7 research outputs found
The Amsterdam Studies of Acute Psychiatry - II (ASAP-II): a comparative study of psychiatric intensive care units in the Netherlands
- Author
- A Smith
- A Zigmond
- AE Vaaler
- Alexander Achilles
- André Klaassen
- Annett Hornbach
- Cecile Gijsbers van Wijk
- CJ Wallace
- CL Mulder
- D Lachar
- D Wynaden
- Emile Barkhof
- EO Noorthoorn
- GD Mitchell
- H Kunze
- H Kunze
- Hans Nusselder
- HJ Salize
- HJ Salize
- Igor Maksimovic
- Inspectie Geestelijke Gezondheidszorg
- Jack Dekker
- Janine van Venrooij
- JE Overall
- K Sundquist
- L Bowers
- L Bowers
- L Citrome
- LB Bigelow
- Lvd Post
- Lvd Post
- M Michalon
- Marieke van Egmond
- Marjan van Herrewaarden
- MD Beer
- N Crowhurst
- NC Stefanis
- P Muller
- PM Dingemans
- R Baker
- Robert Schoevers
- S Pereira
- SM Pereira
- SM Pereira
- SM Pereira
- TW Kallert
- Vincent Koppelmans
- W Mulder
- W Mulder
- WB Crenshaw
- Wijnand Mulder
- WW Eaton
- Yan Bijpost
- Publication venue
- BioMed Central
- Publication date
- 01/01/2009
- Field of study
Background The number of patients in whom mental illness progresses to stages in which acute, and often forced treatment is warranted, is on the increase across Europe. As a consequence, more patients are involuntarily admitted to Psychiatric Intensive Care Units (PICU). From several studies and reports it has become evident that important dissimilarities exist between PICU's. The current study seeks to describe organisational as well as clinical and patient related factors across ten PICU's in and outside the Amsterdam region, adjusted for or stratified by level of urbanization. Method/Design This paper describes the design of the Amsterdam Studies of Acute Psychiatry II (ASAP-II). This study is a prospective observational cohort study comparing PICU's in and outside the Amsterdam region on various patient characteristics, treatment aspects and recovery related variables. Dissimilarities were measured by means of collecting standardized forms which were filled out in the framework of care as usual, by means of questionnaires filled out by mental health care professionals and by means of extracting data from patient files for every consecutive patient admitted at participating PICU's during a specific time period. Urbanization levels for every PICU were calculated conform procedures as proposed by the Dutch Central Bureau for Statistics (CBS). Discussion The current study may provide a deeper understanding of the differences between psychiatric intensive care units that can be used to promote best practice and benchmarking procedures, and thus improve the standard of care
Binary Black Hole Mergers in the first Advanced LIGO Observing Run
- Author
- a DTO
- a MC
- Abbott BP
- Abbott R
- Abbott TD
- Abernathy MR
- Acernese F
- Ackley K
- Adams C
- Adams T
- Addesso P
- Adhikari RX
- Adya VB
- Affeldt C
- Agathos M
- Agatsuma K
- Aggarwal N
- Aguiar OD
- Aiello L
- Ain A
- Ajith P
- Allen B
- Allocca A
- Altin PA
- Anderson SB
- Anderson WG
- Arai K
- Araya MC
- Arceneaux CC
- Areeda JS
- Arnaud N
- Arun KG
- Ascenzi S
- Ashton G
- Ast M
- Aston SM
- Astone P
- Aufmuth P
- Aulbert C
- Babak S
- Bacon P
- Bader MKM
- Baiardi LC
- Bakel NV
- Baker PT
- Baldaccini F
- Ballardin G
- Ballmer SW
- Barayoga JC
- Barclay SE
- Barish BC
- Barker D
- Barone F
- Barr B
- Barsotti L
- Barsuglia M
- Barta D
- Bartlett J
- Bartos I
- Bassiri R
- Basti A
- Batch JC
- Baune C
- Bavigadda V
- Bazzan M
- Bejger M
- Bell AS
- Berger BK
- Bergmann G
- Berry CPL
- Bersanetti D
- Bertolini A
- Betzwieser J
- Beuzekom MV
- Bhagwat S
- Bhandare R
- Bilenko IA
- Billingsley G
- Birch J
- Birney R
- Birnholtz O
- Biscans S
- Bisht A
- Bitossi M
- Biwer C
- Bizouard MA
- Blackburn JK
- Blair CD
- Blair DG
- Blair RM
- Bloemen S
- Bock O
- Boer M
- Bogaert G
- Bogan C
- Bohe A
- Bond C
- Bondu F
- Bonnand R
- Boom BA
- Bork R
- Boschi V
- Bose S
- Bouffanais Y
- Bozzi A
- Bradaschia C
- Brady PR
- Braginsky VB
- Branchesi M
- Brand JFJVD
- Brau JE
- Briant T
- Brillet A
- Brinkmann M
- Brisson V
- Brockill P
- Broeck CVD
- Broida JE
- Brooks AF
- Brown DA
- Brown DD
- Brown NM
- Brunett S
- Buchanan CC
- Buikema A
- Bulik T
- Bulten HJ
- Buonanno A
- Buskulic D
- Bustillo JC
- Buy C
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- Cabero M
- Cadonati L
- Cagnoli G
- Cahillane C
- Callister T
- Calloni E
- Camp JB
- Cannon KC
- Canton TD
- Cao J
- Capano CD
- Capocasa E
- Carbognani F
- Caride S
- Casentini C
- Castro JMG
- Caudill S
- Cavalier F
- Cavalieri R
- Cella G
- Cepeda CB
- Cerretani G
- Cesarini E
- Chamberlin SJ
- Chan M
- Chao S
- Charlton P
- Chassande-Mottin E
- Cheeseboro BD
- Chen HY
- Chen Y
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- Chincarini A
- Chiummo A
- Cho HS
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- Christensen N
- Chu Q
- Chua S
- Chung S
- Ciani G
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- Cleva F
- Coccia E
- Cohadon P-F
- Colla A
- Collaboration TLIGOS
- Collaboration TV
- Collette CG
- Cominsky L
- Conte A
- Conti L
- Cook D
- Corbitt TR
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- Corsi A
- Cortese S
- Costa CA
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- Coulon J-P
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- Cowan EE
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- Cowart MJ
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- Crowder SG
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- Zangrando L
- Zanolin M
- Zendri J-P
- Zertuche LM
- Zevin M
- Zhang L
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- Zhang Y
- Zhao C
- Zhou M
- Zhou Z
- Zhu XJ
- zny AZ
- Zucker ME
- Zuraw SE
- Zweizig J
- Publication venue
- 'American Physical Society (APS)'
- Publication date
- 01/01/2016
- Field of study
The first observational run of the Advanced LIGO detectors, from September 12, 2015 to January 19, 2016, saw the first detections of gravitational waves from binary black hole mergers. In this paper we present full results from a search for binary black hole merger signals with total masses up to 100Mââ and detailed implications from our observations of these systems. Our search, based on general-relativistic models of gravitational wave signals from binary black hole systems, unambiguously identified two signals, GW150914 and GW151226, with a significance of greater than 5Ï over the observing period. It also identified a third possible signal, LVT151012, with substantially lower significance, which has a 87% probability of being of astrophysical origin. We provide detailed estimates of the parameters of the observed systems. Both GW150914 and GW151226 provide an unprecedented opportunity to study the two-body motion of a compact-object binary in the large velocity, highly nonlinear regime. We do not observe any deviations from general relativity, and place improved empirical bounds on several high-order post-Newtonian coefficients. From our observations we infer stellar-mass binary black hole merger rates lying in the range 9â240Gpcâ3yrâ1. These observations are beginning to inform astrophysical predictions of binary black hole formation rates, and indicate that future observing runs of the Advanced detector network will yield many more gravitational wave detections
Localization and broadband follow-up of the gravitational-wave transient GW150914
- Author
- Abbott BP
- Abbott FTBOOTESCTMC
- Abdalla FB
- Abe FTINF
- Ackermann FTFGBMCM
- Ackley K
- Adame JA
- Adams C
- Adams T
- Addesso P
- Adhikari RX
- Adya VB
- Affeldt C
- Agathos M
- Agatsuma K
- Aggarwal N
- Aguiar OD
- Aiello L
- Ain A
- Ajello M
- Ajith P
- Albert A
- Allam S
- Allen B
- Allen WH
- Allison TVCJ
- Allocca A
- Altin PA
- Amati L
- Anderson B
- Anderson JP
- Anderson SB
- Anderson WG
- Annis J
- Antonelli LA
- Aptekar RL
- Arai K
- Araya MC
- Arceneaux CC
- Areeda JS
- Armstrong R
- Arnaud N
- Array FTLF
- Array FTMW-F
- Arun KG
- Ascenzi S
- Ashton G
- Ast M
- Aston SM
- Astone P
- Atwood WB
- Aufmuth P
- Aulbert C
- Axelsson M
- Babak S
- Bacon P
- Bader MKM
- Bai J
- Baiardi LC
- Bakel NV
- Baker PT
- Balanutsa P
- Baldaccini F
- Baldini L
- Ballardin G
- Ballmer SW
- Baltay FTJ-GEMCC
- Banerji M
- Bannister K
- Barayoga JC
- Barbiellini G
- Barclay SE
- Barish BC
- Barker D
- Barlow T
- Barone F
- Barr B
- Barsotti L
- Barsuglia M
- Barta D
- Barthelmy S
- Bartlett J
- Bartos I
- Bassiri R
- Basti A
- Bastieri D
- Batch JC
- Baune C
- Bavigadda V
- Bazzan M
- Bazzano A
- Behnke B
- Bejger M
- Bell AS
- Bell CJ
- Bell ME
- Bellazzini R
- Bellm E
- Benacquista M
- Benoit-LĂ©vy A
- Berger BK
- Berger E
- Bergman J
- Bergmann G
- Bernstein RA
- Beroiz CCM
- Berry CPL
- Bersanetti D
- Bersier D
- Bertin E
- Bertolini A
- Betzwieser J
- Beuzekom MV
- Bhagwat S
- Bhalerao V
- Bhandare R
- Bhat PN
- Bilenko IA
- Billingsley G
- Birch J
- Birney R
- Biscans S
- Bisht A
- Bissaldi E
- Bissaldi E
- Bitossi M
- Biwer C
- Bizouard MA
- Blackburn JK
- Blackburn L
- Blair CD
- Blair DG
- Blair RM
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- Conte A
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- Copperwheat CM
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- Costa CA
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- Countryman ST
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- Äwiek FTPESSTOCA
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- IOP PUBLISHING LTD
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- Field of study
A gravitational-wave transient was identified in data recorded by the Advanced LIGO detectors on 2015 September 14. The event candidate, initially designated G184098 and later given the name GW150914, is described in detail elsewhere. By prior arrangement, preliminary estimates of the time, significance, and sky location of the event were shared with 63 teams of observers covering radio, optical, near-infrared, X-ray, and gamma-ray wavelengths with ground- and space-based facilities. In this Letter we describe the low-latency analysis of the gravitational wave data and present the sky localization of the first observed compact binary merger. We summarize the follow-up observations reported by 25 teams via private Gamma-ray Coordinates Network Circulars, giving an overview of the participating facilities, the gravitational wave sky localization coverage, the timeline and depth of the observations. As this event turned out to be a binary black hole merger, there is little expectation of a detectable electromagnetic signature. Nevertheless, this first broadband campaign to search for a counterpart of an Advanced LIGO source represents a milestone and highlights the broad capabilities of the transient astronomy community and the observing strategies that have been developed to pursue neutron star binary merger events. Detailed investigations of the electromagnetic data and results of the electromagnetic follow-up campaign will be disseminated in the papers of the individual teams
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- 'Springer Science and Business Media LLC'
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Das Lipoidsyndrom und die essentielle HyperlipÀmie
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- Field of study
Supplement: "The rate of binary black hole mergers inferred from advanced LIGO observations surrounding GW150914â (2016, ApJL, 833, L1)
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- Naticchioni L
- Nayak RK
- Necula V
- Nedkova K
- Nelemans G
- Neri M
- Neunzert A
- Newton G
- Nguyen TT
- Nielsen AB
- Nissanke S
- Nitz A
- Nocera F
- Nolting D
- Normandin ME
- Nuttall LK
- Oberling J
- Ochsner E
- ODell J
- Oelker E
- Ogin GH
- Oh JJ
- Oh SH
- Ohme F
- Oliver M
- Oppermann P
- Oram RJ
- Ottaway DJ
- Ottens RS
- Overmier H
- Owen BJ
- OâReilly B
- OâShaughnessy R
- Pace SD
- Pai A
- Pai SA
- Pal-Singh A
- Palamos JR
- Palashov O
- Palma ID
- Palomba C
- Pan H
- Pankow C
- Pannarale F
- Pant BC
- Paoletti F
- Paoli A
- Papa MA
- Paris HR
- Parker W
- Pascucci D
- Pasqualetti A
- Passaquieti R
- Passuello D
- Patricelli B
- Patrick Z
- Pearlstone BL
- Pedraza M
- Pedurand R
- Pekowsky L
- Pele A
- Penn S
- Perreca A
- Phelps M
- Piccinni O
- Pichot M
- Piergiovanni F
- Pierro V
- Pillant G
- Pinard L
- Pinto IM
- Pitkin M
- Poggiani R
- Popolizio P
- Porter EK
- Post A
- Powell J
- Pozzo WD
- Prasad J
- Predoi V
- Premachandra SS
- Prestegard T
- Price LR
- Prijatelj M
- Principe M
- Privitera S
- Prodi GA
- Prokhorov L
- Puncken O
- Punturo M
- Puppo P
- PĂŒrrer M
- Qi H
- Qin J
- Quetschke V
- Quintero EA
- Quitzow-James R
- Raab FJ
- Rabeling DS
- Radkins H
- Raffai P
- Raja S
- Rakhmanov M
- Rapagnani P
- Raymond V
- Razzano M
- Re V
- Read J
- Reed CM
- Regimbau T
- Rei L
- Reid S
- Reitze DH
- Rew H
- Reyes SD
- Ricci F
- Riles K
- Robertson NA
- Robie R
- Robinet F
- Rocchi A
- Rolland L
- Rollins JG
- Roma VJ
- Romano R
- Romanov G
- Romie JH
- Rosa RD
- Rosi?ska D
- Rowan S
- Ruggi P
- Ryan K
- RĂŒdiger A
- Sachdev S
- Sadecki T
- Sadeghian L
- Salconi L
- Saleem M
- Salemi F
- Samajdar A
- Sammut L
- Sampson L
- Sanchez EJ
- Sandberg V
- Sandeen B
- Sanders JR
- Sassolas B
- Sathyaprakash BS
- Saulson PR
- Sauter O
- Savage RL
- Sawadsky A
- Schaaf Lvd
- Schale P
- Schilling R
- Schmidt J
- Schmidt P
- Schnabel R
- Schofield RMS
- Schreiber E
- Schuette D
- Schutz BF
- Schönbeck A
- Scott J
- Scott SM
- Sellers D
- Sengupta AS
- Sentenac D
- Sequino V
- Sergeev A
- Serna G
- Setyawati Y
- Sevigny A
- Shaddock DA
- Shah S
- Shahriar MS
- Shaltev M
- Shao Z
- Shapiro B
- Shawhan P
- Sheperd A
- Shoemaker DH
- Shoemaker DM
- Siellez K
- Siemens X
- Sigg D
- Silva AD
- Simakov D
- Singer A
- Singer LP
- Singh A
- Singh R
- Singhal A
- Sintes AM
- Slagmolen BJJ
- Smith JR
- Smith ND
- Smith RJE
- Son EJ
- Sorazu B
- Sorrentino F
- Souradeep T
- Srivastava AK
- Staley A
- Steinke M
- Steinlechner J
- Steinlechner S
- Steinmeyer D
- Stephens BC
- Stevenson S
- Stone R
- Strain KA
- Straniero N
- Stratta G
- Strauss NA
- Strigin S
- Sturani R
- Stuver AL
- Summerscales TZ
- Sun L
- Sutton PJ
- Swinkels BL
- Szczepa?czyk MJ
- Tacca M
- Talukder D
- Tanner DB
- Tarabrin SP
- Taracchini A
- Taylor R
- Theeg T
- Thirugnanasambandam MP
- Thomas EG
- Thomas M
- Thomas P
- Thorne KA
- Thorne KS
- Thrane E
- Tiwari S
- Tiwari V
- Tokmakov KV
- Tomlinson C
- Tonelli M
- Torres CV
- Torrie CI
- Travasso F
- Traylor G
- TrifirĂČ D
- Tringali MC
- Trozzo L
- Tse M
- Turconi M
- Tuyenbayev D
- TĂĄpai M
- TöyrÀ D
- Ugolini D
- Unnikrishnan CS
- Urban AL
- Usman SA
- Vahlbruch H
- Vajente G
- Valdes G
- Vallisneri M
- van den Brand JFJ
- Vander-Hyde DC
- Vardaro M
- Vass S
- VasĂșth M
- Vaulin R
- Vecchio A
- Vedovato G
- Veggel AAv
- Veitch J
- Veitch PJ
- Venkateswara K
- Verkindt D
- Vetrano F
- Viceré A
- Vinciguerra S
- Vine DJ
- Vinet J
- Virgilio AD
- Vitale S
- Vo T
- Vocca H
- Vorvick C
- Voss D
- Vousden WD
- Vyatchanin SP
- Wade AR
- Wade LE
- Wade M
- Walker M
- Wallace L
- Walsh S
- Wang G
- Wang H
- Wang M
- Wang X
- Wang Y
- Ward RL
- Warner J
- Was M
- Weaver B
- Wei L
- Weinert M
- Weinstein AJ
- Weiss R
- Welborn T
- Wen L
- Wesels P
- Westphal T
- Wette K
- Whelan JT
- White DJ
- Whiting BF
- Williams RD
- Williamson AR
- Willis JL
- Willke B
- Wimmer MH
- Winkler W
- Wipf CC
- Wittel H
- Woan G
- Worden J
- Wright JL
- Wu G
- Yablon J
- Yam W
- Yamamoto H
- Yancey CC
- Yap MJ
- Yu H
- Yvert M
- Zadro?ny A
- Zangrando L
- Zanolin M
- Zendri J
- Zevin M
- Zhang F
- Zhang L
- Zhang M
- Zhang Y
- Zhao C
- Zhou M
- Zhou Z
- Zhu XJ
- Zucker ME
- Zuraw SE
- Zweizig J
- Publication venue
- Publication date
- 01/01/2016
- Field of study
SUPPLEMENT: âTHE RATE OF BINARY BLACK HOLE MERGERS INFERRED FROM ADVANCED LIGO OBSERVATIONS SURROUNDING GW150914â (2016, ApJL, 833, L1)
- Author
- Abbott BP
- Abbott R
- Abbott TD
- Abernathy MR
- Acernese F
- Ackley K
- Adams C
- Adams T
- Addesso P
- Adhikari RX
- Adya VB
- Affeldt C
- Agathos M
- Agatsuma K
- Aggarwal N
- Aguiar OD
- Aiello L
- Ain A
- Ajith P
- Allen B
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- Altin PA
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- Anderson WG
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- Araya MC
- Arceneaux CC
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- Arnaud N
- Arun KG
- Ascenzi S
- Ashton G
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- Aston SM
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- Baiardi LC
- Bakel NV
- Baker PT
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- Bizouard MA
- Blackburn JK
- Blair CD
- Blair DG
- Blair RM
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- Bodiya TP
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- Boom BA
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- Bradaschia C
- Brady PR
- Braginsky VB
- Branchesi M
- Brau JE
- Briant T
- Brillet A
- Brinkmann M
- Brisson V
- Brockill P
- Broeck CVD
- Brooks AF
- Brown DA
- Brown DD
- Brown NM
- Buchanan CC
- Buikema A
- Bulik T
- Bulten HJ
- Buonanno A
- Buskulic D
- Bustillo JC
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- Canton TD
- Cao J
- Capano CD
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- CavagliĂ M
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- Chalermsongsak T
- Chamberlin SJ
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- Chao S
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- Chincarini A
- Chiummo A
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- Cho M
- Chow JH
- Christensen N
- Chu Q
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- Cohadon P-F
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- Collette CG
- Cominsky L
- Constancio M
- Conte A
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- Cook D
- Corbitt TR
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- Corsi A
- Cortese S
- Costa CA
- Coughlin MW
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- Coulon J-P
- Countryman ST
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- Coward DM
- Cowart MJ
- Coyne DC
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- Creighton JDE
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- Crowder SG
- Cumming A
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- Cuoco E
- Danilishin SL
- Danzmann K
- Darman NS
- Dattilo V
- Dave I
- Daveloza HP
- Davier M
- Davies GS
- Daw EJ
- Day R
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- DeBra D
- Debreczeni G
- Degallaix J
- Deléglise S
- Denker T
- Dent T
- Dereli H
- Dergachev V
- DeRosa RT
- DeSalvo R
- Dhurandhar S
- Diaz JC
- Dojcinoski G
- Dolique V
- Donovan F
- Dooley KL
- Doravari S
- Douglas R
- Downes TP
- Drago M
- Drever RWP
- Driggers JC
- Du Z
- Ducrot M
- Dwyer SE
- DĂaz MC
- DâAntonio S
- Edo TB
- Edwards MC
- Effler A
- Eggenstein H-B
- Ehrens P
- Eichholz J
- Eikenberry SS
- Engels W
- Essick RC
- Etzel T
- Evans M
- Evans TM
- Everett R
- Factourovich M
- Fafone V
- Fair H
- Fairhurst S
- Fan X
- Fang Q
- Farinon S
- Farr B
- Farr WM
- Favata M
- Fays M
- Fehrmann H
- Fejer MM
- Ferrante I
- Ferreira EC
- Ferrini F
- Fidecaro F
- Fiore LD
- Fiori I
- Fiorucci D
- Fisher RP
- Flaminio R
- Fletcher M
- Fong H
- Fournier J-D
- Franco S
- Frasca S
- Frasconi F
- Frei Z
- Freise A
- Frey R
- Frey V
- Fricke TT
- Fritschel P
- Frolov VV
- Fulda P
- Fyffe M
- Gabbard HAG
- Gair JR
- Gammaitoni L
- Gaonkar SG
- Garufi F
- Gatto A
- Gaur G
- Gehrels N
- Gemme G
- Gendre B
- Genin E
- Gennai A
- George J
- Gergely L
- Germain V
- Ghosh A
- Ghosh S
- Giaime JA
- Giardina KD
- Giazotto A
- Gill K
- Giovanni MD
- Glaefke A
- Goetz E
- Goetz R
- Gondan L
- Gonzalez Castro JM
- GonzĂĄlez G
- Gopakumar A
- Gordon NA
- Gorodetsky ML
- Gossan SE
- Gosselin M
- Gouaty R
- Graef C
- Graff PB
- Granata M
- Grant A
- Gras S
- Gray C
- Greco G
- Green AC
- Groot P
- Grote H
- Grunewald S
- Guidi GM
- Guo X
- Gupta A
- Gupta MK
- Gushwa KE
- Gustafson EK
- Gustafson R
- Hacker JJ
- Hall BR
- Hall ED
- Hammond G
- Haney M
- Hanke MM
- Hanks J
- Hanna C
- Hannam MD
- Hanson J
- Hardwick T
- Harms J
- Harry GM
- Harry IW
- Hart MJ
- Hartman MT
- Haster C-J
- Haughian K
- Heidmann A
- Heijningen JVV
- Heintze MC
- Heitmann H
- Hello P
- Hemming G
- Hendry M
- Heng IS
- Hennig J
- Heptonstall AW
- Heurs M
- Hild S
- Hoak D
- Hodge KA
- Hofman D
- Hollitt SE
- Holt K
- Holz DE
- Hopkins P
- Hosken DJ
- Hough J
- Houston EA
- Howell EJ
- Hu YM
- Huang S
- Huerta EA
- Huet D
- Hughey B
- Husa S
- Huttner SH
- Huynh-Dinh T
- Idrisy A
- Indik N
- Ingram DR
- Inta R
- Isa HN
- Isac J-M
- Isi M
- Islas G
- Isogai T
- Iyer BR
- Izumi K
- Jacqmin T
- Jang H
- Jani K
- Jaranowski P
- Jawahar S
- Jiménez-Forteza F
- Johnson WW
- Jones DI
- Jones R
- Jonker RJG
- Ju L
- K H
- Kalaghatgi CV
- Kalogera V
- Kandhasamy S
- Kang G
- Kanner JB
- Karki S
- Kasprzack M
- Katsavounidis E
- Katzman W
- Kaufer S
- Kaur T
- Kawabe K
- Kawazoe F
- Kehl MS
- Keitel D
- Kelley DB
- Kells W
- Kennedy R
- Key JS
- Khalaidovski A
- Khalili FY
- Khan I
- Khan S
- Khan Z
- Khazanov EA
- Kijbunchoo N
- Kim C
- Kim J
- Kim K
- Kim N
- Kim N-G
- Kim Y-M
- King EJ
- King PJ
- Kinzel DL
- Kissel JS
- Kleybolte L
- Klimenko S
- Koehlenbeck SM
- Kokeyama K
- Koley S
- Kondrashov V
- Kontos A
- Korobko M
- Korth WZ
- Kowalska I
- Kozak DB
- Kringel V
- Krishnan B
- Krueger C
- KrĂłlak A
- Kuehn G
- Kumar P
- Kuo L
- Kutynia A
- Kéfélian F
- Lackey BD
- Landry M
- Lange J
- Lantz B
- Lasky PD
- Laurentis MD
- Lazzarini A
- Lazzaro C
- Leaci P
- Leavey S
- Lebigot EO
- Lee CH
- Lee HK
- Lee HM
- Lee K
- Lenon A
- Leonardi M
- Leong JR
- Leroy N
- Letendre N
- Levin Y
- Levine BM
- Li TGF
- Libson A
- Lieto AD
- Littenberg TB
- Lockerbie NA
- Logue J
- Lombardi AL
- Lord JE
- Lorenzini M
- Loriette V
- Lormand M
- Losurdo G
- Lough JD
- Lundgren AP
- Luo J
- Lynch R
- LĂŒck H
- Ma Y
- MacDonald T
- Machenschalk B
- MacInnis M
- Macleod DM
- Magaña-Sandoval F
- Magee RM
- Mageswaran M
- Majorana E
- Maksimovic I
- Malvezzi V
- Man N
- Mandel I
- Mandic V
- Mangano V
- Mansell GL
- Manske M
- Mantovani M
- Marchesoni F
- Marion F
- Markosyan AS
- Maros E
- Martelli F
- Martellini L
- Martin IW
- Martin RM
- Martynov DV
- Marx JN
- Mason K
- Masserot A
- Massinger TJ
- Masso-Reid M
- Matichard F
- Matone L
- Mavalvala N
- Mazumder N
- Mazzolo G
- McCarthy R
- McClelland DE
- McCormick S
- McGuire SC
- McIntyre G
- McIver J
- McManus DJ
- McWilliams ST
- Meacher D
- Meadors GD
- Meidam J
- Melatos A
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- Mendoza-Gandara D
- Mercer RA
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- Merzougui M
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- Messick C
- Meyers PM
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- Middleton H
- Mikhailov EE
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- Millhouse M
- Minenkov Y
- Ming J
- Mirshekari S
- Mishra C
- Mitra S
- Mitrofanov VP
- Mitselmakher G
- Mittleman R
- Moggi A
- Mohan M
- Mohapatra SRP
- Montani M
- Moore BC
- Moore CJ
- Moraru D
- Moreno G
- Morriss SR
- Mossavi K
- Mours B
- Mow-Lowry CM
- Mueller CL
- Mueller G
- Muir AW
- Mukherjee A
- Mukherjee D
- Mukherjee S
- Mukund N
- Mullavey A
- Munch J
- Murphy DJ
- Murray PG
- Mytidis A
- MĂĄrka S
- MĂĄrka Z
- Nardecchia I
- Naticchioni L
- Nayak RK
- Necula V
- Nedkova K
- Nelemans G
- Neri M
- Neunzert A
- Newton G
- Nguyen TT
- Nielsen AB
- Nissanke S
- Nitz A
- Nocera F
- Nolting D
- Normandin ME
- Nuttall LK
- Oberling J
- Ochsner E
- Oelker E
- Ogin GH
- Oh JJ
- Oh SH
- Ohme F
- Oliver M
- Oppermann P
- Oram RJ
- Ottaway DJ
- Ottens RS
- Overmier H
- Owen BJ
- OâDell J
- OâReilly B
- OâShaughnessy R
- Pace SD
- Pai A
- Pai SA
- Pal-Singh A
- Palamos JR
- Palashov O
- Palma ID
- Palomba C
- Pan H
- Pankow C
- Pannarale F
- Pant BC
- Paoletti F
- Paoli A
- Papa MA
- Paris HR
- Parker W
- Pascucci D
- Pasqualetti A
- Passaquieti R
- Passuello D
- Patricelli B
- Patrick Z
- Pearlstone BL
- Pedraza M
- Pedurand R
- Pekowsky L
- Pele A
- Penn S
- Perreca A
- Phelps M
- Piccinni O
- Pichot M
- Piergiovanni F
- Pierro V
- Pillant G
- Pinard L
- Pinto IM
- Pitkin M
- Poggiani R
- Popolizio P
- Porter EK
- Post A
- Powell J
- Pozzo WD
- Prasad J
- Predoi V
- Premachandra SS
- Prestegard T
- Price LR
- Prijatelj M
- Principe M
- Privitera S
- Prodi GA
- Prokhorov L
- Puncken O
- Punturo M
- Puppo P
- PĂŒrrer M
- Qi H
- Qin J
- Quetschke V
- Quintero EA
- Quitzow-James R
- Raab FJ
- Rabeling DS
- Radkins H
- Raffai P
- Raja S
- Rakhmanov M
- Rapagnani P
- Raymond V
- Razzano M
- Re V
- Read J
- Reed CM
- Regimbau T
- Rei L
- Reid S
- Reitze DH
- Rew H
- Reyes SD
- Ricci F
- Riles K
- Robertson NA
- Robie R
- Robinet F
- Rocchi A
- Rolland L
- Rollins JG
- Roma VJ
- Romano R
- Romanov G
- Romie JH
- Rosa RD
- RosiĆska D
- Rowan S
- Ruggi P
- Ryan K
- RĂŒdiger A
- Sachdev S
- Sadecki T
- Sadeghian L
- Salconi L
- Saleem M
- Salemi F
- Samajdar A
- Sammut L
- Sampson L
- Sanchez EJ
- Sandberg V
- Sandeen B
- Sanders JR
- Sassolas B
- Sathyaprakash BS
- Saulson PR
- Sauter O
- Savage RL
- Sawadsky A
- Schaaf LVD
- Schale P
- Schilling R
- Schmidt J
- Schmidt P
- Schnabel R
- Schofield RMS
- Schreiber E
- Schuette D
- Schutz BF
- Schönbeck A
- Scott J
- Scott SM
- Sellers D
- Sengupta AS
- Sentenac D
- Sequino V
- Sergeev A
- Serna G
- Setyawati Y
- Sevigny A
- Shaddock DA
- Shah S
- Shahriar MS
- Shaltev M
- Shao Z
- Shapiro B
- Shawhan P
- Sheperd A
- Shoemaker DH
- Shoemaker DM
- Siellez K
- Siemens X
- Sigg D
- Silva AD
- Simakov D
- Singer A
- Singer LP
- Singh A
- Singh R
- Singhal A
- Sintes AM
- Slagmolen BJJ
- Smith JR
- Smith ND
- Smith RJE
- Son EJ
- Sorazu B
- Sorrentino F
- Souradeep T
- Srivastava AK
- Staley A
- Steinke M
- Steinlechner J
- Steinlechner S
- Steinmeyer D
- Stephens BC
- Stevenson S
- Stone R
- Strain KA
- Straniero N
- Stratta G
- Strauss NA
- Strigin S
- Sturani R
- Stuver AL
- Summerscales TZ
- Sun L
- Sutton PJ
- Swinkels BL
- SzczepaĆczyk MJ
- Tacca M
- Talukder D
- Tanner DB
- Tarabrin SP
- Taracchini A
- Taylor R
- Theeg T
- Thirugnanasambandam MP
- Thomas EG
- Thomas M
- Thomas P
- Thorne KA
- Thorne KS
- Thrane E
- Tiwari S
- Tiwari V
- Tokmakov KV
- Tomlinson C
- Tonelli M
- Torres CV
- Torrie CI
- Travasso F
- Traylor G
- TrifirĂČ D
- Tringali MC
- Trozzo L
- Tse M
- Turconi M
- Tuyenbayev D
- TĂĄpai M
- TöyrÀ D
- Ugolini D
- Unnikrishnan CS
- Urban AL
- Usman SA
- Vahlbruch H
- Vajente G
- Valdes G
- Vallisneri M
- van den Brand JFJ
- Vander-Hyde DC
- Vardaro M
- Vass S
- VasĂșth M
- Vaulin R
- Vecchio A
- Vedovato G
- Veggel AAV
- Veitch J
- Veitch PJ
- Venkateswara K
- Verkindt D
- Vetrano F
- Viceré A
- Vinciguerra S
- Vine DJ
- Vinet J-Y
- Virgilio AD
- Vitale S
- Vo T
- Vocca H
- Vorvick C
- Voss D
- Vousden WD
- Vyatchanin SP
- Wade AR
- Wade LE
- Wade M
- Walker M
- Wallace L
- Walsh S
- Wang G
- Wang H
- Wang M
- Wang X
- Wang Y
- Ward RL
- Warner J
- Was M
- Weaver B
- Wei L-W
- Weinert M
- Weinstein AJ
- Weiss R
- Welborn T
- Wen L
- Wesels P
- Westphal T
- Wette K
- Whelan JT
- White DJ
- Whiting BF
- Williams RD
- Williamson AR
- Willis JL
- Willke B
- Wimmer MH
- Winkler W
- Wipf CC
- Wittel H
- Woan G
- Worden J
- Wright JL
- Wu G
- Yablon J
- Yam W
- Yamamoto H
- Yancey CC
- Yap MJ
- Yu H
- Yvert M
- ZadroĆŒny A
- Zangrando L
- Zanolin M
- Zendri J-P
- Zevin M
- Zhang F
- Zhang L
- Zhang M
- Zhang Y
- Zhao C
- Zhou M
- Zhou Z
- Zhu XJ
- Zucker ME
- Zuraw SE
- Zweizig J
- Publication venue
- 'American Astronomical Society'
- Publication date
- 01/12/2016
- Field of study
This article provides supplemental information for a Letter reporting the rate of (BBH) coalescences inferred from 16 days of coincident Advanced LIGO observations surrounding the transient (GW) signal GW150914. In that work we reported various rate estimates whose 90% confidence intervals fell in the range 2â600 Gpcâ3 yrâ1. Here we give details on our method and computations, including information about our search pipelines, a derivation of our likelihood function for the analysis, a description of the astrophysical search trigger distribution expected from merging BBHs, details on our computational methods, a description of the effects and our model for calibration uncertainty, and an analytic method for estimating our detector sensitivity, which is calibrated to our measurements