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Sky Tower stair challenge.
McIntyre W. McIntyre W. Nurs N Z. 2016 Feb;22(1):4. Nurs N Z. 2016. PMID: 27039555 No abstract available.
All-sky LIGO search for periodic gravitational waves in the early fifth-science-run data.
Abbott BP, Abbott R, Adhikari R, Ajith P, Allen B, Allen G, Amin RS, Anderson SB, Anderson WG, Arain MA, Araya M, Armandula H, Armor P, Aso Y, Aston S, Aufmuth P, Aulbert C, Babak S, Baker P, Ballmer S, Bantilan H, Barish BC, Barker C, Barker D, Barr B, Barriga P, Barsotti L, Barton MA, Bartos I, Bassiri R, Bastarrika M, Behnke B, Benacquista M, Betzwieser J, Beyersdorf PT, Bilenko IA, Billingsley G, Biswas R, Black E, Blackburn JK, Blackburn L, Blair D, Bland B, Bodiya TP, Bogue L, Bork R, Boschi V, Bose S, Brady PR, Braginsky VB, Brau JE, Brinkmann M, Brooks AF, Brown DA, Brunet G, Bullington A, Buonanno A, Burmeister O, Byer RL, Cadonati L, Cagnoli G, Camp JB, Cannizzo J, Cannon KC, Cao J, Cardenas L, Cardoso V, Caride S, Casebolt T, Castaldi G, Caudill S, Cavaglià M, Cepeda C, Chalkley E, Charlton P, Chatterji S, Chelkowski S, Chen Y, Christensen N, Clark D, Clark J, Clayton JH, Cokelaer T, Conte R, Cook D, Corbitt TR, Cornish N, Coyne DC, Creighton JD, Creighton TD, Cruise AM, Cumming A, Cunningham L, Cutler RM, Danzmann K, Daudert B, Davies G, Debra D, Degallaix J, Dergachev V, Desai S, Desalvo R, Dhurandhar S, Díaz M, Dickson J, Dietz A, Donovan F, Dooley KL, Doomes EE, Dre… See abstract for full author list ➔ Abbott BP, et al. Phys Rev Lett. 2009 Mar 20;102(11):111102. doi: 10.1103/PhysRevLett.102.111102. Epub 2009 Mar 20. Phys Rev Lett. 2009. PMID: 19392186 Free article.
We report on an all-sky search with the LIGO detectors for periodic gravitational waves in the frequency range 50-1100 Hz and with the frequency's time derivative in the range -5 x 10{-9}-0 Hz s{-1}. ...
We report on an all-sky search with the LIGO detectors for periodic gravitational waves in the frequency range 50-1100 Hz and with th …
Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA.
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, Akutsu T, Allen B, Allocca A, Altin PA, Ananyeva A, Anderson SB, Anderson WG, Ando M, Appert S, Arai K, Araya A, Araya MC, Areeda JS, Arnaud N, Arun KG, Asada H, Ascenzi S, Ashton G, Aso Y, Ast M, Aston SM, Astone P, Atsuta S, Aufmuth P, Aulbert C, Avila-Alvarez A, Awai K, Babak S, Bacon P, Bader MKM, Baiotti L, 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, Barton MA, Bartos I, Bassiri R, Basti A, Batch JC, Baune C, Bavigadda V, Bazzan M, Bécsy B, Beer C, Bejger M, Belahcene I, Belgin M, Bell AS, Berger BK, Bergmann G, Berry CPL, Bersanetti D, Bertolini A, Betzwieser J, Bhagwat S, Bhandare R, Bilenko IA, Billingsley G, Billman CR, Birch J, Birney R, Birnholtz O, Biscans S, Bisht A, Bitossi M, Biwer C, Bizouard MA, Blackburn JK, Blackman J, Blair CD, Blair DG, Blair RM, Bloemen S, Bock O, Boer M, Bogaert G, Bohe A, Bondu F, Bonnand R, Boom BA, Bork R, Boschi V, Bose S, Bou… See abstract for full author list ➔ Abbott BP, et al. Living Rev Relativ. 2018;21(1):3. doi: 10.1007/s41114-018-0012-9. Epub 2018 Apr 26. Living Rev Relativ. 2018. PMID: 29725242 Free PMC article. Review.
We estimate the sensitivity of the network to transient gravitational-wave signals, and study the capability of the network to determine the sky location of the source. We report our findings for gravitational-wave transients, with particular focus on gravitational-wave si …
We estimate the sensitivity of the network to transient gravitational-wave signals, and study the capability of the network to determine the …
Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO and Advanced Virgo.
Abbott BP; LIGO Scientific Collaboration; Virgo Collaboration; 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, Ain A, Ajith P, Allen B, Allocca A, Altin PA, Amariutei DV, Anderson SB, Anderson WG, Arai K, Araya MC, Arceneaux CC, Areeda JS, Arnaud N, Arun KG, Ashton G, Ast M, Aston SM, Astone P, Aufmuth P, Aulbert C, Babak S, 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, Behnke B, Bejger M, Belczynski C, Bell AS, Bell CJ, Berger BK, Bergman J, Bergmann G, Berry CP, Bersanetti D, Bertolini A, Betzwieser J, Bhagwat S, Bhandare R, Bilenko IA, Billingsley G, Birch J, Birney R, Biscans S, Bisht A, Bitossi M, Biwer C, Bizouard MA, Blackburn JK, Blair CD, Blair D, Blair RM, Bloemen S, Bock O, Bodiya TP, Boer M, Bogaert G, Bogan C, Bohe A, Bojtos P, Bond C, Bondu F, Bonnand R, Bork R, Boschi V, Bose S, Bozzi A, Bradaschia C, Brady PR, Braginsky VB, Branchesi M, Brau JE, Briant T, Brillet A, Br… See abstract for full author list ➔ Abbott BP, et al. Living Rev Relativ. 2016;19(1):1. doi: 10.1007/lrr-2016-1. Epub 2016 Feb 8. Living Rev Relativ. 2016. PMID: 28179853 Free PMC article. Review.
We determine the expected sensitivity of the network to transient gravitational-wave signals, and study the capability of the network to determine the sky location of the source. We report our findings for gravitational-wave transients, with particular focus on gravitation …
We determine the expected sensitivity of the network to transient gravitational-wave signals, and study the capability of the network to det …
A gravitational-wave standard siren measurement of the Hubble constant.
LIGO Scientific Collaboration and The Virgo Collaboration; 1M2H Collaboration; Dark Energy Camera GW-EM Collaboration and the DES Collaboration; DLT40 Collaboration; Las Cumbres Observatory Collaboration; VINROUGE Collaboration; MASTER Collaboration. LIGO Scientific Collaboration and The Virgo Collaboration, et al. Nature. 2017 Nov 2;551(7678):85-88. doi: 10.1038/nature24471. Epub 2017 Oct 16. Nature. 2017. PMID: 29094696 Free article.
Less than two seconds after the merger, a gamma-ray burst (GRB 170817A) was detected within a region of the sky consistent with the LIGO-Virgo-derived location of the gravitational-wave source. This sky region was subsequently observed by optical astronomy facilitie …
Less than two seconds after the merger, a gamma-ray burst (GRB 170817A) was detected within a region of the sky consistent with the L …
Directional limits on persistent gravitational waves using LIGO S5 science data.
Abadie J, Abbott BP, Abbott R, Abernathy M, Accadia T, Acernese F, Adams C, Adhikari R, Ajith P, Allen B, Allen GS, Ceron EA, Amin RS, Anderson SB, Anderson WG, Antonucci F, Arain MA, Araya MC, Aronsson M, Arun KG, Aso Y, Aston SM, Astone P, Atkinson D, Aufmuth P, Aulbert C, Babak S, Baker P, Ballardin G, Ballmer S, Barker D, Barnum S, Barone F, Barr B, Barriga P, Barsotti L, Barsuglia M, Barton MA, Bartos I, Bassiri R, Bastarrika M, Bauchrowitz J, Bauer TS, Behnke B, Beker MG, Belletoile A, Benacquista M, Bertolini A, Betzwieser J, Beveridge N, Beyersdorf PT, Bigotta S, Bilenko IA, Billingsley G, Birch J, Birindelli S, Biswas R, Bitossi M, Bizouard MA, Black E, Blackburn JK, Blackburn L, Blair D, Bland B, Blom M, Boccara C, Bock O, Bodiya TP, Bondarescu R, Bondu F, Bonelli L, Bonnand R, Bork R, Born M, Bose S, Bosi L, Bouhou B, Boyle M, Braccini S, Bradaschia C, Brady PR, Braginsky VB, Brau JE, Breyer J, Bridges DO, Brillet A, Brinkmann M, Brisson V, Britzger M, Brooks AF, Brown DA, Budzyński R, Bulik T, Bulten HJ, Buonanno A, Burguet-Castell J, Burmeister O, Buskulic D, Buy C, Byer RL, Cadonati L, Cagnoli G, Cain J, Calloni E, Camp JB, Campagna E, Campsie P, Cannizzo J, Cannon K… See abstract for full author list ➔ Abadie J, et al. Phys Rev Lett. 2011 Dec 30;107(27):271102. doi: 10.1103/PhysRevLett.107.271102. Epub 2011 Dec 29. Phys Rev Lett. 2011. PMID: 22243300 Free article.
The gravitational-wave (GW) sky may include nearby pointlike sources as well as stochastic backgrounds. ...
The gravitational-wave (GW) sky may include nearby pointlike sources as well as stochastic backgrounds. ...
Sex hormone binding globulin and verbal memory in older men.
Takayanagi Y, Spira AP, McIntyre RS, Eaton WW. Takayanagi Y, et al. Am J Geriatr Psychiatry. 2015 Mar;23(3):253-60. doi: 10.1016/j.jagp.2013.02.003. Epub 2013 Jun 22. Am J Geriatr Psychiatry. 2015. PMID: 23800538 Free PMC article.
Search for gravitational waves associated with γ-ray bursts detected by the interplanetary network.
Aasi J, Abbott BP, Abbott R, Abbott T, Abernathy MR, Acernese F, Ackley K, Adams C, Adams T, Addesso P, Adhikari RX, Affeldt C, Agathos M, Aggarwal N, Aguiar OD, Ajith P, Alemic A, Allen B, Allocca A, Amariutei D, Andersen M, Anderson RA, Anderson SB, Anderson WG, Arai K, Araya MC, Arceneaux C, Areeda JS, Ast S, Aston SM, Astone P, Aufmuth P, Augustus H, Aulbert C, Aylott BE, Babak S, Baker PT, Ballardin G, Ballmer SW, Barayoga JC, Barbet M, Barish BC, Barker D, Barone F, Barr B, Barsotti L, Barsuglia M, Barton MA, Bartos I, Bassiri R, Basti A, Batch JC, Bauchrowitz J, Bauer TS, Baune C, Bavigadda V, Behnke B, Bejger M, Beker MG, Belczynski C, Bell AS, Bell C, Bergmann G, Bersanetti D, Bertolini A, Betzwieser J, Bilenko IA, Billingsley G, Birch J, Biscans S, Bitossi M, Biwer C, Bizouard MA, Black E, Blackburn JK, Blackburn L, Blair D, Bloemen S, Bock O, Bodiya TP, Boer M, Bogaert G, Bogan C, Bond C, Bondu F, Bonelli L, Bonnand R, Bork R, Born M, Boschi V, Bose S, Bosi L, Bradaschia C, Brady PR, Braginsky VB, Branchesi M, Brau JE, Briant T, Bridges DO, Brillet A, Brinkmann M, Brisson V, Brooks AF, Brown DA, Brown DD, Brückner F, Buchman S, Buikema A, Bulik T, Bulten HJ, Buonanno A,… See abstract for full author list ➔ Aasi J, et al. Phys Rev Lett. 2014 Jul 4;113(1):011102. doi: 10.1103/PhysRevLett.113.011102. Epub 2014 Jun 30. Phys Rev Lett. 2014. PMID: 25032916 Free article.
We present the results of a search for gravitational waves associated with 223 gamma-ray bursts (GRBs) detected by the InterPlanetary Network (IPN) in 2005-2010 during LIGO's fifth and sixth science runs and Virgo's first, second, and third science runs. The IPN satellites provid …
We present the results of a search for gravitational waves associated with 223 gamma-ray bursts (GRBs) detected by the InterPlanetary Networ …
GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral.
Abbott BP, Abbott R, Abbott TD, Acernese F, Ackley K, Adams C, Adams T, Addesso P, Adhikari RX, Adya VB, Affeldt C, Afrough M, Agarwal B, Agathos M, Agatsuma K, Aggarwal N, Aguiar OD, Aiello L, Ain A, Ajith P, Allen B, Allen G, Allocca A, Altin PA, Amato A, Ananyeva A, Anderson SB, Anderson WG, Angelova SV, Antier S, Appert S, Arai K, Araya MC, Areeda JS, Arnaud N, Arun KG, Ascenzi S, Ashton G, Ast M, Aston SM, Astone P, Atallah DV, Aufmuth P, Aulbert C, AultONeal K, Austin C, Avila-Alvarez A, Babak S, Bacon P, Bader MKM, Bae S, Bailes M, Baker PT, Baldaccini F, Ballardin G, Ballmer SW, Banagiri S, Barayoga JC, Barclay SE, Barish BC, Barker D, Barkett K, Barone F, Barr B, Barsotti L, Barsuglia M, Barta D, Barthelmy SD, Bartlett J, Bartos I, Bassiri R, Basti A, Batch JC, Bawaj M, Bayley JC, Bazzan M, Bécsy B, Beer C, Bejger M, Belahcene I, Bell AS, Berger BK, Bergmann G, Bernuzzi S, Bero JJ, Berry CPL, Bersanetti D, Bertolini A, Betzwieser J, Bhagwat S, Bhandare R, Bilenko IA, Billingsley G, Billman CR, Birch J, Birney R, Birnholtz O, Biscans S, Biscoveanu S, Bisht A, Bitossi M, Biwer C, Bizouard MA, Blackburn JK, Blackman J, Blair CD, Blair DG, Blair RM, Bloemen S, Bock O, Bode N,… See abstract for full author list ➔ Abbott BP, et al. Phys Rev Lett. 2017 Oct 20;119(16):161101. doi: 10.1103/PhysRevLett.119.161101. Epub 2017 Oct 16. Phys Rev Lett. 2017. PMID: 29099225 Free article.
Restricting the component spins to the range inferred in binary neutron stars, we find the component masses to be in the range 1.17-1.60 M_{}, with the total mass of the system 2.74_{-0.01}^{+0.04}M_{}. The source was localized within a sky region of 28 deg^{2} (90% probab …
Restricting the component spins to the range inferred in binary neutron stars, we find the component masses to be in the range 1.17-1.60 M_{ …
GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence.
Abbott BP, Abbott R, Abbott TD, Acernese F, Ackley K, Adams C, Adams T, Addesso P, Adhikari RX, Adya VB, Affeldt C, Afrough M, Agarwal B, Agathos M, Agatsuma K, Aggarwal N, Aguiar OD, Aiello L, Ain A, Ajith P, Allen B, Allen G, Allocca A, Altin PA, Amato A, Ananyeva A, Anderson SB, Anderson WG, Angelova SV, Antier S, Appert S, Arai K, Araya MC, Areeda JS, Arnaud N, Arun KG, Ascenzi S, Ashton G, Ast M, Aston SM, Astone P, Atallah DV, Aufmuth P, Aulbert C, AultONeal K, Austin C, Avila-Alvarez A, Babak S, Bacon P, Bader MKM, Bae S, Baker PT, Baldaccini F, Ballardin G, Ballmer SW, Banagiri S, Barayoga JC, Barclay SE, Barish BC, Barker D, Barkett K, Barone F, Barr B, Barsotti L, Barsuglia M, Barta D, Barthelmy SD, Bartlett J, Bartos I, Bassiri R, Basti A, Batch JC, Bawaj M, Bayley JC, Bazzan M, Bécsy B, Beer C, Bejger M, Belahcene I, Bell AS, Berger BK, Bergmann G, Bero JJ, Berry CPL, Bersanetti D, Bertolini A, Betzwieser J, Bhagwat S, Bhandare R, Bilenko IA, Billingsley G, Billman CR, Birch J, Birney R, Birnholtz O, Biscans S, Biscoveanu S, Bisht A, Bitossi M, Biwer C, Bizouard MA, Blackburn JK, Blackman J, Blair CD, Blair DG, Blair RM, Bloemen S, Bock O, Bode N, Boer M, Bogaert G, Bo… See abstract for full author list ➔ Abbott BP, et al. Phys Rev Lett. 2017 Oct 6;119(14):141101. doi: 10.1103/PhysRevLett.119.141101. Epub 2017 Oct 6. Phys Rev Lett. 2017. PMID: 29053306 Free article.
The luminosity distance of the source is 540_{-210}^{+130} Mpc, corresponding to a redshift of z=0.11_{-0.04}^{+0.03}. A network of three detectors improves the sky localization of the source, reducing the area of the 90% credible region from 1160 deg^{2} using only the tw …
The luminosity distance of the source is 540_{-210}^{+130} Mpc, corresponding to a redshift of z=0.11_{-0.04}^{+0.03}. A network of three de …
12 results