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Book ; Online: Validating Monte Carlo simulations for an analysis chain in H.E.S.S

Leuschner, Fabian / Schäfer, Johannes / Steinmassl, Simon / Holch, Tim Lukas / Bernlöhr, Konrad / Funk, Stefan / Hinton, Jim / Ohm, Stefan / Pühlhofer, Gerd

2023

Abstract: Imaging Air Cherenkov Telescopes (IACTs) detect very high energetic (VHE) gamma rays. They observe the Cherenkov light emitted in electromagnetic shower cascades that gamma rays induce in the atmosphere. A precise reconstruction of the primary photon ... ...

Abstract	Imaging Air Cherenkov Telescopes (IACTs) detect very high energetic (VHE) gamma rays. They observe the Cherenkov light emitted in electromagnetic shower cascades that gamma rays induce in the atmosphere. A precise reconstruction of the primary photon energy and the source flux depends heavily on accurate Monte Carlo (MC) simulations of the shower propagation and the detector response, and therefore also on adequate assumptions about the atmosphere at the site and time of a measurement. Here, we present the results of an extensive validation of the MC simulations for an analysis chain of the H.E.S.S. experiment with special focus on the recently installed FlashCam camera on the large 28 m telescope. One goal of this work was to create a flexible and easy-to-use framework to facilitate the detailed validation of MC simulations also for past and future phases of the H.E.S.S. experiment. Guided by the underlying physics, the detector simulation and the atmospheric transmission profiles were gradually improved until low level parameters such as cosmic ray (CR) trigger rates matched within a few percent between simulations and observational data. This led to instrument response functions (IRFs) with which the analysis of current H.E.S.S. data can ultimately be carried out within percent accuracy, substantially improving earlier simulations. Comment: 8 pages, 4 figures, 1 table. Accepted as Proceeding of the 7th Heidelberg International Symposium on High-Energy Gamma-Ray Astronomy (Gamma2022)
Keywords	Astrophysics - Instrumentation and Methods for Astrophysics ; Astrophysics - High Energy Astrophysical Phenomena
Subject code	612
Publishing date	2023-03-01
Publishing country	us
Document type	Book ; Online
Database	BASE - Bielefeld Academic Search Engine (life sciences selection)

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Book: Abschlussbericht an den DLR-PT zum Vorhaben "Röntgenmorphologie von neu entdeckten Gammaquellen mit XMM - Charakterisierung der hochenergetischen Teilchenpopulationen in neu identifizierten, potentiellen Beschleunigern der kosmischen Strahlung"

Pühlhofer, Gerd

Bewilligungszeitraum: 01.07.2005 - 31.12.2008

2009

Title variant	Röntgenmorphologie von neu entdeckten Gammaquellen mit XMM - Charakterisierung der hochenergetischen Teilchenpopulationen in neu identifizierten, potentiellen Beschleunigern der kosmischen Strahlung ; X-ray morphology of newly discovered gamma-ray sources with XMM - characterising the high energy particle population in newly identified, potential cosmic ray accelerators
Author's details	[Autoren des Berichts/]Projektleiter: Gerd Pühlhofer
Language	German
Size	23 S., Ill., graph. Darst.
Publisher	Univ
Publishing place	Heidelberg
Document type	Book
Note	Auch als elektronische Ressource vorh. ; Förderkennzeichen BMWi 50 OR 0502. - Engl. Zsfassung u.d.T.: X-ray morphology of newly discovered gamma-ray sources with XMM - characterising the high energy particle population in newly identified, potential cosmic ray accelerators ; Unterschiede zwischen dem gedruckten Dokument und der elektronischen Ressource können nicht ausgeschlossen werden
Database	Library catalogue of the German National Library of Science and Technology (TIB), Hannover

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Article ; Online: Acceleration and transport of relativistic electrons in the jets of the microquasar SS 433.

Aharonian, F / Benkhali, F Ait / Aschersleben, J / Ashkar, H / Backes, M / Martins, V Barbosa / Batzofin, R / Becherini, Y / Berge, D / Bernlöhr, K / Bi, B / Böttcher, M / Boisson, C / Bolmont, J / de Lavergne, M de Bony / Borowska, J / Bouyahiaoui, M / Breuhaus, M / Brose, R /

Brown, A M / Brun, F / Bruno, B / Bulik, T / Burger-Scheidlin, C / Caroff, S / Casanova, S / Cecil, R / Celic, J / Cerruti, M / Chand, T / Chandra, S / Chen, A / Chibueze, J / Chibueze, O / Cotter, G / Dai, S / Mbarubucyeye, J Damascene / Djannati-Ataï, A / Dmytriiev, A / Doroshenko, V / Egberts, K / Einecke, S / Ernenwein, J-P / Filipovic, M / Fontaine, G / Füßling, M / Funk, S / Gabici, S / Ghafourizadeh, S / Giavitto, G / Glawion, D / Glicenstein, J-F / Grolleron, G / Haerer, L / Hinton, J A / Hofmann, W / Holch, T L / Holler, M / Horns, D / Jamrozy, M / Jankowsky, F / Jardin-Blicq, A / Joshi, V / Jung-Richardt, I / Kasai, E / Katarzyński, K / Khatoon, R / Khélifi, B / Klepser, S / Kluźniak, W / Komin, Nu / Kosack, K / Kostunin, D / Kundu, A / Lang, R G / Le Stum, S / Leitl, F / Lemière, A / Lenain, J-P / Leuschner, F / Lohse, T / Luashvili, A / Lypova, I / Mackey, J / Malyshev, D / Marandon, V / Marchegiani, P / Marcowith, A / Martí-Devesa, G / Marx, R / Mehta, A / Mitchell, A / Moderski, R / Mohrmann, L / Montanari, A / Moulin, E / Murach, T / Nakashima, K / de Naurois, M / Niemiec, J / Noel, A Priyana / Ohm, S / Olivera-Nieto, L / de Ona Wilhelmi, E / Ostrowski, M / Panny, S / Panter, M / Parsons, R D / Peron, G / Prokhorov, D A / Pühlhofer, G / Punch, M / Quirrenbach, A / Reichherzer, P / Reimer, A / Reimer, O / Ren, H / Renaud, M / Reville, B / Rieger, F / Rowell, G / Rudak, B / Ricarte, H Rueda / Ruiz-Velasco, E / Sahakian, V / Salzmann, H / Santangelo, A / Sasaki, M / Schäfer, J / Schüssler, F / Schwanke, U / Shapopi, J N S / Sol, H / Specovius, A / Spencer, S / Stawarz, L / Steenkamp, R / Steinmassl, S / Steppa, C / Streil, K / Sushch, I / Suzuki, H / Takahashi, T / Tanaka, T / Taylor, A M / Terrier, R / Tsirou, M / Tsuji, N / Unbehaun, T / van Eldik, C / Vecchi, M / Veh, J / Venter, C / Vink, J / Wach, T / Wagner, S J / Werner, F / White, R / Wierzcholska, A / Wong, Yu Wun / Zacharias, M / Zargaryan, D / Zdziarski, A A / Zech, A / Zouari, S / Żywucka, N

Science (New York, N.Y.)

2024 Volume 383, Issue 6681, Page(s) 402–406

Abstract: SS 433 is a microquasar, a stellar binary system that launches collimated relativistic jets. We observed SS 433 in gamma rays using the High Energy Stereoscopic System (H.E.S.S.) and found an energy-dependent shift in the apparent position of the gamma- ... ...

Abstract	SS 433 is a microquasar, a stellar binary system that launches collimated relativistic jets. We observed SS 433 in gamma rays using the High Energy Stereoscopic System (H.E.S.S.) and found an energy-dependent shift in the apparent position of the gamma-ray emission from the parsec-scale jets. These observations trace the energetic electron population and indicate that inverse Compton scattering is the emission mechanism of the gamma rays. Our modeling of the energy-dependent gamma-ray morphology constrains the location of particle acceleration and requires an abrupt deceleration of the jet flow. We infer the presence of shocks on either side of the binary system, at distances of 25 to 30 parsecs, and that self-collimation of the precessing jets forms the shocks, which then efficiently accelerate electrons.
Language	English
Publishing date	2024-01-25
Publishing country	United States
Document type	Journal Article
ZDB-ID	128410-1
ISSN	1095-9203 ; 0036-8075
ISSN (online)	1095-9203
ISSN	0036-8075
DOI	10.1126/science.adi2048
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Zs.MG 77: Show issues

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Article ; Online: Search for Dark Matter Annihilation Signals in the H.E.S.S. Inner Galaxy Survey.

Abdalla, H / Aharonian, F / Benkhali, F Ait / Angüner, E O / Armand, C / Ashkar, H / Backes, M / Baghmanyan, V / Martins, V Barbosa / Batzofin, R / Becherini, Y / Berge, D / Bernlöhr, K / Bi, B / Böttcher, M / Bolmont, J / de Lavergne, M de Bony / Brose, R / Brun, F /

Cangemi, F / Caroff, S / Cerruti, M / Chand, T / Chen, A / Cotter, G / Mbarubucyeye, J Damascene / Devin, J / Djannati-Ataï, A / Dmytriiev, A / Doroshenko, V / Egberts, K / Fiasson, A / de Clairfontaine, G Fichet / Fontaine, G / Funk, S / Gabici, S / Giavitto, G / Glawion, D / Glicenstein, J F / Grondin, M-H / Hinton, J A / Hofmann, W / Holch, T L / Holler, M / Horns, D / Huang, Zhiqiu / Jamrozy, M / Jankowsky, F / Kasai, E / Katarzyński, K / Katz, U / Khélifi, B / Kluźniak, W / Komin, Nu / Kosack, K / Kostunin, D / Lamanna, G / Lemoine-Goumard, M / Lenain, J-P / Leuschner, F / Lohse, T / Luashvili, A / Lypova, I / Mackey, J / Malyshev, D / Marandon, V / Marchegiani, P / Martí-Devesa, G / Marx, R / Maurin, G / Meyer, M / Mitchell, A / Moderski, R / Montanari, A / Moulin, E / Muller, J / de Naurois, M / Niemiec, J / Noel, A Priyana / Ohm, S / Olivera-Nieto, L / Wilhelmi, E de Ona / Ostrowski, M / Panny, S / Panter, M / Parsons, R D / Peron, G / Poireau, V / Prokoph, H / Pühlhofer, G / Punch, M / Quirrenbach, A / Reichherzer, P / Reimer, A / Reimer, O / Renaud, M / Rieger, F / Rowell, G / Rudak, B / Ricarte, H Rueda / Ruiz-Velasco, E / Sahakian, V / Salzmann, H / Santangelo, A / Sasaki, M / Schüssler, F / Schutte, H M / Schwanke, U / Senniappan, M / Shapopi, J N S / Sol, H / Specovius, A / Spencer, S / Stawarz, Ł / Stegmann, C / Steinmassl, S / Steppa, C / Takahashi, T / Tanaka, T / Terrier, R / Thorpe-Morgan, C / Tluczykont, M / Tsirou, M / Tsuji, N / Uchiyama, Y / van Eldik, C / Veh, J / Vink, J / Wagner, S J / White, R / Wierzcholska, A / Wong, Yu Wun / Zacharias, M / Zargaryan, D / Zdziarski, A A / Zech, A / Zhu, S J / Zouari, S / Żywucka, N

Physical review letters

2022 Volume 129, Issue 11, Page(s) 111101

Abstract: The central region of the Milky Way is one of the foremost locations to look for dark matter (DM) signatures. We report the first results on a search for DM particle annihilation signals using new observations from an unprecedented γ-ray survey of the ... ...

Abstract	The central region of the Milky Way is one of the foremost locations to look for dark matter (DM) signatures. We report the first results on a search for DM particle annihilation signals using new observations from an unprecedented γ-ray survey of the Galactic Center (GC) region, i.e., the Inner Galaxy Survey, at very high energies (≳100 GeV) performed with the H.E.S.S. array of five ground-based Cherenkov telescopes. No significant γ-ray excess is found in the search region of the 2014-2020 dataset and a profile likelihood ratio analysis is carried out to set exclusion limits on the annihilation cross section ⟨σv⟩. Assuming Einasto and Navarro-Frenk-White (NFW) DM density profiles at the GC, these constraints are the strongest obtained so far in the TeV DM mass range. For the Einasto profile, the constraints reach ⟨σv⟩ values of 3.7×10^{-26} cm^{3} s^{-1} for 1.5 TeV DM mass in the W^{+}W^{-} annihilation channel, and 1.2×10^{-26} cm^{3} s^{-1} for 0.7 TeV DM mass in the τ^{+}τ^{-} annihilation channel. With the H.E.S.S. Inner Galaxy Survey, ground-based γ-ray observations thus probe ⟨σv⟩ values expected from thermal-relic annihilating TeV DM particles.
Language	English
Publishing date	2022-09-26
Publishing country	United States
Document type	Journal Article
ZDB-ID	208853-8
ISSN	1079-7114 ; 0031-9007
ISSN (online)	1079-7114
ISSN	0031-9007
DOI	10.1103/PhysRevLett.129.111101
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Article ; Online: Time-resolved hadronic particle acceleration in the recurrent nova RS Ophiuchi.

Aharonian, F / Ait Benkhali, F / Angüner, E O / Ashkar, H / Backes, M / Baghmanyan, V / Barbosa Martins, V / Batzofin, R / Becherini, Y / Berge, D / Bernlöhr, K / Bi, B / Böttcher, M / Boisson, C / Bolmont, J / de Bony de Lavergne, M / Breuhaus, M / Brose, R / Brun, F /

Caroff, S / Casanova, S / Cerruti, M / Chand, T / Chen, A / Cotter, G / Damascene Mbarubucyeye, J / Djannati-Ataï, A / Dmytriiev, A / Doroshenko, V / Duffy, C / Egberts, K / Ernenwein, J-P / Fegan, S / Feijen, K / Fiasson, A / Fichet de Clairfontaine, G / Fontaine, G / Füßling, M / Funk, S / Gabici, S / Gallant, Y A / Ghafourizadeh, S / Giavitto, G / Giunti, L / Glawion, D / Glicenstein, J F / Grondin, M-H / Hermann, G / Hinton, J A / Hörbe, M / Hofmann, W / Hoischen, C / Holch, T L / Holler, M / Horns, D / Huang, Zhiqiu / Jamrozy, M / Jankowsky, F / Jung-Richardt, I / Kasai, E / Katarzyński, K / Katz, U / Khangulyan, D / Khélifi, B / Klepser, S / Kluźniak, W / Komin, Nu / Konno, R / Kosack, K / Kostunin, D / Le Stum, S / Lemière, A / Lemoine-Goumard, M / Lenain, J-P / Leuschner, F / Lohse, T / Luashvili, A / Lypova, I / Mackey, J / Malyshev, D / Marandon, V / Marchegiani, P / Marcowith, A / Martí-Devesa, G / Marx, R / Maurin, G / Meyer, M / Mitchell, A / Moderski, R / Mohrmann, L / Montanari, A / Moulin, E / Muller, J / Murach, T / Nakashima, K / de Naurois, M / Nayerhoda, A / Niemiec, J / Priyana Noel, A / O'Brien, P / Ohm, S / Olivera-Nieto, L / de Ona Wilhelmi, E / Ostrowski, M / Panny, S / Panter, M / Parsons, R D / Peron, G / Pita, S / Poireau, V / Prokhorov, D A / Prokoph, H / Pühlhofer, G / Punch, M / Quirrenbach, A / Reichherzer, P / Reimer, A / Reimer, O / Renaud, M / Reville, B / Rieger, F / Rowell, G / Rudak, B / Rueda Ricarte, H / Ruiz-Velasco, E / Sahakian, V / Sailer, S / Salzmann, H / Sanchez, D A / Santangelo, A / Sasaki, M / Schäfer, J / Schüssler, F / Schutte, H M / Schwanke, U / Senniappan, M / Shapopi, J N S / Simoni, R / Sinha, A / Sol, H / Specovius, A / Spencer, S / Stawarz, Ł / Steinmassl, S / Steppa, C / Takahashi, T / Tanaka, T / Taylor, A M / Terrier, R / Thorpe-Morgan, C / Tsirou, M / Tsuji, N / Tuffs, R / Uchiyama, Y / Unbehaun, T / van Eldik, C / van Soelen, B / Veh, J / Venter, C / Vink, J / Wagner, S J / Werner, F / White, R / Wierzcholska, A / Wong, Yu Wun / Yusafzai, A / Zacharias, M / Zargaryan, D / Zdziarski, A A / Zech, A / Zhu, S J / Zouari, S / Żywucka, N

Science (New York, N.Y.)

2022 Volume 376, Issue 6588, Page(s) 77–80

Abstract: Recurrent novae are repeating thermonuclear explosions in the outer layers of white dwarfs, due to the accretion of fresh material from a binary companion. The shock generated when ejected material slams into the companion star's wind can accelerate ... ...

Abstract	Recurrent novae are repeating thermonuclear explosions in the outer layers of white dwarfs, due to the accretion of fresh material from a binary companion. The shock generated when ejected material slams into the companion star's wind can accelerate particles. We report very-high-energy (VHE; [Formula: see text]) gamma rays from the recurrent nova RS Ophiuchi, up to 1 month after its 2021 outburst, observed using the High Energy Stereoscopic System (H.E.S.S.). The temporal profile of VHE emission is similar to that of lower-energy giga-electron volt emission, indicating a common origin, with a 2-day delay in peak flux. These observations constrain models of time-dependent particle energization, favoring a hadronic emission scenario over the leptonic alternative. Shocks in dense winds provide favorable environments for efficient acceleration of cosmic rays to very high energies.
Language	English
Publishing date	2022-03-10
Publishing country	United States
Document type	Journal Article ; Research Support, Non-U.S. Gov't
ZDB-ID	128410-1
ISSN	1095-9203 ; 0036-8075
ISSN (online)	1095-9203
ISSN	0036-8075
DOI	10.1126/science.abn0567
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Article ; Online: Revealing x-ray and gamma ray temporal and spectral similarities in the GRB 190829A afterglow.

Abdalla, H / Aharonian, F / Ait Benkhali, F / Angüner, E O / Arcaro, C / Armand, C / Armstrong, T / Ashkar, H / Backes, M / Baghmanyan, V / Barbosa Martins, V / Barnacka, A / Barnard, M / Becherini, Y / Berge, D / Bernlöhr, K / Bi, B / Bissaldi, E / Böttcher, M /

Boisson, C / Bolmont, J / de Bony de Lavergne, M / Breuhaus, M / Brun, F / Brun, P / Bryan, M / Büchele, M / Bulik, T / Bylund, T / Caroff, S / Carosi, A / Casanova, S / Chand, T / Chandra, S / Chen, A / Cotter, G / Curyło, M / Damascene Mbarubucyeye, J / Davids, I D / Davies, J / Deil, C / Devin, J / Dirson, L / Djannati-Ataï, A / Dmytriiev, A / Donath, A / Doroshenko, V / Dreyer, L / Duffy, C / Dyks, J / Egberts, K / Eichhorn, F / Einecke, S / Emery, G / Ernenwein, J-P / Feijen, K / Fegan, S / Fiasson, A / Fichet de Clairfontaine, G / Fontaine, G / Funk, S / Füßling, M / Gabici, S / Gallant, Y A / Giavitto, G / Giunti, L / Glawion, D / Glicenstein, J F / Grondin, M-H / Hahn, J / Haupt, M / Hermann, G / Hinton, J A / Hofmann, W / Hoischen, C / Holch, T L / Holler, M / Hörbe, M / Horns, D / Huber, D / Jamrozy, M / Jankowsky, D / Jankowsky, F / Jardin-Blicq, A / Joshi, V / Jung-Richardt, I / Kasai, E / Kastendieck, M A / Katarzyński, K / Katz, U / Khangulyan, D / Khélifi, B / Klepser, S / Kluźniak, W / Komin, Nu / Konno, R / Kosack, K / Kostunin, D / Kreter, M / Lamanna, G / Lemière, A / Lemoine-Goumard, M / Lenain, J-P / Leuschner, F / Levy, C / Lohse, T / Lypova, I / Mackey, J / Majumdar, J / Malyshev, D / Marandon, V / Marchegiani, P / Marcowith, A / Mares, A / Martí-Devesa, G / Marx, R / Maurin, G / Meintjes, P J / Meyer, M / Mitchell, A / Moderski, R / Mohrmann, L / Montanari, A / Moore, C / Morris, P / Moulin, E / Muller, J / Murach, T / Nakashima, K / Nayerhoda, A / de Naurois, M / Ndiyavala, H / Niemiec, J / Oakes, L / O'Brien, P / Odaka, H / Ohm, S / Olivera-Nieto, L / de Ona Wilhelmi, E / Ostrowski, M / Panny, S / Panter, M / Parsons, R D / Peron, G / Peyaud, B / Piel, Q / Pita, S / Poireau, V / Priyana Noel, A / Prokhorov, D A / Prokoph, H / Pühlhofer, G / Punch, M / Quirrenbach, A / Raab, S / Rauth, R / Reichherzer, P / Reimer, A / Reimer, O / Remy, Q / Renaud, M / Rieger, F / Rinchiuso, L / Romoli, C / Rowell, G / Rudak, B / Ruiz-Velasco, E / Sahakian, V / Sailer, S / Salzmann, H / Sanchez, D A / Santangelo, A / Sasaki, M / Scalici, M / Schäfer, J / Schüssler, F / Schutte, H M / Schwanke, U / Seglar-Arroyo, M / Senniappan, M / Seyffert, A S / Shafi, N / Shapopi, J N S / Shiningayamwe, K / Simoni, R / Sinha, A / Sol, H / Specovius, A / Spencer, S / Spir-Jacob, M / Stawarz, Ł / Sun, L / Steenkamp, R / Stegmann, C / Steinmassl, S / Steppa, C / Takahashi, T / Tam, T / Tavernier, T / Taylor, A M / Terrier, R / Thiersen, J H E / Tiziani, D / Tluczykont, M / Tomankova, L / Tsirou, M / Tuffs, R / Uchiyama, Y / van der Walt, D J / van Eldik, C / van Rensburg, C / van Soelen, B / Vasileiadis, G / Veh, J / Venter, C / Vincent, P / Vink, J / Völk, H J / Wadiasingh, Z / Wagner, S J / Watson, J / Werner, F / White, R / Wierzcholska, A / Wong, Yu Wun / Yusafzai, A / Zacharias, M / Zanin, R / Zargaryan, D / Zdziarski, A A / Zech, A / Zhu, S J / Zorn, J / Zouari, S / Żywucka, N / Evans, P / Page, K

Science (New York, N.Y.)

2021 Volume 372, Issue 6546, Page(s) 1081–1085

Abstract: Gamma-ray bursts (GRBs), which are bright flashes of gamma rays from extragalactic sources followed by fading afterglow emission, are associated with stellar core collapse events. We report the detection of very-high-energy (VHE) gamma rays from the ... ...

Abstract	Gamma-ray bursts (GRBs), which are bright flashes of gamma rays from extragalactic sources followed by fading afterglow emission, are associated with stellar core collapse events. We report the detection of very-high-energy (VHE) gamma rays from the afterglow of GRB 190829A, between 4 and 56 hours after the trigger, using the High Energy Stereoscopic System (H.E.S.S.). The low luminosity and redshift of GRB 190829A reduce both internal and external absorption, allowing determination of its intrinsic energy spectrum. Between energies of 0.18 and 3.3 tera-electron volts, this spectrum is described by a power law with photon index of 2.07 ± 0.09, similar to the x-ray spectrum. The x-ray and VHE gamma-ray light curves also show similar decay profiles. These similar characteristics in the x-ray and gamma-ray bands challenge GRB afterglow emission scenarios.
Language	English
Publishing date	2021-05-25
Publishing country	United States
Document type	Journal Article ; Research Support, Non-U.S. Gov't
ZDB-ID	128410-1
ISSN	1095-9203 ; 0036-8075
ISSN (online)	1095-9203
ISSN	0036-8075
DOI	10.1126/science.abe8560
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Article ; Online: A very-high-energy component deep in the γ-ray burst afterglow.

Abdalla, H / Adam, R / Aharonian, F / Ait Benkhali, F / Angüner, E O / Arakawa, M / Arcaro, C / Armand, C / Ashkar, H / Backes, M / Barbosa Martins, V / Barnard, M / Becherini, Y / Berge, D / Bernlöhr, K / Bissaldi, E / Blackwell, R / Böttcher, M / Boisson, C /

Bolmont, J / Bonnefoy, S / Bregeon, J / Breuhaus, M / Brun, F / Brun, P / Bryan, M / Büchele, M / Bulik, T / Bylund, T / Capasso, M / Caroff, S / Carosi, A / Casanova, S / Cerruti, M / Chand, T / Chandra, S / Chen, A / Colafrancesco, S / Curyło, M / Davids, I D / Deil, C / Devin, J / deWilt, P / Dirson, L / Djannati-Ataï, A / Dmytriiev, A / Donath, A / Doroshenko, V / Dyks, J / Egberts, K / Emery, G / Ernenwein, J-P / Eschbach, S / Feijen, K / Fegan, S / Fiasson, A / Fontaine, G / Funk, S / Füßling, M / Gabici, S / Gallant, Y A / Gaté, F / Giavitto, G / Giunti, L / Glawion, D / Glicenstein, J F / Gottschall, D / Grondin, M-H / Hahn, J / Haupt, M / Heinzelmann, G / Henri, G / Hermann, G / Hinton, J A / Hofmann, W / Hoischen, C / Holch, T L / Holler, M / Horns, D / Huber, D / Iwasaki, H / Jamrozy, M / Jankowsky, D / Jankowsky, F / Jardin-Blicq, A / Jung-Richardt, I / Kastendieck, M A / Katarzyński, K / Katsuragawa, M / Katz, U / Khangulyan, D / Khélifi, B / King, J / Klepser, S / Kluźniak, W / Komin, Nu / Kosack, K / Kostunin, D / Kreter, M / Lamanna, G / Lemière, A / Lemoine-Goumard, M / Lenain, J-P / Leser, E / Levy, C / Lohse, T / Lypova, I / Mackey, J / Majumdar, J / Malyshev, D / Marandon, V / Marcowith, A / Mares, A / Mariaud, C / Martí-Devesa, G / Marx, R / Maurin, G / Meintjes, P J / Mitchell, A M W / Moderski, R / Mohamed, M / Mohrmann, L / Moore, C / Moulin, E / Muller, J / Murach, T / Nakashima, S / de Naurois, M / Ndiyavala, H / Niederwanger, F / Niemiec, J / Oakes, L / O'Brien, P / Odaka, H / Ohm, S / de Ona Wilhelmi, E / Ostrowski, M / Oya, I / Panter, M / Parsons, R D / Perennes, C / Petrucci, P-O / Peyaud, B / Piel, Q / Pita, S / Poireau, V / Priyana Noel, A / Prokhorov, D A / Prokoph, H / Pühlhofer, G / Punch, M / Quirrenbach, A / Raab, S / Rauth, R / Reimer, A / Reimer, O / Remy, Q / Renaud, M / Rieger, F / Rinchiuso, L / Romoli, C / Rowell, G / Rudak, B / Ruiz-Velasco, E / Sahakian, V / Sailer, S / Saito, S / Sanchez, D A / Santangelo, A / Sasaki, M / Schlickeiser, R / Schüssler, F / Schulz, A / Schutte, H M / Schwanke, U / Schwemmer, S / Seglar-Arroyo, M / Senniappan, M / Seyffert, A S / Shafi, N / Shiningayamwe, K / Simoni, R / Sinha, A / Sol, H / Specovius, A / Spir-Jacob, M / Stawarz, Ł / Steenkamp, R / Stegmann, C / Steppa, C / Takahashi, T / Tavernier, T / Taylor, A M / Terrier, R / Tiziani, D / Tluczykont, M / Trichard, C / Tsirou, M / Tsuji, N / Tuffs, R / Uchiyama, Y / van der Walt, D J / van Eldik, C / van Rensburg, C / van Soelen, B / Vasileiadis, G / Veh, J / Venter, C / Vincent, P / Vink, J / Völk, H J / Vuillaume, T / Wadiasingh, Z / Wagner, S J / White, R / Wierzcholska, A / Yang, R / Yoneda, H / Zacharias, M / Zanin, R / Zdziarski, A A / Zech, A / Ziegler, A / Zorn, J / Żywucka, N / de Palma, F / Axelsson, M / Roberts, O J

Nature

2019 Volume 575, Issue 7783, Page(s) 464–467

Abstract: Gamma-ray bursts (GRBs) are brief flashes of γ-rays and are considered to be the most energetic explosive phenomena in the ... ...

Abstract	Gamma-ray bursts (GRBs) are brief flashes of γ-rays and are considered to be the most energetic explosive phenomena in the Universe
Language	English
Publishing date	2019-11-20
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/s41586-019-1743-9
Database	MEDical Literature Analysis and Retrieval System OnLINE

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Book ; Online: The Control Unit of the KM3NeT Data Acquisition System

Aiello, S. / Ameli, F. / Andre, M. / Androulakis, G. / Anghinolfi, M. / Anton, G. / Ardid, M. / Aublin, J. / Bagatelas, C. / Barbarino, G. / Baret, B. / Pree, S. Basegmez du / Bendahman, M. / Berbee, E. / Berg, A. M. van den / Bertin, V. / Biagi, S. / Biagioni, A. / Bissinger, M. /

Boumaaza, J. / Bourret, S. / Bouta, M. / Bouvet, G. / Bouwhuis, M. / Bozza, C. / Branzas, H. / Bruchner, M. / Bruijn, R. / Brunner, J. / Buis, E. / Buompane, R. / Busto, J. / Calvo, D. / Capone, A. / Celli, S. / Chabab, M. / Chau, N. / Cherubini, S. / Chiarella, V. / Chiarusi, T. / Circella, M. / Cocimano, R. / Coelho, J. A. B. / Coleiro, A. / Molla, M. Colomer / Coniglione, R. / Coyle, P. / Creusot, A. / Cuttone, G. / D'Onofrio, A. / Dallier, R. / De Palma, M. / Di Palma, I. / Díaz, A. F. / Diego-Tortosa, D. / Distefano, C. / Domi, A. / Donà, R. / Donzaud, C. / Dornic, D. / Dörr, M. / Durocher, M. / Eberl, T. / Bojaddaini, I. El / Eljarrari, H. / Elsaesser, D. / Enzenhöfer, A. / Fermani, P. / Ferrara, G. / Filipovic, M. D. / Franco, A. / Fusco, L. A. / Gal, T. / Soto, A. Garcia / Garufi, F. / Gialanella, L. / Giorgio, E. / Gozzini, S. R. / Gracia, R. / Graf, K. / Grasso, D. / Grégoire, T. / Grella, G. / Guderian, D. / Guidi, C. / Hallmann, S. / Hamdaoui, H. / van Haren, H. / Heijboer, A. / Hekalo, A. / Hernández-Rey, J. J. / Hofestädt, J. / Huang, F. / Illuminati, G. / James, C. W. / de Jong, M. / de Jong, P. / Kadler, M. / Kalaczynski, P. / Kalekin, O. / Katz, U. F. / Chowdhury, N. R. Khan / van der Knaap, F. / Koffeman, E. N. / Kooijman, P. / Kouchner, A. / Kulikovskiy, V. / Lahmann, R. / Larosa, G. / Breton, R. Le / Leone, F. / Leonora, E. / Levi, G. / Lincetto, M. / Lonardo, A. / Longhitano, F. / Lopez-Coto, D. / Maggi, G. / Manczak, J. / Mannheim, K. / Margiotta, A. / Marinelli, A. / Markou, C. / Martignac, G. / Martin, L. / Martínez-Mora, J. A. / Martini, A. / Marzaioli, F. / Mazzou, S. / Mele, R. / Melis, K. W. / Migliozzi, P. / Migneco, E. / Mijakowski, P. / Miranda, L. S. / Mollo, C. M. / Morganti, M. / Moser, M. / Moussa, A. / Muller, R. / Musumeci, M. / Nauta, L. / Navas, S. / Nicolau, C. A. / Nielsen, C. / Fearraigh, B. O' / Organokov, M. / Orlando, A. / Panagopoulos, V. / Papalashvili, G. / Papaleo, R. / Pastore, C. / Pavalas, G. E. / Pellegrino, C. / Perrin-Terrin, M. / Piattelli, P. / Pieterse, C. / Pikounis, K. / Pisanti, O. / Poirè, C. / Polydefki, G. / Popa, V. / Post, M. / Pradier, T. / Puhlhofer, G. / Pulvirenti, S. / Quinn, L. / Raffaelli, F. / Randazzo, N. / Rapicavoli, A. / Razzaque, S. / Real, D. / Reck, S. / Reubelt, J. / Riccobene, G. / Richer, M. / Rigalleau, L. / Rovelli, A. / Salvadori, I. / Samtleben, D. F. E. / Losa, A. Sánchez / Sanguineti, M. / Santangelo, A. / Santonocito, D. / Sapienza, P. / Schnabel, J. / Sciacca, V. / Seneca, J. / Sgura, I. / Shanidze, R. / Sharma, A. / Simeone, F. / Sinopoulou, A. / Spisso, B. / Spurio, M. / Stavropoulos, D. / Steijger, J. / Stellacci, S. M. / Strandberg, B. / Stransky, D. / Taiuti, M. / Tayalati, Y. / Tenllado, E. / Thakore, T. / Tingay, S. / Tzamariudaki, E. / Tzanetatos, D. / Van Elewyck, V. / Vannoye, G. / Versari, F. / Viola, S. / Vivolo, D. / de Wasseige, G. / Wilms, J. / Wojaczynski, R. / de Wolf, E. / Zaborov, D. / Zegarelli, A. / Zornoza, J. D. / Zúñiga, J.

2019

Abstract: The KM3NeT Collaboration runs a multi-site neutrino observatory in the Mediterranean Sea. Water Cherenkov particle detectors, deep in the sea and far off the coasts of France and Italy, are already taking data while incremental construction progresses. ... ...

Abstract	The KM3NeT Collaboration runs a multi-site neutrino observatory in the Mediterranean Sea. Water Cherenkov particle detectors, deep in the sea and far off the coasts of France and Italy, are already taking data while incremental construction progresses. Data Acquisition Control software is operating off-shore detectors as well as testing and qualification stations for their components. The software, named Control Unit, is highly modular. It can undergo upgrades and reconfiguration with the acquisition running. Interplay with the central database of the Collaboration is obtained in a way that allows for data taking even if Internet links fail. In order to simplify the management of computing resources in the long term, and to cope with possible hardware failures of one or more computers, the KM3NeT Control Unit software features a custom dynamic resource provisioning and failover technology, which is especially important for ensuring continuity in case of rare transient events in multi-messenger astronomy. The software architecture relies on ubiquitous tools and broadly adopted technologies and has been successfully tested on several operating systems.
Keywords	Astrophysics - Instrumentation and Methods for Astrophysics ; High Energy Physics - Experiment
Subject code	303
Publishing date	2019-09-30
Publishing country	us
Document type	Book ; Online
Database	BASE - Bielefeld Academic Search Engine (life sciences selection)

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Article ; Online: Search for γ-Ray Line Signals from Dark Matter Annihilations in the Inner Galactic Halo from 10 Years of Observations with H.E.S.S.

Abdallah, H / Abramowski, A / Aharonian, F / Ait Benkhali, F / Angüner, E O / Arakawa, M / Arrieta, M / Aubert, P / Backes, M / Balzer, A / Barnard, M / Becherini, Y / Becker Tjus, J / Berge, D / Bernhard, S / Bernlöhr, K / Blackwell, R / Böttcher, M / Boisson, C /

Bolmont, J / Bonnefoy, S / Bordas, P / Bregeon, J / Brun, F / Brun, P / Bryan, M / Büchele, M / Bulik, T / Capasso, M / Caroff, S / Carosi, A / Carr, J / Casanova, S / Cerruti, M / Chakraborty, N / Chaves, R C G / Chen, A / Chevalier, J / Colafrancesco, S / Condon, B / Conrad, J / Davids, I D / Decock, J / Deil, C / Devin, J / deWilt, P / Dirson, L / Djannati-Ataï, A / Domainko, W / Donath, A / Drury, L O'C / Dutson, K / Dyks, J / Edwards, T / Egberts, K / Eger, P / Emery, G / Ernenwein, J-P / Eschbach, S / Farnier, C / Fegan, S / Fernandes, M V / Fiasson, A / Fontaine, G / Förster, A / Funk, S / Füßling, M / Gabici, S / Gallant, Y A / Garrigoux, T / Gaté, F / Giavitto, G / Giebels, B / Glawion, D / Glicenstein, J F / Gottschall, D / Grondin, M-H / Hahn, J / Haupt, M / Hawkes, J / Heinzelmann, G / Henri, G / Hermann, G / Hinton, J A / Hofmann, W / Hoischen, C / Holch, T L / Holler, M / Horns, D / Ivascenko, A / Iwasaki, H / Jacholkowska, A / Jamrozy, M / Janiak, M / Jankowsky, D / Jankowsky, F / Jingo, M / Jouvin, L / Jung-Richardt, I / Kastendieck, M A / Katarzyński, K / Katsuragawa, M / Katz, U / Kerszberg, D / Khangulyan, D / Khélifi, B / King, J / Klepser, S / Klochkov, D / Kluźniak, W / Komin, Nu / Kosack, K / Krakau, S / Kraus, M / Krüger, P P / Laffon, H / Lamanna, G / Lau, J / Lees, J-P / Lefaucheur, J / Lemière, A / Lemoine-Goumard, M / Lenain, J-P / Leser, E / Liu, R / Lohse, T / Lorentz, M / López-Coto, R / Lypova, I / Malyshev, D / Marandon, V / Marcowith, A / Mariaud, C / Marx, R / Maurin, G / Maxted, N / Mayer, M / Meintjes, P J / Meyer, M / Mitchell, A M W / Moderski, R / Mohamed, M / Mohrmann, L / Morå, K / Moulin, E / Murach, T / Nakashima, S / de Naurois, M / Ndiyavala, H / Niederwanger, F / Niemiec, J / Oakes, L / O'Brien, P / Odaka, H / Ohm, S / Ostrowski, M / Oya, I / Padovani, M / Panter, M / Parsons, R D / Pekeur, N W / Pelletier, G / Perennes, C / Petrucci, P-O / Peyaud, B / Piel, Q / Pita, S / Poireau, V / Poon, H / Prokhorov, D / Prokoph, H / Pühlhofer, G / Punch, M / Quirrenbach, A / Raab, S / Rauth, R / Reimer, A / Reimer, O / Renaud, M / de Los Reyes, R / Rieger, F / Rinchiuso, L / Romoli, C / Rowell, G / Rudak, B / Rulten, C B / Sahakian, V / Saito, S / Sanchez, D A / Santangelo, A / Sasaki, M / Schandri, M / Schlickeiser, R / Schüssler, F / Schulz, A / Schwanke, U / Schwemmer, S / Seglar-Arroyo, M / Settimo, M / Seyffert, A S / Shafi, N / Shilon, I / Shiningayamwe, K / Simoni, R / Sol, H / Spanier, F / Spir-Jacob, M / Stawarz, Ł / Steenkamp, R / Stegmann, C / Steppa, C / Sushch, I / Takahashi, T / Tavernet, J-P / Tavernier, T / Taylor, A M / Terrier, R / Tibaldo, L / Tiziani, D / Tluczykont, M / Trichard, C / Tsirou, M / Tsuji, N / Tuffs, R / Uchiyama, Y / van der Walt, J / van Eldik, C / van Rensburg, C / van Soelen, B / Vasileiadis, G / Veh, J / Venter, C / Viana, A / Vincent, P / Vink, J / Voisin, F / Völk, H J / Vuillaume, T / Wadiasingh, Z / Wagner, S J / Wagner, P / Wagner, R M / White, R / Wierzcholska, A / Willmann, P / Wörnlein, A / Wouters, D / Yang, R / Zaborov, D / Zacharias, M / Zanin, R / Zdziarski, A A / Zech, A / Zefi, F / Ziegler, A / Zorn, J / Żywucka, N

Physical review letters

2018 Volume 120, Issue 20, Page(s) 201101

Abstract: Spectral lines are among the most powerful signatures for dark matter (DM) annihilation searches in very-high-energy γ rays. The central region of the Milky Way halo is one of the most promising targets given its large amount of DM and proximity to Earth. ...

Abstract	Spectral lines are among the most powerful signatures for dark matter (DM) annihilation searches in very-high-energy γ rays. The central region of the Milky Way halo is one of the most promising targets given its large amount of DM and proximity to Earth. We report on a search for a monoenergetic spectral line from self-annihilations of DM particles in the energy range from 300 GeV to 70 TeV using a two-dimensional maximum likelihood method taking advantage of both the spectral and spatial features of the signal versus background. The analysis makes use of Galactic center observations accumulated over ten years (2004-2014) with the H.E.S.S. array of ground-based Cherenkov telescopes. No significant γ-ray excess above the background is found. We derive upper limits on the annihilation cross section ⟨σv⟩ for monoenergetic DM lines at the level of 4×10^{-28} cm^{3} s^{-1} at 1 TeV, assuming an Einasto DM profile for the Milky Way halo. For a DM mass of 1 TeV, they improve over the previous ones by a factor of 6. The present constraints are the strongest obtained so far for DM particles in the mass range 300 GeV-70 TeV. Ground-based γ-ray observations have reached sufficient sensitivity to explore relevant velocity-averaged cross sections for DM annihilation into two γ-ray photons at the level expected from the thermal relic density for TeV DM particles.
Language	English
Publishing date	2018-05-18
Publishing country	United States
Document type	Journal Article
ZDB-ID	208853-8
ISSN	1079-7114 ; 0031-9007
ISSN (online)	1079-7114
ISSN	0031-9007
DOI	10.1103/PhysRevLett.120.201101
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Article ; Online: Constraints on an annihilation signal from a core of constant dark matter density around the milky way center with H.E.S.S.

Abramowski, A / Aharonian, F / Ait Benkhali, F / Akhperjanian, A G / Angüner, E O / Backes, M / Balenderan, S / Balzer, A / Barnacka, A / Becherini, Y / Becker Tjus, J / Berge, D / Bernhard, S / Bernlöhr, K / Birsin, E / Biteau, J / Böttcher, M / Boisson, C / Bolmont, J /

Bordas, P / Bregeon, J / Brun, F / Brun, P / Bryan, M / Bulik, T / Carrigan, S / Casanova, S / Chadwick, P M / Chakraborty, N / Chalme-Calvet, R / Chaves, R C G / Chrétien, M / Colafrancesco, S / Cologna, G / Conrad, J / Couturier, C / Cui, Y / Davids, I D / Degrange, B / Deil, C / deWilt, P / Djannati-Ataï, A / Domainko, W / Donath, A / Drury, L O'C / Dubus, G / Dutson, K / Dyks, J / Dyrda, M / Edwards, T / Egberts, K / Eger, P / Espigat, P / Farnier, C / Fegan, S / Feinstein, F / Fernandes, M V / Fernandez, D / Fiasson, A / Fontaine, G / Förster, A / Füßling, M / Gabici, S / Gajdus, M / Gallant, Y A / Garrigoux, T / Giavitto, G / Giebels, B / Glicenstein, J F / Gottschall, D / Grondin, M-H / Grudzińska, M / Hadasch, D / Häffner, S / Hahn, J / Harris, J / Heinzelmann, G / Henri, G / Hermann, G / Hervet, O / Hillert, A / Hinton, J A / Hofmann, W / Hofverberg, P / Holler, M / Horns, D / Ivascenko, A / Jacholkowska, A / Jahn, C / Jamrozy, M / Janiak, M / Jankowsky, F / Jung-Richardt, I / Kastendieck, M A / Katarzyński, K / Katz, U / Kaufmann, S / Khélifi, B / Kieffer, M / Klepser, S / Klochkov, D / Kluźniak, W / Kolitzus, D / Komin, Nu / Kosack, K / Krakau, S / Krayzel, F / Krüger, P P / Laffon, H / Lamanna, G / Lefaucheur, J / Lefranc, V / Lemière, A / Lemoine-Goumard, M / Lenain, J-P / Lohse, T / Lopatin, A / Lu, C-C / Marandon, V / Marcowith, A / Marx, R / Maurin, G / Maxted, N / Mayer, M / McComb, T J L / Méhault, J / Meintjes, P J / Menzler, U / Meyer, M / Mitchell, A M W / Moderski, R / Mohamed, M / Morå, K / Moulin, E / Murach, T / de Naurois, M / Niemiec, J / Nolan, S J / Oakes, L / Odaka, H / Ohm, S / Opitz, B / Ostrowski, M / Oya, I / Panter, M / Parsons, R D / Paz Arribas, M / Pekeur, N W / Pelletier, G / Petrucci, P-O / Peyaud, B / Pita, S / Poon, H / Pühlhofer, G / Punch, M / Quirrenbach, A / Raab, S / Reichardt, I / Reimer, A / Reimer, O / Renaud, M / de Los Reyes, R / Rieger, F / Romoli, C / Rosier-Lees, S / Rowell, G / Rudak, B / Rulten, C B / Sahakian, V / Salek, D / Sanchez, D A / Santangelo, A / Schlickeiser, R / Schüssler, F / Schulz, A / Schwanke, U / Schwarzburg, S / Schwemmer, S / Sol, H / Spanier, F / Spengler, G / Spies, F / Stawarz, Ł / Steenkamp, R / Stegmann, C / Stinzing, F / Stycz, K / Sushch, I / Tavernet, J-P / Tavernier, T / Taylor, A M / Terrier, R / Tluczykont, M / Trichard, C / Valerius, K / van Eldik, C / van Soelen, B / Vasileiadis, G / Veh, J / Venter, C / Viana, A / Vincent, P / Vink, J / Völk, H J / Volpe, F / Vorster, M / Vuillaume, T / Wagner, S J / Wagner, P / Wagner, R M / Ward, M / Weidinger, M / Weitzel, Q / White, R / Wierzcholska, A / Willmann, P / Wörnlein, A / Wouters, D / Yang, R / Zabalza, V / Zaborov, D / Zacharias, M / Zdziarski, A A / Zech, A / Zechlin, H-S

Physical review letters

2015 Volume 114, Issue 8, Page(s) 81301

Abstract: An annihilation signal of dark matter is searched for from the central region of the Milky Way. Data acquired in dedicated on-off observations of the Galactic center region with H.E.S.S. are analyzed for this purpose. No significant signal is found in a ... ...

Abstract	An annihilation signal of dark matter is searched for from the central region of the Milky Way. Data acquired in dedicated on-off observations of the Galactic center region with H.E.S.S. are analyzed for this purpose. No significant signal is found in a total of ∼9 h of on-off observations. Upper limits on the velocity averaged cross section, ⟨σv⟩, for the annihilation of dark matter particles with masses in the range of ∼300 GeV to ∼10 TeV are derived. In contrast to previous constraints derived from observations of the Galactic center region, the constraints that are derived here apply also under the assumption of a central core of constant dark matter density around the center of the Galaxy. Values of ⟨σv⟩ that are larger than 3×10^{-24} cm^{3}/s are excluded for dark matter particles with masses between ∼1 and ∼4 TeV at 95% C.L. if the radius of the central dark matter density core does not exceed 500 pc. This is the strongest constraint that is derived on ⟨σv⟩ for annihilating TeV mass dark matter without the assumption of a centrally cusped dark matter density distribution in the search region.
Language	English
Publishing date	2015-02-27
Publishing country	United States
Document type	Journal Article
ZDB-ID	208853-8
ISSN	1079-7114 ; 0031-9007
ISSN (online)	1079-7114
ISSN	0031-9007
DOI	10.1103/PhysRevLett.114.081301
Database	MEDical Literature Analysis and Retrieval System OnLINE

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