Swift follow-Up Observations of Candidate Gravitational-Wave Transient Events. Evans, P A, Fridriksson, J K, Gehrels, N, Homan, J, Osborne, J P, Siegel, M, Beardmore, A, Handbauer, P, Gelbord, J, Kennea, J A, Smith, M, Zhu, Q, the LIGO Scientific Collaboration, Collaboration, V., Aasi, J, Abadie, J., Abbott, B P, Abbott, R, Abbott, T. D, Abernathy, M., Accadia, T, Acernese, F, Adams, C, Adams, T. S, Addesso, P, Adhikari, R., Affeldt, C, Agathos, M, Agatsuma, K., Ajith, P, Allen, B., Allocca, A, Amador Ceron, E, Amariutei, D, Anderson, S. B, Anderson, W. G, Arai, K., Araya, M C, Ast, S, Aston, S M, Astone, P., Atkinson, D, Aufmuth, P, Aulbert, C., Aylott, B E, Babak, S, Baker, P, Ballardin, G, Ballmer, S., Bao, Y, Barayoga, J C B, Barker, D., Barone, F, Barr, B, Barsotti, L., Barsuglia, M, Barton, M A, Bartos, I, Bassiri, R, Bastarrika, M, Basti, A, Batch, J, Bauchrowitz, J, Bauer, T. S, Bebronne, M, Beck, D, Behnke, B, Bejger, M, Beker, M G, Bell, A S, Bell, C, Belopolski, I, Benacquista, M, Berliner, J M, Bertolini, A., Betzwieser, J, Beveridge, N, Beyersdorf, P T, Bhadbade, T, Bilenko, I A, Billingsley, G, Birch, J, Biswas, R, Bitossi, M, Bizouard, M A, Black, E, Blackburn, J K, Blackburn, L, Blair, D G, Bland, B, Blom, M, Bock, O, Bodiya, T P, Bogan, C, Bond, C, Bondarescu, R, Bondu, F, Bonelli, L, Bonnand, R, Bork, R, Born, M, Boschi, V, Bose, S., Bosi, L, Bouhou, B, Braccini, S, Bradaschia, C, Brady, P R, Braginsky, V B, Branchesi, M, Brau, J E, Breyer, J, Briant, T, Bridges, D O, Brillet, A, Brinkmann, M, Brisson, V, Britzger, M, Brooks, A F, Brown, D. A, Bulik, T, Bulten, H J, Buonanno, A., Burguet--Castell, J, Buskulic, D, Buy, C, Byer, R L, Cadonati, L, Cagnoli, G, Calloni, E, Camp, J B, Campsie, P, Cannon, K. C, Canuel, B, Cao, J, Capano, C. 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Swift follow-Up Observations of Candidate Gravitational-Wave Transient Events [link]Paper  doi  abstract   bibtex   
We present the first multi-wavelength follow-up observations of two candidate gravitational-wave (GW) transient events recorded by LIGO and Virgo in their 2009-2010 science run. The events were selected with low latency by the network of GW detectors (within less than 10 minutes) and their candidate sky locations were observed by the Swift observatory (within 12 hr). Image transient detection was used to analyze the collected electromagnetic data, which were found to be consistent with background. Off-line analysis of the GW data alone has also established that the selected GW events show no evidence of an astrophysical origin; one of them is consistent with background and the other one was a test, part of a blind injection challenge. With this work we demonstrate the feasibility of rapid follow-ups of GW transients and establish the sensitivity improvement joint electromagnetic and GW observations could bring. This is a first step toward an electromagnetic follow-up program in the regime of routine detections with the advanced GW instruments expected within this decade. In that regime, multi-wavelength observations will play a significant role in completing the astrophysical identification of GW sources. We present the methods and results from this first combined analysis and discuss its implications in terms of sensitivity for the present and future instruments.
@article{evans_swift_2012,
	title = {Swift follow-{Up} {Observations} of {Candidate} {Gravitational}-{Wave} {Transient} {Events}},
	volume = {203},
	url = {http://stacks.iop.org/0067-0049/203/i=2/a=28?key=crossref.948837d1419a06cc020c4384967e09e3},
	doi = {10.1088/0067-0049/203/2/28},
	abstract = {We present the first multi-wavelength follow-up observations of two candidate gravitational-wave (GW) transient events recorded by LIGO and Virgo in their 2009-2010 science run. The events were selected with low latency by the network of GW detectors (within less than 10 minutes) and their candidate sky locations were observed by the Swift observatory (within 12 hr). Image transient detection was used to analyze the collected electromagnetic data, which were found to be consistent with background. Off-line analysis of the GW data alone has also established that the selected GW events show no evidence of an astrophysical origin; one of them is consistent with background and the other one was a test, part of a blind injection challenge. With this work we demonstrate the feasibility of rapid follow-ups of GW transients and establish the sensitivity improvement joint electromagnetic and GW observations could bring. This is a first step toward an electromagnetic follow-up program in the regime of routine detections with the advanced GW instruments expected within this decade. In that regime, multi-wavelength observations will play a significant role in completing the astrophysical identification of GW sources. We present the methods and results from this first combined analysis and discuss its implications in terms of sensitivity for the present and future instruments.},
	number = {2},
	journal = {The Astrophysical Journal Supplement Series},
	author = {Evans, P A and Fridriksson, J K and Gehrels, N and Homan, J and Osborne, J P and Siegel, M and Beardmore, A and Handbauer, P and Gelbord, J and Kennea, J A and Smith, M and Zhu, Q and {the LIGO Scientific Collaboration and Virgo Collaboration} and Aasi, J and Abadie, Joshua and Abbott, B P and Abbott, R and Abbott, Thomas D and Abernathy, Matthew and Accadia, T and Acernese, F and Adams, C and Adams, Thomas S and Addesso, P and Adhikari, Rana and Affeldt, C and Agathos, M and Agatsuma, Kazuhiro and Ajith, P and Allen, Bruce and Allocca, A and Amador Ceron, E and Amariutei, D and Anderson, Stuart B and Anderson, Warren G and Arai, Koji and Araya, M C and Ast, S and Aston, S M and Astone, Pia and Atkinson, D and Aufmuth, P and Aulbert, Carsten and Aylott, B E and Babak, S and Baker, P and Ballardin, G and Ballmer, Stefan and Bao, Y and Barayoga, J C B and Barker, David and Barone, F and Barr, B and Barsotti, Lisa and Barsuglia, M and Barton, M A and Bartos, I and Bassiri, R and Bastarrika, M and Basti, A and Batch, J and Bauchrowitz, J and Bauer, Th S and Bebronne, M and Beck, D and Behnke, B and Bejger, M and Beker, M G and Bell, A S and Bell, C and Belopolski, I and Benacquista, M and Berliner, J M and Bertolini, Alessandro and Betzwieser, J and Beveridge, N and Beyersdorf, P T and Bhadbade, T and Bilenko, I A and Billingsley, G and Birch, J and Biswas, R and Bitossi, M and Bizouard, M A and Black, E and Blackburn, J K and Blackburn, L and Blair, D G and Bland, B and Blom, M and Bock, O and Bodiya, T P and Bogan, C and Bond, C and Bondarescu, R and Bondu, F and Bonelli, L and Bonnand, R and Bork, R and Born, M and Boschi, V and Bose, Sukanta and Bosi, L and Bouhou, B and Braccini, S and Bradaschia, C and Brady, P R and Braginsky, V B and Branchesi, M and Brau, J E and Breyer, J and Briant, T and Bridges, D O and Brillet, A and Brinkmann, M and Brisson, V and Britzger, M and Brooks, A F and Brown, Duncan A and Bulik, T and Bulten, H J and Buonanno, Alessandra and Burguet--Castell, J and Buskulic, D and Buy, C and Byer, R L and Cadonati, L and Cagnoli, G and Calloni, E and Camp, J B and Campsie, P and Cannon, Kipp C and Canuel, B and Cao, J and Capano, Collin D and Carbognani, F and Carbone, L and Caride, S and Caudill, Sarah and Cavaglia, Marco and Cavalier, Fabien and Cavalieri, R and Cella, G and Cepeda, C and Cesarini, E and Chalermsongsak, T and Charlton, Philip and Chassande-Mottin, Eric and Chen, W and Chen, X and Chen, Yan-bei and Chincarini, A and Chiummo, A and Cho, H S and Chow, J and Christensen, Nelson and Chua, S S Y and Chung, C T Y and Chung, S and Ciani, G and Clara, F and Clark, D E and Clark, James and Clayton, Jessica H and Cleva, F and Coccia, E and Cohadon, P F and Colacino, C N and Colla, A and Colombini, M and Conte, A and Conte, R and Cook, D and Corbitt, Thomas R and Cordier, M and Cornish, Neil and Corsi, A and Costa, C A and Coughlin, M and Coulon, J-P and Couvares, P and Coward, D M and Cowart, M and Coyne, D C and Creighton, Jolien D E and Creighton, Teviot D and Cruise, A M and Cumming, A and Cunningham, L and Cuoco, E and Cutler, R M and Dahl, K and Damjanic, M and Danilishin, S L and D'Antonio, S and Danzmann, K and Dattilo, V and Daudert, B and Daveloza, H and Davier, M and Daw, E J and Day, R and Dayanga, T and De Rosa, R and DeBra, D and Debreczeni, G and Degallaix, J and Del Pozzo, W and Dent, T and Dergachev, V and DeRosa, R and Dhurandhar, Sanjeev V and Di Fiore, L and Di Lieto, A and Di Palma, Irene and Di Paolo Emilio, M and Di Virgilio, A and Díaz, M and Dietz, A and Donovan, F and Dooley, K L and Doravari, S and Dorsher, S and Drago, M and Drever, R W P and Driggers, J C and Du, Z and Dumas, J-C and Dwyer, S and Eberle, T and Edgar, M and Edwards, M and Effler, A and Ehrens, P and Eikenberry, S and Endröczi, G and Engel, R and Etzel, T and Evans, K and Evans, M and Evans, T and Factourovich, M and Fafone, V and Fairhurst, Stephen and Farr, B F and Favata, M and Fazi, D and Fehrmann, H and Feldbaum, D and Ferrante, I and Ferrini, F and Fidecaro, F and Finn, Lee Samuel and Fiori, I and Fisher, R P and Flaminio, R and Foley, S and Forsi, E and Forte, L A and Fotopoulos, N and Fournier, J-D and Franc, J and Franco, S and Frasca, S and Frasconi, F and Frede, M and Frei, M A and Frei, Z and Freise, A and Frey, R and Fricke, Tobin T and Friedrich, D and Fritschel, Peter and Frolov, V V and Fujimoto, Masa-Katsu and Fulda, P J and Fyffe, M and Gair, J and Galimberti, M and Gammaitoni, L and Garcia, J and Garufi, F and Gáspár, M E and Gelencser, G and Gemme, G and Genin, E and Gennai, A and Gergely, L Á and Ghosh, S and Giaime, J A and Giampanis, S and Giardina, K D and Giazotto, A and Gil-Casanova, S and Gill, C and Gleason, J and Goetz, E and González, Gabriela and Gorodetsky, M L and Goßler, S and Gouaty, R and Graef, C and Graff, P B and Granata, M and Grant, A and Gray, C and Greenhalgh, R J S and Gretarsson, A M and Griffo, C and Grote, H and Grover, K and Grunewald, S and Guidi, Gianluca M and Guido, C and Gupta, R and Gustafson, E K and Gustafson, R and Hallam, J M and Hammer, D and Hammond, Giles and Hanks, J and Hanna, Chad and Hanson, J and Harms, Jan and Harry, Gregory M and Harry, Ian W and Harstad, E D and Hartman, M T and Haughian, K and Hayama, K and Hayau, J F and Heefner, J and Heidmann, A and Heintze, M C and Heitmann, H and Hello, Patrice and Hemming, G and Hendry, M A and Heng, I S and Heptonstall, A W and Herrera, V and Heurs, M and Hewitson, Martin and Hild, S and Hoak, D and Hodge, K A and Holt, K and Holtrop, M and Hong, T and Hooper, S and Hough, J and Howell, E J and Hughey, Brennan and Husa, S and Huttner, S H and Huynh-Dinh, T and Ingram, D R and Inta, R and Isogai, Tomoki and Ivanov, A and Izumi, K and Jacobson, M and James, E and Jang, Y J and Jaranowski, P and Jesse, E and Johnson, W W and Jones, D I and Jones, R and Jonker, R J G and Ju, L and Kalmus, P and Kalogera, Vicky and Kandhasamy, S and Kang, G and Kanner, J B and Kasprzack, M and Kasturi, R and Katsavounidis, E and Katzman, W and Kaufer, H and Kaufman, K and Kawabe, K and Kawamura, Seiji and Kawazoe, F and Keitel, D and Kelley, D and Kells, W and Keppel, Drew Garvin and Keresztes, Z and Khalaidovski, A and Khalili, F Y and Khazanov, E A and Kim, B K and Kim, C and Kim, H and Kim, K and Kim, N and Kim, Y M and King, P J and Kinzel, D L and Kissel, J S and Klimenko, S and Kline, J and Kokeyama, Keiko and Kondrashov, V and Koranda, S and Korth, W Z and Kowalska, I and Kozak, D and Kringel, V and Krishnan, Badri and Królak, A and Kuehn, G and Kumar, P and Kumar, R and Kurdyumov, R and Kwee, P and Lam, P K and Landry, Michael and Langley, A and Lantz, B and Lastzka, N and Lawrie, C and Lazzarini, A and Le Roux, A and Leaci, P and Lee, C H and Lee, H K and Lee, H M and Leong, J R and Leonor, Isabel and Leroy, Nicolas and Letendre, N and Lhuillier, V and Li, J and Li, T G F and Lindquist, P E and Litvine, V and Liu, Y and Liu, Z and 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	month = nov,
	year = {2012},
	pages = {28}
}
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