228 research outputs found
Gravitational wave searches associated with galactic core-collapse supernovae
- Author
- Publication venue
- Publication date
- Field of study
Understanding the mechanism by which stars become supernovae is a major unsolved problem in astrophysics. They are driven by the release of gravitational energy,
which is expelled largely in the form of neutrinos. After almost 40 years of numerical simulations, it is still unclear how and why large stars explode. A core-collapse
supernova (CCSN) begins when its core collapses and drives a shock wave outwards. Due to the emission of neutrinos and the inward pressure of the core collapse, the shock wave briefly subsides. The mechanism for the revival of the shock wave and subsequent supernova explosion is presently unknown. Proposed mechanisms include the neutrino, magnetorotational, and the acoustic mechanisms. Gravitational Waves (GWs) will help answer how large stars explode. The violent motions of dense matter in the stars core produce GWs, and their shape is determined by that motion. Therefore, the physical processes (i.e. either the neutrino, magnetorotational, or the acoustic mechanisms) can be inferred by studying the GWs. Estimates from numerical simulations indicate that the GWs from a supernova anywhere in the Milky Way would be strong enough to be detectable by advanced LIGO. A large burst of neutrino particles is also emitted in the core collapse; together with the GWs, these can determine the location of the supernova on the sky before the shock breakout, giving astronomers a chance to see the earliest stages of the explosion. Because the Galactic supernova rate is no larger than about one every thirty years, it is necessary for a search to be ready from the beginning of the operation of advanced LIGO. This search should include the ability to detect any plausible GW polarization that could arise from a CCSN. Speci�cally, the knowledge of the precise time and sky location of the SN provided by neutrino and optical detection respectively constrains how the GW signal will appear in a network of detectors. Thus, deviations from the expected detector response could reveal if GWs contain polarizations beyond those predicted by GR. This thesis explores the ability of aLIGO to detect scalar polarizedGWs from CCSNe and other possible galactic sources
All-sky search for long-duration gravitational wave transients with initial LIGO
- Author
- Publication venue
- 'American Physical Society (APS)'
- Publication date
- 15/02/2016
- Field of study
We present the results of a search for long-duration gravitational wave transients in two sets of data collected by the LIGO Hanford and LIGO Livingston detectors between November 5, 2005 and September 30, 2007, and July 7, 2009 and October 20, 2010, with a total observational time of 283.0 days and 132.9 days, respectively. The search targets gravitational wave transients of duration 10–500 s in a frequency band of 40–1000 Hz, with minimal assumptions about the signal waveform, polarization, source direction, or time of occurrence. All candidate triggers were consistent with the expected background; as a result we set 90% confidence upper limits on the rate of long-duration gravitational wave transients for different types of gravitational wave signals. For signals from black hole accretion disk instabilities, we set upper limits on the source rate density between 3.4×10−5 and 9.4×10−4 Mpc−3 yr−1 at 90% confidence. These are the first results from an all-sky search for unmodeled long-duration transient gravitational wave
Search of the Orion spur for continuous gravitational waves using a loosely coherent algorithm on data from LIGO interferometers
- Author
- Publication venue
- 'American Physical Society (APS)'
- Publication date
- 17/02/2016
- Field of study
We report results of a wideband search for periodic gravitational waves from isolated neutron stars within the Orion spur towards both the inner and outer regions of our Galaxy. As gravitational waves interact very weakly with matter, the search is unimpeded by dust and concentrations of stars. One search disk (A) is 6.87° in diameter and centered on 20h10m54.71s+33°33′25.29′′, and the other (B) is 7.45° in diameter and centered on 8h35m20.61s−46°49′25.151′′. We explored the frequency range of 50–1500 Hz and frequency derivative from 0 to −5×10−9 Hz/s. A multistage, loosely coherent search program allowed probing more deeply than before in these two regions, while increasing coherence length with every stage. Rigorous follow-up parameters have winnowed the initial coincidence set to only 70 candidates, to be examined manually. None of those 70 candidates proved to be consistent with an isolated gravitational-wave emitter, and 95% confidence level upper limits were placed on continuous-wave strain amplitudes. Near 169 Hz we achieve our lowest 95% C.L. upper limit on the worst-case linearly polarized strain amplitude h0 of 6.3×10−25, while at the high end of our frequency range we achieve a worst-case upper limit of 3.4×10−24 for all polarizations and sky location
Accelerated surgery versus standard care in hip fracture (HIP ATTACK): an international, randomised, controlled trial
- Author
- Abarca Javiera
- Abarca Luis
- Abdlaziz Ihab
- Abraham Valsamma
- Accetta Riccardo
- Adhye Bharati Anil
- Adili Anthony
- Adinarayanan S
- Aframian Arash
- Aguado Hector J
- Aguilar Marc
- Ahmed Tashfeen
- Ahn Henry
- Ali Arif
- Almas Ayesha
- Alvarado Kim A
- Ambroży Wojciech
- Anaya Rafael
- Andres-Peiro Jose-Vicente
- Anjum Anila
- Arnuntasupakul Vanlapa
- Arroyo Marta
- Ashraf Mohammed
- Ashraf Muhammad
- Atrey Amit
- Avram Victoria RA
- Balaguer-Castro Mariano
- Balasubramanian Kumar
- Balonov Konstantin
- Bangdiwala Shrikant I
- Bardana Davide D
- Barnawal Satish Prasad
- Bartley Debra
- Baños Victoria
- Beaupre Lauren
- Begum Dilshad
- Belley-Cote Emilie P
- Bentoumi Souad
- Beretta Luigi
- Bergese Sergio D
- Bernaus Martí
- Beroud Sebastien
- Bhandari Mohit
- Bhutia Jigme Tshering
- Biccard Bruce M
- Bicknell Ryan T
- Bidkar Prasanna Udupi
- Bilchod Prashanth Nabhirajappa
- Binda Mirko
- Biscardi Anna
- Bisland Stuart
- Bogallo Jose Manuel
- Bohm Eric R
- Bokhari Syedah Saira
- Bonadies Marika
- Boon Huck Wee
- Borate Madhav Pandurang
- Borges Flavia K
- Brokelman Roy B.G.
- Campbell Aaron R
- Campbell Ryan Jonathan
- Cano Juan Ramon
- Carey Timothy
- Carreras-Castañer Anna
- Cassidy Charles
- Castillón Pablo
- Cecconi Maurizio
- Chalacheewa Theerawat
- Chandran Nitheesh
- Chaudier Philippe
- Chaw Sook Hui
- Chee KH
- Chen Brian P-J
- Chetty Sean
- Chin Im Im
- Choi Stephen
- Chouhan Devendra K
- Clark Molly E
- Clinckaert Carol
- Cobben Jan-Hein MG
- Coles Chad P
- Colnaghi Eleonora
- Colombo Chiara
- Colomina Maria J
- Comstock Curt
- Conen David
- Cornu Olivier
- Correia Patricia
- Coughlin Ryan
- Coupal Stephanie A
- Cowan David D
- Crawford Gordon A
- Cruz Encarnacion
- Cullinan Claude
- Cámara-Cabrera Jaume
- Daniels Timothy R
- Dashputra Ravi Prabhakar
- David Jean Stephane
- de Beer Justin
- De Blasio Giuseppe
- De Caso Julio
- De Clippeleir Dirk
- Dealbert Alfred
- Deheshi Benjamin
- Dehghan Niloofar
- Denaro Giuseppe
- Devereaux PJ
- Dhillon Mandeep S
- Dillane Derek
- Dillingham Sally
- Ding Anthony
- Dongre Himanshu Vijaykumar
- Douplat Marion
- Dragic-Taylor Sanela
- Dresser George K
- Droll Kurt
- Duncan Andrew W
- Dąbek Piotr
- Elnaggar Mohamed
- Elskamp-Meijerman Hannie F
- Estrada Cristina
- Fang Christian Xinshuo
- Farooque Kamran
- Farrell Janet C
- Fayet Jean Marie
- Feibel Robert J
- Feijoo-Massó Carlos
- Fergusson Dean A
- Fessy Michel Henri
- Firth Gregory Bodley
- Flikweert Elvira R
- Flint Margot
- Foo Li Lian
- Forget Patrice
- Fourtounas Maria
- Fozzato Stefania
- Fraguas-Castany Antoni
- Frank Christopher C
- Friggeri Arnaud
- Furgan Ahmad
- Gallant Catherine
- Gamangati Shivanand
- Garcia-Sanchez Yaiza
- Garg Amit X
- Garrido Clua Miriam
- Gattu Uttam Vaidya
- Gauthier Leslie P
- George Carolin Elizabeth
- George Preetha Elizabeth
- Georgekutty AM
- Giardina Giuseppe
- Giilck Stephen M
- Gnanadurai Kingsly Robert
- Gonzalez Posada MA
- Gonzalez Zacarias Alicia A
- Grant Heather
- Greene James
- Gregus Krysten K
- Grzelak Adrian
- Gucwa Jaroslaw
- Guerado Enrique
- Guerra-Farfan Ernesto
- Guilabert Patricia
- Gupta Babita
- Guy Pierre
- Guyatt Gordon H
- Guzzetti Luca
- Gómez Olga
- Hadden William J
- Haider Syed Y
- Haire Kevin
- Hall Jeremy A
- Halman Samantha
- Harrison Mark M
- Harvey Valerie
- Hashmi Pervaiz Mehmood
- Henry Patrick DG
- Herranz Susana
- Herrera-Mateo Sergio
- Higa-Sansone JL
- Hiremath Santosh Angad
- Horst Maarten R
- Hunt Stephen B
- Hupel Tom
- Imbuldeniya Arjuna
- Iqbal Muhammad Nasir
- Irwin Marleen
- Ivanov Alexia
- Jacka Michael J
- Jaeger Melanie T
- Janjua Kholood Abid
- Jawali Abhijit
- Jenkinson Richard J
- John Bobby
- John Joby
- Jornet-Gibert Monsant
- Joseph Katherine
- Joseph Philip G
- Juman Naveed Muhammed
- K Varghese Zachariah
- Kadry Miriam Adel
- Karbassi Arsha
- Karera Mwalimu
- Kearon Clive
- Khan Abdus Salam
- Khan Eraj Khurshid
- Khan Hammad Naqi
- Khan Moin
- Khan Muhammad Kashif
- Khan Robyna Irshad
- Khan Siddra Ahmed
- Khanna Vickas
- Khattak Mujahid Jamil
- Khor HM
- Khoshbin Amir
- Kishta Waleed
- Kleinlugtenbelt Ydo V
- Koo Kevin
- KP Mary KP
- Kreder Hans J
- Kudrimoti Kiran Bhalchandra
- Kulachote Noratep
- Kumar CS
- Kumoń Adam
- Kunz Monica R
- Labrador Gregorio
- Lai Hou Yee
- Lakdawala Riaz Hussain
- Lal Purushotham
- Lalueza-Broto Pilar
- Lamy Andre
- Landais Paul
- Landman Ellie BM
- Landoni Giovanni
- Lavand'homme Patricia
- Lawendy Abdel-Rahman
- Lawrence Kelly H
- Le Manach Yannick
- le Polain de Waroux Bernard
- Lee Jacques S
- Lee Meng-Li
- Lefrancois Tina
- Leong Darryl P
- Leung Frankie Ka Li
- León Ricardo
- Liu Yang
- Loh PS
- Louboutin Lucie
- M Niranjan
- MacDonald Anne Marie
- MacDonald Shelley
- Machala Waldemar
- Macho Oscar
- Macleod Mark D
- Maddipati Tatarao
- Magloire Patrick
- Malhotra Rajesh
- Maluleke Matimba Lenny
- Mann Stephen M
- Maqungo Sithombo
- Marcantonio Andrew J
- Marcato Anna
- Marcucci Maura
- Marion Travis
- Marmor Meir T
- Martin Nuria
- Martinez-Municio Gonzalo
- Martinez-Ripol Pedro
- Martínez-Sañudo Luis
- Mateo Llorenç
- Mathur Purva
- Matityahu Amir
- Maxwell Chelsea
- Mayor Amy SE
- McClellan Robert Trigg
- McGillion Michael H
- McIlquham Katie
- McLean Lisa M
- McMahon Stephen J
- Menon Jagdish
- Menon Matthew
- Menon Prem Haridas
- Mestre-Torres Jaume
- Millan Angelica
- Minguell-Monyart Joan
- Mishra Sandeep Kumar
- Mittal Samarth
- Molero-Garcia Vicente
- Moller Carien
- Molnar Sarah
- Moppett Iain K
- Morelli Ilaria
- Mozzon Lise
- Mustafa Khawaja Junaid
- Muñoz Juan Manuel
- Naidoo Rubendren
- Nam Diane
- Nanjayan Shashi Kumar
- Naratreekoon Bundit
- Narayan Ravi
- Nauth Aaron
- NC Madhusudhan
- Neary John D
- Nejthardt Marcin B
- Ngim Joanne HL
- Nhlapo Lerato
- Nicholson Laura
- Noordin Shahryar
- Nousiainen Markku
- Novellas Marga
- Nur Aamer Nabi
- Nuñez Camarena Jorge
- O'Brien Peter J
- O'Sullivan Susan
- O'Toole Robert
- Olivieri Loretta
- Omran Sherif
- Orakzai Sajjad Hassan
- Oxner William
- Oyenubi Ademilola N
- Pandey Ritesh Arvind
- Parker Martyn J
- Patel Ameen
- Patil Atul Ashok
- Patil Sharanu
- Patil Shashank
- Payendeh Jubin
- Paños Gozalo M Luisa
- Peig-Font Anna
- Pengrung Nachapan
- Perazzo Paolo
- Pettit Shirley M
- Pey Borja
- Phieffer Laura S
- Piccirillo Fabio
- Pino Fabio
- Piriou Vincent
- Placella Giacomo
- Ploeg Leone
- Popova Ekaterine
- Porcel-Vazquez Juan A
- Pradhan Chetan Vijay
- Prakasam Komella
- Puram Chetan Prabhakar
- Puskas David
- Quintas Saioa
- Quraishi Faraaz A
- Rahate Prashant Vitthal
- Rajkumar Arti
- Ramokgopa Mmampapatla T
- Ramokgopa Mmampapatla Thomas
- Rashid Haroon Ur
- Rashid Rizwan Haroon
- Ravi Bheeshma
- Reul Maike
- Riaz Muhammad Mehmood
- Richardson C Glen
- Ricol Laura
- Roerdink Herbert W
- Ruggiero Sara
- Ryan Scott P
- Rycombel Jacek
- Sa-ngasoongsong Paphon
- Sadoughi Mehdi
- Salini Vincenzo
- Salomó-Domènech Mònica
- Salvador Jordi
- Sancheti Parag K
- Sancheti Parag Kantilal
- Sanchez-Raya Judith
- Sanders David W
- Santiago-Maniega Silvia
- Santone David J
- Satora Wojciech
- Sawhney Chavi
- Schemitsch Emil
- Schemitsch Emil H
- Sciadini Marcus
- Selga Marsa Jordi
- Serrano-Sanz Jorge
- Shadowitz Steven
- Shan Lei
- Shanthanna Harsha
- Sharma Achal
- Sharma Deep
- Sharma Vijay
- Shirali Hemant R
- Shiraz Muhammad
- Shrikumar Mopina
- Sianes-Gallén Mònica
- Sigamani Alben
- Sigamani Alen
- Simpson Diane L
- Singh Simmrat
- Singh Surya Udai
- Singh Virsen
- Sirisreetreerux Norachart
- Sivilotti Marco LA
- Slobogean Gerard
- Smith Christopher A
- Smith Crystal A
- Sohail Mian Amjad
- Stella Daniele
- Stephen David JG
- Stephen Manesh
- Stiegelmahr Robert
- Sulthan Ahamad Shaheel
- Swaminathan Srinivasan
- Szczeklik Wojciech
- Tan Kit Mun
- Tandon Vikas
- Teixidor-Serra Jordi
- Thayaparan Surendini
- Thiruganasambandamoorth Venkatesh
- Tiboni Maria E
- Tieszer Christina
- Tomas-Hernandez Jordi
- Toogood Paul
- Torner Pere
- Torra Mercè
- Touil Nassim
- Tran Sarah
- Trask Kelly
- Trenholm J Andrew I
- Tribak Karim
- Tripathy Vijaylaxmi
- Tuazon Ravianne
- Turgeon Thomas R
- Turiel Maurizio
- Tushinski Daniel M
- Umar Muhammad
- Umer Masood
- Usua Gemma
- Valldosera Esther
- Vasarhelyi Edward
- Veevaete Laurent
- Villar-Casares Maria del Mar
- Vincent Jessica
- Vizcaychipi Marcela Paola
- Wahab Hussain
- Wang Chew Yin
- Ward Sarah E
- Wasserstein David
- Watts Evan
- Wells Jennifer R
- Whelan Daniel B
- White Neil J
- Whitlock Richard
- Wikkerink Spencer
- Wilson David AJ
- Winemaker Mitchell
- Wong Steven CW
- Wood Gavin CA
- Wood Thomas J
- Worster Andrew
- Wright Douglas Steven
- Wu Anshi
- Yach Jeff D
- Yee Allan J
- Yee Dennis King Hang
- Yela-Verdú Christian
- Yingchoncharoen Teerapat
- Yombi Jean Cyr
- Yuste Antoni
- Yusuf Salim
- Zabalza Ana
- Zaki Amna
- Zhao Yanrui
- Zhou Junlin
- Ślęczka Paweł
- Święch Mariusz
- Publication venue
- 'Elsevier BV'
- Publication date
- 29/02/2020
- Field of study
Search for gravitational waves from Scorpius X-1 in the second Advanced LIGO observing run with an improved hidden Markov model
- Author
- Abbott Bp
- Abbott R
- Abbott Td
- Abraham S
- Acernese F
- Ackley K
- Adams C
- Adhikari Rx
- Adya Vb
- Affeldt C
- Agathos M
- Agatsuma K
- Aggarwal N
- Aguiar Od
- Aiello L
- Ain A
- Ajith P
- Allen G
- Allocca A
- Aloy Ma
- Altin Pa
- Amato A
- Anand S
- Ananyeva A
- Anderson Sb
- Anderson Wg
- Angelova Sv
- Antier S
- Appert S
- Arai K
- Araya Mc
- Areeda Js
- Arene M
- Arnaud N
- Aronson Sm
- Ascenzi S
- Ashton G
- Aston Sm
- Astone P
- Aubin F
- Aufmuth P
- AultONeal K
- Austin C
- Avendano V
- Avila-Alvarez A
- Babak S
- Bacon P
- Badaracco F
- Bader Mkm
- Bae S
- Baird J
- Baker Pt
- Baldaccini F
- Ballardin G
- Ballmer Sw
- Bals A
- Banagiri S
- Barayoga Jc
- Barbieri C
- Barclay Se
- Barish Bc
- 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 Jc
- Bazzan M
- Becsy B
- Bejger M
- Belahcene I
- Bell As
- Beniwal D
- Benjamin Mg
- Berger Bk
- Bergmann G
- Bernuzzi S
- Berry Cpl
- Bersanetti D
- Bertolini A
- Betzwieser J
- Bhandare R
- Bidler J
- Biggs E
- Bilenko Ia
- Bilgili Sa
- Billingsley G
- Birney R
- Birnholtz O
- Biscans S
- Bischi M
- Biscoveanu S
- Bisht A
- Bitossi M
- Bizouard Ma
- Blackburn Jk
- Blackman J
- Blair Cd
- Blair Dg
- Blair Rm
- Bloemen S
- Bobba F
- Bode N
- Boer M
- Boetzel Y
- Bogaert G
- Bondu F
- Bonnand R
- Booker P
- Boom Ba
- Bork R
- Boschi V
- Bose S
- Bossilkov V
- Bosveld J
- Bouffanais Y
- Bozzi A
- Bradaschia C
- Brady Pr
- Bramley A
- Branchesi M
- Brau Je
- Breschi M
- Briant T
- Briggs Jh
- Brighenti F
- Brillet A
- Brinkmann M
- Brockill P
- Brooks Af
- Brooks J
- Brown Dd
- Brunett S
- Buikema A
- Bulik T
- Bulten Hj
- Buonanno A
- Buskulic D
- Bustillo Jc
- Buy C
- Byer Rl
- Cabero M
- Cadonati L
- Cagnoli G
- Cahillane C
- Callister Ta
- Calloni E
- Camp Jb
- Campbell Wa
- Cannon Kc
- Cao H
- Cao J
- Carapella G
- Carbognani F
- Caride S
- Carney Mf
- Carullo G
- Casentini C
- Castro Jmg
- Caudill S
- Cavaglia M
- Cavalier F
- Cavalieri R
- Cella G
- Cerda-Duran P
- Cesarini E
- Chaibi O
- Chakravarti K
- Chamberlin Sj
- Chan M
- Chao S
- Charlton P
- Chase Ea
- Chassande-Mottin E
- Chatterjee D
- Chaturvedi M
- Cheeseboro Bd
- Chen Hy
- Chen X
- Chen Y
- Cheng Hp
- Cheong Ck
- Chia Hy
- Chiadini F
- Chincarini A
- Chiummo A
- Cho G
- Cho Hs
- Cho M
- Christensen N
- Chu Q
- Chua S
- Chung Kw
- Chung S
- Ciani G
- Cieslar M
- Ciobanu Aa
- Ciolfi R
- Cipriano F
- Cirone A
- Clara F
- Clark Ja
- Clearwater P
- Cleva F
- Coccia E
- Cohadon Pf
- Cohen D
- Colleoni M
- Collette Cg
- Collins C
- Colpi M
- Cominsky Lr
- Constancio M
- Conti L
- Cooper Sj
- Corban P
- Corbitt Tr
- Cordero-Carrion I
- Corezzi S
- Corley Kr
- Cornish N
- Corre D
- Corsi A
- Cortese S
- Costa Ca
- Costa Cfd
- Cotesta R
- Coughlin Mw
- Coughlin Sb
- Coulon Jp
- Countryman St
- Couvares P
- Covas Pb
- Cowan Ee
- Coward Dm
- Cowart Mj
- Coyne Dc
- Coyne R
- Creighton Jde
- Creighton Td
- Cripe J
- Croquette M
- Crowder Sg
- Cullen Tj
- Cumming A
- Cunningham L
- Cuoco E
- D'Angelo B
- D'Antonio S
- Dal Canton T
- Dalya G
- Danilishin Sl
- Danzmann K
- Dasgupta A
- Datrier Leh
- Dattilo V
- Dave I
- Davier M
- Davis D
- Daw Ej
- De Laurentis M
- De Pietri R
- De Rosa R
- De Rossi C
- de Varona O
- DeBra D
- Deenadayalan M
- Degallaix J
- Del Pozzo W
- Deleglise S
- DeMarchi Lm
- Demos N
- Dent T
- DeSalvo R
- Dhurandhar S
- Di Fiore L
- Di Giorgio C
- Di Giovanni F
- Di Giovanni M
- Di Girolamo T
- Di Lieto A
- Di Pace S
- Di Palma I
- Di Renzo F
- Diaz Jc
- Diaz Mc
- Dietrich T
- DiFronzo C
- Ding B
- Divakarla Ak
- Dmitriev A
- Doctor Z
- Donovan F
- Dooley Kl
- Doravari S
- Dorrington I
- Downes Tp
- Drago M
- Driggers Jc
- Du Z
- Ducoin Jg
- Dupej P
- Durante O
- Dwyer Se
- Easter Pj
- Eddolls G
- Edo Tb
- Effler A
- Ehrens P
- Eichholz J
- Eikenberry Ss
- Eisenmann M
- Eisenstein Ra
- Errico L
- Essick Rc
- Estelles H
- Estevez D
- Etienne Zb
- Etzel T
- Evans M
- Evans Tm
- Fafone V
- Fairhurst S
- Fan X
- Farinon S
- Farr B
- Farr Wm
- Fauchon-Jones Ej
- Favata M
- Fays M
- Fazio M
- Fee C
- Feicht J
- Fejer Mm
- Feng F
- Fernandez-Galiana A
- Ferrante I
- Ferreira Ec
- Ferreira Ta
- Fidecaro F
- Fiori I
- Fiorucci D
- Fishbach M
- Fisher Rp
- Fishner Jm
- Fittipaldi R
- Fitz-Axen M
- Fiumara V
- Flaminio R
- Fletcher M
- Floden E
- Flynn E
- Fong H
- Font Ja
- Forsyth Pwf
- Fournier Jd
- Frasca S
- Frasconi F
- Frei Z
- Freise A
- Frey R
- Frey V
- Fritschel P
- Frolov Vv
- Fronze G
- Fulda P
- Fyffe M
- Gabbard Ha
- Gadre Bu
- Gaebel Sm
- Gair Jr
- Gammaitoni L
- Gaonkar Sg
- 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 Ja
- Giardina Kd
- Gibson Dr
- Gill K
- Glover L
- Gniesmer J
- Godwin P
- Goetz E
- Goetz R
- Goncharov B
- Gonzalez G
- Gopakumar A
- Gossan Se
- Gosselin M
- Gouaty R
- Grace B
- Grado A
- Granata M
- Grant A
- Gras S
- Grassia P
- Gray C
- Gray R
- Greco G
- Green Ac
- Green R
- Gretarsson Em
- Grimaldi A
- Grimm Sj
- Groot P
- Grote H
- Grunewald S
- Gruning P
- Guidi Gm
- Gulati Hk
- Guo Y
- Gupta A
- Gupta A
- Gupta P
- Gustafson Ek
- Gustafson R
- Haegel L
- Halim O
- Hall Br
- Hall Ed
- Hamilton Ez
- Hammond G
- Haney M
- Hanke Mm
- Hanks J
- Hanna C
- Hannuksela Oa
- Hansen Tj
- Hanson J
- Harder T
- Hardwick T
- Haris K
- Harms J
- Harry Gm
- Harry Iw
- Hasskew Rk
- Haster Cj
- Haughian K
- Hayes Fj
- Healy J
- Heidmann A
- Heintze Mc
- Heitmann H
- Hellman F
- Hello P
- Hemming G
- Hendry M
- Heng Is
- Hennig J
- Hernandez Im
- Heurs M
- Hild S
- Hinderer T
- Hochheim S
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- Zimmerman Ab
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- Zweizig J
- Publication venue
- College Park, MD : American Physical Society
- Publication date
- 01/01/2019
- Field of study
We present results from a semicoherent search for continuous gravitational waves from the low-mass x-ray binary Scorpius X-1, using a hidden Markov model (HMM) to track spin wandering. This search improves on previous HMM-based searches of LIGO data by using an improved frequency domain matched filter, the J-statistic, and by analyzing data from Advanced LIGO's second observing run. In the frequency range searched, from 60 to 650 Hz, we find no evidence of gravitational radiation. At 194.6 Hz, the most sensitive search frequency, we report an upper limit on gravitational wave strain (at 95% confidence) of h095%=3.47×10-25 when marginalizing over source inclination angle. This is the most sensitive search for Scorpius X-1, to date, that is specifically designed to be robust in the presence of spin wandering. © 2019 American Physical Society
Search for gravitational waves from Scorpius X-1 in the second Advanced LIGO observing run with an improved hidden Markov model
- Author
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- Zweizig J
- Publication venue
- 'American Physical Society (APS)'
- Publication date
- 01/01/2019
- Field of study
We present results from a semicoherent search for continuous gravitational waves from the low-mass x-ray binary Scorpius X-1, using a hidden Markov model (HMM) to track spin wandering. This search improves on previous HMM-based searches of LIGO data by using an improved frequency domain matched filter, the J-statistic, and by analyzing data from Advanced LIGO’s second observing run. In the frequency range searched, from 60 to 650 Hz, we find no evidence of gravitational radiation. At 194.6 Hz, the most sensitive search frequency, we report an upper limit on gravitational wave strain (at 95% confidence) of h95%0=3.47×10−25 when marginalizing over source inclination angle. This is the most sensitive search for Scorpius X-1, to date, that is specifically designed to be robust in the presence of spin wandering
Erratum: "A Gravitational-wave Measurement of the Hubble Constant Following the Second Observing Run of Advanced LIGO and Virgo" (2021, ApJ, 909, 218)
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- Publication venue
- London : Institute of Physics Publ.
- Publication date
- 01/01/2021
- Field of study
[no abstract available
Erratum: “Searches for Gravitational Waves from Known Pulsars at Two Harmonics in 2015–2017 LIGO Data” (2019, ApJ, 879, 10)
- Author
- Abbott B. P.
- Abbott R.
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- Publication venue
- 'American Astronomical Society'
- Publication date
- 01/01/2019
- Field of study
Due to an error at the publisher, in the published article the number of pulsars presented in the paper is incorrect in multiple places throughout the text. Specifically, "222" pulsars should be "221." Additionally, the number of pulsars for which we have EM observations that fully overlap with O1 and O2 changes from "168" to "167." Elsewhere, in the machine-readable table of Table 1 and in Table 2, the row corresponding to pulsar J0952-0607 should be excised as well. Finally, in the caption for Table 2 the number of pulsars changes from "188" to "187.
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