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  1. Article ; Online: Photon-counting hexagonal pixel array CdTe detector: Spatial resolution characteristics for image-guided interventional applications.

    Vedantham, Srinivasan / Shrestha, Suman / Karellas, Andrew / Shi, Linxi / Gounis, Matthew J / Bellazzini, Ronaldo / Spandre, Gloria / Brez, Alessandro / Minuti, Massimo

    Medical physics

    2017  Volume 43, Issue 5, Page(s) 2118

    Abstract: Purpose: High-resolution, photon-counting, energy-resolved detector with fast-framing capability can facilitate simultaneous acquisition of precontrast and postcontrast images for subtraction angiography without pixel registration artifacts and can ... ...

    Abstract Purpose: High-resolution, photon-counting, energy-resolved detector with fast-framing capability can facilitate simultaneous acquisition of precontrast and postcontrast images for subtraction angiography without pixel registration artifacts and can facilitate high-resolution real-time imaging during image-guided interventions. Hence, this study was conducted to determine the spatial resolution characteristics of a hexagonal pixel array photon-counting cadmium telluride (CdTe) detector.
    Methods: A 650 μm thick CdTe Schottky photon-counting detector capable of concurrently acquiring up to two energy-windowed images was operated in a single energy-window mode to include photons of 10 keV or higher. The detector had hexagonal pixels with apothem of 30 μm resulting in pixel pitch of 60 and 51.96 μm along the two orthogonal directions. The detector was characterized at IEC-RQA5 spectral conditions. Linear response of the detector was determined over the air kerma rate relevant to image-guided interventional procedures ranging from 1.3 nGy/frame to 91.4 μGy/frame. Presampled modulation transfer was determined using a tungsten edge test device. The edge-spread function and the finely sampled line spread function accounted for hexagonal sampling, from which the presampled modulation transfer function (MTF) was determined. Since detectors with hexagonal pixels require resampling to square pixels for distortion-free display, the optimal square pixel size was determined by minimizing the root-mean-squared-error of the aperture functions for the square and hexagonal pixels up to the Nyquist limit.
    Results: At Nyquist frequencies of 8.33 and 9.62 cycles/mm along the apothem and orthogonal to the apothem directions, the modulation factors were 0.397 and 0.228, respectively. For the corresponding axis, the limiting resolution defined as 10% MTF occurred at 13.3 and 12 cycles/mm, respectively. Evaluation of the aperture functions yielded an optimal square pixel size of 54 μm. After resampling to 54 μm square pixels using trilinear interpolation, the presampled MTF at Nyquist frequency of 9.26 cycles/mm was 0.29 and 0.24 along the orthogonal directions and the limiting resolution (10% MTF) occurred at approximately 12 cycles/mm. Visual analysis of a bar pattern image showed the ability to resolve close to 12 line-pairs/mm and qualitative evaluation of a neurovascular nitinol-stent showed the ability to visualize its struts at clinically relevant conditions.
    Conclusions: Hexagonal pixel array photon-counting CdTe detector provides high spatial resolution in single-photon counting mode. After resampling to optimal square pixel size for distortion-free display, the spatial resolution is preserved. The dual-energy capabilities of the detector could allow for artifact-free subtraction angiography and basis material decomposition. The proposed high-resolution photon-counting detector with energy-resolving capability can be of importance for several image-guided interventional procedures as well as for pediatric applications.
    MeSH term(s) Alloys ; Angiography, Digital Subtraction/methods ; Blood Vessels/diagnostic imaging ; Cadmium Compounds ; Fingers/diagnostic imaging ; Humans ; Linear Models ; Models, Anatomic ; Phantoms, Imaging ; Photons ; Polymethyl Methacrylate ; Radiometry/instrumentation ; Radiometry/methods ; Stents ; Tellurium ; Therapy, Computer-Assisted/instrumentation ; Therapy, Computer-Assisted/methods ; Wrist/diagnostic imaging ; X-Rays
    Chemical Substances Alloys ; Cadmium Compounds ; nitinol (2EWL73IJ7F) ; Polymethyl Methacrylate (9011-14-7) ; Tellurium (NQA0O090ZJ) ; cadmium telluride (STG188WO13)
    Language English
    Publishing date 2017-04-18
    Publishing country United States
    Document type Journal Article
    ZDB-ID 188780-4
    ISSN 2473-4209 ; 0094-2405
    ISSN (online) 2473-4209
    ISSN 0094-2405
    DOI 10.1118/1.4944868
    Database MEDical Literature Analysis and Retrieval System OnLINE

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  2. Article ; Online: X-ray polarization evidence for a 200-year-old flare of Sgr A

    Marin, Frédéric / Churazov, Eugene / Khabibullin, Ildar / Ferrazzoli, Riccardo / Di Gesu, Laura / Barnouin, Thibault / Di Marco, Alessandro / Middei, Riccardo / Vikhlinin, Alexey / Costa, Enrico / Soffitta, Paolo / Muleri, Fabio / Sunyaev, Rashid / Forman, William / Kraft, Ralph / Bianchi, Stefano / Donnarumma, Immacolata / Petrucci, Pierre-Olivier / Enoto, Teruaki /
    Agudo, Iván / Antonelli, Lucio A / Bachetti, Matteo / Baldini, Luca / Baumgartner, Wayne H / Bellazzini, Ronaldo / Bongiorno, Stephen D / Bonino, Raffaella / Brez, Alessandro / Bucciantini, Niccolò / Capitanio, Fiamma / Castellano, Simone / Cavazzuti, Elisabetta / Chen, Chien-Ting / Ciprini, Stefano / De Rosa, Alessandra / Del Monte, Ettore / Di Lalla, Niccolò / Doroshenko, Victor / Dovčiak, Michal / Ehlert, Steven R / Evangelista, Yuri / Fabiani, Sergio / Garcia, Javier A / Gunji, Shuichi / Hayashida, Kiyoshi / Heyl, Jeremy / Ingram, Adam / Iwakiri, Wataru / Jorstad, Svetlana G / Kaaret, Philip / Karas, Vladimir / Kitaguchi, Takao / Kolodziejczak, Jeffery J / Krawczynski, Henric / La Monaca, Fabio / Latronico, Luca / Liodakis, Ioannis / Maldera, Simone / Manfreda, Alberto / Marinucci, Andrea / Marscher, Alan P / Marshall, Herman L / Massaro, Francesco / Matt, Giorgio / Mitsuishi, Ikuyuki / Mizuno, Tsunefumi / Negro, Michela / Ng, C-Y / O'Dell, Stephen L / Omodei, Nicola / Oppedisano, Chiara / Papitto, Alessandro / Pavlov, George G / Peirson, Abel L / Perri, Matteo / Pesce-Rollins, Melissa / Pilia, Maura / Possenti, Andrea / Poutanen, Juri / Puccetti, Simonetta / Ramsey, Brian D / Rankin, John / Ratheesh, Ajay / Roberts, Oliver J / Romani, Roger W / Sgrò, Carmelo / Slane, Patrick / Spandre, Gloria / Swartz, Doug / Tamagawa, Toru / Tavecchio, Fabrizio / Taverna, Roberto / Tawara, Yuzuru / Tennant, Allyn F / Thomas, Nicholas E / Tombesi, Francesco / Trois, Alessio / Tsygankov, Sergey S / Turolla, Roberto / Vink, Jacco / Weisskopf, Martin C / Wu, Kinwah / Xie, Fei / Zane, Silvia

    Nature

    2023  Volume 619, Issue 7968, Page(s) 41–45

    Abstract: The centre of the Milky Way Galaxy hosts a black hole with a solar mass of about 4 million (Sagittarius ... ...

    Abstract The centre of the Milky Way Galaxy hosts a black hole with a solar mass of about 4 million (Sagittarius A
    Language English
    Publishing date 2023-06-21
    Publishing country England
    Document type Journal Article
    ZDB-ID 120714-3
    ISSN 1476-4687 ; 0028-0836
    ISSN (online) 1476-4687
    ISSN 0028-0836
    DOI 10.1038/s41586-023-06064-x
    Database MEDical Literature Analysis and Retrieval System OnLINE

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  3. Article ; Online: Vela pulsar wind nebula X-rays are polarized to near the synchrotron limit.

    Xie, Fei / Di Marco, Alessandro / La Monaca, Fabio / Liu, Kuan / Muleri, Fabio / Bucciantini, Niccolò / Romani, Roger W / Costa, Enrico / Rankin, John / Soffitta, Paolo / Bachetti, Matteo / Di Lalla, Niccolò / Fabiani, Sergio / Ferrazzoli, Riccardo / Gunji, Shuichi / Latronico, Luca / Negro, Michela / Omodei, Nicola / Pilia, Maura /
    Trois, Alessio / Watanabe, Eri / Agudo, Iván / Antonelli, Lucio A / Baldini, Luca / Baumgartner, Wayne H / Bellazzini, Ronaldo / Bianchi, Stefano / Bongiorno, Stephen D / Bonino, Raffaella / Brez, Alessandro / Capitanio, Fiamma / Castellano, Simone / Cavazzuti, Elisabetta / Ciprini, Stefano / De Rosa, Alessandra / Del Monte, Ettore / Di Gesu, Laura / Donnarumma, Immacolata / Doroshenko, Victor / Dovčiak, Michal / Ehlert, Steven R / Enoto, Teruaki / Evangelista, Yuri / Garcia, Javier A / Hayashida, Kiyoshi / Heyl, Jeremy / Iwakiri, Wataru / Jorstad, Svetlana G / Karas, Vladimir / Kitaguchi, Takao / Kolodziejczak, Jeffery J / Krawczynski, Henric / Liodakis, Ioannis / Maldera, Simone / Manfreda, Alberto / Marin, Frédéric / Marinucci, Andrea / Marscher, Alan P / Marshall, Herman L / Massaro, Francesco / Matt, Giorgio / Mitsuishi, Ikuyuki / Mizuno, Tsunefumi / Ng, C-Y / O'Dell, Stephen L / Oppedisano, Chiara / Papitto, Alessandro / Pavlov, George G / Peirson, Abel L / Perri, Matteo / Pesce-Rollins, Melissa / Petrucci, Pierre-Olivier / Possenti, Andrea / Poutanen, Juri / Puccetti, Simonetta / Ramsey, Brian D / Ratheesh, Ajay / Sgró, Carmelo / Slane, Patrick / Spandre, Gloria / Tamagawa, Toru / Tavecchio, Fabrizio / Taverna, Roberto / Tawara, Yuzuru / Tennant, Allyn F / Thomas, Nicolas E / Tombesi, Francesco / Tsygankov, Sergey S / Turolla, Roberto / Vink, Jacco / Weisskopf, Martin C / Wu, Kinwah / Zane, Silvia

    Nature

    2022  Volume 612, Issue 7941, Page(s) 658–660

    Abstract: Pulsar wind nebulae are formed when outflows of relativistic electrons and positrons hit the surrounding supernova remnant or interstellar medium at a shock front. The Vela pulsar wind nebula is powered by a young pulsar (B0833-45, aged 11,000 years) ...

    Abstract Pulsar wind nebulae are formed when outflows of relativistic electrons and positrons hit the surrounding supernova remnant or interstellar medium at a shock front. The Vela pulsar wind nebula is powered by a young pulsar (B0833-45, aged 11,000 years)
    Language English
    Publishing date 2022-12-21
    Publishing country England
    Document type Journal Article ; Research Support, Non-U.S. Gov't ; Research Support, U.S. Gov't, Non-P.H.S.
    ZDB-ID 120714-3
    ISSN 1476-4687 ; 0028-0836
    ISSN (online) 1476-4687
    ISSN 0028-0836
    DOI 10.1038/s41586-022-05476-5
    Database MEDical Literature Analysis and Retrieval System OnLINE

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  4. Article ; Online: Polarized x-rays from a magnetar.

    Taverna, Roberto / Turolla, Roberto / Muleri, Fabio / Heyl, Jeremy / Zane, Silvia / Baldini, Luca / González-Caniulef, Denis / Bachetti, Matteo / Rankin, John / Caiazzo, Ilaria / Di Lalla, Niccolò / Doroshenko, Victor / Errando, Manel / Gau, Ephraim / Kırmızıbayrak, Demet / Krawczynski, Henric / Negro, Michela / Ng, Mason / Omodei, Nicola /
    Possenti, Andrea / Tamagawa, Toru / Uchiyama, Keisuke / Weisskopf, Martin C / Agudo, Ivan / Antonelli, Lucio A / Baumgartner, Wayne H / Bellazzini, Ronaldo / Bianchi, Stefano / Bongiorno, Stephen D / Bonino, Raffaella / Brez, Alessandro / Bucciantini, Niccolò / Capitanio, Fiamma / Castellano, Simone / Cavazzuti, Elisabetta / Ciprini, Stefano / Costa, Enrico / De Rosa, Alessandra / Del Monte, Ettore / Di Gesu, Laura / Di Marco, Alessandro / Donnarumma, Immacolata / Dovčiak, Michal / Ehlert, Steven R / Enoto, Teruaki / Evangelista, Yuri / Fabiani, Sergio / Ferrazzoli, Riccardo / Garcia, Javier A / Gunji, Shuichi / Hayashida, Kiyoshi / Iwakiri, Wataru / Jorstad, Svetlana G / Karas, Vladimir / Kitaguchi, Takao / Kolodziejczak, Jeffery J / La Monaca, Fabio / Latronico, Luca / Liodakis, Ioannis / Maldera, Simone / Manfreda, Alberto / Marin, Frédéric / Marinucci, Andrea / Marscher, Alan P / Marshall, Herman L / Matt, Giorgio / Mitsuishi, Ikuyuki / Mizuno, Tsunefumi / Ng, Stephen C-Y / O'Dell, Stephen L / Oppedisano, Chiara / Papitto, Alessandro / Pavlov, George G / Peirson, Abel L / Perri, Matteo / Pesce-Rollins, Melissa / Pilia, Maura / Poutanen, Juri / Puccetti, Simonetta / Ramsey, Brian D / Ratheesh, Ajay / Romani, Roger W / Sgrò, Carmelo / Slane, Patrick / Soffitta, Paolo / Spandre, Gloria / Tavecchio, Fabrizio / Tawara, Yuzuru / Tennant, Allyn F / Thomas, Nicholas E / Tombesi, Francesco / Trois, Alessio / Tsygankov, Sergey S / Vink, Jacco / Wu, Kinwah / Xie, Fei

    Science (New York, N.Y.)

    2022  Volume 378, Issue 6620, Page(s) 646–650

    Abstract: Magnetars are neutron stars with ultrastrong magnetic fields, which can be observed in x-rays. Polarization measurements could provide information on their magnetic fields and surface properties. We observed polarized x-rays from the magnetar 4U 0142+61 ... ...

    Abstract Magnetars are neutron stars with ultrastrong magnetic fields, which can be observed in x-rays. Polarization measurements could provide information on their magnetic fields and surface properties. We observed polarized x-rays from the magnetar 4U 0142+61 using the Imaging X-ray Polarimetry Explorer and found a linear polarization degree of 13.5 ± 0.8% averaged over the 2- to 8-kilo-electron volt band. The polarization changes with energy: The degree is 15.0 ± 1.0% at 2 to 4 kilo-electron volts, drops below the instrumental sensitivity ~4 to 5 kilo-electron volts, and rises to 35.2 ± 7.1% at 5.5 to 8 kilo-electron volts. The polarization angle also changes by 90° at ~4 to 5 kilo-electron volts. These results are consistent with a model in which thermal radiation from the magnetar surface is reprocessed by scattering off charged particles in the magnetosphere.
    Language English
    Publishing date 2022-11-03
    Publishing country United States
    Document type Journal Article ; Research Support, Non-U.S. Gov't ; Research Support, U.S. Gov't, Non-P.H.S.
    ZDB-ID 128410-1
    ISSN 1095-9203 ; 0036-8075
    ISSN (online) 1095-9203
    ISSN 0036-8075
    DOI 10.1126/science.add0080
    Database MEDical Literature Analysis and Retrieval System OnLINE

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  5. Article ; Online: Polarized blazar X-rays imply particle acceleration in shocks.

    Liodakis, Ioannis / Marscher, Alan P / Agudo, Iván / Berdyugin, Andrei V / Bernardos, Maria I / Bonnoli, Giacomo / Borman, George A / Casadio, Carolina / Casanova, Vı Ctor / Cavazzuti, Elisabetta / Rodriguez Cavero, Nicole / Di Gesu, Laura / Di Lalla, Niccoló / Donnarumma, Immacolata / Ehlert, Steven R / Errando, Manel / Escudero, Juan / Garcı A-Comas, Maya / Agı S-González, Beatriz /
    Husillos, César / Jormanainen, Jenni / Jorstad, Svetlana G / Kagitani, Masato / Kopatskaya, Evgenia N / Kravtsov, Vadim / Krawczynski, Henric / Lindfors, Elina / Larionova, Elena G / Madejski, Grzegorz M / Marin, Frédéric / Marchini, Alessandro / Marshall, Herman L / Morozova, Daria A / Massaro, Francesco / Masiero, Joseph R / Mawet, Dimitri / Middei, Riccardo / Millar-Blanchaer, Maxwell A / Myserlis, Ioannis / Negro, Michela / Nilsson, Kari / O'Dell, Stephen L / Omodei, Nicola / Pacciani, Luigi / Paggi, Alessandro / Panopoulou, Georgia V / Peirson, Abel L / Perri, Matteo / Petrucci, Pierre-Olivier / Poutanen, Juri / Puccetti, Simonetta / Romani, Roger W / Sakanoi, Takeshi / Savchenko, Sergey S / Sota, Alfredo / Tavecchio, Fabrizio / Tinyanont, Samaporn / Vasilyev, Andrey A / Weaver, Zachary R / Zhovtan, Alexey V / Antonelli, Lucio A / Bachetti, Matteo / Baldini, Luca / Baumgartner, Wayne H / Bellazzini, Ronaldo / Bianchi, Stefano / Bongiorno, Stephen D / Bonino, Raffaella / Brez, Alessandro / Bucciantini, Niccoló / Capitanio, Fiamma / Castellano, Simone / Ciprini, Stefano / Costa, Enrico / De Rosa, Alessandra / Del Monte, Ettore / Di Marco, Alessandro / Doroshenko, Victor / Dovčiak, Michal / Enoto, Teruaki / Evangelista, Yuri / Fabiani, Sergio / Ferrazzoli, Riccardo / Garcia, Javier A / Gunji, Shuichi / Hayashida, Kiyoshi / Heyl, Jeremy / Iwakiri, Wataru / Karas, Vladimir / Kitaguchi, Takao / Kolodziejczak, Jeffery J / La Monaca, Fabio / Latronico, Luca / Maldera, Simone / Manfreda, Alberto / Marinucci, Andrea / Matt, Giorgio / Mitsuishi, Ikuyuki / Mizuno, Tsunefumi / Muleri, Fabio / Ng, Stephen C-Y / Oppedisano, Chiara / Papitto, Alessandro / Pavlov, George G / Pesce-Rollins, Melissa / Pilia, Maura / Possenti, Andrea / Ramsey, Brian D / Rankin, John / Ratheesh, Ajay / Sgró, Carmelo / Slane, Patrick / Soffitta, Paolo / Spandre, Gloria / Tamagawa, Toru / Taverna, Roberto / Tawara, Yuzuru / Tennant, Allyn F / Thomas, Nicolas E / Tombesi, Francesco / Trois, Alessio / Tsygankov, Sergey / Turolla, Roberto / Vink, Jacco / Weisskopf, Martin C / Wu, Kinwah / Xie, Fei / Zane, Silvia

    Nature

    2022  Volume 611, Issue 7937, Page(s) 677–681

    Abstract: Most of the light from blazars, active galactic nuclei with jets of magnetized plasma that point nearly along the line of sight, is produced by high-energy particles, up to around 1 TeV. Although the jets are known to be ultimately powered by a ... ...

    Abstract Most of the light from blazars, active galactic nuclei with jets of magnetized plasma that point nearly along the line of sight, is produced by high-energy particles, up to around 1 TeV. Although the jets are known to be ultimately powered by a supermassive black hole, how the particles are accelerated to such high energies has been an unanswered question. The process must be related to the magnetic field, which can be probed by observations of the polarization of light from the jets. Measurements of the radio to optical polarization-the only range available until now-probe extended regions of the jet containing particles that left the acceleration site days to years earlier
    Language English
    Publishing date 2022-11-23
    Publishing country England
    Document type Journal Article
    ZDB-ID 120714-3
    ISSN 1476-4687 ; 0028-0836
    ISSN (online) 1476-4687
    ISSN 0028-0836
    DOI 10.1038/s41586-022-05338-0
    Database MEDical Literature Analysis and Retrieval System OnLINE

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  6. Article ; Online: Polarized x-rays constrain the disk-jet geometry in the black hole x-ray binary Cygnus X-1.

    Krawczynski, Henric / Muleri, Fabio / Dovčiak, Michal / Veledina, Alexandra / Rodriguez Cavero, Nicole / Svoboda, Jiri / Ingram, Adam / Matt, Giorgio / Garcia, Javier A / Loktev, Vladislav / Negro, Michela / Poutanen, Juri / Kitaguchi, Takao / Podgorný, Jakub / Rankin, John / Zhang, Wenda / Berdyugin, Andrei / Berdyugina, Svetlana V / Bianchi, Stefano /
    Blinov, Dmitry / Capitanio, Fiamma / Di Lalla, Niccolò / Draghis, Paul / Fabiani, Sergio / Kagitani, Masato / Kravtsov, Vadim / Kiehlmann, Sebastian / Latronico, Luca / Lutovinov, Alexander A / Mandarakas, Nikos / Marin, Frédéric / Marinucci, Andrea / Miller, Jon M / Mizuno, Tsunefumi / Molkov, Sergey V / Omodei, Nicola / Petrucci, Pierre-Olivier / Ratheesh, Ajay / Sakanoi, Takeshi / Semena, Andrei N / Skalidis, Raphael / Soffitta, Paolo / Tennant, Allyn F / Thalhammer, Phillipp / Tombesi, Francesco / Weisskopf, Martin C / Wilms, Joern / Zhang, Sixuan / Agudo, Iván / Antonelli, Lucio A / Bachetti, Matteo / Baldini, Luca / Baumgartner, Wayne H / Bellazzini, Ronaldo / Bongiorno, Stephen D / Bonino, Raffaella / Brez, Alessandro / Bucciantini, Niccolò / Castellano, Simone / Cavazzuti, Elisabetta / Ciprini, Stefano / Costa, Enrico / De Rosa, Alessandra / Del Monte, Ettore / Di Gesu, Laura / Di Marco, Alessandro / Donnarumma, Immacolata / Doroshenko, Victor / Ehlert, Steven R / Enoto, Teruaki / Evangelista, Yuri / Ferrazzoli, Riccardo / Gunji, Shuichi / Hayashida, Kiyoshi / Heyl, Jeremy / Iwakiri, Wataru / Jorstad, Svetlana G / Karas, Vladimir / Kolodziejczak, Jeffery J / La Monaca, Fabio / Liodakis, Ioannis / Maldera, Simone / Manfreda, Alberto / Marscher, Alan P / Marshall, Herman L / Mitsuishi, Ikuyuki / Ng, Chi-Yung / O'Dell, Stephen L / Oppedisano, Chiara / Papitto, Alessandro / Pavlov, George G / Peirson, Abel L / Perri, Matteo / Pesce-Rollins, Melissa / Pilia, Maura / Possenti, Andrea / Puccetti, Simonetta / Ramsey, Brian D / Romani, Roger W / Sgrò, Carmelo / Slane, Patrick / Spandre, Gloria / Tamagawa, Toru / Tavecchio, Fabrizio / Taverna, Roberto / Tawara, Yuzuru / Thomas, Nicholas E / Trois, Alessio / Tsygankov, Sergey / Turolla, Roberto / Vink, Jacco / Wu, Kinwah / Xie, Fei / Zane, Silvia

    Science (New York, N.Y.)

    2022  Volume 378, Issue 6620, Page(s) 650–654

    Abstract: A black hole x-ray binary (XRB) system forms when gas is stripped from a normal star and accretes onto a black hole, which heats the gas sufficiently to emit x-rays. We report a polarimetric observation of the XRB Cygnus X-1 using the Imaging X-ray ... ...

    Abstract A black hole x-ray binary (XRB) system forms when gas is stripped from a normal star and accretes onto a black hole, which heats the gas sufficiently to emit x-rays. We report a polarimetric observation of the XRB Cygnus X-1 using the Imaging X-ray Polarimetry Explorer. The electric field position angle aligns with the outflowing jet, indicating that the jet is launched from the inner x-ray-emitting region. The polarization degree is 4.01 ± 0.20% at 2 to 8 kiloelectronvolts, implying that the accretion disk is viewed closer to edge-on than the binary orbit. These observations reveal that hot x-ray-emitting plasma is spatially extended in a plane perpendicular to, not parallel to, the jet axis.
    Language English
    Publishing date 2022-11-03
    Publishing country United States
    Document type Journal Article ; Research Support, U.S. Gov't, Non-P.H.S.
    ZDB-ID 128410-1
    ISSN 1095-9203 ; 0036-8075
    ISSN (online) 1095-9203
    ISSN 0036-8075
    DOI 10.1126/science.add5399
    Database MEDical Literature Analysis and Retrieval System OnLINE

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  7. Article ; Online: Einstein@Home discovers a radio-quiet gamma-ray millisecond pulsar.

    Clark, Colin J / Pletsch, Holger J / Wu, Jason / Guillemot, Lucas / Kerr, Matthew / Johnson, Tyrel J / Camilo, Fernando / Salvetti, David / Allen, Bruce / Anderson, David / Aulbert, Carsten / Beer, Christian / Bock, Oliver / Cuéllar, Andres / Eggenstein, Heinz-Bernd / Fehrmann, Henning / Kramer, Michael / Kwang, Shawn A / Machenschalk, Bernd /
    Nieder, Lars / Ackermann, Markus / Ajello, Marco / Baldini, Luca / Ballet, Jean / Barbiellini, Guido / Bastieri, Denis / Bellazzini, Ronaldo / Bissaldi, Elisabetta / Blandford, Roger D / Bloom, Elliott D / Bonino, Raffaella / Bottacini, Eugenio / Brandt, Terri J / Bregeon, Johan / Bruel, Philippe / Buehler, Rolf / Burnett, Toby H / Buson, Sara / Cameron, Rob A / Caputo, Regina / Caraveo, Patrizia A / Cavazzuti, Elisabetta / Cecchi, Claudia / Charles, Eric / Chekhtman, Alexandre / Ciprini, Stefano / Cominsky, Lynn R / Costantin, Denise / Cutini, Sara / D'Ammando, Filippo / De Luca, Andrea / Desiante, Rachele / Di Venere, Leonardo / Di Mauro, Mattia / Di Lalla, Niccolò / Digel, Seth W / Favuzzi, Cecilia / Ferrara, Elizabeth C / Franckowiak, Anna / Fukazawa, Yasushi / Funk, Stefan / Fusco, Piergiorgio / Gargano, Fabio / Gasparrini, Dario / Giglietto, Nico / Giordano, Francesco / Giroletti, Marcello / Gomez-Vargas, Germán A / Green, David / Grenier, Isabelle A / Guiriec, Sylvain / Harding, Alice K / Hewitt, John W / Horan, Deirdre / Jóhannesson, Guðlaugur / Kensei, Shiki / Kuss, Michael / La Mura, Giovanni / Larsson, Stefan / Latronico, Luca / Li, Jian / Longo, Francesco / Loparco, Francesco / Lovellette, Michael N / Lubrano, Pasquale / Magill, Jeffrey D / Maldera, Simone / Manfreda, Alberto / Mazziotta, Mario N / McEnery, Julie E / Michelson, Peter F / Mirabal, Nestor / Mitthumsiri, Warit / Mizuno, Tsunefumi / Monzani, Maria Elena / Morselli, Aldo / Moskalenko, Igor V / Nuss, Eric / Ohsugi, Takashi / Omodei, Nicola / Orienti, Monica / Orlando, Elena / Palatiello, Michele / Paliya, Vaidehi S / de Palma, Francesco / Paneque, David / Perkins, Jeremy S / Persic, Massimo / Pesce-Rollins, Melissa / Porter, Troy A / Principe, Giacomo / Rainò, Silvia / Rando, Riccardo / Ray, Paul S / Razzano, Massimiliano / Reimer, Anita / Reimer, Olaf / Romani, Roger W / Saz Parkinson, Pablo M / Sgrò, Carmelo / Siskind, Eric J / Smith, David A / Spada, Francesca / Spandre, Gloria / Spinelli, Paolo / Thayer, Jana B / Thompson, David J / Torres, Diego F / Troja, Eleonora / Vianello, Giacomo / Wood, Kent / Wood, Matthew

    Science advances

    2018  Volume 4, Issue 2, Page(s) eaao7228

    Abstract: Millisecond pulsars (MSPs) are old neutron stars that spin hundreds of times per second and appear to pulsate as their emission beams cross our line of sight. To date, radio pulsations have been detected from all rotation-powered MSPs. In an attempt to ... ...

    Abstract Millisecond pulsars (MSPs) are old neutron stars that spin hundreds of times per second and appear to pulsate as their emission beams cross our line of sight. To date, radio pulsations have been detected from all rotation-powered MSPs. In an attempt to discover radio-quiet gamma-ray MSPs, we used the aggregated power from the computers of tens of thousands of volunteers participating in the Einstein@Home distributed computing project to search for pulsations from unidentified gamma-ray sources in Fermi Large Area Telescope data. This survey discovered two isolated MSPs, one of which is the only known rotation-powered MSP to remain undetected in radio observations. These gamma-ray MSPs were discovered in completely blind searches without prior constraints from other observations, raising hopes for detecting MSPs from a predicted Galactic bulge population.
    Language English
    Publishing date 2018-02
    Publishing country United States
    Document type Journal Article
    ZDB-ID 2810933-8
    ISSN 2375-2548 ; 2375-2548
    ISSN (online) 2375-2548
    ISSN 2375-2548
    DOI 10.1126/sciadv.aao7228
    Database MEDical Literature Analysis and Retrieval System OnLINE

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