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A SLUGGS and Gemini/GMOS combined study of the elliptical galaxy M60: wide-field photometry and kinematics of the globular cluster system
Pota, Vincenzo; Brodie, Jean P.; Bridges, Terry; Strader, Jay; Romanowsky, Aaron J.; Villaume, Alexa; Jennings, Zach; Faifer, Favio Raúl; Pastorello, Nicola; Forbes, Duncan A.; Campbell, Ainsley; Usher, Christopher; Foster, Caroline; Spitler, Lee R.; Caldwell, Nelson; Forte, Juan Carlos.; Norris, Mark A.; Zepf, Stephen E.; Beasley, Michael A.; Gebhardt, Karl; Hanes, David A.; Sharples, Ray M.; Arnold, Jacob A. (Wiley, 2015-03)
We present new wide-field photometry and spectroscopy of the globular clusters (GCs) around NGC 4649 (M60), the third brightest galaxy in the Virgo cluster. Imaging of NGC 4649 was assembled from a recently-obtained ...
Multimessenger astronomy with gravitational waves and high-energy neutrinos
Ando, Shin’ichiro; Baret, Bruny; Bartos, Imre; Bouhou, Boutayeb; Chassande Mottin, Eric; Corsi, Alessandra; Di Palma, Irene; Dietz, Alexander; Donzaud, Corinne; Eichler, David; Finley, Chad; Guetta, Dafne; Halzen, Francis; Jones, Gareth; Kandhasamy, Shivaraj; Kotake, Kei; Kouchner, Antoine; Mandic, Vuk; Marka, Szabolcs; Marka, Zsuzsa; Moscoso, Luciano; Papa, Maria Alessandra; Piran, Tsvi; Pradier, Thierry; Romero, Gustavo Esteban; Sutton, Patrick; Thrane, Eric; Van Elewyck, Veronique; Waxman, Eli (American Physical Society, 2013-10)
Many of the astrophysical sources and violent phenomena observed in our Universe are potential emitters of gravitational waves and high-energy cosmic radiation, including photons, hadrons, and presumably also neutrinos. ...
A DARK ENERGY CAMERA SEARCH FOR MISSING SUPERGIANTS IN THE LMC AFTER THE ADVANCED LIGO GRAVITATIONAL-WAVE EVENT GW150914
Fermilab Natl Accelerator Lab; Harvard Smithsonian Ctr Astrophys; Univ Penn; Univ Chicago; Ohio Univ; Univ Illinois; STScI; Univ Southampton; Univ Arizona; Universidade Estadual Paulista (Unesp); Natl Opt Astron Observ; UCL; Rhodes Univ; CNRS; Univ Paris 06; Carnegie Observ; Stanford Univ; SLAC Natl Accelerator Lab; Univ Portsmouth; Lab Interinst & Astron LIneA; Observ Nacl; IEEC CSIC; Barcelona Inst Sci & Technol; NASA; Univ Maryland; Excellence Cluster Universe; Univ Munich; CALTECH; Univ Michigan; Penn State Univ; Los Alamos Natl Lab; CIEMAT; Univ Calif Berkeley; Ohio State Univ; Australian Astron Observ; Texas A&M Univ; Universidade de São Paulo (USP); Columbia Univ; Inst Catalana Recerca & Estudis Avancats; Max Planck Inst Extraterr Phys; Univ Sussex; Univ Fed Rio Grande do Sul; Brookhaven Natl Lab; Argonne Natl Lab (Iop Publishing Ltd, 2016-06-01)
The collapse of a stellar core is expected to produce gravitational waves (GWs), neutrinos, and in most cases a luminous supernova. Sometimes, however, the optical event could be significantly less luminous than a supernova ...
Search for Gravitational Waves Associated with gamma-ray Bursts Detected by the Interplanetary Network
CALTECH; Louisiana State Univ; Univ Salerno; Complesso Univ Monte S Angelo; Univ Florida; LIGO Livingston Observ; Cardiff Univ; Univ Sannio Benevento; INFN; Max Planck Inst Gravitat Phys; Nikhef; MIT; Instituto Nacional de Pesquisas Espaciais (INPE); Tata Inst Fundamental Res; Syracuse Univ; Univ Wisconsin Milwaukee; Leibniz Univ Hannover; Univ Siena; Stanford Univ; University of Mississippi; Calif State Univ Fullerton; Ist Nazl Fis Nucl; Univ Birmingham; Max Planck Inst Gravitat phys; Montana State Univ; European Gravitat Observ EGO; Hanford Observ; Univ Glasgow; Univ Paris Diderot; Columbia University; Univ Pisa; CAMK PAN; Warsaw Univ; Univ Genoa; Moscow MV Lomonosov State Univ; Univ Paris 11; NASA; Univ Western Australia; Radboud Univ Nijmegen; Univ Nice Sophia Antipolis; Univ Rennes 1; Univ Savoie; Washington State Univ; Inter Univ Ctr Astron & Astrophys; Kyoto Univ; Univ Urbino; Univ Oregon; Univ Paris 06; Vrije Univ Amsterdam; University of Maryland; Univ Massachusetts Amherst; Univ Lyon; Univ Illes Balears; Univ Naples Federico II; Univ Toronto; Tsinghua Univ; University of Michigan; Natl Tsing Hua Univ; Charles Sturt Univ; Caltech CaRT; Pusan Natl Univ; Australian Natl Univ; Carleton Coll; Univ Roma Tor Vergata; Univ Roma La Sapienza; Univ Brussels; Sonoma State Univ; George Washington Univ; Univ Cambridge; Univ Minnesota; Univ Texas Brownsville; Univ Sheffield; RMKI; Argentinian Gravitat Wave Grp; Univ Trent; NW Univ; Montclair State Univ; Penn State Univ; Eotvos Lorand Univ; Univ Perugia; HSIC; Embry Riddle Aeronaut Univ; Seoul Natl Univ; Perimeter Inst Theoret Phys; Amer Univ; Coll William & Mary; Univ Adelaide; Raman Res Inst; Korea Inst Sci & Technol Informat; Bialystok Univ; Univ Southampton; IISER TVM; Inst Phys Appl; Hanyang Univ; NCBJ; IM PAN; Inst Plasma Res; Univ Melbourne; Monash Univ; Univ Strathclyde; Louisiana Tech University; CNRS; Univ Camerino; S Univ & A& M Coll; IISER Kolkata; Natl Inst Mat Sci; Hobart & William Smith Coll; RRCAT; Univ W Scotland; Inst Astron; Indian Inst Technol; Universidade Estadual Paulista (Unesp); Andrews Univ; Trinity Univ; University of Washington; Rochester Inst Technol; SE Louisiana Univ; Abilene Christian Univ; AF Ioffe Phys Tech Inst; Univ Toulouse; Univ Alabama Huntsville; Univ Calif Berkeley; CRESST; Univ Space Res Assoc; INAF IASF Bologna; St Petersburg State Polytechn Univ; Los Alamos Natl Lab; Saitama Univ; Max Planck Inst f extraterrest Phys (Amer Physical Soc, 2014-06-30)
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, ...
First all-sky search for continuous gravitational waves from unknown sources in binary systems
LIGO-California Institute of Technology; Louisiana State University; CNRS/IN2P3; Complesso Universitario di Monte S. Angelo; Università di Salerno; University of Florida; LIGO-Livingston Observatory; Cardiff University; Max-Planck-Institut für Gravitationsphysik; Nikhef; LIGO-Massachusetts Institute of Technology; Instituto Nacional de Pesquisas Espaciais; Inter-University Centre for Astronomy and Astrophysics; Tata Institute for Fundamental Research; Syracuse University; University of Wisconsin-Milwaukee; Leibniz Universität Hannover; Sezione di Pisa; Università di Siena; Stanford University; University of Mississippi; California State University Fullerton; Sezione di Roma; University of Birmingham; Montana State University; European Gravitational Observatory (EGO); LIGO-Hanford Observatory; University of Glasgow; Sorbonne Paris Cité; Columbia University; Università di Pisa; CAMK-PAN; Astronomical Observatory Warsaw University; Sezione di Genova; Università degli Studi di Genova; San Jose State University; Lomonosov Moscow State University; IN2P3/CNRS; NASA/Goddard Space Flight Center; University of Western Australia; Radboud University Nijmegen; Observatoire de la Côte d'Azur; Université de Rennes 1; Université de Lyon; Washington State University; Sezione di Perugia; Sezione di Firenze; Università degli Studi di Urbino Carlo Bo; University of Oregon; Université Pierre et Marie Curie; VU University Amsterdam; University of Maryland; University of Massachusetts-Amherst; Universitat de les Illes Balears; University of Toronto; Tsinghua University; University of Michigan; Rochester Institute of Technology; Sezione di Roma Tor Vergata; National Tsing Hua University; Charles Sturt University; Caltech-CaRT; Pusan National University; Australian National University; Carleton College; Gran Sasso Science Institute; Università di Roma Tor Vergata; Università di Roma La Sapienza; University of Brussels; Sonoma State University; Embry-Riddle Aeronautical University; George Washington University; University of Cambridge; Northwestern University; University of Texas at Brownsville; University of Minnesota; University of Sheffield; RMKI; University of Sannio at Benevento; Gruppo Collegato di Trento; Università di Trento; Montclair State University; Pennsylvania State University; Lendulet A.R.G.; Università di Perugia; HSIC; Perimeter Institute for Theoretical Physics; American University; University of Adelaide; Raman Research Institute; Korea Institute of Science and Technology Information; Białystok University; University of Southampton; CET Campus; Institute of Applied Physics; Seoul National University; Hanyang University; IM-PAN; NCBJ; Institute for Plasma Research; University of Melbourne; Sezione di Padova; Monash University; University of Strathclyde; CNRS; Cordoba; Dipartimento di Fisica; University of Texas at Austin; A and M College; College of William and Mary; IISER-Kolkata; National Institute for Mathematical Sciences; Hobart and William Smith Colleges; RRCAT; University of the West of Scotland; Institute of Astronomy; Indian Institute of Technology; Universidade Estadual Paulista (UNESP); Andrews University; Trinity University; University of Washington; Southeastern Louisiana University; Abilene Christian University (2014-09-15)
We present the first results of an all-sky search for continuous gravitational waves from unknown spinning neutron stars in binary systems using LIGO and Virgo data. Using a specially developed analysis program, the TwoSpect ...
First targeted search for gravitational-wave bursts from core-collapse supernovae in data of first-generation laser interferometer detectors
California Institute of Technology; Louisiana State University; Università di Salerno; Complesso Universitario di Monte S.Angelo; University of Florida; LIGO Livingston Observatory; CNRS/IN2P3; University of Sannio at Benevento; Max-Planck-Institut für Gravitationsphysik; Nikhef; Massachusetts Institute of Technology; Instituto Nacional de Pesquisas Espaciais; Gran Sasso Science Institute; Sezione di Roma Tor Vergata; Inter-University Centre for Astronomy and Astrophysics; Tata Institute of Fundamental Research; University of Wisconsin-Milwaukee; Leibniz Universität Hannover; Università di Pisa; Sezione di Pisa; Australian National University; University of Mississippi; California State University Fullerton; Université Paris-Saclay; Chennai Mathematical Institute; Università di Roma Tor Vergata; University of Southampton; Universität Hamburg; Sezione di Roma; Sorbonne Paris Cité; Montana State University; Università di Perugia; Sezione di Perugia; European Gravitational Observatory (EGO); Syracuse University; University of Glasgow; LIGO Hanford Observatory; RMKI; Columbia University; Stanford University; Dipartimento di Fisica e Astronomia; Sezione di Padova; CAMK-PAN; University of Birmingham; Università degli Studi di Genova; Sezione di Genova; RRCAT; Lomonosov Moscow State University; University of the West of Scotland; University of Western Australia; Radboud University Nijmegen; Observatoire Côte d'Azur; Lendulet Astrophysics Research Group; Université de Rennes 1; Washington State University; Università degli Studi di Urbino Carlo Bo; Sezione di Firenze; University of Oregon; Collège de France; Astronomical Observatory Warsaw University; VU University Amsterdam; University of Maryland; Georgia Institute of Technology; Université Claude Bernard Lyon 1; IAC3-IEEC; NASA/Goddard Space Flight Center; University of Toronto; Tsinghua University; University of Michigan; National Tsing Hua University; Charles Sturt University; University of Chicago; Caltech CaRT; Korea Institute of Science and Technology Information; Carleton College; Università di Roma la Sapienza; University of Brussels; Sonoma State University; Texas Tech University; Cardiff University; University of Minnesota; University of Melbourne; University of Texas Rio Grande Valley; University of Sheffield; Dipartimento di Fisica; Trento Institute for Fundamental Physics and Applications; Montclair State University; Pennsylvania State University; National Astronomical Observatory of Japan; University of Edinburgh; Indian Institute of Technology; Institute for Plasma Research; University of Szeged; Embry-Riddle Aeronautical University; Osservatorio Astronomico di Capodimonte; American University; University of Massachusetts-Amherst; University of Adelaide; West Virginia University; University of Białystok; University of Strathclyde; CET Campus; Northwestern University; Institute of Applied Physics; Pusan National University; Hanyang University; NCBJ; IM-PAN; Rochester Institute of Technology; Monash University; Seoul National University; University of Alabama in Huntsville; CNRS; AandM College; College of William and Mary; Universidade Estadual Paulista (UNESP); University of Cambridge; IISER-Kolkata; HSIC; Whitman College; National Institute for Mathematical Sciences; Université de Lyon; Hobart and William Smith Colleges; University of Zielona Góra; Andrews University; Università di Siena; Trinity University; University of Washington; Kenyon College; Abilene Christian University; Sezione di Napoli (2016-11-15)
We present results from a search for gravitational-wave bursts coincident with two core-collapse supernovae observed optically in 2007 and 2011. We employ data from the Laser Interferometer Gravitational-wave Observatory ...
GW150914: Implications for the stochastic gravitational-wave background from binary black holes
California Institute of Technology; Louisiana State University; Università di Salerno; Complesso Universitario di Monte sant'Angelo; University of Florida; LIGO Livingston Observatory; CNRS/IN2P3; Max-Planck-Institut für Gravitationsphysik; Science Park; Massachusetts Institute of Technology; Instituto Nacional de Pesquisas Espaciais; Gran Sasso Science Institute; Sezione di Roma Tor Vergata; Inter-University Centre for Astronomy and Astrophysics; Tata Institute of Fundamental Research; University of Wisconsin-Milwaukee; Leibniz Universität Hannover; Università di Pisa; Sezione di Pisa; Australian National University; University of Mississippi; California State University Fullerton; Université Paris-Saclay; Chennai Mathematical Institute; Università di Roma Tor Vergata; University of Southampton; Universität Hamburg; Sezione di Roma; Sorbonne Paris Cité; Montana State University; Università di Perugia; Sezione di Perugia; European Gravitational Observatory (EGO); Syracuse University; University of Glasgow; LIGO Hanford Observatory; RMKI; Columbia University; Stanford University; Dipartimento di Fisica e Astronomia; Sezione di Padova; CAMK-PAN; Astronomical Observatory Warsaw University; University of Birmingham; Università degli Studi di Genova; Sezione di Genova; RRCAT; Lomonosov Moscow State University; University of the West of Scotland; University of Western Australia; Radboud University Nijmegen; CNRS; Lendulet Astrophysics Research Group; Université de Rennes 1; Washington State University; Università degli Studi di Urbino Carlo Bo; Sezione di Firenze; University of Oregon; Collège de France; VU University Amsterdam; University of Maryland; Georgia Institute of Technology; UMR CNRS 5306; Université de Lyon; IAC3 - IEEC; NASA/Goddard Space Flight Center; University of Toronto; Tsinghua University; Texas Tech University; Pennsylvania State University; National Tsing Hua University; Charles Sturt University; University of Chicago; Caltech CaRT; Korea Institute of Science and Technology Information; Carleton College; Università di Roma la Sapienza; University of Brussels; Sonoma State University; Northwestern University; University of Minnesota; University of Melbourne; University of Texas Rio Grande Valley; University of Sheffield; University of Sannio at Benevento; Montclair State University; Dipartimento di Fisica; Trento Institute for Fundamental Physics and Applications; Cardiff University; National Astronomical Observatory of Japan; University of Edinburgh; Gandhinagar Ahmedabad; Institute for Plasma Research; University of Szeged; Embry-Riddle Aeronautical University; University of Michigan; American University; University of Massachusetts-Amherst; University of Adelaide; West Virginia University; University of Biał Ystok; University of Strathclyde; CET Campus; Institute of Applied Physics; Pusan National University; Hanyang University; NCBJ; IM-PAN; Rochester Institute of Technology; Monash University; Seoul National University; University of Alabama in Huntsville; AandM College; College of William and Mary; Universidade Estadual Paulista (UNESP); University of Cambridge; IISER-Kolkata; HSIC; Whitman College; National Institute for Mathematical Sciences; Hobart and William Smith Colleges; University of Zielona Góra; Andrews University; Università di Siena; Trinity University; University of Washington; Kenyon College; Abilene Christian University; Sezione di Napoli (2016-03-31)
The LIGO detection of the gravitational wave transient GW150914, from the inspiral and merger of two black holes with masses 30M, suggests a population of binary black holes with relatively high mass. This observation ...
Search for gravitational waves associated with γ-ray bursts detected by the interplanetary network
LIGO, California Institute of Technology; Louisiana State University; Università di Salerno; INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo; University of Florida; LIGO Livingston Observatory; Cardiff University; University of Sannio at Benevento; Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik; Nikhef; LIGO, Massachusetts Institute of Technology; Instituto Nacional de Pesquisas Espaciais; International Centre for Theoretical Sciences, Tata Institute of Fundamental Research; Syracuse University; University of Wisconsin-Milwaukee; Leibniz Universität Hannover; Università di Siena; INFN, Sezione di Pisa; Stanford University; University of Mississippi; California State University Fullerton; INFN, Sezione di Roma; University of Birmingham; Montana State University; European Gravitational Observatory (EGO); LIGO Hanford Observatory; SUPA, University of Glasgow; APC, AstroParticule et Cosmologie, Université Paris Diderot, Observatoire de Paris; Columbia University; Università di Pisa; CAMK-PAN; Astronomical Observatory Warsaw University; Università Degli Studi di Genova; INFN, Sezione di Genova; Faculty of Physics, Lomonosov Moscow State University; LAL, Université Paris-Sud, IN2P3/CNRS; NASA/Goddard Space Flight Center; University of Western Australia; Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur; Institut de Physique de Rennes, CNRS, Université de Rennes 1; Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3; Washington State University; Inter-University Centre for Astronomy and Astrophysics; INFN, Sezione di Perugia; Yukawa Institute for Theoretical Physics, Kyoto University; Università Degli Studi di Urbino Carlo Bo; INFN, Sezione di Firenze; University of Oregon; Laboratoire Kastler Brossel, UPMC, Université Pierre et Marie Curie; VU University Amsterdam; University of Maryland; University of Massachusetts Amherst; Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon; Universitat de les Illes Balears; Università di Napoli 'Federico II', Complesso Universitario di Monte S. Angelo; Canadian Institute for Theoretical Astrophysics, University of Toronto; Tsinghua University; University of Michigan; INFN, Sezione di Roma Tor Vergata; National Tsing Hua University; Charles Sturt University; Caltech-CaRT; Pusan National University; Australian National University; Carleton College; Università di Roma Tor Vergata; INFN, Gran Sasso Science Institute; Università di Roma 'La Sapienza'; University of Brussels; Sonoma State University; George Washington University; University of Cambridge; University of Minnesota; University of Texas at Brownsville; University of Sheffield; Wigner RCP, RMKI; Argentinian Gravitational Wave Group; Università di Trento; INFN, Gruppo Collegato di Trento; Northwestern University; Montclair State University; Pennsylvania State University; MTA Eötvös University, Lendulet A. R. G.; Università di Perugia; Rutherford Appleton Laboratory, HSIC; Embry-Riddle Aeronautical University; Seoul National University; Perimeter Institute for Theoretical Physics; American University; College of William and Mary; University of Adelaide; Raman Research Institute; Korea Institute of Science and Technology Information; Białystok University; University of Southampton; IISER-TVM, CET Campus; Institute of Applied Physics; Hanyang University; NCBJ; IM-PAN; Institute for Plasma Research; University of Melbourne; INFN, Sezione di Padova; Monash University; SUPA, University of Strathclyde; Louisiana Tech University; ESPCI, CNRS; Università di Camerino, Dipartimento di Fisica; Southern University and AandM College; IISER-Kolkata; National Institute for Mathematical Sciences; Hobart and William Smith Colleges; RRCAT; Tata Institute for Fundamental Research; SUPA, University of the West of Scotland; Institute of Astronomy; Indian Institute of Technology; Universidade Estadual Paulista (UNESP); Andrews University; Trinity University; University of Washington; Rochester Institute of Technology; Southeastern Louisiana University; Abilene Christian University; Ioffe Physical-Technical Institute; Université de Toulouse, UPS-OMP, IRAP; CNRS, IRAP; CSPAR, University of Alabama in Huntsville; University of California-Berkeley, Space Sciences Lab; Center for Research and Exploration in Space Science and Technology (CRESST), NASA Goddard Space Flight Center; Universities Space Research Association; INAF-IASF Bologna; Saint Petersburg State Polytechnical University; Los Alamos National Laboratory; Graduate School of Science and Engineering, Saitama University; Max-Planck-Institut für Extraterrestrische Physik; INFN, Sezione di Napoli (2014-06-30)
We present the results of a search for gravitational waves associated with 223 γ-ray bursts (GRBs) detected by the InterPlanetary Network (IPN) in 2005-2010 during LIGO's fifth and sixth science runs and Virgo's first, ...
Search for continuous gravitational waves from neutron stars in globular cluster NGC 6544
CALTECH; Louisiana State Univ; Amer Univ; Univ Salerno; Complesso Univ Monte S Angelo; Univ Florida; LIGO Livingston Observ; Univ Savoie Mont Blanc; Univ Sannio Benevento; Ist Nazl Fis Nucl; Albert Einstein Inst; Nikhef; MIT; Inst Nacl Pesquisas Espaciais; Inter Univ Ctr Astron & Astrophys; Tata Inst Fundamental Res; Univ Wisconsin; Leibniz Univ Hannover; Univ Pisa; Australian Natl Univ; Univ Mississippi; Calif State Univ Fullerton; Univ Paris 11; Chennai Math Inst; Univ Roma Tor Vergata; Univ Southampton; Univ Hamburg; Max Planck Inst Gravitat Phys; Universidade de São Paulo (USP); Montana State Univ; Univ Perugia; European Gravitat Observ; Syracuse Univ; Univ Glasgow; LIGO Hanford Observ; Wigner RCP; Columbia Univ; Stanford Univ; Univ Padua; CAMK PAN; Univ Birmingham; Univ Genoa; RRCAT; Lomonosov Moscow State Univ; Univ West Scotland; Univ Western Australia; Radboud Univ Nijmegen; Univ Cote Azur; Univ Rennes 1; Washington State Univ; Univ Urbino Carlo Bo; Univ Oregon; UPMC; Carleton Coll; Warsaw Univ; Vrije Univ Amsterdam; Univ Maryland; Georgia Inst Technol; CNRS; Univ Lyon 1; Univ Naples Federico II; Goddard Space Flight Ctr; Univ Tokyo; Tsinghua Univ; Texas Tech Univ; Penn State Univ; Natl Tsing Hua Univ; Charles Sturt Univ; West Virginia Univ; Univ Chicago; Caltech CaRT; Korea Inst Sci & Technol Informat; Univ Roma La Sapienza; Univ Brussels; Sonoma State Univ; Northwestern Univ; Univ Minnesota; Univ Melbourne; Inst Plasma Res; Univ Sheffield; Univ Texas Rio Grande Valley; Univ Trento; Cardiff Univ; Montclair State Univ; MTA Eotvos Univ; Natl Astron Observ Japan; Univ Edinburgh; Indian Inst Technol; Univ Szeged; Embry Riddle Aeronaut Univ; INAF; Univ Michigan; Rochester Inst Technol; Univ Illinois; Univ Illes Balears; Univ Bialystok; Univ Strathclyde; IISER TVM; Univ Toronto; Inst Appl Phys; Pusan Natl Univ; Hanyang Univ; Univ Adelaide; NCBJ; IM PAN; Monash Univ; Seoul Natl Univ; Chinese Univ Hong Kong; Univ Alabama; Univ Massachusetts; Univ Camerino; Southern Univ; A&M Coll; Coll William & Mary; Universidade Estadual Paulista (Unesp); Univ Cambridge; IISER Kolkata; Rutherford Appleton Lab; Whitman Coll; Natl Inst Math Sci; Univ Lyon; Hobart & William Smith Coll; Univ Zielona Gora; Univ London; Andrews Univ; Univ Siena; Trinity Univ; Univ Washington; Kenyon Coll; Abilene Christian Univ (Amer Physical Soc, 2017-04-19)
We describe a directed search for continuous gravitational waves in data from the sixth initial LIGO science run. The target was the nearby globular cluster NGC 6544 at a distance of approximate to 2.7 kpc. The search ...
First low frequency all-sky search for continuous gravitational wave signals
CALTECH; Louisiana State Univ; Univ Salerno; Ist Nazl Fis Nucl; Univ Florida; LIGO Livingston Observ Livingston; Cardiff Univ; Univ Savoie Mt Blanc; Univ Sannio Benevento; INFN; Max Planck Inst Gravitat Phys; Nikhef; MIT; Inst Nacl Pesquisas Espaciais; Interuniv Ctr Astron & Astrophys; Tata Inst Fundamental Res; Univ Wisconsin; Leibniz Univ Hannover; Univ Siena; Stanford Univ; Univ Mississippi; Calif State Univ Fullerton; Univ Paris 11; Univ Southampton; Montana State Univ; Univ Perugia; EGO; Syracuse Univ; Univ Glasgow; LIGO Hanford Observ; Universidade de São Paulo (USP); Columbia Univ; Univ Pisa; CAMK PAN; Warsaw Univ; Univ Birmingham; Univ Genoa; RRCAT; Moscow MV Lomonosov State Univ; Univ West Scotland; Univ Western Australia; Radboud Univ Nijmegen; Univ Nice Sophia Antipolis; Observ Cote Azur; Eotvos Lorand Univ; Univ Rennes 1; Washington State Univ; Univ Urbino Carlo Bo; Embry Riddle Aeronaut Univ; Univ Oregon; ENS PSL Res Univ; Vrije Univ Amsterdam; Univ Maryland; Georgia Inst Technol; Univ Lyon; Univ Illes Balears; Univ Naples Federico II; NASA; Univ Toronto; Tsinghua Univ; Univ Michigan; Univ Roma Tor Vergata; Natl Tsing Hua Univ; Charles Sturt Univ; Pusan Natl Univ; Australian Natl Univ; Carleton Coll; Univ Roma La Sapienza; Univ Brussels; Texas Tech Univ; Univ Minnesota; Univ Melbourne; Univ Texas Brownsville; Univ Sheffield; RMKI; Montclair State Univ; Argentinian Gravitat Wave Grp; Univ Trento; Penn State Univ; Univ Chicago; Univ Cambridge; Univ Szeged; Inst Plasma Res; Amer Univ; Univ Massachusetts; Univ Adelaide; W Virginia Univ; Korea Inst Sci & Technol Informat; Univ Bialystok; Univ Strathclyde; IISER TVM; Northwestern Univ; Inst Appl Phys; Hanyang Univ; NCBJ; IM PAN; Monash Univ; Seoul Natl Univ; CNRS; Univ Camerino; Southern Univ; A&M Coll; Coll William & Mary; Universidade Estadual Paulista (Unesp); IISER Kolkata; Rutherford Appleton Lab; Whitman Coll; Natl Inst Math Sci; Rochester Inst Technol; Hobart & William Smith Coll; Inst Astron; Andrews Univ; Trinity Univ; Univ Padua; Univ Washington; Abilene Christian Univ (Amer Physical Soc, 2016-02-25)
In this paper we present the results of the first low frequency all-sky search of continuous gravitational wave signals conducted on Virgo VSR2 and VSR4 data. The search covered the full sky, a frequency range between 20 ...