25. HIGH PRESSURE N2O LASER : DISCHARGE PROPERTIES, GAIN AND SPECTRA

Author: IONIN, A. A., primary, KELNER, M. S., additional, LOBANOV, A. N., additional, OKHRIMENKO, D. B., additional, SINITSIN, D. V., additional, and SUCHKOV, A. F., additional
Published: 1991
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26. Preclinical Evaluation of Illudins as Anticancer Agents: Basis for Selective Cytotoxicity

Author: Kelner, M. J., primary, McMorris, T. C., additional, and Taetle, R., additional
Published: 1990
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27. Alteration of endogenous glutathione peroxidase, manganese superoxide dismutase, and glutathione transferase activity in cells transfected with a copper-zinc superoxide dismutase expression vector. Explanation for variations in paraquat resistance.

Author: Kelner, M J, primary and Bagnell, R, additional
Published: 1990
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28. Thioureas react with superoxide radicals to yield a sulfhydryl compound. Explanation for protective effect against paraquat.

Author: Kelner, M J, primary, Bagnell, R, additional, and Welch, K J, additional
Published: 1990
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29. Moving forward? Complementary and alternative practitioners seeking self-regulation.

Author: Welsh S, Kelner M, Wellman B, and Boon H
Subjects: *ALTERNATIVE medicine, *ACUPUNCTURISTS, *HOMEOPATHIC physicians, *MEDICAL sciences
Abstract: Complementary and alternative medicine (CAM) occupations continue to struggle towards achieving professional status, especially in the form of statutory regulation. Many consider professional status a worthwhile goal for CAM occupations, yet it is a process fraught with tensions. In this paper we present in-depth interview data from the leaders of three CAM groups (naturopaths, traditional Chinese medicine practitioners acupuncturists, and homeopaths) in Ontario, Canada that demonstrate four main strategies used by these groups to professionalize. The strategies discussed are related to how the knowledge base of each group is organised and transmitted. These strategies include: improving educational standards, improving practice standards, engaging in peer-reviewed research and increasing group cohesion. At the core of these strategies is the demarcation of who is qualified to practice, and a signalling to 'outsiders', such as medicine and the government, that practitioners are qualified and legitimate. Across the three groups, the leaders referred to the inclusion of medical science as a basis for distinguishing between 'science' and 'non-science' as well as who should practice and who should not. We highlight how internal battles over the infusion of medical science into the knowledge base are part of the process for establishing legitimacy for the three CAM groups in our study. We end with a brief discussion of the implications of these internal battles over medical science knowledge for the future of CAM groups. [ABSTRACT FROM AUTHOR]
Published: 2004
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30. Health care and consumer choice: medical and alternative therapies.

Author: Kelner M and Wellman B
Abstract: This paper reports on research conducted in a large Canadian city during 1994-1995. The study examines the motivations of patients who choose to seek care from one of five different types of practitioners: family physicians, chiropractors, acupuncturists/traditional Chinese doctors, naturopaths and Reiki practitioners. We use the Andersen socio-behavioural model to help explain why people choose orthodox medicine or a type of alternative care. The data are derived from face to face interviews with 300 patients: 60 from each of the five modes of treatment. The findings demonstrate that this model can explain the use of alternative as well as orthodox medical services. Patients choose specific kinds of practitioners for particular problems, and some use a mixture of practitioners to treat a specific complaint. The choice of type of practitioner(s) is multidimensional and cannot solely be explained either by disenchantment with medicine or by an 'alternative ideology'. [ABSTRACT FROM AUTHOR]
Published: 1997
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31. The integration of behavioral science theory and clinical experience for second-year medical students.

Author: Taylor, K M, Shapiro, M, and Kelner, M
Published: 1983
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32. Preparation and Biological Activity of Amino Acid and Peptide Conjugates of Antitumor Hydroxymethylacylfulvene

Author: McMorris, T. C., Yu, J., Ngo, H.-T., Wang, H., and Kelner, M. J.
Abstract: The primary hydroxyl group in hydroxymethylacylfulvene, a potent antitumor drug, is readily replaced by thiols including cysteine, N-acetylcysteine, homocysteine, and glutathione. Best yields are obtained when reaction is carried out in the presence of dilute sulfuric acid. A variety of sulfur-containing analogues have been prepared, and their toxicity to tumor cells was examined.
Published: 2000

33. Structural organization of the microsomal glutathione S-transferase gene (MGST1) on chromosome 12p13.1-13.2. Identification of the correct promoter region and demonstration of transcriptional regulation in response to oxidative stress.

Author: Kelner, M J, Bagnell, R D, Montoya, M A, Estes, L A, Forsberg, L, and Morgenstern, R
Abstract: The structure and regulation of the microsomal glutathione S-transferase gene (MGST1) are considerably more complex than originally perceived to be. The MGST1 gene has two alternative first exons and is located in the 12p13.1-13.2 region. Two other potential first exons were determined to be nonfunctional. The region between the functional first exons cannot direct transcription. Thus, one common promoter element directing transcription exists, and RNA splicing occurs such that only one of the first exons (containing only untranslated mRNA) is incorporated into each mRNA species with common downstream exons. MGST1 expression and regulation are therefore similar to those of other hepatic xenobiotic handling enzymes, which also produce mRNA species differing only in the 5'-untranslated regions to yield identical proteins. MGST1 was previously considered a "housekeeping" gene, as non-oxidant inducers had little effect on activity. However, the promoter region immediately upstream of the dominant first exon transcriptionally responds to oxidative stress. In this respect, MGST1 is similar to glutathione peroxidases that also transcriptionally respond to oxidative stress. The discovery that MGST1 utilizes alternative first exon splicing eliminates a problem with the first description of MGST1 cDNA in that it appeared that MGST1 expression was in violation of the ribosomal scanning model. The identification that the first exon originally noted is in fact a minor alternative first exon far downstream of the primary first exon eliminates this conundrum.
Published: 2000

34. Structural organization of the human gastrointestinal glutathione peroxidase (GPX2) promoter and 3prime-nontranscribed region: transcriptional response to exogenous redox agents

Author: Kelner, M. J., Bagnell, R. D., Montoya, M. A., and Lanham, K. A.
Published: 2000
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35. Metabolism of antitumor acylfulvene by rat liver cytosol

Author: McMorris, T. C., Elayadi, A. N., Yu, J., and Kelner, M. J.
Published: 1999
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36. Efficacy of MGI 114 (6-hydroxymethylacylfulvene, HMAF) Against the mdr1/gp170 Metastatic MV522 Lung Carcinoma Xenograft

Author: Kelner, M. J., McMorris, T. C., Estes, L., Samson, K. M., Bagnell, R. D., and Taetle, R.
Published: 1998
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37. Methylene blue directly oxidizes glutathione without the intermediate formation of hydrogen peroxide.

Author: Kelner, M J and Alexander, N M
Abstract: Methylene blue stimulates the oxidation of glutathione in red blood cells in vitro and in vivo. This oxidation has been attributed to hydrogen peroxide that is generated from the autooxidation of leucomethylene blue arising from the reduction of methylene blue by NADPH. In this report we present evidence that methylene blue directly oxidizes glutathione and that oxidation of glutathione by hydrogen peroxide is a secondary reaction. Moreover, superoxide dismutase has no effect on the oxidation. Under aerobic conditions, methylene blue oxidizes glutathione 30 times faster than the spontaneous autooxidation of glutathione. Under anaerobic conditions the stoichiometry of the reaction of methylene blue with glutathione supports a direct chemical reaction. The reaction rates between glutathione and methylene blue suggest a second order reaction over the conditions tested. That neither oxygen radical formation nor significant amounts of hydrogen peroxide are produced by methylene blue, even in the presence of added glucose, is further confirmed by the failure to detect significant amounts of lipid peroxidation products, or hemolysis, in red blood cells incubated with the dye.
Published: 1985
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38. Inhibition of erythrocyte superoxide dismutase by diethyldithiocarbamate also results in oxyhemoglobin-catalyzed glutathione depletion and methemoglobin production.

Author: Kelner, M J and Alexander, N M
Abstract: N,N-Diethyldithiocarbamate (DDC), a copper-chelating agent, not only inhibits superoxide dismutase activity in the red cell, but also depletes glutathione and promotes the production of methemoglobin, sulfhemoglobin, and small amounts of lipid peroxidation products. DDC reacts with oxyhemoglobin to yield disulfiram, hydrogen peroxide, and methemoglobin. Disulfiram and hydrogen peroxide both convert GSH to GSSG, while DDC reduces methemoglobin to oxyhemoglobin. Although disulfiram also reacts with the hemoglobin sulfhydryl groups, this reaction does not play a role in the conversion of GSH to GSSG. Other hemoglobin derivatives, ferrous, and ferric ions do not catalyze the oxidation of GSH by DDC. These results support the conclusion that DDC reacts with the super-oxo-ferriheme complex of oxyhemoglobin to generate hydrogen peroxide and disulfiram and that the cyclic conversion of oxyhemoglobin to methemoglobin and DDC and disulfiram results in the net oxidation of GSH. Thus, damage to DDC-treated erythrocytes exposed to a putative superoxide-generating toxin, such as 1,4-naphthoquinone-2-sulfonate, may actually be due to diminished GSH concentration and hemoglobin oxidation rather than to superoxide radicals. Glucose added to the incubation medium of DDC-treated erythrocytes fully prevented glutathione depletion but not the oxidation of oxyhemoglobin to methemoglobin. Several other copper-chelating agents either failed to inhibit the activity of purified superoxide dismutase or when incubated with erythrocytes produced more extensive GSH depletion and hemoglobin oxidation than DDC. It is concluded that the interpretation of results with erythrocytes exposed to copper-chelating agents must consider their effects on GSH and hemoglobin as well as on superoxide dismutase inhibition. Moreover, one must be mindful of the interference by DDC in the analysis of GSH with 5,5'-dithiobis-(2-nitrobenzoic acid) in the absence of sufficient quantities of metaphosphoric acid to destroy DDC and that contamination of DDC with trace quantities of disulfiram may be a significant problem.
Published: 1986
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39. Elevation in the ratio of Cu/Zn-superoxide dismutase to glutathione peroxidase activity induces features of cellular senescence and this effect is mediated by hydrogen peroxide.

Author: de Haan, J B, Cristiano, F, Iannello, R, Bladier, C, Kelner, M J, and Kola, I
Abstract: Although reactive oxygen species have been proposed to play a major role in the aging process, the exact molecular mechanisms remain elusive. In this study we investigate the effects of a perturbation in the ratio of Cu/Zn-superoxide dismutase activity (Sod1 dismutases .O2-to H2O2) to glutathione peroxidase activity (Gpx1 catalyses H2O2 conversion to H2O) on cell growth and development. Our data demonstrate that Sod1 transfected cell lines that have an elevation in the ratio of Sod1 activity to Gpx1 activity produce higher levels of H2O2 and exhibit well characterised markers of cellular senescence viz. slower proliferation and altered morphology. On the contrary, Sod1 transfected cell lines that have an unaltered ratio in the activity of these two enzymes, have unaltered levels of H2O2 and fail to show characteristics of senescence. Furthermore, fibroblasts established from individuals with Down syndrome have an increase in the ratio of Sod1 to Gpx1 activity compared with corresponding controls and senesce earlier. Interestingly, cells treated with H2O2 also show features of senescence and/or senesce earlier. We also show that Cip1 mRNA levels are elevated in Down syndrome cells, Sod1 transfectants with an altered Sod1 to Gpx1 activity ratio and those treated with H2O2, thus suggesting that the slow proliferation may be mediated by Cip1. Furthermore, our data demonstrate that Cip1 mRNA levels are induced by exposure of cells to H2O2. These data give valuable insight into possible molecular mechanisms that contribute tribute to cellular senescence and may be useful in the evolution of therapeutic strategies for aging.
Published: 1996
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40. Mice with a homozygous null mutation for the most abundant glutathione peroxidase, Gpx1, show increased susceptibility to the oxidative stress-inducing agents paraquat and hydrogen peroxide.

Author: de Haan, J B, Bladier, C, Griffiths, P, Kelner, M, O'Shea, R D, Cheung, N S, Bronson, R T, Silvestro, M J, Wild, S, Zheng, S S, Beart, P M, Hertzog, P J, and Kola, I
Abstract: Glutathione peroxidases have been thought to function in cellular antioxidant defense. However, some recent studies on Gpx1 knockout (-/-) mice have failed to show a role for Gpx1 under conditions of oxidative stress such as hyperbaric oxygen and the exposure of eye lenses to high levels of H2O2. These findings have, unexpectedly, raised the issue of the role of Gpx1, especially under conditions of oxidative stress. Here we demonstrate a role for Gpx1 in protection against oxidative stress by showing that Gpx1 (-/-) mice are highly sensitive to the oxidant paraquat. Lethality was already detected within 24 h in mice exposed to paraquat at 10 mg.kg-1 (approximately (1)/(7) the LD50 of wild-type controls). The effects of paraquat were dose-related. In the 30 mg.kg-1-treated group, 100% of mice died within 5 h, whereas the controls showed no evidence of toxicity. We further demonstrate that paraquat transcriptionally up-regulates Gpx1 in normal cells, reinforcing a role for Gpx1 in protection against paraquat toxicity. Finally, we show that cortical neurons from Gpx1 (-/-) mice are more susceptible to H2O2; 30% of neurons from Gpx1 (-/-) mice were killed when exposed to 65 microM H2O2, whereas the wild-type controls were unaffected. These data establish a function for Gpx1 in protection against some oxidative stressors and in protection of neurons against H2O2. Further, they emphasize the need to elucidate the role of Gpx1 in protection against different oxidative stressors and in different disease states and suggest that Gpx1 (-/-) mice may be valuable for studying the role of H2O2 in neurodegenerative disorders.
Published: 1998

41. Heterologous Expression of Carbonyl Reductase: Demonstration of Prostaglandin 9-Ketoreductase Activity and Paraquat Resistance

Author: Kelner, M. J., Estes, L., Rutherford, M., Uglik, S. F., and Peitzke, J. A.
Published: 1997
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42. (Hydroxymethyl)acylfulvene: An Illudin Derivative with Superior Antitumor Properties

Author: McMorris, T. C., Kelner, M. J., Wang, W., Yu, J., Estes, L. A., and Taetle, R.
Abstract: Reaction of the fungal sesquiterpene illudin S with excess paraformaldehyde in dilute H2SO4 gives (hydroxymethyl)acylfulvene. The primary allylic hydroxyl thus formed can undergo very facile replacement by a variety of nucleophiles. (Hydroxymethyl)acylfulvene (MGI.114) was more toxic than a precursor, acylfulvene, but less toxic than the parent compound illudin S to HL 60 cells.
Published: 1996

43. Rhodamine B ingestion as a cause of fluorescent red urine

Author: Kelner, M J
Subjects: Adult, Male, Adolescent, Xanthenes, Food, Pregnancy, Rhodamines, Humans, Female, Urine, Fluorescence, Research Article
Published: 1985

44. Understanding physicians' response to AIDS

Author: Taylor, K M, Shapiro, M, Skinner, H A, Eakin, J, and Kelner, M
Subjects: Acquired Immunodeficiency Syndrome, Physician-Patient Relations, Attitude of Health Personnel, Physicians, Public Opinion, North America, Health Resources, Humans, Professional Practice, Delivery of Health Care, Health Education, Prejudice, Research Article
Abstract: Attempts to comprehend physicians' extreme reaction to AIDS (acquired immune deficiency syndrome) have met with great difficulty since the disease brings into question traditional norms and assumptions. As the medical profession struggles to develop guidelines and policies to help it deal with this disease, it can draw on very little systematic research on the effect of AIDS on physicians' attitudes and practices. We suggest a framework developed from the literature on physicians' and society's response to other disorders that would provide a basis for organizing the ever-increasing amount of information on physicians and AIDS and would guide systematic research aimed at understanding and predicting physicians' participation in the prevention and management of AIDS. Within this framework we consider how characteristics of the disease, elements of the health care system and physicians' attitudes interact to influence clinical and personal practices. AIDS had led to new delineations of physicians' responsibility, modification of prevailing beliefs about physician autonomy and thus a redefinition of the role of the physician in North America.
Published: 1989

45. American Pediatrics: The Social Dynamics of Professionalism, 1880-1980. Sydney Halpern

Author: Kelner, M. J.
Published: 1989

46. Reaction of Irofulven with Zinc and Acid

Author: McMorris, T. C., Moon, S.-S., and Kelner, M. J.
Abstract: Reaction of antitumor agent irofulven (1) with zinc and acetic acid yielded several new indene derivatives (6, 7, 8, 10) as well as the known indene (9). These all have greatly reduced toxicity to human leukemia (HL60) cells compared to irofulven.
Published: 2003

47. Sesquiterpenes from the Basidiomycete Omphalotus illudens

Author: McMorris, T. C., Lira, R., Gantzel, P. K., Kelner, M. J., and Dawe, R.
Abstract: A new sesquiterpene, omphadiol (4), has been isolated from cultures of Omphalotus illudens. Several known compounds, including illudosin (1), were also obtained. Structures were determined using MS, NMR, and X-ray techniques.
Published: 2000

48. Complementary and alternative therapies for pain in older adults

Author: Burford-Mason, A., Dryden, T., Kelner, M., Saunders, P. R., and Mark Ware

49. BEATING THE SPIN-DOWN LIMIT ON GRAVITATIONAL WAVE EMISSION FROM THE VELA PULSAR

Author: Abadie, J., Abbott, B. P., Abbott, R., Abernathy, M., Accadia, T., Acernese, F., Adams, C., Adhikari, R., Affeldt, C., Allen, B., Allen, G. S., Ceron, E. A., Amariutei, D., Amin, R. S., Anderson, S. B., Anderson, W. G., Antonucci, F., Arai, K., Arain, M. A., Araya, M. C., Aston, S. M., Astone, P., Atkinson, D., Aufmuth, P., Aulbert, C., Aylott, B. E., Babak, S., Baker, P., Ballardin, G., Ballmer, S., Barker, D., Barnum, S., Barone, F., Barr, B., Barriga, P., Barsotti, L., Barsuglia, M., Barton, M. A., Bartos, I., Bassiri, R., Bastarrika, M., Basti, A., Bauchrowitz, J., Bauer, T. S., Behnke, B., Bejger, M., Beker, M. G., Bell, A. S., Belletoile, A., Belopolski, I., Benacquista, M., Bertolini, A., Betzwieser, J., Beveridge, N., Beyersdorf, P. T., Bilenko, I. A., Billingsley, G., Birch, J., Birindelli, S., Biswas, R., Bitossi, M., Bizouard, M. A., Black, E., Blackburn, J. K., Blackburn, L., Blair, D., Bland, B., Blom, M., Bock, O., Bodiya, T. P., Bogan, C., Bondarescu, R., Bondu, F., Bonelli, L., Bonnand, R., Bork, R., Born, M., Boschi, V., Bose, S., Bosi, L., Bouhou, B., Boyle, M., Braccini, S., Bradaschia, C., Brady, P. R., Braginsky, V. B., Brau, J. E., Breyer, J., Bridges, D. O., Brillet, A., Brinkmann, M., Brisson, V., Britzger, M., Brooks, A. F., Brown, D. A., Brummit, A., Budzynski, R., Bulik, T., Bulten, H. J., Buonanno, A., Burguet-Castell, J., Burmeister, O., Buskulic, D., Buy, C., Byer, R. L., Cadonati, L., Cagnoli, G., Cain, J., Calloni, E., Camp, J. B., Campagna, E., Campsie, P., Cannizzo, J., Cannon, K., Canuel, B., Cao, J., Capano, C., Carbognani, F., Caride, S., Caudill, S., Cavaglia, M., Cavalier, F., Cavalieri, R., Cella, G., Cepeda, C., Cesarini, E., Chaibi, O., Chalermsongsak, T., Chalkley, E., Charlton, P., Chassande-Mottin, E., Chelkowski, S., Chen, Y., Chincarini, A., Christensen, N., S. S. Y., C. T. Y., Chung, S., Clara, F., Clark, D., Clark, J., Clayton, J. H., Cleva, F., Coccia, E., Colacino, C. N., Colas, J., Colla, A., Colombini, M., Conte, R., Cook, D., Corbitt, T. R., Cornish, N., Corsi, A., Costa, C. A., Coughlin, M., Coulon, J., Coward, D. M., Coyne, D. C., J. D. E., Creighton, T. D., Cruise, A. M., Culter, R. M., Cumming, A., Cunningham, L., Cuoco, E., Dahl, K., Danilishin, S. L., Dannenberg, R., Antonio, S. D., Danzmann, K., Das, K., Dattilo, V., Daudert, B., Daveloza, H., Davier, M., Davies, G., Daw, E. J., Day, R., Dayanga, T., Rosa, R. D., Debra, D., Debreczeni, G., Degallaix, J., Prete, M. D., Dent, T., Dergachev, V., Derosa, R., Desalvo, R., Dhurandhar, S., Fiore, L. D., Lieto, A. D., Palma, I. D., Paolo, M. D., Virgilio, A. D., Diaz, M., Dietz, A., Donovan, F., Dooley, K. L., Dorsher, S., E. S. D., Drago, M., R. W. P., Driggers, J. C., Dumas, J., Dwyer, S., Eberle, T., Edgar, M., Edwards, M., Effler, A., Ehrens, P., Engel, R., Etzel, T., Evans, M., Evans, T., Factourovich, M., Fafone, V., Fairhurst, S., Fan, Y., Farr, B. F., Fazi, D., Fehrmann, H., Feldbaum, D., Ferrante, I., Fidecaro, F., Finn, L. S., Fiori, I., Flaminio, R., Flanigan, M., Foley, S., Forsi, E., Forte, L. A., Fotopoulos, N., Fournier, J., Franc, J., Frasca, S., Frasconi, F., Frede, M., Frei, M., Frei, Z., Freise, A., Frey, R., Fricke, T. T., Friedrich, D., Fritschel, P., Frolov, V. V., Fulda, P., Fyffe, M., Galimberti, M., Gammaitoni, L., Garcia, J., Garofoli, J. A., Garufi, F., Gaspar, M. E., Gemme, G., Genin, E., Gennai, A., Ghosh, S., Giaime, J. A., Giampanis, S., Giardina, K. D., Giazotto, A., Gill, C., Goetz, E., Goggin, L. M., Gonzalez, G., Gorodetsky, M. L., Gossler, S., Gouaty, R., Graef, C., Granata, M., Grant, A., Gras, S., Gray, C., R. J. S., Gretarsson, A. M., Greverie, C., Grosso, R., Grote, H., Grunewald, S., Guidi, G. M., Guido, C., Gupta, R., Gustafson, E. K., Gustafson, R., Hage, B., Hallam, J. M., Hammer, D., Hammond, G., Hanks, J., Hanna, C., Hanson, J., Harms, J., Harry, G. M., Harry, I. W., Harstad, E. D., Hartman, M. T., Haughian, K., Hayama, K., Hayau, J., Hayler, T., Heefner, J., Heitmann, H., Hello, P., Hendry, M. A., Heng, I. S., Heptonstall, A. W., Herrera, V., Hewitson, M., Hild, S., Hoak, D., Hodge, K. A., Holt, K., Hong, T., Hooper, S., Hosken, D. J., Hough, J., Howell, E. J., Huet, D., Hughey, B., Husa, S., Huttner, S. H., Ingram, D. R., Inta, R., Isogai, T., Ivanov, A., Jaranowski, P., Johnson, W. W., Jones, D. I., Jones, G., Jones, R., Ju, L., Kalmus, P., Kalogera, V., Kandhasamy, S., Kanner, J. B., Katsavounidis, E., Katzman, W., Kawabe, K., Kawamura, S., Kawazoe, F., Kells, W., Kelner, M., Keppel, D. G., Khalaidovski, A., Khalili, F. Y., Khazanov, E. A., Kim, H., Kim, N., King, P. J., Kinzel, D. L., Kissel, J. S., Klimenko, S., Kondrashov, V., Kopparapu, R., Koranda, S., Korth, W. Z., Kowalska, I., Kozak, D., Kringel, V., Krishnamurthy, S., Krishnan, B., Krolak, A., Kuehn, G., Kumar, R., Kwee, P., Landry, M., Lantz, B., Lastzka, N., Lazzarini, A., Leaci, P., Leong, J., Leonor, I., Leroy, N., Letendre, N., Li, J., T. G. F., Liguori, N., Lindquist, P. E., Lockerbie, N. A., Lodhia, D., Lorenzini, M., Loriette, V., Lormand, M., Losurdo, G., Lu, P., Luan, J., Lubinski, M., Lueck, H., Lundgren, A. P., Macdonald, E., Machenschalk, B., Macinnis, M., Mageswaran, M., Mailand, K., Majorana, E., Maksimovic, I., Man, N., Mandel, I., Mandic, V., Mantovani, M., Marandi, A., Marchesoni, F., Marion, F., Marka, S., Marka, Z., Maros, E., Marque, J., Martelli, F., Martin, I. W., Martin, R. M., Marx, J. N., Mason, K., Masserot, A., Matichard, F., Matone, L., Matzner, R. A., Mavalvala, N., Mccarthy, R., Mcclelland, D. E., Mcguire, S. C., Mcintyre, G., D. J. A., Meadors, G., Mehmet, M., Meier, T., Melatos, A., Melissinos, A. C., Mendell, G., Mercer, R. A., Merill, L., Meshkov, S., Messenger, C., Meyer, M. S., Miao, H., Michel, C., Milano, L., Miller, J., Minenkov, Y., Mino, Y., Mitrofanov, V. P., Mitselmakher, G., Mittleman, R., Miyakawa, O., Moe, B., Moesta, P., Mohan, M., Mohanty, S. D., S. R. P., Moraru, D., Moreno, G., Morgado, N., Morgia, A., Mosca, S., Moscatelli, V., Mossavi, K., Mours, B., Mow-Lowry, C. M., Mueller, G., Mukherjee, S., Mullavey, A., Mueller-Ebhardt, H., Munch, J., Murray, P. G., Nash, T., Nawrodt, R., Nelson, J., Neri, I., Newton, G., Nishida, E., Nishizawa, A., Nocera, F., Nolting, D., Ochsner, E., J. O'Dell, Ogin, G. H., Oldenburg, R. G., Reilly, B. O., Shaughnessy, R. O., Osthelder, C., Ott, C. D., Ottaway, D. J., Ottens, R. S., Overmier, H., Owen, B. J., Page, A., Pagliaroli, G., Palladino, L., Palomba, C., Pan, Y., Pankow, C., Paoletti, F., Papa, M. A., Parameswaran, A., Pardi, S., Parisi, M., Pasqualetti, A., Passaquieti, R., Passuello, D., Patel, P., Pathak, D., Pedraza, M., Pekowsky, L., Penn, S., Peralta, C., Perreca, A., Persichetti, G., Phelps, M., Pichot, M., Pickenpack, M., Piergiovanni, F., Pietka, M., Pinard, L., Pinto, I. M., Pitkin, M., Pletsch, H. J., Plissi, M. V., Podkaminer, J., Poggiani, R., Poeld, J., Postiglione, F., Prato, M., Predoi, V., Price, L. R., Prijatelj, M., Principe, M., Privitera, S., Prix, R., Prodi, G. A., Prokhorov, L., Puncken, O., Punturo, M., Puppo, P., Quetschke, V., Raab, F. J., Rabeling, D. S., Racz, I., Radkins, H., Raffai, P., Rakhmanov, M., Ramet, C. R., Rankins, B., Rapagnani, P., Raymond, V., Re, V., Redwine, K., Reed, C. M., Reed, T., Regimbau, T., Reid, S., Reitze, D. H., Ricci, F., Riesen, R., Riles, K., Roberts, P., Robertson, N. A., Robinet, F., Robinson, C., Robinson, E. L., Rocchi, A., Roddy, S., Rolland, L., Rollins, J., Romano, J. D., Romano, R., Romie, J. H., Rosinska, D., Roever, C., Rowan, S., Ruediger, A., Ruggi, P., Ryan, K., Sakata, S., Sakosky, M., Salemi, F., Salit, M., Sammut, L., L. S. de, Sandberg, V., Sannibale, V., Santamaria, L., Santiago-Prieto, I., Santostasi, G., Saraf, S., Sassolas, B., Sathyaprakash, B. S., Sato, S., Satterthwaite, M., Saulson, P. R., Savage, R., Schilling, R., Schlamminger, S., Schnabel, R., R. M. S., Schulz, B., Schutz, B. F., Schwinberg, P., Scott, J., Scott, S. M., Searle, A. C., Seifert, F., Sellers, D., Sengupta, A. S., Sentenac, D., Sergeev, A., Shaddock, D. A., Shaltev, M., Shapiro, B., Shawhan, P., Weerathunga, T. S., Shoemaker, D. H., Sibley, A., Siemens, X., Sigg, D., Singer, A., Singer, L., Sintes, A. M., Skelton, G., B. J. J., Slutsky, J., Smith, J. R., Smith, M. R., Smith, N. D., Smith, R., Somiya, K., Sorazu, B., Soto, J., Speirits, F. C., Sperandio, L., Stefszky, M., Stein, A. J., Steinlechner, J., Steinlechner, S., Steplewski, S., Stochino, A., Stone, R., Strain, K. A., Strigin, S., Stroeer, A. S., Sturani, R., Stuver, A. L., Summerscales, T. Z., Sung, M., Susmithan, S., Sutton, P. J., Swinkels, B., Szokoly, G. P., Tacca, M., Talukder, D., Tanner, D. B., Tarabrin, S. P., Taylor, J. R., Taylor, R., Thomas, P., Thorne, K. A., Thorne, K. S., Thrane, E., Thuering, A., Titsler, C., Tokmakov, K. V., Toncelli, A., Tonelli, M., Torre, O., Torres, C., Torrie, C. I., Tournefier, E., Travasso, F., Traylor, G., Trias, M., Tseng, K., Turner, L., Ugolini, D., Urbanek, K., Vahlbruch, H., Vaishnav, B., Vajente, G., Vallisneri, M., J. F. J., Den, C. V., S. v. der, M. V. van, A. A. van, Vass, S., Vasuth, M., Vaulin, R., Vavoulidis, M., Vecchio, A., Vedovato, G., Veitch, J., Veitch, P. J., Veltkamp, C., Verkindt, D., Vetrano, F., Vicere, A., Villar, A. E., Vinet, J., Vocca, H., Vorvick, C., Vyachanin, S. P., Waldman, S. J., Wallace, L., Wanner, A., Ward, R. L., Was, M., Wei, P., Weinert, M., Weinstein, A. J., Weiss, R., Wen, L., Wen, S., Wessels, P., West, M., Westphal, T., Wette, K., Whelan, J. T., Whitcomb, S. E., White, D., Whiting, B. F., Wilkinson, C., Willems, P. A., Williams, H. R., Williams, L., Willke, B., Winkelmann, L., Winkler, W., Wipf, C. C., Wiseman, A. G., Woan, G., Wooley, R., Worden, J., Yablon, J., Yakushin, I., Yamamoto, H., Yamamoto, K., Yang, H., Yeaton-Massey, D., Yoshida, S., Yu, P., Yvert, M., Zanolin, M., Zhang, L., Zhang, Z., Zhao, C., Zotov, N., Zucker, M. E., Zweizig, J., Buchner, S., Hotan, A., Palfreyman, J., Collaboration, L. S., Collaboration, V., Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), APC - Cosmologie, AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Observatoire de la Côte d'Azur (OCA), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Institut de Physique de Rennes (IPR), Université de Rennes 1 (UR1), Université de Rennes (UNIV-RENNES)-Université de Rennes (UNIV-RENNES)-Centre National de la Recherche Scientifique (CNRS), Laboratoire des matériaux avancés (LMA), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon, APC - Gravitation (APC-Gravitation), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Max-Planck-Gesellschaft-Max-Planck-Gesellschaft, Ecole Superieure de Physique et de Chimie Industrielles de la Ville de Paris (ESPCI Paris), Université Paris sciences et lettres (PSL), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université de Rennes (UR)-Centre National de la Recherche Scientifique (CNRS), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Laboratoire d'Annecy de Physique des Particules ( LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules ), Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Savoie Mont Blanc ( USMB [Université de Savoie] [Université de Chambéry] ) -Centre National de la Recherche Scientifique ( CNRS ), Physique Corpusculaire et Cosmologie - Collège de France ( PCC ), Collège de France ( CdF ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Paris Diderot - Paris 7 ( UPD7 ) -Centre National de la Recherche Scientifique ( CNRS ) -Collège de France ( CdF ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Paris Diderot - Paris 7 ( UPD7 ) -Centre National de la Recherche Scientifique ( CNRS ) -AstroParticule et Cosmologie ( APC - UMR 7164 ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Centre National de la Recherche Scientifique ( CNRS ) -Observatoire de Paris-Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ), Observatoire de la Côte d'Azur ( OCA ), Centre National de la Recherche Scientifique ( CNRS ), Laboratoire de l'Accélérateur Linéaire ( LAL ), Université Paris-Sud - Paris 11 ( UP11 ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ), Institut de Physique de Rennes ( IPR ), Université de Rennes 1 ( UR1 ), Université de Rennes ( UNIV-RENNES ) -Université de Rennes ( UNIV-RENNES ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire des matériaux avancés ( LMA ), Université Claude Bernard Lyon 1 ( UCBL ), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ) -Centre National de la Recherche Scientifique ( CNRS ), AstroParticule et Cosmologie ( APC - UMR 7164 ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ), APC - Gravitation ( APC-Gravitation ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut), Max-Planck-Institut-Max-Planck-Institut, Ecole Supérieure de Physique et de Chimie Industrielles ( ESPCI ), Mairie de Paris, (Astro)-Particles Physics, Student Lab and Education, Laboratoire d'Annecy de Physique des Particules (LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules), Physique Corpusculaire et Cosmologie - Collège de France (PCC), Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-AstroParticule et Cosmologie (APC (UMR_7164)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Centre National de la Recherche Scientifique (CNRS), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Ecole Supérieure de Physique et de Chimie Industrielles (ESPCI), F., Acernese, F., Barone, Calloni, Enrico, DE ROSA, Rosario, L., Di Fiore, Garufi, Fabio, Milano, Leopoldo, S., Mosca, M., Parisi, G., Persichetti, R., Romano, Pinto, Innocenzo, The LIGO Scientific Collaboration, and The Virgo Collaboration
Subjects: [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], NEUTRON-STARS, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, DEFORMATIONS, Vela, pulsars: individual (PSR J0835-4510), 01 natural sciences, General Relativity and Quantum Cosmology, [ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], gravitational waves, stars: neutron, Settore FIS/05 - Astronomia e Astrofisica, Pulsar, TIMING PACKAGE, SEARCH, 0103 physical sciences, QC176, Limit (mathematics), neutron star, 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, Spin-½, pulsars, pulsars: individual (psr j0835-4510), High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Degree (graph theory), 010308 nuclear & particles physics, Gravitational wave, [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Settore FIS/01 - Fisica Sperimentale, [ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Astronomy and Astrophysics, Polarization (waves), Orientation (vector space), pulsars: individual, Gravitational waves, Space and Planetary Science, [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], [ SDU.ASTR.HE ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Astrophysics - High Energy Astrophysical Phenomena, TEMPO2
Abstract: We present direct upper limits on continuous gravitational wave emission from the Vela pulsar using data from the Virgo detector's second science run. These upper limits have been obtained using three independent methods that assume the gravitational wave emission follows the radio timing. Two of the methods produce frequentist upper limits for an assumed known orientation of the star's spin axis and value of the wave polarization angle of, respectively, $1.9\ee{-24}$ and $2.2\ee{-24}$, with 95% confidence. The third method, under the same hypothesis, produces a Bayesian upper limit of $2.1\ee{-24}$, with 95% degree of belief. These limits are below the indirect {\it spin-down limit} of $3.3\ee{-24}$ for the Vela pulsar, defined by the energy loss rate inferred from observed decrease in Vela's spin frequency, and correspond to a limit on the star ellipticity of $\sim 10^{-3}$. Slightly less stringent results, but still well below the spin-down limit, are obtained assuming the star's spin axis inclination and the wave polarization angles are unknown., Comment: 37 pages, 6 figures corrected typo in the Authors field

50. Definitive liquid-chromatographic demonstration that N-ethylglycine is the metabolite of lidocaine that interferes in the Kodak sarcosine oxidase-coupled method for creatinine.

Author: Roberts, R T, primary, Alexander, N M, primary, and Kelner, M J, primary
Published: 1988
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