J/ApJ/886/75 Search for GW signals associated with GRBs (Abbott+, 2019)
Search for gravitational-wave signals associated with gamma-ray bursts during
the second observing run of Advanced LIGO and Advanced Virgo.
Abbott B.P., Abbott R., Abbott T.D., Abraham S., Acernese F., Ackley K.,
Adams C., Adhikari R.X., Adya V.B., Affeldt C., Agathos M., Agatsuma K.,
Aggarwal N., Aguiar O.D., Aiello L., Ain A., Ajith P., Allen G., Allocca A.,
Aloy M.A., Altin P.A., Amato A., Anand S., Ananyeva A., Anderson S.B.,
Anderson W.G., Angelova S.V., Antier S., Appert S., Arai K., Araya M.C.,
Areeda J.S., Arene M., Arnaud N., Aronson S.M., Ascenzi S., Ashton G.,
Aston S.M., Astone P., Aubin F., Aufmuth P., AultONeal K., Austin C.,
Avendano V., Avila-Alvarez A., Babak S., Bacon P., Badaracco F.,
Bader M.K.M., Bae S., Baird J., Baker P.T., Baldaccini F., Ballardin G.,
Ballmer S.W., Bals A., Banagiri S., Barayoga J.C., Barbieri C.,
Barclay S.E., Barish B.C., Barker D., Barkett K., Barnum S., Barone F.,
Barr B., Barsotti L., Barsuglia M., Barta D., Bartlett J., Bartos I.,
Bassiri R., Basti A., Bawaj M., Bayley J.C., Bazzan M., Becsy B., Bejger M.,
Belahcene I., Bell A.S., Beniwal D., Benjamin M.G., Berger B.K.,
Bergmann G., Bernuzzi S., Berry C.P.L., Bersanetti D., Bertolini A.,
Betzwieser J., Bhandare R., Bidler J., Biggs E., Bilenko I.A., Bilgili S.A.,
Billingsley G., Birney R., Birnholtz O., Biscans S., Bischi M.,
Biscoveanu S., Bisht A., Bitossi M., Bizouard M.A., Blackburn J.K.,
Blackman J., Blair C.D., Blair D.G., Blair R.M., Bloemen S., Bobba F.,
Bode N., Boer M., Boetzel Y., Bogaert G., Bondu F., Bonnand R., Booker P.,
Boom B.A., Bork R., Boschi V., Bose S., Bossilkov V., Bosveld J.,
Bouffanais Y., Bozzi A., Bradaschia C., Brady P.R., Bramley A.,
Branchesi M., Brau J.E., Breschi M., Briant T., Briggs J.H., Brighenti F.,
Brillet A., Brinkmann M., Brockill P., Brooks A.F., Brooks J., Brown D.D.,
Brunett S., Buikema A., Bulik T., Bulten H.J., Buonanno A., Buskulic D.,
Buy C., Byer R.L., Cabero M., Cadonati L., Cagnoli G., Cahillane C.,
Bustillo J.C., Callister T.A., Calloni E., Camp J.B., Campbell W.A.,
Canepa M., Cannon K.C., Cao H., Cao J., Carapella G., Carbognani F.,
Caride S., Carney M.F., Carullo G., Diaz J.C., Casentini C., Caudill S.,
Cavaglia M., Cavalier F., Cavalieri R., Cella G., Cerda-Duran P.,
Cesarini E., Chaibi O., Chakravarti K., Chamberlin S.J., Chan M., Chao S.,
Charlton P., Chase E.A., Chassande-Mottin E., Chatterjee D., Chaturvedi M.,
Cheeseboro B.D., Chen H.Y., Chen X., Chen Y., Cheng H.-P., Cheong C.K.,
Chia H.Y., Chiadini F., Chincarini A., Chiummo A., Cho G., Cho H.S., Cho M.,
Christensen N., Chu Q., Chua S., Chung K.W., Chung S., Ciani G., Cieslar M.,
Ciobanu A.A., Ciolfi R., Cipriano F., Cirone A., Clara F., Clark J.A.,
Clearwater P., Cleva F., Coccia E., Cohadon P.-F., Cohen D., Colleoni M.,
Collette C.G., Collins C., Colpi M., Cominsky L.R., Constancio M., Conti L.,
Cooper S.J., Corban P., Corbitt T.R., Cordero-Carrion I., Corezzi S.,
Corley K.R., Cornish N., Corre D., Corsi A., Cortese S., Costa C.A.,
Cotesta R., Coughlin M.W., Coughlin S.B., Coulon J.-P., Countryman S.T.,
Couvares P., Covas P.B., Cowan E.E., Coward D.M., Cowart M.J., Coyne D.C.,
Coyne R., Creighton J.D.E., Creighton T.D., Cripe J., Croquette M.,
Crowder S.G., Cullen T.J., Cumming A., Cunningham L., Cuoco E., Canton T.D.,
Dalya G., D'Angelo B., Danilishin S.L., D'Antonio S., Danzmann K.,
Dasgupta A., Da Silva Costa C.F., Datrier L.E.H., Dattilo V., Dave I.,
Davier M., Davis D., Daw E.J., DeBra D., Deenadayalan M., Degallaix J., De
Laurentis M., Deleglise S., Del Pozzo W., DeMarchi L.M., Demos N., Dent T.,
De Pietri R., De Rosa R., De Rossi C., DeSalvo R., de Varona O.,
Dhurandhar S., Diaz M.C., Dietrich T., Di Fiore L., DiFronzo C., Di
Giorgio C., Di Giovanni F., Di Giovanni M., Di Girolamo T., Di Lieto A.,
Ding B., Di Pace S., Di Palma I., Di Renzo F., Divakarla A.K., Dmitriev A.,
Doctor Z., Donovan F., Dooley K.L., Doravari S., Dorrington I., Downes T.P.,
Drago M., Driggers J.C., Du Z., Ducoin J.-G., Dupej P., Durante O.,
Dwyer S.E., Easter P.J., Eddolls G., Edo T.B., Effler A., Ehrens P.,
Eichholz J., Eikenberry S.S., Eisenmann M., Eisenstein R.A., Errico L.,
Essick R.C., Estelles H., Estevez D., Etienne Z.B., Etzel T., Evans M.,
Evans T.M., Fafone V., Fairhurst S., Fan X., Farinon S., Farr B., Farr W.M.,
Fauchon-Jones E.J., Favata M., Fays M., Fazio M., Fee C., Feicht J.,
Fejer M.M., Feng F., Fernandez-Galiana A., Ferrante I., Ferreira E.C.,
Ferreira T.A., Fidecaro F., Fiori I., Fiorucci D., Fishbach M., Fisher R.P.,
Fishner J.M., Fittipaldi R., Fitz-Axen M., Fiumara V., Flaminio R.,
Fletcher M., Floden E., Flynn E., Fong H., Font J.A., Forsyth P.W.F.,
Fournier J.-D., Vivanco F.H., Frasca S., Frasconi F., Frei Z., Freise A.,
Frey R., Frey V., Fritschel P., Frolov V.V., Fronze G., Fulda P., Fyffe M.,
Gabbard H.A., Gadre B.U., Gaebel S.M., Gair J.R., Gammaitoni L.,
Gaonkar S.G., Garcia-Quiros C., Garufi F., Gateley B., Gaudio S., Gaur G.,
Gayathri V., Gemme G., Genin E., Gennai A., George D., George J.,
Gergely L., Ghonge S., Ghosh A., Ghosh A., Ghosh S., Giacomazzo B.,
Giaime J.A., Giardina K.D., Gibson D.R., Gill K., Glover L., Gniesmer J.,
Godwin P., Goetz E., Goetz R., Goncharov B., Gonzalez G., Castro J.M.G.,
Gopakumar A., Gossan S.E., Gosselin M., Gouaty R., Grace B., Grado A.,
Granata M., Grant A., Gras S., Grassia P., Gray C., Gray R., Greco G.,
Green A.C., Green R., Gretarsson E.M., Grimaldi A., Grimm S.J., Groot P.,
Grote H., Grunewald S., Gruning P., Guidi G.M., Gulati H.K., Guo Y.,
Gupta A., Gupta A., Gupta P., Gustafson E.K., Gustafson R., Haegel L.,
Halim O., Hall B.R., Hall E.D., Hamilton E.Z., Hammond G., Haney M.,
Hanke M.M., Hanks J., Hanna C., Hannam M.D., Hannuksela O.A., Hansen T.J.,
Hanson J., Harder T., Hardwick T., Haris K., Harms J., Harry G.M.,
Harry I.W., Hasskew R.K., Haster C.J., Haughian K., Hayes F.J., Healy J.,
Heidmann A., Heintze M.C., Heitmann H., Hellman F., Hello P., Hemming G.,
Hendry M., Heng I.S., Hennig J., Heurs M., Hild S., Hinderer T.,
Hochheim S., Hofman D., Holgado A.M., Holland N.A., Holt K., Holz D.E.,
Hopkins P., Horst C., Hough J., Howell E.J., Hoy C.G., Huang Y.,
Hubner M.T., Huerta E.A., Huet D., Hughey B., Hui V., Husa S., Huttner S.H.,
Huynh-Dinh T., Idzkowski B., Iess A., Inchauspe H., Ingram C., Inta R.,
Intini G., Irwin B., Isa H.N., Isac J.-M., Isi M., Iyer B.R., Jacqmin T.,
Jadhav S.J., Jani K., Janthalur N.N., Jaranowski P., Jariwala D.,
Jenkins A.C., Jiang J., Johnson D.S., Jones A.W., Jones D.I., Jones J.D.,
Jones R., Jonker R.J.G., Ju L., Junker J., Kalaghatgi C.V., Kalogera V.,
Kamai B., Kandhasamy S., Kang G., Kanner J.B., Kapadia S.J., Karki S.,
Kashyap R., Kasprzack M., Katsanevas S., Katsavounidis E., Katzman W.,
Kaufer S., Kawabe K., Keerthana N.V., Kefelian F., Keitel D., Kennedy R.,
Key J.S., Khalili F.Y., Khan I., Khan S., Khazanov E.A., Khetan N.,
Khursheed M., Kijbunchoo N., Kim C., Kim J.C., Kim K., Kim W., Kim W.S.,
Kim Y.-M., Kimball C., King P.J., Kinley-Hanlon M., Kirchhoff R.,
Kissel J.S., Kleybolte L., Klika J.H., Klimenko S., Knowles T.D., Koch P.,
Koehlenbeck S.M., Koekoek G., Koley S., Kondrashov V., Kontos A., Koper N.,
Korobko M., Korth W.Z., Kovalam M., Kozak D.B., Kramer C., Kringel V.,
Krishnendu N., Krolak A., Krupinski N., Kuehn G., Kumar A., Kumar P.,
Kumar R., Kumar R., Kuo L., Kutynia A., Kwang S., Lackey B.D., Laghi D.,
Lai K.H., Lam T.L., Landry M., Lane B.B., Lang R.N., Lange J., Lantz B.,
Lanza R.K., Lartaux-Vollard A., Lasky P.D., Laxen M., Lazzarini A.,
Lazzaro C., Leaci P., Leavey S., Lecoeuche Y.K., Lee C.H., Lee H.K.,
Lee H.M., Lee H.W., Lee J., Lee K., Lehmann J., Lenon A.K., Leroy N.,
Letendre N., Levin Y., Li A., Li J., Li K.J.L., Li T.G.F., Li X., Lin F.,
Linde F., Linker S.D., Littenberg T.B., Liu J., Liu X., Llorens-
Monteagudo M., Lo R.K.L., London L.T., Longo A., Lorenzini M., Loriette V.,
Lormand M., Losurdo G., Lough J.D., Lousto C.O., Lovelace G., Lower M.E.,
Luck H., Lumaca D., Lundgren A.P., Lynch R., Ma Y., Macas R., Macfoy S.,
MacInnis M., Macleod D.M., Macquet A., Hernandez I.M., Magana-Sandoval F.,
Magee R.M., Majorana E., Maksimovic I., Malik A., Man N., Mandic V.,
Mangano V., Mansell G.L., Manske M., Mantovani M., Mapelli M.,
Marchesoni F., Marion F., Marka S., Marka Z., Markakis C., Markosyan A.S.,
Markowitz A., Maros E., Marquina A., Marsat S., Martelli F., Martin I.W.,
Martin R.M., Martinez V., Martynov D.V., Masalehdan H., Mason K.,
Massera E., Masserot A., Massinger T.J., Masso-Reid M., Mastrogiovanni S.,
Matas A., Matichard F., Matone L., Mavalvala N., McCann J.J., McCarthy R.,
McClelland D.E., McCormick S., McCuller L., McGuire S.C., McIsaac C.,
McIver J., McManus D.J., McRae T., McWilliams S.T., Meacher D.,
Meadors G.D., Mehmet M., Mehta A.K., Meidam J., Villa E.M., Melatos A.,
Mendell G., Mercer R.A., Mereni L., Merfeld K., Merilh E.L., Merzougui M.,
Meshkov S., Messenger C., Messick C., Messina F., Metzdorff R., Meyers P.M.,
Meylahn F., Miani A., Miao H., Michel C., Middleton H., Milano L.,
Miller A.L., Millhouse M., Mills J.C., Milovich-Goff M.C., Minazzoli O.,
Minenkov Y., Mishkin A., Mishra C., Mistry T., Mitra S., Mitrofanov V.P.,
Mitselmakher G., Mittleman R., Mo G., Moffa D., Mogushi K.,
Mohapatra S.R.P., Molina-Ruiz M., Mondin M., Montani M., Moore C.J.,
Moraru D., Morawski F., Moreno G., Morisaki S., Mours B., Mow-Lowry C.M.,
Muciaccia F., Mukherjee A., Mukherjee D., Mukherjee S., Mukherjee S.,
Mukund N., Mullavey A., Munch J., Muniz E.A., Muratore M., Murray P.G.,
Nardecchia I., Naticchioni L., Nayak R.K., Neil B.F., Neilson J.,
Nelemans G., Nelson T.J.N., Nery M., Neunzert A., Nevin L., Ng K.Y., Ng S.,
Nguyen C., Nguyen P., Nichols D., Nichols S.A., Nissanke S., Nocera F.,
North C., Nuttall L.K., Obergaulinger M., Oberling J., O'Brien B.D.,
Oganesyan G., Ogin G.H., Oh J.J., Oh S.H., Ohme F., Ohta H., Okada M.A.,
Oliver M., Oppermann P., Oram R.J., O'Reilly B., Ormiston R.G., Ortega L.F.,
O'Shaughnessy R., Ossokine S., Ottaway D.J., Overmier H., Owen B.J.,
Pace A.E., Pagano G., Page M.A., Pagliaroli G., Pai A., Pai S.A.,
Palamos J.R., Palashov O., Palomba C., Pan H., Panda P.K., Pang P.T.H.,
Pankow C., Pannarale F., Pant B.C., Paoletti F., Paoli A., Parida A.,
Parker W., Pascucci D., Pasqualetti A., Passaquieti R., Passuello D.,
Patil M., Patricelli B., Payne E., Pearlstone B.L., Pechsiri T.C.,
Pedersen A.J., Pedraza M., Pedurand R., Pele A., Penn S., Perego A.,
Perez C.J., Perigois C., Perreca A., Petermann J., Pfeiffer H.P., Phelps M.,
Phukon K.S., Piccinni O.J., Pichot M., Piergiovanni F., Pierro V.,
Pillant G., Pinard L., Pinto I.M., Pirello M., Pitkin M., Plastino W.,
Poggiani R., Pong D.Y.T., Ponrathnam S., Popolizio P., Powell J.,
Prajapati A.K., Prasad J., Prasai K., Prasanna R., Pratten G.,
Prestegard T., Principe M., Prodi G.A., Prokhorov L., Punturo M., Puppo P.,
Purrer M., Qi H., Quetschke V., Quinonez P.J., Raab F.J., Raaijmakers G.,
Radkins H., Radulesco N., Raffai P., Raja S., Rajan C., Rajbhandari B.,
Rakhmanov M., Ramirez K.E., Ramos-Buades A., Rana J., Rao K., Rapagnani P.,
Raymond V., Razzano M., Read J., Regimbau T., Rei L., Reid S., Reitze D.H.,
Rettegno P., Ricci F., Richardson C.J., Richardson J.W., Ricker P.M.,
Riemenschneider G., Riles K., Rizzo M., Robertson N.A., Robinet F.,
Rocchi A., Rolland L., Rollins J.G., Roma V.J., Romanelli M., Romano R.,
Romel C.L., Romie J.H., Rose C.A., Rose D., Rose K., Rosinska D.,
Rosofsky S.G., Ross M.P., Rowan S., Rudiger A., Ruggi P., Rutins G.,
Ryan K., Sachdev S., Sadecki T., Sakellariadou M., Salafia O.S., Salconi L.,
Saleem M., Samajdar A., Sammut L., Sanchez E.J., Sanchez L.E., Sanchis-
Gual N., Sanders J.R., Santiago K.A., Santos E., Sarin N., Sassolas B.,
Sathyaprakash B.S., Sauter O., Savage R.L., Schale P., Scheel M.,
Scheuer J., Schmidt P., Schnabel R., Schofield R.M.S., Schonbeck A.,
Schreiber E., Schulte B.W., Schutz B.F., Scott J., Scott S.M., Seidel E.,
Sellers D., Sengupta A.S., Sennett N., Sentenac D., Sequino V., Sergeev A.,
Setyawati Y., Shaddock D.A., Shaffer T., Shahriar M.S., Shaner M.B.,
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Shoemaker D.M., Shukla K., ShyamSundar S., Siellez K., Sieniawska M.,
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Sitmukhambetov S., Skliris V., Slagmolen B.J.J., Slaven-Blair T.J.,
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Zhang L., Zhang T., Zhao C., Zhao G., Zhou M., Zhou Z., Zhu X.J.,
Zucker M.E., Zweizig J.,
(The LIGO Scientific Collaboration and the Virgo Collaboration),
Aptekar R.L., Boynton W.V., Frederiks D.D., Golenetskii S.V., Golovin D.V.,
Hurley K., Kozlova A.V., Litvak M.L., Mitrofanov I.G., Sanin A.B.,
Svinkin D.S., (The IPN Collaboration), Carotenuto F., Krishnan B.
<Astrophys. J., 886, 75 (2019)>
=2019ApJ...886...75A 2019ApJ...886...75A
ADC_Keywords: GRB; Gravitational wave
Keywords: Burst astrophysics ; Gamma-ray bursts ; Gravitational wave astronomy ;
Gravitational wave sources ; Gravitational waves ;
High energy astrophysics ; LIGO
Abstract:
We present the results of targeted searches for gravitational-wave
transients associated with gamma-ray bursts during the second
observing run of Advanced LIGO and Advanced Virgo, which took place
from 2016 November to 2017 August. We have analyzed 98 gamma-ray
bursts using an unmodeled search method that searches for generic
transient gravitational waves and 42 with a modeled search method that
targets compact-binary mergers as progenitors of short gamma-ray
bursts. Both methods clearly detect the previously reported binary
merger signal GW170817, with p-values of <9.38x10-6 (modeled) and
3.1x10-4 (unmodeled). We do not find any significant evidence for
gravitational-wave signals associated with the other gamma-ray bursts
analyzed, and therefore we report lower bounds on the distance to each
of these, assuming various source types and signal morphologies. Using
our final modeled search results, short gamma-ray burst observations,
and assuming binary neutron star progenitors, we place bounds on the
rate of short gamma-ray bursts as a function of redshift for z≤1. We
estimate 0.07-1.80 joint detections with Fermi-GBM per year for the
2019-20 LIGO-Virgo observing run and 0.15-3.90 per year when current
gravitational-wave detectors are operating at their design sensitivities.
File Summary:
--------------------------------------------------------------------------------
FileName Lrecl Records Explanations
--------------------------------------------------------------------------------
ReadMe 80 . This file
table3.dat 86 111 Information and limits on associated GW emission
for each of the analyzed GRBs
--------------------------------------------------------------------------------
See also:
J/ApJ/715/1438 : Gravitational-wave bursts with GRBs (Abbott+, 2010)
J/ApJ/760/12 : LIGO/Virgo gravitational-wave bursts with GRBs (Abadie+, 2012)
J/ApJS/211/13 : The second Fermi/GBM GRB catalog (4yr) (von Kienlin+, 2014)
J/ApJS/223/28 : The third Fermi/GBM GRB catalog (6yr) (Bhat+, 2016)
J/ApJ/829/7 : Third Swift/BAT GRB catalog (past ∼11yrs) (BAT3) (Lien+, 2016)
J/ApJ/848/L33 : Opt. follow-up of GW events with LCO (Arcavi+, 2017)
J/ApJ/893/46 : The 4th Fermi-GBM GRB catalog: 10 years (von Kienlin+, 2020)
http://gcn.gsfc.nasa.gov/gcn3_archive.html : GCN circulars archive
http://swift.gsfc.nasa.gov/results/batgrbcat/ : Swift/BAT GRB online catalog
http://swift.gsfc.nasa.gov/archive/grb_table/ : Swift GRBs online catalog
http://heasarc.gsfc.nasa.gov/W3Browse/fermi/fermigbrst.html : Fermi/GBM online
catalog home page
Byte-by-byte Description of file: table3.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 9 A9 --- Name GRB name
11 A1 --- f_Name Flag on Name (1)
13- 20 A8 --- Time UTC time
22- 23 I2 h RAh Hour of right ascension (J2000)
25- 26 I2 min RAm Minute of right ascension (J2000)
28- 29 I2 s RAs Second of right ascension (J2000)
31 A1 --- DE- Sign of declination (J2000)
32- 33 I2 deg DEd Degree of declination (J2000)
35- 36 I2 arcmin DEm Arcminute of declination (J2000)
38- 42 A5 --- Inst Instrument whose sky localization was used
for the purposes of analysis
44- 52 A9 --- Type Source type
54- 65 A12 --- Network GW detector network used in the analysis
of each GRB (2)
67 A1 --- f_Network Flag on Network (1)
69- 71 I3 Mpc BNS [9/171]? The 90% confidence exclusion distance
to the GRB (D90) for BNS scenario
73- 75 I3 Mpc NS-BH-g [22/254]? The 90% confidence exclusion distance
to the GRB (D90) for generic NS-BH scenario
77- 79 I3 Mpc NS-BH-a [0/304]? The 90% confidence exclusion distance
to the GRB (D90) for aligned-spin NS-BH
scenario
81- 82 I2 Mpc ADI-A [3/58]? The 90% confidence exclusion distance
to the GRB (D90) for ADI-A scenario
84- 86 I3 Mpc CSG [14/166]? The 90% confidence exclusion distance
to the GRB (D90) for CSG GW burst at 150Hz
scenario with total radiated energy
EGW=M☉c2
--------------------------------------------------------------------------------
Note (1): Flag as follows:
a = GRB 170113A has a redshift of z=1.968 (Xu+ 2017GCN.20458....1X 2017GCN.20458....1X)
b = GRB 170125102 occurred when the Livingston detector was not in its
nominal observing state; however, the data were deemed suitable for the
purposes of the unmodeled analysis.
c = GRB 170202A has a redshift of z=3.645
(de Ugarte Postigo+ 2017GCN.20584....1D 2017GCN.20584....1D)
d = cases in which the on-source window of the generic transient search
is extended to cover the GRB duration (T90>60s).
e = GRB 170428A has a redshift of z=0.454 (Izzo+ 2017GCN.21059....1I 2017GCN.21059....1I)
f = GRB 170705A has a redshift of z=2.01
(de Ugarte Postigo+ 2017GCN.21359....1D 2017GCN.21359....1D)
g = GRB 170714A has a redshift of z=0.793
(de Ugarte Postigo+ 2017GCN.21298....1D 2017GCN.21298....1D)
h = GRB 170803172: Virgo data did not meet the data quality requirements of
X-Pipeline.
i = GRB 170803B occurred near the null of the Virgo detector (see note b). In
addition, Livingston data did not meet the data quality requirements of
X-Pipeline, so this GRB was not subject to the unmodeled analysis.
j = GRB 170816599 occurred near the null of the Livingston detector
(see note b).
l = GRB 170305256 occurred near the null of the Hanford detector, and
inclusion of its data degraded the PyGRB search sensitivity compared to
a Livingston-only analysis.
Note (2): GW detector network as follows:
H1 = LIGO Hanford;
L1 = LIGO Livingston;
V1 = Virgo
In cases where each analysis used a different network, parentheses indicate
the network used for PyGRB analysis, and detail is provided in the
flag column.
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History:
From electronic version of the journal
(End) Emmanuelle Perret [CDS] 12-Apr-2021