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by Scholten, Olaf and van den Berg, Aiaan and Las Cumbres Observatory Grp and ATCA Australia Telescope and LIGO Sci Collaboration & Virgo and KU Collaboration and GROUND and RIMAS RATIR and AGILE Team and ASKAP Australian SKA Pathfinder and IPN Collaboration and LOFAR Collaboration and Salt Grp and VINROUGE Collaboration and Nordic Optical Telescope and MAXI Team and Fermi GBM and Fermi Large Area Telescope and J-GEM and IceCube Collaboration and BOOTES Collaboration and Pi Sky Collaboration and Pan-STARRS and LWA Long Wavelength Array and SKA South Africa MeerKAT and CALET Collaboration and AstroSat Cadmium Zinc Telluride and HAWC Collaboration and GROWTH JAGWAR CALTECH and ATLAS and ePESSTO and DFN Desert Fireball Network and Insight-Hxmt Collaboration and Texas Tech Univ and MASTER Collaboration and TZAC Consortium and Dark Energy Camera GW-EM and GRAWITA GRAvitational Wave and INTERGRAL and Toros Transient Robotic Observat and Chandra Team McGill Univ and H E S S Collaboration and Swift Collaboration and Pierre Auger Collaboration and OzGrav DWF Deeper Wider Faster and IKI-GW Follow-up Collaboration and Euro VLBI Team and High Time Resolution Universe and ANTARES Collaboration and DLT40 Collaboration and ALMA Collaboration and The 1M2H Team and MWA Murchison Widefield Array and The Insight-HXMT Collaboration and The MAXI Team and The Swift Collaboration and The Fermi Large Area Telescope Collaboration and GROND and TOROS: Transient Robotic Observatory of the South Collaboration and Texas Tech University and OzGrav, DWF (Deeper, Wider, Faster program), AST3, and CAASTRO Collaborations and MWA: Murchison Widefield Array and GROWTH, JAGWAR, Caltech-NRAO, TTU-NRAO, and NuSTAR Collaborations and INTEGRAL and RIMAS and RATIR and Pi of the Sky Collaboration and The Chandra Team at McGill University and LWA: Long Wavelength Array and The DLT40 Collaboration and DFN: Desert Fireball Network and LIGO Scientific Collaboration and Virgo Collaboration and ASKAP: Australian SKA Pathfinder and AstroSat Cadmium Zinc Telluride Imager Team and The BOOTES Collaboration and The Pierre Auger Collaboration and ATCA: Australia Telescope Compact Array and SALT Group and H.E.S.S. Collaboration and The Dark Energy Camera GW-EM Collaboration and the DES Collaboration and High Time Resolution Universe Survey and Las Cumbres Observatory Group and GRAWITA: GRAvitational Wave Inaf TeAm and The VINROUGE Collaboration and The CALET Collaboration and SLAC National Accelerator Lab., Menlo Park, CA (United States) and Brookhaven National Lab. (BNL), Upton, NY (United States) and Los Alamos National Lab. (LANL), Los Alamos, NM (United States) and Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States) and Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States) and Lawrence Berkeley National Laboratory-National Energy Research Scientific Computing Center (NERSC) and Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States) and Fysikum and Naturvetenskapliga fakulteten and Institutionen för astronomi and Stockholms universitet and Oskar Klein-centrum för kosmopartikelfysik (OKC)
Astrophysical Journal Letters, ISSN 2041-8205, 10/2017, Volume 848, Issue 2, p. L12
Journal Article
by Abbott, B. P and Abbott, R and Abbott, T. D and Acernese, F and Ackley, K and Adams, C and Adams, T and Addesso, P and Adhikari, R. X and Adya, V. B and Affeldt, C and Afrough, M and Agarwal, B and Agathos, M and Agatsuma, K and Aggarwal, N and Aguiar, O. D and Aiello, L and Ain, A and Ajith, P and Allen, B and Allen, G and Allocca, A and Altin, P. A and Amato, A and Ananyeva, A and Anderson, S. B and Anderson, W. G and Angelova, S. V and Antier, S and Appert, S and Arai, K and Araya, M. C and Areeda, J. S and Arnaud, N and Arun, K. G and Ascenzi, S and Ashton, G and Ast, M and Aston, S. M and Astone, P and Atallah, D. V and Aufmuth, P and Aulbert, C and AultONeal, K and Austin, C and Avila-Alvarez, A and Babak, S and Bacon, P and Bader, M. K. M and Bae, S and Baker, P. T and Baldaccini, F and Ballardin, G and Ballmer, S. W and Banagiri, S and Barayoga, J. C and Barclay, S. E and Barish, B. C and Barker, D and Barkett, K and Barone, F and Barr, B and Barsotti, L and Barsuglia, M and Barta, D and Barthelmy, S. D and Bartlett, J and Bartos, I and Bassiri, R and Basti, A and Batch, J. C and Bawaj, M and Bayley, J. C and Bazzan, M and Bécsy, B and Beer, C and Bejger, M and Belahcene, I and Bell, A. S and Berger, B. K and Bergmann, G and Bero, J. J and Berry, C. P. L and Bersanetti, D and Bertolini, A and Betzwieser, J and Bhagwat, S and Bhandare, R and Bilenko, I. A and Billingsley, G and Billman, C. R and Birch, J and Birney, R and Birnholtz, O and Biscans, S and Biscoveanu, S and Bisht, A and Bitossi, M and Biwer, C and ... and Institutionen för fysik och astronomi and Teknisk-naturvetenskapliga vetenskapsområdet and Högenergifysik and Uppsala universitet and Fysiska sektionen
Astrophysical Journal Letters, ISSN 1538-4357, 2017, Volume 848, Issue 2
Journal Article
The archetypical very-high-energy gamma-ray blazar Mrk 421 was monitored for more than 3 years with the Gas Slit Camera onboard Monitor of All Sky X-ray Image... 
Physics - High Energy Astrophysical Phenomena
Journal Article
We present the light curve data of a remarkable blazer 3C 454.3 (z=0.859) in optical, X-ray, and gamma-ray bands. Since January 2008, we have been monitoring... 
Physics - High Energy Astrophysical Phenomena
Journal Article
Astrophysical Journal Supplement Series, ISSN 0067-0049, 2016, Volume 225, Issue 1, pp. 1 - 8
This Supplement provides supporting material for Abbott et al. (2016a). We briefly summarize past electromagnetic (EM) follow-up efforts as well as the... 
Journal Article
Astrophysical Journal Letters, ISSN 2041-8205, 07/2016, Volume 826, Issue 1
A gravitational-wave (GW) transient was identified in data recorded by the Advanced Laser Interferometer Gravitational-wave Observatory (LIGO) detectors on... 
Journal Article
Journal Article
AIP Conference Proceedings, ISSN 0094-243X, 2012, Volume 1427, pp. 294 - 295
Using unbiased observations of MAXI/GSC the potential contribution of stellar flares and CVs to GRXE luminosity is estimated in the energy range of 2 - 10 keV.... 
Thermal spectrum | Stellar flares | Diffuse X-ray emission | Galactic ridge | Physics - High Energy Astrophysical Phenomena
Conference Proceeding
日本物理学会講演概要集, ISSN 2189-079X, 03/2015, Volume 70
Journal Article
日本物理学会講演概要集, ISSN 1342-8349, 08/2014, Volume 69
Journal Article
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