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Liepert J, Stürner J, Büsching I, Sehle A, Schoenfeld MA. Effects of a single mental chronometry training session in subacute stroke patients - a randomized controlled trial. BMC Sports Sci Med Rehabil 2020; 12:66. [PMID: 33101692 PMCID: PMC7579870 DOI: 10.1186/s13102-020-00212-w] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Journal Information] [Subscribe] [Scholar Register] [Received: 03/29/2020] [Accepted: 10/05/2020] [Indexed: 11/10/2022]
Abstract
Background Motor imagery training might be helpful in stroke rehabilitation. This study explored if a single session of motor imagery (MI) training induces performance changes in mental chronometry (MC), motor execution, or changes of motor excitability. Methods Subacute stroke patients (n = 33) participated in two training sessions. The order was randomized. One training consisted of a mental chronometry task, the other training was a hand identification task, each lasting 30 min. Before and after the training session, the Box and Block Test (BBT) was fully executed and also performed as a mental version which served as a measure of MC. A subgroup analysis based on the presence of sensory deficits was performed. Patients were allocated to three groups (no sensory deficits, moderate sensory deficits, severe sensory deficits). Motor excitability was measured by transcranial magnetic stimulation (TMS) pre and post training. Amplitudes of motor evoked potentials at rest and during pre-innervation as well as the duration of cortical silent period were measured in the affected and the non-affected hand. Results Pre-post differences of MC showed an improved MC after the MI training, whereas MC was worse after the hand identification training. Motor execution of the BBT was significantly improved after mental chronometry training but not after hand identification task training. Patients with severe sensory deficits performed significantly inferior in BBT execution and MC abilities prior to the training session compared to patients without sensory deficits or with moderate sensory deficits. However, pre-post differences of MC were similar in the 3 groups. TMS results were not different between pre and post training but showed significant differences between affected and unaffected side. Conclusion Even a single training session can modulate MC abilities and BBT motor execution in a task-specific way. Severe sensory deficits are associated with poorer motor performance and poorer MC ability, but do not have a negative impact on training-associated changes of mental chronometry. Studies with longer treatment periods should explore if the observed changes can further be expanded. Trial registration DRKS, DRKS00020355, registered March 9th, 2020, retrospectively registered
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Affiliation(s)
- Joachim Liepert
- Department of Neurorehabilitation, Kliniken Schmieder, Zum Tafelholz 8, 78476 Allensbach, Germany
| | - Jana Stürner
- Department of Neurorehabilitation, Kliniken Schmieder, Zum Tafelholz 8, 78476 Allensbach, Germany
| | | | - Aida Sehle
- Department of Neurorehabilitation, Kliniken Schmieder, Zum Tafelholz 8, 78476 Allensbach, Germany
| | - Mircea A Schoenfeld
- Department of Neurorehabilitation, Kliniken Schmieder, Heidelberg, Germany.,Department of Experimental Neurology, Medical Faculty, Otto-von-Guericke University Magdeburg, Magdeburg, Germany.,Department of Behavioral Neurology, Leibniz Institute for Neurobiology, Magdeburg, Germany
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Büsching I, Sehle A, Stürner J, Liepert J. Using an upper extremity exoskeleton for semi-autonomous exercise during inpatient neurological rehabilitation- a pilot study. J Neuroeng Rehabil 2018; 15:72. [PMID: 30068372 PMCID: PMC6090973 DOI: 10.1186/s12984-018-0415-6] [Citation(s) in RCA: 7] [Impact Index Per Article: 1.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 03/25/2018] [Accepted: 07/12/2018] [Indexed: 11/23/2022] Open
Abstract
Background Motor deficits are the most common symptoms after stroke. There is some evidence that intensity and amount of exercises influence the degree of improvement of functions within the first 6 months after the injury. The purpose of this pilot study was to evaluate the feasibility and acceptance of semi-autonomous exercises with an upper extremity exoskeleton in addition to an inpatient rehabilitation program. In addition, changes of motor functions were examined. Methods Ten stroke patients with a severe upper extremity paresis were included. They were offered to perform a semi-autonomous training with a gravity-supported, computer-enhanced device (Armeo®Spring, Hocoma AG) six times per week for 4 weeks. Feasibility was evaluated by weekly structured interviews with patients and supervisors. Motor functions were assessed before and after the training period using the Wolf Motor Function Test (WMFT). The Wilcoxon Signed Rank Test was used for assessing pre-post differences. The Pearson correlation co-efficient was used for correlating the number of completed sessions with the change in motor function. Acceptance of the device and the level of satisfaction with the training were determined by a questionnaire based on visual analogue scales. Results Neither patients nor supervisors reported side effects. However, one patient had to be excluded from analysis because of transportation difficulties from the ward to the treatment facility. Therefore, analysis was based on nine patients. On average, 13.2 (55%) sessions were realized. WMFT results showed significant improvements of proximal arm functions. The number of sessions correlated with the degree of shoulder force improvement. Patients rated the exercises to be motivating, and enjoyable and would continue using the Armeo®Spring at home if they had the opportunity. Conclusion Using an upper extremity exoskeleton for semi-autonomous training in an inpatient setting is feasible without side effects and is positively rated by the patients. It might further support the recovery of upper extremity function. Trial registration The trial was retrospectively registered. Registration number ISRCTN42633681.
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Affiliation(s)
- Imke Büsching
- Department of Neurorehabilitation, Kliniken Schmieder, Zum Tafelholz 8, D- 78476, Allensbach, Germany.,Reha-Klinik Bellikon, Mutschellenstrasse 2, 5454, Bellikon, Switzerland
| | - Aida Sehle
- Department of Neurorehabilitation, Kliniken Schmieder, Zum Tafelholz 8, D- 78476, Allensbach, Germany
| | - Jana Stürner
- Department of Neurorehabilitation, Kliniken Schmieder, Zum Tafelholz 8, D- 78476, Allensbach, Germany
| | - Joachim Liepert
- Department of Neurorehabilitation, Kliniken Schmieder, Zum Tafelholz 8, D- 78476, Allensbach, Germany.
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Braun N, Kranczioch C, Liepert J, Dettmers C, Zich C, Büsching I, Debener S. Motor Imagery Impairment in Postacute Stroke Patients. Neural Plast 2017; 2017:4653256. [PMID: 28458926 PMCID: PMC5387846 DOI: 10.1155/2017/4653256] [Citation(s) in RCA: 22] [Impact Index Per Article: 3.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 12/09/2016] [Accepted: 02/14/2017] [Indexed: 01/26/2023] Open
Abstract
Not much is known about how well stroke patients are able to perform motor imagery (MI) and which MI abilities are preserved after stroke. We therefore applied three different MI tasks (one mental chronometry task, one mental rotation task, and one EEG-based neurofeedback task) to a sample of postacute stroke patients (n = 20) and age-matched healthy controls (n = 20) for addressing the following questions: First, which of the MI tasks indicate impairment in stroke patients and are impairments restricted to the paretic side? Second, is there a relationship between MI impairment and sensory loss or paresis severity? And third, do the results of the different MI tasks converge? Significant differences between the stroke and control groups were found in all three MI tasks. However, only the mental chronometry task and EEG analysis revealed paresis side-specific effects. Moreover, sensitivity loss contributed to a performance drop in the mental rotation task. The findings indicate that although MI abilities may be impaired after stroke, most patients retain their ability for MI EEG-based neurofeedback. Interestingly, performance in the different MI measures did not strongly correlate, neither in stroke patients nor in healthy controls. We conclude that one MI measure is not sufficient to fully assess an individual's MI abilities.
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Affiliation(s)
- Niclas Braun
- Neuropsychology Lab, Department of Psychology, University of Oldenburg, Oldenburg, Germany
| | - Cornelia Kranczioch
- Neuropsychology Lab, Department of Psychology, University of Oldenburg, Oldenburg, Germany
| | | | | | - Catharina Zich
- Neuropsychology Lab, Department of Psychology, University of Oldenburg, Oldenburg, Germany
| | | | - Stefan Debener
- Neuropsychology Lab, Department of Psychology, University of Oldenburg, Oldenburg, Germany
- Research Center Neurosensory Science, University of Oldenburg, Oldenburg, Germany
- Cluster of Excellence Hearing4All, University of Oldenburg, Oldenburg, Germany
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Dettmers C, Braun N, Büsching I, Hassa T, Debener S, Liepert J. [Neurofeedback-based motor imagery training for rehabilitation after stroke]. Nervenarzt 2017; 87:1074-1081. [PMID: 27573884 DOI: 10.1007/s00115-016-0185-y] [Citation(s) in RCA: 3] [Impact Index Per Article: 0.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 11/28/2022]
Abstract
Mental training, including motor observation and motor imagery, has awakened much academic interest. The presumed functional equivalence of motor imagery and motor execution has given hope that mental training could be used for motor rehabilitation after a stroke. Results obtained from randomized controlled trials have shown mixed results. Approximately half of the studies demonstrate positive effects of motor imagery training but the rest do not show an additional benefit. Possible reasons why motor imagery training has so far not become established as a robust therapeutic approach are discussed in detail. Moreover, more recent approaches, such as neurofeedback-based motor imagery or closed-loop systems are presented and the potential importance for motor learning and rehabilitation after a stroke is discussed.
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Affiliation(s)
- C Dettmers
- Kliniken Schmieder Konstanz, Eichhornstr.68, 78464, Konstanz, Deutschland.
| | - N Braun
- Abteilung für Neuropsychologie, Department für Psychologie, Fakultät VI - Medizin und Gesundheitswissenschaften, Universität Oldenburg, Oldenburg, Deutschland
| | - I Büsching
- Kliniken Schmieder Allensbach, Allensbach, Deutschland
| | - T Hassa
- Kliniken Schmieder Allensbach, Allensbach, Deutschland.,Lurija Institut, Konstanz, Deutschland
| | - S Debener
- Abteilung für Neuropsychologie, Department für Psychologie, Fakultät VI - Medizin und Gesundheitswissenschaften, Universität Oldenburg, Oldenburg, Deutschland
| | - J Liepert
- Kliniken Schmieder Allensbach, Allensbach, Deutschland
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Liepert J, Büsching I, Sehle A, Schoenfeld MA. Mental chronometry and mental rotation abilities in stroke patients with different degrees of sensory deficit. Restor Neurol Neurosci 2016; 34:907-914. [PMID: 27689548 DOI: 10.3233/rnn-160640] [Citation(s) in RCA: 11] [Impact Index Per Article: 1.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/15/2022]
Abstract
BACKGROUND Motor imagery is used for treatment of motor deficits after stroke. Clinical observations suggested that motor imagery abilities might be reduced in patients with severe sensory deficits. This study investigated the influence of somatosensory deficits on temporal (mental chronometry, MC) and spatial aspects of motor imagery abilities. METHODS Stroke patients (n = 70; <6 months after stroke) were subdivided into 3 groups according to their somatosensory functions. Group 1 (n = 31) had no sensory deficits, group 2 (n = 27) had a mild to moderate sensory impairment and group 3 (n = 12) had severe sensory deficits. Patients and a healthy age-matched control group (n = 23) participated in a mental chronometry task (Box and Block Test, BBT) and a mental rotation task (Hand Identification Test, HIT). MC abilities were expressed as a ratio (motor execution time-motor imagery time/motor execution time). RESULTS MC for the affected hand was significantly impaired in group 3 in comparison to stroke patients of group 1 (p = 0.006), group 2 (p = 0.005) and healthy controls (p < 0.001). For the non-affected hand MC was similar across all groups. Stroke patients had a slower BBT motor execution than healthy controls (p < 0.001), and group 1 executed the task faster than group 3 (p = 0.002). The percentage of correct responses in the HIT was similar for all groups. CONCLUSION Severe sensory deficits impair mental chronometry abilities but have no impact on mental rotation abilities. Future studies should explore whether the presence of severe sensory deficits in stroke patients reduces the benefit from motor imagery therapy.
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Affiliation(s)
- Joachim Liepert
- Department of Neurorehabilitation, Kliniken Schmieder, Allensbach, Germany
| | - Imke Büsching
- Department of Neurorehabilitation, Kliniken Schmieder, Allensbach, Germany
| | - Aida Sehle
- Department of Neurorehabilitation, Kliniken Schmieder, Allensbach, Germany
| | - Mircea Ariel Schoenfeld
- Department of Behavioural Neurology, Leibniz Institute for Neurobiology, Magdeburg, Germany.,Department of Neurology, Otto-von-Guericke University, Magdeburg, Germany
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Sehle A, Büsching I, Vogt E, Liepert J. Temporary deafferentation evoked by cutaneous anesthesia: behavioral and electrophysiological findings in healthy subjects. J Neural Transm (Vienna) 2016; 123:473-80. [PMID: 26983925 DOI: 10.1007/s00702-016-1537-2] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 10/20/2015] [Accepted: 02/28/2016] [Indexed: 01/31/2023]
Abstract
Motor function and motor excitability can be modulated by changes of somatosensory input. Here, we performed a randomized single-blind trial to investigate behavioral and neurophysiological changes during temporary deafferentation of left upper arm and forearm in 31 right-handed healthy adults. Lidocaine cream was used to anesthetize the skin from wrist to shoulder, sparing the hand. As control condition, on a different day, a neutral cream was applied to the same skin area. The sequence (first Lidocaine, then placebo or vice versa) was randomized. Behavioral measures included the Grating Orientation Task, the Von Frey hair testing and the Nine-hole-peg-test. Transcranial magnetic stimulation was used to investigate short-interval intracortical inhibition, stimulus response curves, motor evoked potential amplitudes during pre-innervation and the cortical silent period (CSP). Recordings were obtained from left first dorsal interosseous muscle and from left flexor carpi radialis muscle. During deafferentation, the threshold of touch measured at the forearm was significantly worse. Other behavioral treatment-related changes were not found. The CSP showed a significant interaction between treatment and time in first dorsal interosseous muscle. CSP duration was longer during Lidocaine application and shorter during placebo exposure. We conclude that, in healthy subjects, temporary cutaneous deafferentation of upper and lower arm may have minor effects on motor inhibition, but not on sensory or motor function for the adjacent non-anesthetized hand.
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Affiliation(s)
- Aida Sehle
- Kliniken Schmieder Allensbach, Lurija Institut, Zum Tafelholz 8, 78476, Allensbach, Germany.
| | - Imke Büsching
- Kliniken Schmieder Allensbach, Lurija Institut, Zum Tafelholz 8, 78476, Allensbach, Germany
| | - Eva Vogt
- Kliniken Schmieder Allensbach, Lurija Institut, Zum Tafelholz 8, 78476, Allensbach, Germany
| | - Joachim Liepert
- Kliniken Schmieder Allensbach, Lurija Institut, Zum Tafelholz 8, 78476, Allensbach, Germany
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Büsching I, Sehle A, Liepert J. P153. Correlation of cortical inhibition and motor performance after mental training with the hand in patients after stroke. Clin Neurophysiol 2015. [DOI: 10.1016/j.clinph.2015.04.223] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/16/2022]
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Abramowski A, Acero F, Aharonian F, Akhperjanian AG, Anton G, Barnacka A, de Almeida UB, Bazer-Bachi AR, Becherini Y, Becker J, Behera B, Bernlöhr K, Bochow A, Boisson C, Bolmont J, Bordas P, Borrel V, Brucker J, Brun F, Brun P, Bulik T, Büsching I, Carrigan S, Casanova S, Cerruti M, Chadwick PM, Charbonnier A, Chaves RCG, Cheesebrough A, Chounet LM, Clapson AC, Coignet G, Conrad J, Dalton M, Daniel MK, Davids ID, Degrange B, Deil C, Dickinson HJ, Djannati-Ataï A, Domainko W, Drury LO, Dubois F, Dubus G, Dyks J, Dyrda M, Egberts K, Eger P, Espigat P, Fallon L, Farnier C, Fegan S, Feinstein F, Fernandes MV, Fiasson A, Fontaine G, Förster A, Füssling M, Gallant YA, Gast H, Gérard L, Gerbig D, Giebels B, Glicenstein JF, Glück B, Goret P, Göring D, Hague JD, Hampf D, Hauser M, Heinz S, Heinzelmann G, Henri G, Hermann G, Hinton JA, Hoffmann A, Hofmann W, Hofverberg P, Horns D, Jacholkowska A, de Jager OC, Jahn C, Jamrozy M, Jung I, Kastendieck MA, Katarzyński K, Katz U, Kaufmann S, Keogh D, Kerschhaggl M, Khangulyan D, Khélifi B, Klochkov D, Kluźniak W, Kneiske T, Komin N, Kosack K, Kossakowski R, Laffon H, Lamanna G, Lennarz D, Lohse T, Lopatin A, Lu CC, Marandon V, Marcowith A, Masbou J, Maurin D, Maxted N, McComb TJL, Medina MC, Méhault J, Moderski R, Moulin E, Naumann CL, Naumann-Godo M, de Naurois M, Nedbal D, Nekrassov D, Nguyen N, Nicholas B, Niemiec J, Nolan SJ, Ohm S, Olive JF, Wilhelmi EDO, Opitz B, Ostrowski M, Panter M, Arribas MP, Pedaletti G, Pelletier G, Petrucci PO, Pita S, Pühlhofer G, Punch M, Quirrenbach A, Raue M, Rayner SM, Reimer A, Reimer O, Renaud M, de los Reyes R, Rieger F, Ripken J, Rob L, Rosier-Lees S, Rowell G, Rudak B, Rulten CB, Ruppel J, Ryde F, Sahakian V, Santangelo A, Schlickeiser R, Schöck FM, Schönwald A, Schwanke U, Schwarzburg S, Schwemmer S, Shalchi A, Sikora M, Skilton JL, Sol H, Spengler G, Stawarz Ł, Steenkamp R, Stegmann C, Stinzing F, Sushch I, Szostek A, Tavernet JP, Terrier R, Tibolla O, Tluczykont M, Valerius K, van Eldik C, Vasileiadis G, Venter C, Vialle JP, Viana A, Vincent P, Vivier M, Völk HJ, Volpe F, Vorobiov S, Vorster M, Wagner SJ, Ward M, Wierzcholska A, Zajczyk A, Zdziarski AA, Zech A, Zechlin HS. Search for a dark matter annihilation signal from the galactic center halo with H.E.S.S. Phys Rev Lett 2011; 106:161301. [PMID: 21599352 DOI: 10.1103/physrevlett.106.161301] [Citation(s) in RCA: 10] [Impact Index Per Article: 0.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 11/04/2010] [Revised: 01/12/2011] [Indexed: 05/30/2023]
Abstract
A search for a very-high-energy (VHE; ≥100 GeV) γ-ray signal from self-annihilating particle dark matter (DM) is performed towards a region of projected distance r∼45-150 pc from the Galactic center. The background-subtracted γ-ray spectrum measured with the High Energy Stereoscopic System (H.E.S.S.) γ-ray instrument in the energy range between 300 GeV and 30 TeV shows no hint of a residual γ-ray flux. Assuming conventional Navarro-Frenk-White and Einasto density profiles, limits are derived on the velocity-weighted annihilation cross section (σv) as a function of the DM particle mass. These are among the best reported so far for this energy range and in particular differ only little between the chosen density profile parametrizations. In particular, for the DM particle mass of ∼1 TeV, values for (σv) above 3×10(-25) cm(3) s(-1) are excluded for the Einasto density profile.
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Affiliation(s)
- A Abramowski
- Universität Hamburg, Institut für Experimentalphysik, Hamburg, Germany
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Acero F, Aharonian F, Akhperjanian AG, Anton G, Barres de Almeida U, Bazer-Bachi AR, Becherini Y, Behera B, Bernlöhr K, Bochow A, Boisson C, Bolmont J, Borrel V, Brucker J, Brun F, Brun P, Bühler R, Bulik T, Büsching I, Boutelier T, Chadwick PM, Charbonnier A, Chaves RCG, Cheesebrough A, Chounet LM, Clapson AC, Coignet G, Dalton M, Daniel MK, Davids ID, Degrange B, Deil C, Dickinson HJ, Djannati-Ataï A, Domainko W, Drury LO, Dubois F, Dubus G, Dyks J, Dyrda M, Egberts K, Emmanoulopoulos D, Espigat P, Farnier C, Fegan S, Feinstein F, Fiasson A, Förster A, Fontaine G, Füßling M, Gabici S, Gallant YA, Gérard L, Gerbig D, Giebels B, Glicenstein JF, Glück B, Goret P, Göring D, Hauser D, Hauser M, Heinz S, Heinzelmann G, Henri G, Hermann G, Hinton JA, Hoffmann A, Hofmann W, Hofverberg P, Hoppe S, Horns D, Jacholkowska A, de Jager OC, Jahn C, Jung I, Katarzyński K, Katz U, Kaufmann S, Kerschhaggl M, Khangulyan D, Khélifi B, Keogh D, Klochkov D, Kluźniak W, Kneiske T, Komin N, Kosack K, Kossakowski R, Lamanna G, Lenain JP, Lohse T, Marandon V, Martineau-Huynh O, Marcowith A, Masbou J, Maurin D, McComb TJL, Medina MC, Méhault J, Moderski R, Moulin E, Naumann-Godo M, de Naurois M, Nedbal D, Nekrassov D, Nicholas B, Niemiec J, Nolan SJ, Ohm S, Olive JF, Wilhelmi EDO, Orford KJ, Ostrowski M, Panter M, Arribas MP, Pedaletti G, Pelletier G, Petrucci PO, Pita S, Pühlhofer G, Punch M, Quirrenbach A, Raubenheimer BC, Raue M, Rayner SM, Reimer O, Renaud M, Rieger F, Ripken J, Rob L, Rosier-Lees S, Rowell G, Rudak B, Rulten CB, Ruppel J, Sahakian V, Santangelo A, Schlickeiser R, Schöck FM, Schwanke U, Schwarzburg S, Schwemmer S, Shalchi A, Sikora M, Skilton JL, Sol H, Stawarz Ł, Steenkamp R, Stegmann C, Stinzing F, Superina G, Szostek A, Tam PH, Tavernet JP, Terrier R, Tibolla O, Tluczykont M, van Eldik C, Vasileiadis G, Venter C, Venter L, Vialle JP, Vincent P, Vivier M, Völk HJ, Volpe F, Wagner SJ, Ward M, Zdziarski AA, Zech A. Detection of Gamma Rays from a Starburst Galaxy. Science 2009; 326:1080-2. [DOI: 10.1126/science.1178826] [Citation(s) in RCA: 151] [Impact Index Per Article: 10.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
Affiliation(s)
- F. Acero
- Laboratoire de Physique Théorique et Astroparticules, Université Montpellier 2, CNRS/IN2P3, CC 70, Place Eugène Bataillon, F-34095 Montpellier Cedex 5, France
| | - F. Aharonian
- Max-Planck-Institut für Kernphysik, P.O. Box 103980, D 69029 Heidelberg, Germany
- Dublin Institute for Advanced Studies, 5 Merrion Square, Dublin 2, Ireland
| | - A. G. Akhperjanian
- Yerevan Physics Institute, 2 Alikhanian Brothers Street, 375036 Yerevan, Armenia
| | - G. Anton
- Universität Erlangen-Nürnberg, Physikalisches Institut, Erwin-Rommel-Strasse 1, D 91058 Erlangen, Germany
| | | | - A. R. Bazer-Bachi
- Centre d’Etude Spatiale des Rayonnements, CNRS/UPS, 9 avenue du Colonel Roche, BP 4346, F-31029 Toulouse Cedex 4, France
| | - Y. Becherini
- Astroparticule et Cosmologie (APC), CNRS, Université Paris 7 Denis Diderot, 10, rue Alice Domon et Leonie Duquet, F-75205 Paris Cedex 13, France. UMR 7164 (CNRS, Université Paris VII, CEA, Observatoire de Paris)
| | - B. Behera
- Landessternwarte, Universität Heidelberg, Königstuhl, D 69117 Heidelberg, Germany
| | - K. Bernlöhr
- Max-Planck-Institut für Kernphysik, P.O. Box 103980, D 69029 Heidelberg, Germany
- Institut für Physik, Humboldt-Universität zu Berlin, Newtonstrasse 15, D 12489 Berlin, Germany
| | - A. Bochow
- Max-Planck-Institut für Kernphysik, P.O. Box 103980, D 69029 Heidelberg, Germany
| | - C. Boisson
- Laboratoire Univers et Théories, Observatoire de Paris, CNRS, Université Paris Diderot, 5 Place Jules Janssen, 92190 Meudon, France
| | - J. Bolmont
- Laboratoire de Physique Nucléaire et des Hautes Energies, Université Pierre et Marie Curie Paris 6, Université Denis Diderot Paris 7, CNRS/IN2P3, 4 Place Jussieu, F-75252, Paris Cedex 5, France
| | - V. Borrel
- Centre d’Etude Spatiale des Rayonnements, CNRS/UPS, 9 avenue du Colonel Roche, BP 4346, F-31029 Toulouse Cedex 4, France
| | - J. Brucker
- Universität Erlangen-Nürnberg, Physikalisches Institut, Erwin-Rommel-Strasse 1, D 91058 Erlangen, Germany
| | - F. Brun
- Laboratoire de Physique Nucléaire et des Hautes Energies, Université Pierre et Marie Curie Paris 6, Université Denis Diderot Paris 7, CNRS/IN2P3, 4 Place Jussieu, F-75252, Paris Cedex 5, France
| | - P. Brun
- Institut de Recherche sur les Lois Fondamentales de l’Univers/La Direction des Sciences de la Matière/Commissariat àl’Energie Atomique, CE Saclay, F-91191 Gif-sur-Yvette, Cedex, France
| | - R. Bühler
- Max-Planck-Institut für Kernphysik, P.O. Box 103980, D 69029 Heidelberg, Germany
| | - T. Bulik
- Astronomical Observatory, The University of Warsaw, Al. Ujazdowskie 4, 00-478 Warsaw, Poland
| | - I. Büsching
- Unit for Space Physics, North-West University, Potchefstroom 2520, South Africa
| | - T. Boutelier
- Laboratoire d’Astrophysique de Grenoble, Institut National des Sciences de l’Univers/CNRS, Université Joseph Fourier, BP 53, F-38041 Grenoble Cedex 9, France
| | - P. M. Chadwick
- University of Durham, Department of Physics, South Road, Durham DH1 3LE, UK
| | - A. Charbonnier
- Laboratoire de Physique Nucléaire et des Hautes Energies, Université Pierre et Marie Curie Paris 6, Université Denis Diderot Paris 7, CNRS/IN2P3, 4 Place Jussieu, F-75252, Paris Cedex 5, France
| | - R. C. G. Chaves
- Max-Planck-Institut für Kernphysik, P.O. Box 103980, D 69029 Heidelberg, Germany
| | - A. Cheesebrough
- University of Durham, Department of Physics, South Road, Durham DH1 3LE, UK
| | - L.-M. Chounet
- Laboratoire Leprince-Ringuet, Ecole Polytechnique, CNRS/IN2P3, F-91128 Palaiseau, France
| | - A. C. Clapson
- Max-Planck-Institut für Kernphysik, P.O. Box 103980, D 69029 Heidelberg, Germany
| | - G. Coignet
- Laboratoire d’Annecy-le-Vieux de Physique des Particules, Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - M. Dalton
- Institut für Physik, Humboldt-Universität zu Berlin, Newtonstrasse 15, D 12489 Berlin, Germany
| | - M. K. Daniel
- University of Durham, Department of Physics, South Road, Durham DH1 3LE, UK
| | - I. D. Davids
- Unit for Space Physics, North-West University, Potchefstroom 2520, South Africa
- University of Namibia, Private Bag 13301, Windhoek, Namibia
| | - B. Degrange
- Laboratoire Leprince-Ringuet, Ecole Polytechnique, CNRS/IN2P3, F-91128 Palaiseau, France
| | - C. Deil
- Max-Planck-Institut für Kernphysik, P.O. Box 103980, D 69029 Heidelberg, Germany
| | - H. J. Dickinson
- University of Durham, Department of Physics, South Road, Durham DH1 3LE, UK
| | - A. Djannati-Ataï
- Astroparticule et Cosmologie (APC), CNRS, Université Paris 7 Denis Diderot, 10, rue Alice Domon et Leonie Duquet, F-75205 Paris Cedex 13, France. UMR 7164 (CNRS, Université Paris VII, CEA, Observatoire de Paris)
| | - W. Domainko
- Max-Planck-Institut für Kernphysik, P.O. Box 103980, D 69029 Heidelberg, Germany
| | - L. O’C. Drury
- Dublin Institute for Advanced Studies, 5 Merrion Square, Dublin 2, Ireland
| | - F. Dubois
- Laboratoire d’Annecy-le-Vieux de Physique des Particules, Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - G. Dubus
- Laboratoire d’Astrophysique de Grenoble, Institut National des Sciences de l’Univers/CNRS, Université Joseph Fourier, BP 53, F-38041 Grenoble Cedex 9, France
| | - J. Dyks
- Nicolaus Copernicus Astronomical Center, ul. Bartycka 18, 00-716 Warsaw, Poland
| | - M. Dyrda
- Instytut Fizyki Jadrowej PAN, ul. Radzikowskiego 152, 31-342 Kraków, Poland
| | - K. Egberts
- Max-Planck-Institut für Kernphysik, P.O. Box 103980, D 69029 Heidelberg, Germany
| | - D. Emmanoulopoulos
- Landessternwarte, Universität Heidelberg, Königstuhl, D 69117 Heidelberg, Germany
| | - P. Espigat
- Astroparticule et Cosmologie (APC), CNRS, Université Paris 7 Denis Diderot, 10, rue Alice Domon et Leonie Duquet, F-75205 Paris Cedex 13, France. UMR 7164 (CNRS, Université Paris VII, CEA, Observatoire de Paris)
| | - C. Farnier
- Laboratoire de Physique Théorique et Astroparticules, Université Montpellier 2, CNRS/IN2P3, CC 70, Place Eugène Bataillon, F-34095 Montpellier Cedex 5, France
| | - S. Fegan
- Laboratoire Leprince-Ringuet, Ecole Polytechnique, CNRS/IN2P3, F-91128 Palaiseau, France
| | - F. Feinstein
- Laboratoire de Physique Théorique et Astroparticules, Université Montpellier 2, CNRS/IN2P3, CC 70, Place Eugène Bataillon, F-34095 Montpellier Cedex 5, France
| | - A. Fiasson
- Laboratoire d’Annecy-le-Vieux de Physique des Particules, Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - A. Förster
- Max-Planck-Institut für Kernphysik, P.O. Box 103980, D 69029 Heidelberg, Germany
| | - G. Fontaine
- Laboratoire Leprince-Ringuet, Ecole Polytechnique, CNRS/IN2P3, F-91128 Palaiseau, France
| | - M. Füßling
- Institut für Physik, Humboldt-Universität zu Berlin, Newtonstrasse 15, D 12489 Berlin, Germany
| | - S. Gabici
- Dublin Institute for Advanced Studies, 5 Merrion Square, Dublin 2, Ireland
| | - Y. A. Gallant
- Laboratoire de Physique Théorique et Astroparticules, Université Montpellier 2, CNRS/IN2P3, CC 70, Place Eugène Bataillon, F-34095 Montpellier Cedex 5, France
| | - L. Gérard
- Astroparticule et Cosmologie (APC), CNRS, Université Paris 7 Denis Diderot, 10, rue Alice Domon et Leonie Duquet, F-75205 Paris Cedex 13, France. UMR 7164 (CNRS, Université Paris VII, CEA, Observatoire de Paris)
| | - D. Gerbig
- Institut für Theoretische Physik, Lehrstuhl IV: Weltraum und Astrophysik, Ruhr-Universität Bochum, D 44780 Bochum, Germany
| | - B. Giebels
- Laboratoire Leprince-Ringuet, Ecole Polytechnique, CNRS/IN2P3, F-91128 Palaiseau, France
| | - J. F. Glicenstein
- Institut de Recherche sur les Lois Fondamentales de l’Univers/La Direction des Sciences de la Matière/Commissariat àl’Energie Atomique, CE Saclay, F-91191 Gif-sur-Yvette, Cedex, France
| | - B. Glück
- Universität Erlangen-Nürnberg, Physikalisches Institut, Erwin-Rommel-Strasse 1, D 91058 Erlangen, Germany
| | - P. Goret
- Institut de Recherche sur les Lois Fondamentales de l’Univers/La Direction des Sciences de la Matière/Commissariat àl’Energie Atomique, CE Saclay, F-91191 Gif-sur-Yvette, Cedex, France
| | - D. Göring
- Universität Erlangen-Nürnberg, Physikalisches Institut, Erwin-Rommel-Strasse 1, D 91058 Erlangen, Germany
| | - D. Hauser
- Landessternwarte, Universität Heidelberg, Königstuhl, D 69117 Heidelberg, Germany
| | - M. Hauser
- Landessternwarte, Universität Heidelberg, Königstuhl, D 69117 Heidelberg, Germany
| | - S. Heinz
- Universität Erlangen-Nürnberg, Physikalisches Institut, Erwin-Rommel-Strasse 1, D 91058 Erlangen, Germany
| | - G. Heinzelmann
- Universität Hamburg, Institut für Experimentalphysik, Luruper Chaussee 149, D 22761 Hamburg, Germany
| | - G. Henri
- Laboratoire d’Astrophysique de Grenoble, Institut National des Sciences de l’Univers/CNRS, Université Joseph Fourier, BP 53, F-38041 Grenoble Cedex 9, France
| | - G. Hermann
- Max-Planck-Institut für Kernphysik, P.O. Box 103980, D 69029 Heidelberg, Germany
| | - J. A. Hinton
- School of Physics and Astronomy, University of Leeds, Leeds LS2 9JT, UK
| | - A. Hoffmann
- Institut für Astronomie und Astrophysik, Universität Tübingen, Sand 1, D 72076 Tübingen, Germany
| | - W. Hofmann
- Max-Planck-Institut für Kernphysik, P.O. Box 103980, D 69029 Heidelberg, Germany
| | - P. Hofverberg
- Max-Planck-Institut für Kernphysik, P.O. Box 103980, D 69029 Heidelberg, Germany
| | - S. Hoppe
- Max-Planck-Institut für Kernphysik, P.O. Box 103980, D 69029 Heidelberg, Germany
| | - D. Horns
- Universität Hamburg, Institut für Experimentalphysik, Luruper Chaussee 149, D 22761 Hamburg, Germany
| | - A. Jacholkowska
- Laboratoire de Physique Nucléaire et des Hautes Energies, Université Pierre et Marie Curie Paris 6, Université Denis Diderot Paris 7, CNRS/IN2P3, 4 Place Jussieu, F-75252, Paris Cedex 5, France
| | - O. C. de Jager
- Unit for Space Physics, North-West University, Potchefstroom 2520, South Africa
| | - C. Jahn
- Universität Erlangen-Nürnberg, Physikalisches Institut, Erwin-Rommel-Strasse 1, D 91058 Erlangen, Germany
| | - I. Jung
- Universität Erlangen-Nürnberg, Physikalisches Institut, Erwin-Rommel-Strasse 1, D 91058 Erlangen, Germany
| | - K. Katarzyński
- Toruń Centre for Astronomy, Nicolaus Copernicus University, ul. Gagarina 11, 87-100 Toruń, Poland
| | - U. Katz
- Universität Erlangen-Nürnberg, Physikalisches Institut, Erwin-Rommel-Strasse 1, D 91058 Erlangen, Germany
| | - S. Kaufmann
- Landessternwarte, Universität Heidelberg, Königstuhl, D 69117 Heidelberg, Germany
| | - M. Kerschhaggl
- Institut für Physik, Humboldt-Universität zu Berlin, Newtonstrasse 15, D 12489 Berlin, Germany
| | - D. Khangulyan
- Max-Planck-Institut für Kernphysik, P.O. Box 103980, D 69029 Heidelberg, Germany
| | - B. Khélifi
- Laboratoire Leprince-Ringuet, Ecole Polytechnique, CNRS/IN2P3, F-91128 Palaiseau, France
| | - D. Keogh
- University of Durham, Department of Physics, South Road, Durham DH1 3LE, UK
| | - D. Klochkov
- Institut für Astronomie und Astrophysik, Universität Tübingen, Sand 1, D 72076 Tübingen, Germany
| | - W. Kluźniak
- Nicolaus Copernicus Astronomical Center, ul. Bartycka 18, 00-716 Warsaw, Poland
| | - T. Kneiske
- Universität Hamburg, Institut für Experimentalphysik, Luruper Chaussee 149, D 22761 Hamburg, Germany
| | - Nu. Komin
- Institut de Recherche sur les Lois Fondamentales de l’Univers/La Direction des Sciences de la Matière/Commissariat àl’Energie Atomique, CE Saclay, F-91191 Gif-sur-Yvette, Cedex, France
| | - K. Kosack
- Max-Planck-Institut für Kernphysik, P.O. Box 103980, D 69029 Heidelberg, Germany
| | - R. Kossakowski
- Laboratoire d’Annecy-le-Vieux de Physique des Particules, Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - G. Lamanna
- Laboratoire d’Annecy-le-Vieux de Physique des Particules, Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - J.-P. Lenain
- Laboratoire Univers et Théories, Observatoire de Paris, CNRS, Université Paris Diderot, 5 Place Jules Janssen, 92190 Meudon, France
| | - T. Lohse
- Institut für Physik, Humboldt-Universität zu Berlin, Newtonstrasse 15, D 12489 Berlin, Germany
| | - V. Marandon
- Astroparticule et Cosmologie (APC), CNRS, Université Paris 7 Denis Diderot, 10, rue Alice Domon et Leonie Duquet, F-75205 Paris Cedex 13, France. UMR 7164 (CNRS, Université Paris VII, CEA, Observatoire de Paris)
| | - O. Martineau-Huynh
- Laboratoire de Physique Nucléaire et des Hautes Energies, Université Pierre et Marie Curie Paris 6, Université Denis Diderot Paris 7, CNRS/IN2P3, 4 Place Jussieu, F-75252, Paris Cedex 5, France
| | - A. Marcowith
- Laboratoire de Physique Théorique et Astroparticules, Université Montpellier 2, CNRS/IN2P3, CC 70, Place Eugène Bataillon, F-34095 Montpellier Cedex 5, France
| | - J. Masbou
- Laboratoire d’Annecy-le-Vieux de Physique des Particules, Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - D. Maurin
- Laboratoire de Physique Nucléaire et des Hautes Energies, Université Pierre et Marie Curie Paris 6, Université Denis Diderot Paris 7, CNRS/IN2P3, 4 Place Jussieu, F-75252, Paris Cedex 5, France
| | - T. J. L. McComb
- University of Durham, Department of Physics, South Road, Durham DH1 3LE, UK
| | - M. C. Medina
- Laboratoire Univers et Théories, Observatoire de Paris, CNRS, Université Paris Diderot, 5 Place Jules Janssen, 92190 Meudon, France
| | - J. Méhault
- Laboratoire de Physique Théorique et Astroparticules, Université Montpellier 2, CNRS/IN2P3, CC 70, Place Eugène Bataillon, F-34095 Montpellier Cedex 5, France
| | - R. Moderski
- Nicolaus Copernicus Astronomical Center, ul. Bartycka 18, 00-716 Warsaw, Poland
| | - E. Moulin
- Laboratoire Univers et Théories, Observatoire de Paris, CNRS, Université Paris Diderot, 5 Place Jules Janssen, 92190 Meudon, France
| | - M. Naumann-Godo
- Laboratoire Leprince-Ringuet, Ecole Polytechnique, CNRS/IN2P3, F-91128 Palaiseau, France
| | - M. de Naurois
- Laboratoire de Physique Nucléaire et des Hautes Energies, Université Pierre et Marie Curie Paris 6, Université Denis Diderot Paris 7, CNRS/IN2P3, 4 Place Jussieu, F-75252, Paris Cedex 5, France
| | - D. Nedbal
- Charles University, Faculty of Mathematics and Physics, Institute of Particle and Nuclear Physics, V Holesovickách 2, 180 00, Prague, Czech Republic
| | - D. Nekrassov
- Max-Planck-Institut für Kernphysik, P.O. Box 103980, D 69029 Heidelberg, Germany
| | - B. Nicholas
- School of Chemistry and Physics, University of Adelaide, Adelaide 5005, Australia
| | - J. Niemiec
- Instytut Fizyki Jadrowej PAN, ul. Radzikowskiego 152, 31-342 Kraków, Poland
| | - S. J. Nolan
- University of Durham, Department of Physics, South Road, Durham DH1 3LE, UK
| | - S. Ohm
- Max-Planck-Institut für Kernphysik, P.O. Box 103980, D 69029 Heidelberg, Germany
| | - J-F. Olive
- Centre d’Etude Spatiale des Rayonnements, CNRS/UPS, 9 avenue du Colonel Roche, BP 4346, F-31029 Toulouse Cedex 4, France
| | - E. de Oña Wilhelmi
- Max-Planck-Institut für Kernphysik, P.O. Box 103980, D 69029 Heidelberg, Germany
| | - K. J. Orford
- University of Durham, Department of Physics, South Road, Durham DH1 3LE, UK
| | - M. Ostrowski
- Obserwatorium Astronomiczne, Uniwersytet Jagielloński, ul. Orla 171, 30-244 Kraków, Poland
| | - M. Panter
- Max-Planck-Institut für Kernphysik, P.O. Box 103980, D 69029 Heidelberg, Germany
| | - M. Paz Arribas
- Institut für Physik, Humboldt-Universität zu Berlin, Newtonstrasse 15, D 12489 Berlin, Germany
| | - G. Pedaletti
- Landessternwarte, Universität Heidelberg, Königstuhl, D 69117 Heidelberg, Germany
| | - G. Pelletier
- Laboratoire d’Astrophysique de Grenoble, Institut National des Sciences de l’Univers/CNRS, Université Joseph Fourier, BP 53, F-38041 Grenoble Cedex 9, France
| | - P.-O. Petrucci
- Laboratoire d’Astrophysique de Grenoble, Institut National des Sciences de l’Univers/CNRS, Université Joseph Fourier, BP 53, F-38041 Grenoble Cedex 9, France
| | - S. Pita
- Astroparticule et Cosmologie (APC), CNRS, Université Paris 7 Denis Diderot, 10, rue Alice Domon et Leonie Duquet, F-75205 Paris Cedex 13, France. UMR 7164 (CNRS, Université Paris VII, CEA, Observatoire de Paris)
| | - G. Pühlhofer
- Landessternwarte, Universität Heidelberg, Königstuhl, D 69117 Heidelberg, Germany
- Institut für Astronomie und Astrophysik, Universität Tübingen, Sand 1, D 72076 Tübingen, Germany
| | - M. Punch
- Astroparticule et Cosmologie (APC), CNRS, Université Paris 7 Denis Diderot, 10, rue Alice Domon et Leonie Duquet, F-75205 Paris Cedex 13, France. UMR 7164 (CNRS, Université Paris VII, CEA, Observatoire de Paris)
| | - A. Quirrenbach
- Landessternwarte, Universität Heidelberg, Königstuhl, D 69117 Heidelberg, Germany
| | - B. C. Raubenheimer
- Unit for Space Physics, North-West University, Potchefstroom 2520, South Africa
| | - M. Raue
- Max-Planck-Institut für Kernphysik, P.O. Box 103980, D 69029 Heidelberg, Germany
- European Associated Laboratory for Gamma-Ray Astronomy, 4 Place Jussieu, F-75252, Paris Cedex 5, France
| | - S. M. Rayner
- University of Durham, Department of Physics, South Road, Durham DH1 3LE, UK
| | - O. Reimer
- Institut für Astro und Teilchenphysik, Leopold-Franzens-Universität Innsbruck, A6020 Innsbruck, Austria
- KIPAC Kavli Institute for Particle Physics and Cosmology, Stanford University, Stanford, CA 94305, USA
| | - M. Renaud
- Max-Planck-Institut für Kernphysik, P.O. Box 103980, D 69029 Heidelberg, Germany
- Astroparticule et Cosmologie (APC), CNRS, Université Paris 7 Denis Diderot, 10, rue Alice Domon et Leonie Duquet, F-75205 Paris Cedex 13, France. UMR 7164 (CNRS, Université Paris VII, CEA, Observatoire de Paris)
| | - F. Rieger
- Max-Planck-Institut für Kernphysik, P.O. Box 103980, D 69029 Heidelberg, Germany
- European Associated Laboratory for Gamma-Ray Astronomy, 4 Place Jussieu, F-75252, Paris Cedex 5, France
| | - J. Ripken
- Universität Hamburg, Institut für Experimentalphysik, Luruper Chaussee 149, D 22761 Hamburg, Germany
| | - L. Rob
- Charles University, Faculty of Mathematics and Physics, Institute of Particle and Nuclear Physics, V Holesovickách 2, 180 00, Prague, Czech Republic
| | - S. Rosier-Lees
- Laboratoire d’Annecy-le-Vieux de Physique des Particules, Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - G. Rowell
- School of Chemistry and Physics, University of Adelaide, Adelaide 5005, Australia
| | - B. Rudak
- Nicolaus Copernicus Astronomical Center, ul. Bartycka 18, 00-716 Warsaw, Poland
| | - C. B. Rulten
- University of Durham, Department of Physics, South Road, Durham DH1 3LE, UK
| | - J. Ruppel
- Institut für Theoretische Physik, Lehrstuhl IV: Weltraum und Astrophysik, Ruhr-Universität Bochum, D 44780 Bochum, Germany
| | - V. Sahakian
- Yerevan Physics Institute, 2 Alikhanian Brothers Street, 375036 Yerevan, Armenia
| | - A. Santangelo
- Institut für Astronomie und Astrophysik, Universität Tübingen, Sand 1, D 72076 Tübingen, Germany
| | - R. Schlickeiser
- Institut für Theoretische Physik, Lehrstuhl IV: Weltraum und Astrophysik, Ruhr-Universität Bochum, D 44780 Bochum, Germany
| | - F. M. Schöck
- Universität Erlangen-Nürnberg, Physikalisches Institut, Erwin-Rommel-Strasse 1, D 91058 Erlangen, Germany
| | - U. Schwanke
- Institut für Physik, Humboldt-Universität zu Berlin, Newtonstrasse 15, D 12489 Berlin, Germany
| | - S. Schwarzburg
- Institut für Astronomie und Astrophysik, Universität Tübingen, Sand 1, D 72076 Tübingen, Germany
| | - S. Schwemmer
- Landessternwarte, Universität Heidelberg, Königstuhl, D 69117 Heidelberg, Germany
| | - A. Shalchi
- Institut für Theoretische Physik, Lehrstuhl IV: Weltraum und Astrophysik, Ruhr-Universität Bochum, D 44780 Bochum, Germany
| | - M. Sikora
- Nicolaus Copernicus Astronomical Center, ul. Bartycka 18, 00-716 Warsaw, Poland
| | - J. L. Skilton
- School of Physics and Astronomy, University of Leeds, Leeds LS2 9JT, UK
| | - H. Sol
- Laboratoire Univers et Théories, Observatoire de Paris, CNRS, Université Paris Diderot, 5 Place Jules Janssen, 92190 Meudon, France
| | - Ł. Stawarz
- Obserwatorium Astronomiczne, Uniwersytet Jagielloński, ul. Orla 171, 30-244 Kraków, Poland
| | - R. Steenkamp
- University of Namibia, Private Bag 13301, Windhoek, Namibia
| | - C. Stegmann
- Universität Erlangen-Nürnberg, Physikalisches Institut, Erwin-Rommel-Strasse 1, D 91058 Erlangen, Germany
| | - F. Stinzing
- Universität Erlangen-Nürnberg, Physikalisches Institut, Erwin-Rommel-Strasse 1, D 91058 Erlangen, Germany
| | - G. Superina
- Laboratoire Leprince-Ringuet, Ecole Polytechnique, CNRS/IN2P3, F-91128 Palaiseau, France
| | - A. Szostek
- Laboratoire d’Astrophysique de Grenoble, Institut National des Sciences de l’Univers/CNRS, Université Joseph Fourier, BP 53, F-38041 Grenoble Cedex 9, France
- Obserwatorium Astronomiczne, Uniwersytet Jagielloński, ul. Orla 171, 30-244 Kraków, Poland
| | - P. H. Tam
- Landessternwarte, Universität Heidelberg, Königstuhl, D 69117 Heidelberg, Germany
| | - J.-P. Tavernet
- Laboratoire de Physique Nucléaire et des Hautes Energies, Université Pierre et Marie Curie Paris 6, Université Denis Diderot Paris 7, CNRS/IN2P3, 4 Place Jussieu, F-75252, Paris Cedex 5, France
| | - R. Terrier
- Astroparticule et Cosmologie (APC), CNRS, Université Paris 7 Denis Diderot, 10, rue Alice Domon et Leonie Duquet, F-75205 Paris Cedex 13, France. UMR 7164 (CNRS, Université Paris VII, CEA, Observatoire de Paris)
| | - O. Tibolla
- Max-Planck-Institut für Kernphysik, P.O. Box 103980, D 69029 Heidelberg, Germany
| | - M. Tluczykont
- Universität Hamburg, Institut für Experimentalphysik, Luruper Chaussee 149, D 22761 Hamburg, Germany
| | - C. van Eldik
- Max-Planck-Institut für Kernphysik, P.O. Box 103980, D 69029 Heidelberg, Germany
| | - G. Vasileiadis
- Laboratoire de Physique Théorique et Astroparticules, Université Montpellier 2, CNRS/IN2P3, CC 70, Place Eugène Bataillon, F-34095 Montpellier Cedex 5, France
| | - C. Venter
- Unit for Space Physics, North-West University, Potchefstroom 2520, South Africa
| | - L. Venter
- Laboratoire Univers et Théories, Observatoire de Paris, CNRS, Université Paris Diderot, 5 Place Jules Janssen, 92190 Meudon, France
| | - J. P. Vialle
- Laboratoire d’Annecy-le-Vieux de Physique des Particules, Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - P. Vincent
- Laboratoire de Physique Nucléaire et des Hautes Energies, Université Pierre et Marie Curie Paris 6, Université Denis Diderot Paris 7, CNRS/IN2P3, 4 Place Jussieu, F-75252, Paris Cedex 5, France
| | - M. Vivier
- Institut de Recherche sur les Lois Fondamentales de l’Univers/La Direction des Sciences de la Matière/Commissariat àl’Energie Atomique, CE Saclay, F-91191 Gif-sur-Yvette, Cedex, France
| | - H. J. Völk
- Max-Planck-Institut für Kernphysik, P.O. Box 103980, D 69029 Heidelberg, Germany
| | - F. Volpe
- Max-Planck-Institut für Kernphysik, P.O. Box 103980, D 69029 Heidelberg, Germany
| | - S. J. Wagner
- Landessternwarte, Universität Heidelberg, Königstuhl, D 69117 Heidelberg, Germany
| | - M. Ward
- University of Durham, Department of Physics, South Road, Durham DH1 3LE, UK
| | - A. A. Zdziarski
- Nicolaus Copernicus Astronomical Center, ul. Bartycka 18, 00-716 Warsaw, Poland
| | - A. Zech
- Laboratoire Univers et Théories, Observatoire de Paris, CNRS, Université Paris Diderot, 5 Place Jules Janssen, 92190 Meudon, France
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Acciari VA, Aliu E, Arlen T, Bautista M, Beilicke M, Benbow W, Bradbury SM, Buckley JH, Bugaev V, Butt Y, Byrum K, Cannon A, Celik O, Cesarini A, Chow YC, Ciupik L, Cogan P, Cui W, Dickherber R, Fegan SJ, Finley JP, Fortin P, Fortson L, Furniss A, Gall D, Gillanders GH, Grube J, Guenette R, Gyuk G, Hanna D, Holder J, Horan D, Hui CM, Humensky TB, Imran A, Kaaret P, Karlsson N, Kieda D, Kildea J, Konopelko A, Krawczynski H, Krennrich F, Lang MJ, LeBohec S, Maier G, McCann A, McCutcheon M, Millis J, Moriarty P, Ong RA, Otte AN, Pandel D, Perkins JS, Petry D, Pohl M, Quinn J, Ragan K, Reyes LC, Reynolds PT, Roache E, Roache E, Rose HJ, Schroedter M, Sembroski GH, Smith AW, Swordy SP, Theiling M, Toner JA, Varlotta A, Vincent S, Wakely SP, Ward JE, Weekes TC, Weinstein A, Williams DA, Wissel S, Wood M, Walker RC, Davies F, Hardee PE, Junor W, Ly C, Aharonian F, Akhperjanian AG, Anton G, Barres de Almeida U, Bazer-Bachi AR, Becherini Y, Behera B, Bernlöhr K, Bochow A, Boisson C, Bolmont J, Borrel V, Brucker J, Brun F, Brun P, Bühler R, Bulik T, Büsching I, Boutelier T, Chadwick PM, Charbonnier A, Chaves RCG, Cheesebrough A, Chounet LM, Clapson AC, Coignet G, Dalton M, Daniel MK, Davids ID, Degrange B, Deil C, Dickinson HJ, Djannati-Ataï A, Domainko W, Drury LO, Dubois F, Dubus G, Dyks J, Dyrda M, Egberts K, Emmanoulopoulos D, Espigat P, Farnier C, Feinstein F, Fiasson A, Förster A, Fontaine G, Füssling M, Gabici S, Gallant YA, Gérard L, Gerbig D, Giebels B, Glicenstein JF, Glück B, Goret P, Göhring D, Hauser D, Hauser M, Heinz S, Heinzelmann G, Henri G, Hermann G, Hinton JA, Hoffmann A, Hofmann W, Holleran M, Hoppe S, Horns D, Jacholkowska A, de Jager OC, Jahn C, Jung I, Katarzyński K, Katz U, Kaufmann S, Kendziorra E, Kerschhaggl M, Khangulyan D, Khélifi B, Keogh D, Kluźniak W, Kneiske T, Komin N, Kosack K, Lamanna G, Lenain JP, Lohse T, Marandon V, Martin JM, Martineau-Huynh O, Marcowith A, Maurin D, McComb TJL, Medina MC, Moderski R, Moulin E, Naumann-Godo M, de Naurois M, Nedbal D, Nekrassov D, Nicholas B, Niemiec J, Nolan SJ, Ohm S, Olive JF, de Oña Wilhelmi E, Orford KJ, Ostrowski M, Panter M, Paz Arribas M, Pedaletti G, Pelletier G, Petrucci PO, Pita S, Pühlhofer G, Punch M, Quirrenbach A, Raubenheimer BC, Raue M, Rayner SM, Renaud M, Rieger F, Ripken J, Rob L, Rosier-Lees S, Rowell G, Rudak B, Rulten CB, Ruppel J, Sahakian V, Santangelo A, Schlickeiser R, Schöck FM, Schröder R, Schwanke U, Schwarzburg S, Schwemmer S, Shalchi A, Sikora M, Skilton JL, Sol H, Spangler D, Stawarz Ł, Steenkamp R, Stegmann C, Stinzing F, Superina G, Szostek A, Tam PH, Tavernet JP, Terrier R, Tibolla O, Tluczykont M, van Eldik C, Vasileiadis G, Venter C, Venter L, Vialle JP, Vincent P, Vivier M, Völk HJ, Volpe F, Wagner SJ, Ward M, Zdziarski AA, Zech A, Anderhub H, Antonelli LA, Antoranz P, Backes M, Baixeras C, Balestra S, Barrio JA, Bastieri D, Becerra González J, Becker JK, Bednarek W, Berger K, Bernardini E, Biland A, Bock RK, Bonnoli G, Bordas P, Borla Tridon D, Bosch-Ramon V, Bose D, Braun I, Bretz T, Britvitch I, Camara M, Carmona E, Commichau S, Contreras JL, Cortina J, Costado MT, Covino S, Curtef V, Dazzi F, De Angelis A, De Cea del Pozo E, Delgado Mendez C, De los Reyes R, De Lotto B, De Maria M, De Sabata F, Dominguez A, Dorner D, Doro M, Elsaesser D, Errando M, Ferenc D, Fernández E, Firpo R, Fonseca MV, Font L, Galante N, García López RJ, Garczarczyk M, Gaug M, Goebel F, Hadasch D, Hayashida M, Herrero A, Hildebrand D, Höhne-Mönch D, Hose J, Hsu CC, Jogler T, Kranich D, La Barbera A, Laille A, Leonardo E, Lindfors E, Lombardi S, Longo F, López M, Lorenz E, Majumdar P, Maneva G, Mankuzhiyil N, Mannheim K, Maraschi L, Mariotti M, Martínez M, Mazin D, Meucci M, Miranda JM, Mirzoyan R, Miyamoto H, Moldón J, Moles M, Moralejo A, Nieto D, Nilsson K, Ninkovic J, Oya I, Paoletti R, Paredes JM, Pasanen M, Pascoli D, Pauss F, Pegna RG, Perez-Torres MA, Persic M, Peruzzo L, Prada F, Prandini E, Puchades N, Reichardt I, Rhode W, Ribó M, Rico J, Rissi M, Robert A, Rügamer S, Saggion A, Saito TY, Salvati M, Sanchez-Conde M, Satalecka K, Scalzotto V, Scapin V, Schweizer T, Shayduk M, Shore SN, Sidro N, Sierpowska-Bartosik A, Sillanpää A, Sitarek J, Sobczynska D, Spanier F, Stamerra A, Stark LS, Takalo L, Tavecchio F, Temnikov P, Tescaro D, Teshima M, Torres DF, Turini N, Vankov H, Wagner RM, Zabalza V, Zandanel F, Zanin R, Zapatero J. Radio Imaging of the Very-High-Energy γ-Ray Emission Region in the Central Engine of a Radio Galaxy. Science 2009; 325:444-8. [PMID: 19574351 DOI: 10.1126/science.1175406] [Citation(s) in RCA: 157] [Impact Index Per Article: 10.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/03/2022]
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Aharonian F, Akhperjanian AG, Barres de Almeida U, Bazer-Bachi AR, Becherini Y, Behera B, Benbow W, Bernlöhr K, Boisson C, Bochow A, Borrel V, Braun I, Brion E, Brucker J, Brun P, Brucker R, Bulik T, Büsching I, Boutelier T, Carrigan S, Chadwick PM, Charbonnier A, Chaves RCG, Cheesebrough A, Chounet LM, Clapson AC, Coignet G, Costamante L, Dalton M, Degrange B, Deil C, Dickinson HJ, Djannati-Ataï A, Domainko W, Drury LO, Dubois F, Dubus G, Dyks J, Dyrda M, Egberts K, Emmanoulopoulos D, Espigat P, Farnier C, Feinstein F, Fiasson A, Fontaine G, Füsling M, Gabici S, Gallant YA, Gérard L, Giebels B, Glicenstein JF, Glück B, Goret P, Hadjichristidis C, Hauser D, Hauser M, Heinz S, Heinzelmann G, Henri G, Hermann G, Hinton JA, Hoffmann A, Hofmann W, Holleran M, Hoppe S, Horns D, Jacholkowska A, de Jager OC, Jung I, Katarzyński K, Kaufmann S, Kendziorra E, Kerschhaggl M, Khangulyan D, Khélifi B, Keogh D, Komin N, Kosack K, Lamanna G, Lenain JP, Lohse T, Marandon V, Martin JM, Martineau-Huynh O, Marcowith A, Maurin D, McComb TJL, Medina C, Moderski R, Moulin E, Naumann-Godo M, de Naurois M, Nedbal D, Nekrassov D, Niemiec J, Nolan SJ, Ohm S, Olive JF, de Oña Wilhelmi E, Orford KJ, Osborne JL, Ostrowski M, Panter M, Pedaletti G, Pelletier G, Petrucci PO, Pita S, Pühlhofer G, Punch M, Quirrenbach A, Raubenheimer BC, Raue M, Rayner SM, Renaud M, Rieger F, Ripken J, Rob L, Rosier-Lees S, Rowell G, Rudak B, Rulten CB, Ruppel J, Sahakian V, Santangelo A, Schlickeiser R, Schöck FM, Schröder R, Schwanke U, Schwarzburg S, Schwemmer S, Shalchi A, Skilton JL, Sol H, Spangler D, Stawarz Ł, Steenkamp R, Stegmann C, Superina G, Tam PH, Tavernet JP, Terrier R, Tibolla O, van Eldik C, Vasileiadis G, Venter C, Vialle JP, Vincent P, Vivier M, Völk HJ, Volpe F, Wagner SJ, Ward M, Zdziarski AA, Zech A. Energy spectrum of cosmic-ray electrons at TeV energies. Phys Rev Lett 2008; 101:261104. [PMID: 19437632 DOI: 10.1103/physrevlett.101.261104] [Citation(s) in RCA: 34] [Impact Index Per Article: 2.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/27/2023]
Abstract
The very large collection area of ground-based gamma-ray telescopes gives them a substantial advantage over balloon or satellite based instruments in the detection of very-high-energy (>600 GeV) cosmic-ray electrons. Here we present the electron spectrum derived from data taken with the High Energy Stereoscopic System (H.E.S.S.) of imaging atmospheric Cherenkov telescopes. In this measurement, the first of this type, we are able to extend the measurement of the electron spectrum beyond the range accessible to direct measurements. We find evidence for a substantial steepening in the energy spectrum above 600 GeV compared to lower energies.
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Affiliation(s)
- F Aharonian
- Max-Planck-Institut für Kernphysik, P.O. Box 103980, D 69029 Heidelberg, Germany
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Aharonian F, Akhperjanian AG, Barres de Almeida U, Bazer-Bachi AR, Becherini Y, Behera B, Beilicke M, Benbow W, Bernlöhr K, Boisson C, Bochow A, Borrel V, Braun I, Brion E, Brucker J, Brun P, Bühler R, Bulik T, Büsching I, Boutelier T, Carrigan S, Chadwick PM, Charbonnier A, Chaves RCG, Chounet LM, Clapson AC, Coignet G, Costamante L, Dalton M, Degrange B, Deil C, Dickinson HJ, Djannati-Ataï A, Domainko W, Drury LO, Dubois F, Dubus G, Dyks J, Egberts K, Emmanoulopoulos D, Espigat P, Farnier C, Feinstein F, Fiasson A, Förster A, Fontaine G, Füssling M, Gabici S, Gallant YA, Gérard L, Giebels B, Glicenstein JF, Glück B, Goret P, Hadjichristidis C, Hauser D, Hauser M, Heinz S, Heinzelmann G, Henri G, Hermann G, Hinton JA, Hoffmann A, Hofmann W, Holleran M, Hoppe S, Horns D, Jacholkowska A, de Jager OC, Jung I, Katarzyński K, Kaufmann S, Kendziorra E, Kerschhaggl M, Khangulyan D, Khélifi B, Keogh D, Komin N, Kosack K, Lamanna G, Lenain JP, Lohse T, Marandon V, Martin JM, Martineau-Huynh O, Marcowith A, Maurin D, McComb TJL, Medina C, Moderski R, Moulin E, Naumann-Godo M, de Naurois M, Nedbal D, Nekrassov D, Niemiec J, Nolan SJ, Ohm S, Olive JF, de Oña Wilhelmi E, Orford KJ, Osborne JL, Ostrowski M, Panter M, Pedaletti G, Pelletier G, Petrucci PO, Pita S, Pühlhofer G, Punch M, Quirrenbach A, Raubenheimer BC, Raue M, Rayner SM, Renaud M, Rieger F, Ripken J, Rob L, Rosier-Lees S, Rowell G, Rudak B, Ruppel J, Sahakian V, Santangelo A, Schlickeiser R, Schöck FM, Schröder R, Schwanke U, Schwarzburg S, Schwemmer S, Shalchi A, Skilton JL, Sol H, Spangler D, Stawarz Ł, Steenkamp R, Stegmann C, Superina G, Tam PH, Tavernet JP, Terrier R, Tibolla O, van Eldik C, Vasileiadis G, Venter C, Vialle JP, Vincent P, Vivier M, Völk HJ, Volpe F, Wagner SJ, Ward M, Zdziarski AA, Zech A. Limits on an energy dependence of the speed of light from a flare of the active galaxy PKS 2155-304. Phys Rev Lett 2008; 101:170402. [PMID: 18999724 DOI: 10.1103/physrevlett.101.170402] [Citation(s) in RCA: 10] [Impact Index Per Article: 0.6] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 07/10/2008] [Indexed: 05/27/2023]
Abstract
In the past few decades, several models have predicted an energy dependence of the speed of light in the context of quantum gravity. For cosmological sources such as active galaxies, this minuscule effect can add up to measurable photon-energy dependent time lags. In this Letter a search for such time lags during the High Energy Stereoscopic System observations of the exceptional very high energy flare of the active galaxy PKS 2155-304 on 28 July 2006 is presented. Since no significant time lag is found, lower limits on the energy scale of speed of light modifications are derived.
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Affiliation(s)
- F Aharonian
- Max-Planck-Institut für Kernphysik, Heidelberg, Germany
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Aharonian F, Akhperjanian AG, Bazer-Bachi AR, Beilicke M, Benbow W, Berge D, Bernlöhr K, Boisson C, Bolz O, Borrel V, Braun I, Breitling F, Brown AM, Bühler R, Büsching I, Carrigan S, Chadwick PM, Chounet LM, Cornils R, Costamante L, Degrange B, Dickinson HJ, Djannati-Ataï A, Drury LO, Dubus G, Egberts K, Emmanoulopoulos D, Espigat P, Feinstein F, Ferrero E, Fiasson A, Fontaine G, Funk S, Funk S, Gallant YA, Giebels B, Glicenstein JF, Goret P, Hadjichristidis C, Hauser D, Hauser M, Heinzelmann G, Henri G, Hermann G, Hinton JA, Hofmann W, Holleran M, Horns D, Jacholkowska A, de Jager OC, Khélifi B, Komin N, Konopelko A, Kosack K, Latham IJ, Le Gallou R, Lemière A, Lemoine-Goumard M, Lohse T, Martin JM, Martineau-Huynh O, Marcowith A, Masterson C, McComb TJL, de Naurois M, Nedbal D, Nolan SJ, Noutsos A, Orford KJ, Osborne JL, Ouchrif M, Panter M, Pelletier G, Pita S, Pühlhofer G, Punch M, Raubenheimer BC, Raue M, Rayner SM, Reimer A, Reimer O, Ripken J, Rob L, Rolland L, Rowell G, Sahakian V, Saugé L, Schlenker S, Schlickeiser R, Schwanke U, Sol H, Spangler D, Spanier F, Steenkamp R, Stegmann C, Superina G, Tavernet JP, Terrier R, Théoret CG, Tluczykont M, van Eldik C, Vasileiadis G, Venter C, Vincent P, Völk HJ, Wagner SJ, Ward M. HESS observations of the galactic center region and their possible dark matter interpretation. Phys Rev Lett 2006; 97:221102. [PMID: 17155788 DOI: 10.1103/physrevlett.97.221102] [Citation(s) in RCA: 8] [Impact Index Per Article: 0.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 12/19/2005] [Revised: 08/23/2006] [Indexed: 05/12/2023]
Abstract
The detection of gamma rays from the source HESS J1745-290 in the Galactic Center (GC) region with the High Energy Spectroscopic System (HESS) array of Cherenkov telescopes in 2004 is presented. After subtraction of the diffuse gamma-ray emission from the GC ridge, the source is compatible with a point source with spatial extent less than 1.2;{'}(stat) (95% C.L.). The measured energy spectrum above 160 GeV is compatible with a power law with photon index of 2.25+/-0.04(stat)+/-0.10(syst) and no significant flux variation is detected. It is finally found that the bulk of the very high energy emission must have non-dark-matter origin.
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Affiliation(s)
- F Aharonian
- Max-Planck-Institut für Kernphysik, P.O. Box 103980, D-69029 Heidelberg, Germany
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Strasdeit H, Büsching I, Behrends S, Saak W, Barklage W. Syntheses and properties of zinc and calcium complexes of valinate and isovalinate: metal alpha-amino acidates as possible constituents of the early Earth's chemical inventory. Chemistry 2001; 7:1133-42. [PMID: 11303873 DOI: 10.1002/1521-3765(20010302)7:5<1133::aid-chem1133>3.0.co;2-t] [Citation(s) in RCA: 30] [Impact Index Per Article: 1.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/08/2022]
Abstract
We have studied the ligand behavior of racemic isovalinate (iva) and valinate (val) towards zinc(II) and calcium(II). The following solid metal amino acidates were obtained from aqueous solutions: Zn3Cl2(iva)4 (1), Zn3Cl2(val)4 (2). Zn(val)2 (3), Zn(iva)2 x 2H2O (4), Zn(iva)2 x 3.25H2O (5), Zn(iva)2 (6), Ca(iva)2x xH2O (7), and Ca(val)2 x H2O (8). Except for complex 3, these were hitherto unknown compounds. The conditions under which they formed, together with current ideas of the conditions on early Earth, support the assumption that alpha-amino acidate complexes of zinc and calcium might have belonged to early Earth's prebiotic chemical inventory. The zinc isovalinates 1, 4, and 5 were characterized by X-ray crystal structure analyses. Complex 1 forms a layer structure containing four- and five-coordinate metal atoms, whereas the zinc atoms in 4 and 5 are five-coordinate. Compound 5 possesses an unprecedented nonpolymeric structure built from cyclic [Zn6(iva)12] complexes, which are separated by water molecules. The thermolyses of solids 1. 3, and 8 at 320 degrees C in an N2 atmosphere yielded numerous organic products, including the cyclic dipeptide of valine from 3 and 8. Condensation, C-C bond breaking and bond formation, aromatization, decarboxylation, and deamination reactions occurred during the thermolyses. Such reactions of metal-bound a-amino acidates that are abiotically formed could already have contributed to an organic-geochemical diversity before life appeared on Earth.
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Affiliation(s)
- H Strasdeit
- Fachbereich Chemie der Universität, Oldenburg, Germany.
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Strasdeit H, Büsching I, Duhme AK, Pohl S. Structure of the two-coordinate cadmium complex bis(pentafluorophenyl)cadmium(II), [Cd(C6F5)2]. Acta Crystallogr C 1993. [DOI: 10.1107/s010827019201014x] [Citation(s) in RCA: 11] [Impact Index Per Article: 0.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/10/2022] Open
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