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Journal articles on the topic 'CANGAROO'

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Published: 10 December 2022

Last updated: 29 January 2023

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1

Yukawa, Y., and the CANGAROO Collaboration. "Recent results from CANGAROO-III." Journal of Physics: Conference Series 120, no. 6 (July 1, 2008): 062018. http://dx.doi.org/10.1088/1742-6596/120/6/062018.

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2

Mori for the CANGAROO Team, Masaki. "Recent Status of CANGAROO-III." Journal of the Physical Society of Japan 77, Suppl.B (January 2, 2008): 32–35. http://dx.doi.org/10.1143/jpsjs.77sb.32.

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3

Kubo, H., A. Asahara, G. V. Bicknell, R. W. Clay, Y. Doi, P. G. Edwards, R. Enomoto, et al. "Status of the CANGAROO-III project." New Astronomy Reviews 48, no. 5-6 (April 2004): 323–29. http://dx.doi.org/10.1016/j.newar.2003.12.002.

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4

Dazeley, S. A., P. G. Edwards, J. R. Patterson, G. P. Rowell, M. Sinnott, G. J. Thornton, C. Wilkinson, et al. "Recent Results from the CANGAROO Project." International Astronomical Union Colloquium 160 (1996): 363–64. http://dx.doi.org/10.1017/s0252921100041919.

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TheCollaboration ofAustralia andNippon for aGAmmaRayObservatory in theOutback operates two large telescopes at Woomera (South Australia), which detect the Čerenkov light images produced in the atmosphere by electronpositron cascades initiated by very high energy (~1 TeV or 1012eV) gamma rays. These gamma rays arise from a different mechanism than at EGRET energies: inverse Compton (IC) emission from relativistic electrons.The spoke-like images are recorded by a multi-pixel camera which facilitates the rejection of the large numbers of oblique and ragged cosmic ray images. A field of view ~3.5° is required. The Australian team operates a triple 4 m diameter mirror telescope, BIGRAT, with a 37 photomultiplier tube camera and energy threshold 600 GeV. The Japanese operate a single, highly accurate 3.8 m diameter f/1 telescope and high resolution 256 photomultipler tube camera. In 1998 a new 7 m telescope is planned for Woomera with a design threshold ~;200GeV.

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5

Muraishi, H., T. Tanimori, S. Yanagita, T. Yoshida, T. Kifune, S. A. Dazeley, P. G. Edwards, et al. "Observation of RXJ1713.7-3946 by CANGAROO telescope." Astronomische Nachrichten 320, no. 4-5 (August 1999): 324. http://dx.doi.org/10.1002/1521-3994(199908)320:4/5<324::aid-asna324>3.0.co;2-3.

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6

Nishijima, Kyoshi. "Very High Energy Gamma-ray Observations of AGN with CANGAROO." Publications of the Astronomical Society of Australia 19, no. 1 (2002): 26–28. http://dx.doi.org/10.1071/as01089.

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AbstractWe have observed eight AGN since 1993 in the energy region above several hundred GeV using the CANGAROO telescopes. We observed Mrk 421 for ten nights with the CANGAROO-II 10 m telescope during its active state in early 2001 using the very large zenith angle technique. Our preliminary result implies the detection of gamma-ray emission from Mrk 421 in the energy range above 9.3 TeV. The high energy peaked BL Lacs (HBLs) PKS 2005–489 and PKS 2155–304 have been also observed. No statistically significant signals are found for both HBLs and flux upper limits are obtained. A summary of results of observations of AGN is presented in this paper.

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7

Mori for the CANGAROO Team, Masaki. "CANGAROO Project for High-Energy Gamma-Ray Astrophysics." Progress of Theoretical Physics Supplement 151 (2003): 85–94. http://dx.doi.org/10.1143/ptps.151.85.

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8

Kifune, T. "Very High Energy Gamma Rays from Plerions: CANGAROO Results." Symposium - International Astronomical Union 188 (1998): 125–28. http://dx.doi.org/10.1017/s0074180900114597.

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The current status of very high energy gamma ray astronomy (in ~ 1 TeV region) is described by using as example results of CANGAROO (Collaboration of Australia and Nippon for a GAmma Ray Observatory in the Outback). Gamma rays at TeV energies, emitted through inverse Compton effect of electrons or π0 decay from proton interaction, provide direct evidence on “hot” non-thermal processes of the Universe, as well as environmental features, such as the strength of magnetic field in the emission region, for the non-thermal processes.

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9

Enomoto, R., S. Watanabe, T. Tanimori, A. Asahara, G. V. Bicknell, R. W. Clay, P. G. Edwards, et al. "CANGAROO III Observations of the Supernova Remnant RX J0852.0−4622." Astrophysical Journal 652, no. 2 (December 2006): 1268–76. http://dx.doi.org/10.1086/508531.

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10

Enomoto, R., Y. Higashi, T. Yoshida, T. Tanimori, G. V. Bicknell, R. W. Clay, P. G. Edwards, et al. "CANGAROO‐III Search for Gamma Rays from Kepler’s Supernova Remnant." Astrophysical Journal 683, no. 1 (August 10, 2008): 383–88. http://dx.doi.org/10.1086/589912.

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11

Edwards, P. G., A. G. Gregory, J. R. Patterson, M. D. Roberts, G. P. Rowell, N. I. Smith, G. J. Thornton, et al. "First Test Data from the CANGAROO Project for Stereo Čerenkov Imaging." Publications of the Astronomical Society of Australia 10, no. 4 (1993): 287–90. http://dx.doi.org/10.1017/s1323358000025893.

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AbstractThe CANGAROO project incorporates two Čerenkov imaging telescopes at Woomera to obtain stereo images of very high-energy gamma-ray (and cosmic-ray) showers. The first stereo observations, with one imaging system, were made in March 1992, and preliminary stereo imaging observations began in July 1992. This paper describes the stereo imaging technique, the sources under investigation, and the indications from the first data sets.

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12

Edwards, P. G., A. G. Gregory, J. R. Patterson, M. D. Roberts, G. P. Rowell, N. I. Smith, G. J. Thornton, et al. "The CANGAROO Project: Very High Energy Gamma-ray Astronomy at Woomera." Publications of the Astronomical Society of Australia 10, no. 1 (1992): 27–29. http://dx.doi.org/10.1017/s1323358000019160.

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AbstractIn this paper the Very High Energy (VHE) gamma-ray astronomy program at the University of Adelaide is described. VHE gamma rays with energies above ~5 × 1011eV are observed using the atmospheric Cerenkov technique. Results from the first three years observations at Woomera and the current upgrading of the telecope are described. The CANGAROO project, a collaboration between the University of Adelaide and a number of Japanese institutions, is also introduced.

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13

Sakamoto, Y., K. Nishijima, T. Mizukami, E. Yamazaki, J. Kushida, R. Enomoto, M. Ohishi, et al. "CANGAROO‐III Observations of the 2006 Outburst of PKS 2155−304." Astrophysical Journal 676, no. 1 (March 20, 2008): 113–20. http://dx.doi.org/10.1086/528369.

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14

Yoshikoshi, T., S. A. Dazeley, S. Gunji, S. Hara, T. Hara, J. Holder, J. Jimbo, et al. "Present status of the 7–10 m telescope of CANGAROO II." Astroparticle Physics 11, no. 1-2 (June 1999): 267–69. http://dx.doi.org/10.1016/s0927-6505(99)00063-8.

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15

Kawachi, A., Y. Hayami, J. Jimbo, S. Kamei, T. Kifune, H. Kubo, J. Kushida, et al. "The optical reflector system for the CANGAROO-II imaging atmospheric Cherenkov telescope." Astroparticle Physics 14, no. 4 (January 2001): 261–69. http://dx.doi.org/10.1016/s0927-6505(00)00131-6.

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16

Dazeley, S. A., and J. R. Patterson. "Monte Carlo simulations of the CANGAROO I 3.8 m imaging Čerenkov telescope." Astroparticle Physics 15, no. 3 (June 2001): 305–11. http://dx.doi.org/10.1016/s0927-6505(00)00161-4.

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17

Kabuki, S., K. Tsuchiya, K. Okumura, R. Enomoto, T. Uchida, H. Tsunoo, Shin Hayashi, et al. "Development of an atmospheric Cherenkov imaging camera for the CANGAROO-III experiment." Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 500, no. 1-3 (March 2003): 318–36. http://dx.doi.org/10.1016/s0168-9002(03)00331-0.

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18

Kifune, T. "Gamma-rays of TeV energy from plerions and results of CANGAROO project." Advances in Space Research 25, no. 3-4 (January 2000): 641–46. http://dx.doi.org/10.1016/s0273-1177(99)00816-9.

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19

Kiuchi, R., M. Mori, G. V. Bicknell, R. W. Clay, P. G. Edwards, R. Enomoto, S. Gunji, et al. "CANGAROO-III SEARCH FOR TeV GAMMA RAYS FROM TWO CLUSTERS OF GALAXIES." Astrophysical Journal 704, no. 1 (September 22, 2009): 240–46. http://dx.doi.org/10.1088/0004-637x/704/1/240.

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20

Enomoto, R., G. V. Bicknell, R. W. Clay, P. G. Edwards, S. Gunji, S. Hara, T. Hattori, et al. "CANGAROO‐III Search for Gamma Rays from SN 1987A and the Surrounding Field." Astrophysical Journal 671, no. 2 (December 20, 2007): 1939–43. http://dx.doi.org/10.1086/523100.

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21

Hayashi, Sei, F. Kajino, T. Naito, A. Asahara, G. V. Bicknell, R. W. Clay, Y. Doi, et al. "Search for VHE gamma rays from SS433/W50 with the CANGAROO-II telescope." Astroparticle Physics 32, no. 2 (September 2009): 112–19. http://dx.doi.org/10.1016/j.astropartphys.2009.06.006.

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22

Katagiri, H., R. Enomoto, L. T. Ksenofontov, M. Mori, Y. Adachi, A. Asahara, G. V. Bicknell, et al. "Detection of Gamma Rays around 1 TeV from RX J0852.0-4622 by CANGAROO-II." Astrophysical Journal 619, no. 2 (January 5, 2005): L163—L166. http://dx.doi.org/10.1086/427980.

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23

Kabuki, S., R. Enomoto, G. V. Bicknell, R. W. Clay, P. G. Edwards, S. Gunji, S. Hara, et al. "CANGAROO III Search for Gamma Rays from Centaurus A and the ω Centauri Region." Astrophysical Journal 668, no. 2 (October 20, 2007): 968–73. http://dx.doi.org/10.1086/520767.

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24

Hattori, Takahiro, and Kyoshi Nishijima. "Search for TeV Gamma-Rays from 3EG J1234-1318 with the Cangaroo-II Telescope." Astrophysics and Space Science 297, no. 1-4 (June 2005): 327–34. http://dx.doi.org/10.1007/s10509-005-7671-1.

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25

Enomoto, R., J. Kushida, T. Nakamori, T. Kifune, G. V. Bicknell, R. W. Clay, P. G. Edwards, et al. "CANGAROO-III OBSERVATION OF TeV GAMMA RAYS FROM THE VICINITY OF PSR B1706-44." Astrophysical Journal 703, no. 2 (September 12, 2009): 1725–33. http://dx.doi.org/10.1088/0004-637x/703/2/1725.

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26

Tsuchiya, K., R. Enomoto, L. T. Ksenofontov, M. Mori, T. Naito, A. Asahara, G. V. Bicknell, et al. "Detection of Sub-TeV Gamma Rays from the Galactic Center Direction by CANGAROO-II." Astrophysical Journal 606, no. 2 (April 9, 2004): L115—L118. http://dx.doi.org/10.1086/421292.

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27

Enomoto, R., K. Tsuchiya, Y. Adachi, S. Kabuki, P. G. Edwards, A. Asahara, G. V. Bicknell, et al. "A Search for Sub‐TeV Gamma Rays from the Vela Pulsar Region with CANGAROO‐III." Astrophysical Journal 638, no. 1 (February 10, 2006): 397–408. http://dx.doi.org/10.1086/498858.

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28

Ohishi, M., M. Mori, Y. Adachi, A. Asahara, G. V. Bicknell, R. W. Clay, Y. Doi, et al. "Very high energy gamma-ray observations of the Galactic Plane with the CANGAROO-III telescopes." Astroparticle Physics 30, no. 2 (September 2008): 47–53. http://dx.doi.org/10.1016/j.astropartphys.2008.06.007.

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29

Higashi, Y., H. Kubo, T. Yoshida, R. Enomoto, T. Tanimori, P. G. Edwards, T. Naito, et al. "Observation of Very High Energy Gamma Rays from HESS J1804−216 with CANGAROO‐III Telescopes." Astrophysical Journal 683, no. 2 (August 20, 2008): 957–66. http://dx.doi.org/10.1086/589877.

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30

BILAND, ADRIAN. "GROUND-BASED GAMMA-RAY ASTRONOMY." International Journal of Modern Physics A 20, no. 29 (November 20, 2005): 6981–90. http://dx.doi.org/10.1142/s0217751x05030661.

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Very High Energy Gamma-Ray Astronomy (the measurement of γ above 10 GeV) is a rather young but fast evolving field. In the past 16 years some 20 sources have been discovered, about half of them are firmly established and seen with high significance by more than one experiment. This rather short list already contains very different objects like plerions, supernova remnants and active galactic nuclei. A new generation of instruments (CANGAROO III, HESS, MAGIC, VERITAS) is just starting to take data, and first preliminary results show that the sensitivity is improved by at least a factor of 100. Already during commissioning, some new sources have been discovered. This overview will summarize the techniques used in VHE gamma-ray observations as well discuss briefly some physics topics that can be investigated in this energy range.

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31

Mizukami, T., H. Kubo, T. Yoshida, T. Nakamori, R. Enomoto, T. Tanimori, M. Akimoto, et al. "CANGAROO-III OBSERVATION OF TeV GAMMA RAYS FROM THE UNIDENTIFIED GAMMA-RAY SOURCE HESS J1614–518." Astrophysical Journal 740, no. 2 (October 3, 2011): 78. http://dx.doi.org/10.1088/0004-637x/740/2/78.

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32

Sako, T., Y. Matsubara, Y. Muraki, P. V. Ramanamurthy, S. A. Dazeley, P. G. Edwards, S. Gunji, et al. "Very High Energy Gamma‐Ray Observations of PSR B1509−58 with the CANGAROO 3.8 Meter Telescope." Astrophysical Journal 537, no. 1 (July 2000): 422–28. http://dx.doi.org/10.1086/308998.

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33

Enomoto, R. "Design study of CANGAROO-III, stereoscopic imaging atmospheric Cherenkov telescopes for sub-TeV Î³-ray detection." Astroparticle Physics 16, no. 3 (January 2002): 235–44. http://dx.doi.org/10.1016/s0927-6505(01)00112-8.

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34

Mizumura, Y., J. Kushida, K. Nishijima, G. V. Bicknell, R. W. Clay, P. G. Edwards, S. Gunji, et al. "Searches for very high energy gamma rays from blazars with CANGAROO-III telescope in 2005–2009." Astroparticle Physics 35, no. 9 (April 2012): 563–72. http://dx.doi.org/10.1016/j.astropartphys.2012.01.002.

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35

Rector, Travis, Eric Perlman, Rita Sambruna, Greg Madejski, and Frederik Rantakyro. "Multifrequency Monitoring of the Blazar PKS 2005-489." Publications of the Astronomical Society of Australia 19, no. 1 (2002): 158–60. http://dx.doi.org/10.1071/as01115.

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AbstractWe present a multifrequency monitoring campaign of PKS 2005–489, a bright and highly variable blazar. Simultaneous observations were completed over a 13 day period in the X-ray with RXTE, in the optical at the CTIO 0.9 m telescope, at TeV energies with CANGAROO-II, and at submillimetre wavelengths with SEST. Previous multiwavelength monitoring campaigns of PKS 2005–489 and other blazars have found complex flux and spectral variability behaviour, with different modes and timescales from days to hours and shorter.PKS 2005–489 was observed in transition from a quiescent state into the early stages of a flare. A gradual increase in flux density was observed at optical and X-ray wavelengths during 19–27 August 2000, and a dramatic increase in X-ray emission was observed starting on 2 September 2000. Intraday and spectral variability were not detected during the campaign.

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36

Kifune, T. "The Prospects for Very High Energy Gamma Ray Astronomy." Australian Journal of Physics 48, no. 2 (1995): 305. http://dx.doi.org/10.1071/ph950305.

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Very-high-energy (VHE) gamma rays, with energies .<: 1 TeV = 1012 eV, are observed with ground-based telescopes using the atmospheric Cerenkov technique. This field of astronomy has recently experienced its coming of age, opening a new observational window on the universe after efforts spanning almost 30 years. Recent advances in this field have been aided by the results from satellite detectors with high-energy (HE) gamma ray 'eyes'. Satellite detectors are sensitive to HE gamma rays, up to energies of about 10 GeV = 1010 eV. In this paper, VHE gamma ray astronomy is reviewed, and the 3�8 m diameter telescope of the Japanese-Australian CANGAROO project is used to illustrate the detection techniques. As VHE gamma ray astronomy is closely related to observations in the HE region, results from recent satellite experiments are also discussed.

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37

Nakamori, T., H. Kubo, T. Yoshida, T. Tanimori, R. Enomoto, G. V. Bicknell, R. W. Clay, et al. "Observation of an Extended Very High Energy Gamma‐Ray Emission from MSH 15‐52 with CANGAROO‐III." Astrophysical Journal 677, no. 1 (April 10, 2008): 297–305. http://dx.doi.org/10.1086/529029.

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38

Dazeley, S. A., J. R. Patterson, G. P. Rowell, and P. G. Edwards. "The sensitivity of the CANGAROO I analyses of the Crab and Vela plerions to image selection cuts." Astroparticle Physics 15, no. 3 (June 2001): 313–21. http://dx.doi.org/10.1016/s0927-6505(00)00162-6.

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39

Yoshikoshi, T., M. Mori, P. G. Edwards, S. Gunji, S. Hara, T. Hara, A. Kawachi, et al. "REANALYSIS OF DATA TAKEN BY THE CANGAROO 3.8 METER IMAGING ATMOSPHERIC CHERENKOV TELESCOPE: PSR B1706-44, SN 1006, AND VELA." Astrophysical Journal 702, no. 1 (August 14, 2009): 631–48. http://dx.doi.org/10.1088/0004-637x/702/1/631.

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40

Konopelko, A. "Study of Galaxy Evolution Using VHE γ-ray Observations with Ground-based Čerenkov Telescopes." Symposium - International Astronomical Union 204 (2001): 151. http://dx.doi.org/10.1017/s0074180900225989.

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The spectral distribution of the extragalactic background light (EBL) in the infrared yields important information about the evolution of galaxies. The spectrum of a galaxy in the 0.1–200 μm region is a footprint of the intrinsic starlight at ~ 1μm and its extinction by dust with re-emission at ~ 100 μm. The overall spectral energy distribution of the EBL is then determined by the galaxy luminosity evolution. High-energy γ-rays are absorbed by the EBL photons through γγ → e+e- reactions. Such an effect has been seen recently in the Mkn 501 TeV spectrum measured by the HEGRA (High Energy Gamma Ray Astronomy) collaboration using an advanced system of imaging atmospheric Čerenkov telescopes (IACTs). The intrinsic spectra of AGNs in the 50 GeV-1 TeV energy range may be constrained by the X-ray fluxes measured with satellite instruments aboard missions such as RXTE, XMM, and ASCA. By reducing the energy threshold down to 50 GeV, forthcoming ground-based IACTs systems (CANGAROO IV, H.E.S.S., VERITAS) may be able to study the absorption cutoff in energy spectra of distant AGNs (z< 0.4), to unfold the true galaxy luminosity evolution function.

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41

Kawachi, A., T. Naito, J. R. Patterson, P. G. Edwards, A. Asahara, G. V. Bicknell, R. W. Clay, et al. "A Search for TeV Gamma‐Ray Emission from the PSR B1259−63/SS 2883 Binary System with the CANGAROO‐II 10 Meter Telescope." Astrophysical Journal 607, no. 2 (June 2004): 949–58. http://dx.doi.org/10.1086/383604.

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42

Tanimori, Toru. "Detection of TeV Gamma Rays from SN1006." Symposium - International Astronomical Union 188 (1998): 121–24. http://dx.doi.org/10.1017/s0074180900114585.

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In spite of the recent progress of high energy gamma-ray astronomy, there still remains quite unclear and important problem about the origin of cosmic rays. Supernova remnants (SNRs) are the favoured site for cosmic rays up to 1016 eV, as they satisfy the requirements such as an energy input rate. But direct supporting evidence is sparse. Recently intense non-thermal X-ray emission from the rims of the Type Ia SNR SN1006 (G327.6+14.6) has been observed by ASCA (Koyama et al. 1995)and ROSAT (Willingale et al. 1996), which is considered, by attributing the emission to synchrotron radiation, to be strong evidence of shock acceleration of high energy electrons up to ~100 TeV. If so, TeV gamma rays would also be expected from inverse Compton scattering (IC) of low energy photons (mostly attributable to the 2.7 K cosmic background photons) by these electrons. By assuming the magnetic field strength (B) in the emission region of the SNR, several theorists (Pohl 1996; Mastichiadis 1996; Mastichiadis & de Jager 1996; Yoshida & Yanagita 1997) calculated the expected spectra of TeV gamma rays using the observed radio/X-ray spectra. Observation of TeV gamma rays would thus provide not only the further direct evidence of the existence of very high energy electrons but also the another important information such as the strength of the magnetic field and diffusion coefficient of the shock acceleration. With this motivation, SN1006 was observed by the CANGAROO imaging air Cerenkov telescope in 1996 March and June, also 1997 March and April.

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43

Costa, Ana Paula Rodrigues da. "LUGAR E MEMÓRIA: A VIDA CANGACEIRA DO BANDO DOS MARCELINOS EM BARBALHA - CE." Revista da Casa da Geografia de Sobral (RCGS) 22, no. 1 (April 24, 2020): 52–67. http://dx.doi.org/10.35701/rcgs.v22n1.413.

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O trabalho em questão discorre sobre a abordagem dos conceitos de lugar e memória a partir da geografia humanista, apresentando como objeto de estudo o bando de cangaceiros dos Marcelinos no Cariri cearense, tendo como recorte espacial o município de Barbalha. O texto apresenta um apanhado geral sobre o movimento do cangaço para, em seguida, apresentar o bando dos Marcelinos e alguns lugares de sua atuação em Barbalha. Para contextualizar o tema, apresenta-se a interseção entre lugar e memória como definições relevantes para o entendimento do movimento do cangaço. Palavras-chave: Bando dos Marcelinos; Cangaço; Lugar; Memória; Geografia Humanista. RESUMEN El trabajo en cuestión discurre sobre el abordaje de los conceptos de lugar y memoria a partir de la geografía humanista, presentando como objeto de estudio el bando de “cangaceiros” de los Marcelinos en el Cariri cearense, teniendo como recorte espacial el municipio de Barbalha. El texto presenta un recuento general sobre el movimiento del “cangaço”, enseguida, presentar el bando de los Marcelinos y algunos sitios de su actuación en Barbalha. Para contextualizar el tema, se presenta la intersección entre lugar y memoria como definiciones relevantes para el entendimiento del movimiento del “cangaço”. Palabras clave: Bando de los Marcelinos; Cangaço; Lugar; Memoria; Geografía Humanista. ABSTRACT This work discusses about the concepts’ approach of place and memory from the humanistic geography, presenting as object of study the Marcelinos’ gang in Cariri – Ceará, having as a spatial clipping the city of Barbalha. The text presents a general overview of the cangaço movement to, then, present the Marcelinos’ gang and some of their actuation places in Barbalha. To contextualize the theme, wepresent the intersection between place and memory as relevant definitions for the understanding of the “cangaço” movement. Keywords: Marcelinos’ gang; Cangaço; Place; Memory; Humanistic Geography. RÉSUMÉ Le travail en question discute de l'approche des concepts de lieu et de mémoire de la géographie humaniste, présentant comme objet d'étude la bande de “cangaceiros” des Marcelinos dans le Cariri Ceará, avec la municipalité de Barbalha comme section spatiale. Le texte présente un aperçu du mouvement du “cangaço” puis présente le groupe des Marcelinos et quelques lieux de leur performance à Barbalha. Pour contextualiser le thème, l'intersection entre le lieu et la mémoire est présentée comme des définitions pertinentes pour comprendre le mouvement du “cangaço”. Mots-clés: La bande des Marcelinos; Cangaço; Lieu; Mémoire; Géographie humaniste.

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44

Mansur, João Paulo. "Literatura ou antropologia criminal? O cangaço em Pedra Bonita e Cangaceiros." Mana 25, no. 2 (August 2019): 427–55. http://dx.doi.org/10.1590/1678-49442019v25n2p427.

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Resumo Este artigo investiga as interpretações sociocriminológicas de José Lins do Rego sobre o cangaço que lhe serviram de pano de fundo para desenvolver os romances Pedra Bonita e Cangaceiros. Mostra-se como o romancista se posicionava perante duas teorias criminológicas que, em sua época, tentavam compreender o cangaço: a teoria do banditismo social e a antropologia criminal da Escola Positiva brasileira. Conclui-se que o caminho trilhado por Rego para explicar a gênese do cangaço passava por entendê-lo em função das disputas coronelistas.

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Souza, Felipe Trindade de. "A bibliografia marxista de matriz comunista sobre o cangaço e a tese da singularidade brasileira." Em Tese 17, no. 2 (September 23, 2020): 178–88. http://dx.doi.org/10.5007/1806-5023.2020v17n2p178.

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O presente artigo objetiva debater a bibliografia marxista de matriz comunista do cangaço dentro da tese da singularidade brasileira. Buscando identificar como determinadas “imagens” da realidade social brasileira foram utilizadas pelos trabalhos para explicar o cangaço. Posições que, consequentemente, reafirmam proposições singulares e podem ter implicado em considerações etnocêntricas. Além disso, através deste artigo será possível demonstrar como o Partido Comunista do Brasil exerceu influência na produção de teses sobre o cangaço. Ideias que, em sentido amplo, geraram objeções de um conjunto de trabalhos que também foram influenciados pelo marxismo.

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Aléssio, Renata Lira dos Santos. "A representação social da violência na literatura de cordel sobre cangaço." Psicologia: Ciência e Profissão 24, no. 4 (December 2004): 52–59. http://dx.doi.org/10.1590/s1414-98932004000400007.

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O cangaço é uma forma de banditismo social típica do Nordeste brasileiro, cujas histórias, veiculadas nos folhetos de cordel, transmitem representações acerca dos mais diversos objetos sociais, dentre eles a violência. O objetivo deste trabalho foi investigar a representação social da violência em cordéis sobre o cangaço. Foram pesquisados 12 (doze) folhetos, cuja análise, a partir do software ALCESTE, produziu quatro classes de palavras, agrupadas em dois eixos: o primeiro, ligado à narrativa jornalística do cangaço, e o segundo eixo, fortemente marcado por idéias que indicam um julgamento moral dos atores sociais envolvidos, forjando uma identidade social para nordestinos, sertanejos e cangaceiros.

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Tunggal, Rahmad, Joko Triwanto, and Ramli Ramadhan. "Valuasi Ekonomi Dan Implementasi Pes (Payment For Ecosystem Service) Pada Wisata Pemandian Air Panas Cangar Di Era Pandemi Covid-19." Journal of Forest Science Avicennia 4, no. 2 (February 2, 2022): 86–95. http://dx.doi.org/10.22219/avicennia.v4i2.19645.

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Sejak diumumkanya status pandemi di seluruh indonesia berbagai aktivitas perekonomian mulai dari sektor pariwisata hingga perdagangan terpaksa harus menutup usahanya karena tidak diperbolehkan melakukan aktivitas, tak terkecuali wisata pemandian air panas Cangar yang berada di area taman hutan raya Raden Soeryo hal tersebut akan berdampak terhadap valuasi serta perekonomian kawasan hal terebut juga akan berdampak secara tidak langsung terhadap pelaksanan PES. Penelitian ini bertujuan untuk mengkaji valuasi dan implementasi Pay Ecosystem for Services (PES) dari ekowisata pemandian air panas cangar di era pandemi serta menganalisis permasalahan ekonomi yang timbul akibat penutupan kawasan wisata pemandian air panas cangar. Data yang digunakan dalam penelitian ini yaitu kualitatif deskriptif dari fenomena dan kejadian yang sebenarnya terjadi di lapangan yang dihasilkan dari observasi dan quisioner. Waktu dan tempat penelitian ini dilaksanakan pada bulan Desember 2020-Januari 2021 di pemandian air panas Cangar kawasan tahura R.Soerjo. metode pengambilan sampel yang digunakan dalam penelitian ini adalah menggunakan Teknik Purposive Sampling yaitu teknik pengambilan sampel dari populasi penelitian yang didasarkan atas ciri-ciri dan suatu karakteristik tertentu untuk mencapai tujuan peneliti. Nilai ekonomi total yang dihasilkan pada kawasan pemandian air panas Cangar yaitu sebesar Rp. 5.216.626.830,- per tahun sebelum pandemi dan Rp. 4.188.516.830,- per tahun selama pandemi. Valuasi ekonomi di pemandian air panas Cangar mengalami penurunan dimasa pandemi akibat berkurangnya nilai guna langsung dan nilai pilihan. Implementasi PES telah terlaksana dengan sebagai mana mestinya karena semua unsur parameter sudah terpenuhi

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Almeida, Ricardo Santos de. "Contextualização de Jogo eletrônico para a realidade: as relações espaço-tempo e a geopolítica do cangaço." Revista Interseção 1, no. 1 (August 17, 2020): 113–21. http://dx.doi.org/10.48178/intersecao.v1i1.220.

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RESUMO Este artigo objetiva-se em ressaltar a importância da adaptação de jogos eletrônicos para jogos de tabuleiro, bem como a relação ensino-aprendizagem realizada interdisciplinarmente entre as disciplinas Geografia e História, no Projeto Cangaço, realizado entre dezembro de 2017 a janeiro de 2018 em uma escola pública estadual do Alto Sertão Alagoano estimulando a compreensão das relações espaço-tempo e os contextos geopolíticos em que cada personagem do jogo adaptado encontrava-se, permitindo a participação dos estudantes/jogadores de três turmas da segunda série do Ensino Médio no pátio da escola junto ao docente de Geografia, protagonistas do processo contínuo de aprendizagem. Para o desenvolvimento desta atividade foram realizadas discussões envolvendo a compreensão de cangaço em Hobsbawm (1976), Dutra (2006), e a importância de jogos utilizados como ferramenta didática a partir de Roehrs et al (2017), Santos e Eichler (2016), Tassinari (2016), e Ramos (2014) para a elaboração e aplicação da adaptação do jogo eletrônico Cangaço® (2014) em sala de aula. Palavras-chave: Jogo educativo. Ensino-aprendizado. Interdisciplinaridade. ABSTRACT This article aims to emphasize the importance of adapting electronic games for board games, as well as the interdisciplinary teaching-learning relationship between the disciplines Geography and History, in the Cangaço Project, carried out between December 2017 and January 2018 in a state public school of Alto Sertão Alagoano stimulating the understanding of space-time relations and the geopolitical contexts in which each character of the adapted game was found, allowing the participation of students / players from three classes of the second grade of High School in the schoolyard together with the Geography teacher, protagonists of the continuous learning process. For the development of this activity, discussions were held involving the understanding of cangaço in Hobsbawm (1976), Dutra (2006), and the importance of games used as a didactic tool from Roehrs et al (2017), Santos and Eichler (2016), Tassinari (2016), and Ramos (2014) for the elaboration and application of the adaptation of the electronic game Cangaço® (2014) in the classroom. Keywords: Educational game. Teaching-learning. Interdisciplinarity.

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Costa, Ana Paula Rodrigues. "Geografia do cangaço: concepções conceituais para pensar o banditismo sertanejo." Geography Department University of Sao Paulo 41 (July 23, 2021): e174830. http://dx.doi.org/10.11606/eissn.2236-2878.rdg.2021.174830.

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Este artigo parte de algumas proposições suscitadas ao longo da pesquisa de mestrado objetivando discorrer ideias a respeito do conceito de banditismo social elaborado por Eric Hobsbawm e a costumeira aplicação desse conceito em alguns trabalhos para caracterizar o movimento do cangaço, padronizando, dessa forma, lugares, paisagens e sujeitos sem levar em consideração as implicações ao homogeneizar movimento do cangaço como banditismo social, transferindo, assim, a teoria para conceituar diferentes movimentos sociais e culturais. Pensando nessa discussão, ponderam-se observações de cunho histórico-cultural para a existência de bandos de cangaceiros no sertão nordestino, pontuando as relações que permeavam a sociedade sertaneja da época, correlacionando às questões de honra, valentia e cabra-macho, agregada à conexão de vivência no ambiente da caatinga, que constituiu uma geografia do cangaço, presente no contexto cultural do sujeito sertanejo nordestino com o meio ambiente a partir dos saberes populares que garantiam aos cangaceiros a vivência e a sobrevivência como nômades. A base cultural de vivência sertaneja nordestina, constituída por meio da relação do código moral sertanejo da não desmoralização, culminou, na visão dos sujeitos sertanejos nordestinos, o reconhecimento de uma geografia do cangaço desenvolvida pela atuação dos bandos de cangaceiros que asseguram, até hoje, narrativas, quer sejam de admiração ou de aversão aos bandidos/cangaceiros, atribuindo, sobretudo, um lugar de destaque após episódios de mortes trágicas sofridas por alguns cangaceiros.

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Silva, Leandro. "SERTÕES DAS LETRAS ao cinema nacional: Pedra Bonita e Cangaceiros em Deus e o Diabo na Terra do Sol." Revista Légua & Meia 7, no. 1 (November 10, 2017): 62. http://dx.doi.org/10.13102/lm.v7i1.2157.

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O presente artigo trabalha a relação entre O ciclo do misticismo e do cangaço,fase em que José Lins do Rego traz a lume os livros Pedra Bonita e Cangaceiros no constructo de Deus e o Diabo de Glauber Rocha, a partir da perspectiva de que, tanto as narrativas literárias, como o filme, à guisa do realismo documental que marca o Cinema Novo e o Modernismo, extenuam a busca por uma identidade nacional, a partir dos resgaste do mitos sertanejos, detidamente o cangaço e o beatismo.

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