dc.contributor | LIGO Calif Inst Technol | |
dc.contributor | Louisiana State Univ | |
dc.contributor | Univ Salerno | |
dc.contributor | Complesso Univ Monte S Angelo | |
dc.contributor | Univ Florida | |
dc.contributor | LIGO Livingston Observ | |
dc.contributor | Cardiff Univ | |
dc.contributor | Univ Savoie Mt Blanc | |
dc.contributor | Univ Sannio Benevento | |
dc.contributor | Ist Nazl Fis Nucl | |
dc.contributor | Max Planck Inst Gravitat Phys | |
dc.contributor | NIKHEF H | |
dc.contributor | LIGO Massachusetts Inst Technol | |
dc.contributor | Inst Nacl Pesquisas Espaciais | |
dc.contributor | Interuniv Ctr Astron & Astrophys | |
dc.contributor | Tata Inst Fundamental Res | |
dc.contributor | Univ Wisconsin | |
dc.contributor | Leibniz Univ Hannover | |
dc.contributor | Univ Siena | |
dc.contributor | Stanford Univ | |
dc.contributor | Univ Mississippi | |
dc.contributor | Calif State Univ Fullerton | |
dc.contributor | Univ Paris 11 | |
dc.contributor | Univ Southampton | |
dc.contributor | Montana State Univ | |
dc.contributor | Univ Perugia | |
dc.contributor | EGO | |
dc.contributor | Syracuse Univ | |
dc.contributor | Univ Glasgow | |
dc.contributor | LIGO Hanford Observ | |
dc.contributor | Universidade de São Paulo (USP) | |
dc.contributor | Columbia Univ | |
dc.contributor | Univ Pisa | |
dc.contributor | CAMK PAN | |
dc.contributor | Warsaw Univ | |
dc.contributor | Univ Birmingham | |
dc.contributor | Univ Genoa | |
dc.contributor | RRCAT | |
dc.contributor | Moscow MV Lomonosov State Univ | |
dc.contributor | Univ West Scotland | |
dc.contributor | Univ Western Australia | |
dc.contributor | Radboud Univ Nijmegen | |
dc.contributor | Univ Nice Sophia Antipolis | |
dc.contributor | Observ Cote Azur | |
dc.contributor | MTA Eotvos Univ | |
dc.contributor | Univ Rennes 1 | |
dc.contributor | Washington State Univ | |
dc.contributor | Univ Urbino Carlo Bo | |
dc.contributor | Embry Riddle Aeronaut Univ | |
dc.contributor | Univ Oregon | |
dc.contributor | ENS PSL Res Univ | |
dc.contributor | Vrije Univ Amsterdam | |
dc.contributor | Univ Maryland | |
dc.contributor | Georgia Inst Technol | |
dc.contributor | Univ Lyon | |
dc.contributor | Univ Illes Balears IEEC | |
dc.contributor | Univ Naples Federico II | |
dc.contributor | NASA | |
dc.contributor | Univ Toronto | |
dc.contributor | Tsinghua Univ | |
dc.contributor | Univ Michigan | |
dc.contributor | Univ Roma Tor Vergata | |
dc.contributor | Natl Tsing Hua Univ | |
dc.contributor | Charles Sturt Univ | |
dc.contributor | Caltech CaRT | |
dc.contributor | Pusan Natl Univ | |
dc.contributor | Australian Natl Univ | |
dc.contributor | Carleton Coll | |
dc.contributor | Univ Roma La Sapienza | |
dc.contributor | Univ Brussels | |
dc.contributor | Texas Tech Univ | |
dc.contributor | Univ Minnesota | |
dc.contributor | Univ Melbourne | |
dc.contributor | Univ Texas Brownsville | |
dc.contributor | Univ Sheffield | |
dc.contributor | RMKI | |
dc.contributor | Montclair State Univ | |
dc.contributor | Argentinian Gravitat Wave Grp | |
dc.contributor | Univ Trent | |
dc.contributor | Penn State Univ | |
dc.contributor | Univ Chicago | |
dc.contributor | Univ Cambridge | |
dc.contributor | Univ Szeged | |
dc.contributor | Inst Plasma Res | |
dc.contributor | Amer Univ | |
dc.contributor | Univ Massachusetts | |
dc.contributor | Univ Adelaide | |
dc.contributor | W Virginia Univ | |
dc.contributor | Korea Inst Sci & Technol Informat | |
dc.contributor | Univ Bialystok | |
dc.contributor | Univ Strathclyde | |
dc.contributor | IISER TVM | |
dc.contributor | Northwestern Univ | |
dc.contributor | Inst Appl Phys | |
dc.contributor | Hanyang Univ | |
dc.contributor | NCBJ | |
dc.contributor | IM PAN | |
dc.contributor | Monash Univ | |
dc.contributor | Seoul Natl Univ | |
dc.contributor | CNRS | |
dc.contributor | Univ Camerino | |
dc.contributor | Southern Univ | |
dc.contributor | A&M Coll | |
dc.contributor | Coll William & Mary | |
dc.contributor | Universidade Estadual Paulista (Unesp) | |
dc.contributor | IISER Kolkata | |
dc.contributor | HSIC | |
dc.contributor | Whitman Coll | |
dc.contributor | Nat Inst Math Sci | |
dc.contributor | Rochester Inst Technol | |
dc.contributor | Hobart & William Smith Coll | |
dc.contributor | Astron Inst | |
dc.contributor | Andrews Univ | |
dc.contributor | Trinity Univ | |
dc.contributor | Univ Padua | |
dc.contributor | Univ Washington | |
dc.contributor | Abilene Christian Univ | |
dc.contributor | Emory Univ | |
dc.date.accessioned | 2018-11-26T16:23:44Z | |
dc.date.available | 2018-11-26T16:23:44Z | |
dc.date.created | 2018-11-26T16:23:44Z | |
dc.date.issued | 2016-02-17 | |
dc.identifier | Physical Review D. College Pk: Amer Physical Soc, v. 93, n. 4, 14 p., 2016. | |
dc.identifier | 2470-0010 | |
dc.identifier | http://hdl.handle.net/11449/161214 | |
dc.identifier | 10.1103/PhysRevD.93.042006 | |
dc.identifier | WOS:000370247800001 | |
dc.identifier | WOS000370247800001.pdf | |
dc.description.abstract | 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 degrees in diameter and centered on 20(h)10(m)54.71(s) + 33 degrees 33'25.29 '', and the other (B) is 7.45 degrees in diameter and centered on 8(h)35(m)20.61(s) - 46 degrees 49'25.151 ''. We explored the frequency range of 50-1500 Hz and frequency derivative from 0 to -5 x 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 h(0) of 6.3 x 10(-25), while at the high end of our frequency range we achieve a worst-case upper limit of 3.4 x 10(-24) for all polarizations and sky locations. | |
dc.language | eng | |
dc.publisher | Amer Physical Soc | |
dc.relation | Physical Review D | |
dc.relation | 1,801 | |
dc.rights | Acesso aberto | |
dc.source | Web of Science | |
dc.title | Search of the Orion spur for continuous gravitational waves using a loosely coherent algorithm on data from LIGO interferometers | |
dc.type | Artículos de revistas | |