Magic school abs matter because physical fitness and strength play a significant role in magical abilities. Abs are a crucial indicator of a mage's overall fitness and power. In magic schools, students are taught various spells and techniques to harness their magical abilities. However, in order to perform these spells effectively, a certain level of physical fitness is necessary. Abs are a visible sign of physical strength, endurance, and core stability, which are essential for controlling and channeling magical energy. Strong abs provide the foundation for a mage's magical abilities.
These abs know what’s up. They’re hip to the trend, but aware that it’s silly. More than anything, these abs illustrate that this man’s comfortable with his body, one of the most attractive traits of a MMXXL dancer. And he thinks about ice cream! You know who also thinks about ice cream? Tito. (Well, he wants to open a yogurt food truck and dances an ice cream/candy-based routine so close enough.) Also me.
These ambitious abs have already changed the world by introducing it to this heavily curtained bath tub and a phone roughly the size of two abs, but this sentiment is trite and vague. Abstract Milky Way dwarf spheroidal galaxies dSphs are among the best candidates to search for signals of dark matter annihilation with Imaging Atmospheric Cherenkov Telescopes, given their high mass-to-light ratios and the fact that they are free of astrophysical gamma-ray emitting sources.
Strong abs provide the foundation for a mage's magical abilities. They allow for better control and manipulation of magical energy, resulting in more precise and powerful spellcasting. Without strong abs, a mage may struggle to perform complex spells and may lack the necessary control over their powers.
Title: Combined searches for dark matter in dwarf spheroidal galaxies observed with the MAGIC telescopes, including new data from Coma Berenices and Draco
(9), A. López-Oramas (1), S. Loporchio (21), B. Machado de Oliveira Fraga (10), C. Maggio (25), P. Majumdar (31), M. Makariev (32), M. Mallamaci (11), G. Maneva (32), M. Manganaro (22), K. Mannheim (23), L. Maraschi (3), M. Mariotti (11), M. Martínez (5), D. Mazin (6,15), S. Menchiari (13), S. Mender (7), S. Mićanović (22), D. Miceli (2,45), T. Miener (9), J. M. Miranda (13), R. Mirzoyan (15), E. Molina (17), A. Moralejo (5), D. Morcuende (9), V. Moreno (25), E. Moretti (5), V. Neustroev (33), C. Nigro (5), K. Nilsson (24), D. Ninci (5), K. Nishijima (30), K. Noda (6), S. Nozaki (29), Y. Ohtani (6), T. Oka (29), J. Otero-Santos (1), S. Paiano (3), M. Palatiello (2), D. Paneque (15), R. Paoletti (13), J. M. Paredes (17), L. Pavletić (22), P. Peñil (9), M. Persic (2,46), M. Pihet (15), P. G. Prada Moroni (16), E. Prandini (11), C. Priyadarshi (5), I. Puljak (27), W. Rhode (7), M. Ribó (17), J. Rico (5), C. Righi (3), A. Rugliancich (16), L. Saha (9), N. Sahakyan (26), T. Saito (6), S. Sakurai (6), K. Satalecka (14), F. G. Saturni (3), B. Schleicher (23), K. Schmidt (7), T. Schweizer (15), J. Sitarek (12), I. Šnidarić (34), D. Sobczynska (12), A. Spolon (11), A. Stamerra (3), J. Strišković (28), D. Strom (15), M. Strzys (6), Y. Suda (35), T. Surić (34), M. Takahashi (6), R. Takeishi (6), F. Tavecchio (3), P. Temnikov (32), T. Terzić (22), M. Teshima (15,6), L. Tosti (36), S. Truzzi (13), A. Tutone (3), S. Ubach (25), J. van Scherpenberg (15), G. Vanzo (1), M. Vazquez Acosta (1), S. Ventura (13), V. Verguilov (32), C. F. Vigorito (20), V. Vitale (37), I. Vovk (6), M. Will (15), C. Wunderlich (13), D. Zarić (27) ((1) Instituto de Astrofísica de Canarias and Dpto. de Astrofísica, Universidad de La Laguna (Tenerife), Spain, (2) Universitá di Udine and INFN Trieste, Udine, Italy, (3) INAF - National Institute for Astrophysics, Roma, Italy, (4) ETH Zürich, Institute for Particle Physics, Zürich, Switzerland, (5) Institut de Física d'Altes Energies (IFAE), The Barcelona Institute of Science and Technology (BIST), Bellaterra (Barcelona), Spain, (6) Japanese MAGIC Group: Institute for Cosmic Ray Research (ICRR), The University of Tokyo, Chiba, Japan, (7) Technische Universität Dortmund, Dortmund, Germany, (8) Croatian MAGIC Group: University of Zagreb, Faculty of Electrical Engineering and Computing (FER), Zagreb, Croatia, (9) IPARCOS Institute and EMFTEL Department, Universidad Complutense de Madrid, Madrid, Spain, (10) Centro Brasileiro de Pesquisas Físicas (CBPF), Rio de Janeiro, Brazil, (11) Dipartimento di Fisica e Astronomia dell'Universitá and INFN Padova, Padova, Italy, (12) University of Lodz, Faculty of Physics and Applied Informatics, Department of Astrophysics, Lodz, Poland, (13) Dipartimento SFTA, Sezione di Fisica, Universitá di Siena and INFN Pisa, Siena, Italy, (14) Deutsches Elektronen-Synchrotron (DESY), Zeuthen, Germany, (15) Max-Planck-Institut für Physik, München, Germany, (16) Universitá di Pisa and INFN Pisa, Pisa, Italy, (17) Universitat de Barcelona, ICCUB, IEEC-UB, Barcelona, Spain, (18) Armenian MAGIC Group: A. Alikhanyan National Science Laboratory, Yerevan, Armenia, (19) Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas, Madrid, Spain, (20) INFN MAGIC Group: INFN Sezione di Torino and Universitá degli Studi di Torino, Torino, Italy, (21) INFN MAGIC Group: INFN Sezione di Bari and Dipartimento Interateneo di Fisica dell'Universitá e del Politecnico di Bari, Bari, Italy, (22) Croatian MAGIC Group: University of Rijeka, Department of Physics, Rijeka, Croatia, (23) Institut für Theoretische Physik und Astrophysik, Fakultät für Physik und Astronomie, Universität Würzburg, Würzburg, Germany Universität Würzburg, Würzburg, Germany, (24) Finnish MAGIC Group: Finnish Centre for Astronomy with ESO, University of Turku, Turku, Finland, (25) Departament de Física, and CERES-IEEC, Universitat Autónoma de Barcelona, Bellaterra, Spain, (26) Armenian MAGIC Group: ICRANet-Armenia at NAS RA, Yerevan, Armenia, (27) Croatian MAGIC Group: University of Split, Faculty of Electrical Engineering, Mechanical Engineering and Naval Architecture (FESB), Split, Croatia, (28) Croatian MAGIC Group: Josip Juraj Strossmayer University of Osijek, Department of Physics, Osijek, Croatia (29) Japanese MAGIC Group: Department of Physics, Kyoto University, Kyoto, Japan, (30) Japanese MAGIC Group: Department of Physics, Tokai University, Hiratsuka, Kanagawa, Japan, (31) Saha Institute of Nuclear Physics, HBNI, Kolkata, India, (32) Institute for Nuclear Research and Nuclear Energy, Sofia, Bulgaria, (33) Finnish MAGIC Group: Astronomy Research Unit, University of Oulu, Oulu, Finland, (34) Croatian MAGIC Group: Ruđer Bošković Institute, Zagreb, Croatia, (35) Japanese MAGIC Group: Physics Program, Graduate School of Advanced Science and Engineering, Hiroshima University, Hiroshima, Japan, (36) INFN MAGIC Group: INFN Sezione di Perugia, Perugia, Italy, (37) INFN MAGIC Group: INFN Roma Tor Vergata, Roma, Italy, (38) also at International Center for Relativistic Astrophysics (ICRA), Rome, Italy, (39) now at Department for Physics and Technology, University of Bergen, Norway, (40) now at University of Innsbruck, (41) also at Port d'Informació Científica (PIC), Bellaterra (Barcelona) Spain, (42) now at Ruhr-Universität Bochum, Fakultät für Physik und Astronomie, Astronomisches Institut (AIRUB), Bochum, Germany, (43) now at Department of Astronomy, University of California Berkeley, Berkeley CA, (44) also at Dipartimento di Fisica, Universitá di Trieste, Trieste, Italy, (45) now at Laboratoire d'Annecy de Physique des Particules (LAPP), CNRS-IN2P3, Annecy Cedex, France, (46) also at INAF Trieste and Dept. of Physics and Astronomy, University of Bologna)
Download a PDF of the paper titled Combined searches for dark matter in dwarf spheroidal galaxies observed with the MAGIC telescopes, including new data from Coma Berenices and Draco, by MAGIC Collaboration: V. A. Acciari (1) and 370 other authors
Abstract: Milky Way dwarf spheroidal galaxies (dSphs) are among the best candidates to search for signals of dark matter annihilation with Imaging Atmospheric Cherenkov Telescopes, given their high mass-to-light ratios and the fact that they are free of astrophysical gamma-ray emitting sources. Since 2011, MAGIC has performed a multi-year observation program in search for Weakly Interacting Massive Particles (WIMPs) in dSphs. Results on the observations of Segue 1 and Ursa Major II dSphs have already been published and include some of the most stringent upper limits (ULs) on the velocity-averaged cross-section $\langle \sigma_<\mathrm> v \rangle$ of WIMP annihilation from observations of dSphs. In this work, we report on the analyses of 52.1 h of data of Draco dSph and 49.5 h of Coma Berenices dSph observed with the MAGIC telescopes in 2018 and in 2019 respectively. No hint of a signal has been detected from either of these targets and new constraints on the $\langle \sigma_<\mathrm > v \rangle$ of WIMP candidates have been derived. In order to improve the sensitivity of the search and reduce the effect of the systematic uncertainties due to the $J$-factor estimates, we have combined the data of all dSphs observed with the MAGIC telescopes. Using 354.3 h of dSphs good quality data, 95 % CL ULs on $\langle \sigma_<\mathrm > v \rangle$ have been obtained for 9 annihilation channels. For most of the channels, these results reach values of the order of $10^ $cm$^3$/s at $1$ TeV and are the most stringent limits obtained with the MAGIC telescopes so far.
| Comments: | 17 pages, 5 figures |
| Subjects: | High Energy Astrophysical Phenomena (astro-ph.HE) |
| Cite as: | arXiv:2111.15009 [astro-ph.HE] |
| (or arXiv:2111.15009v1 [astro-ph.HE] for this version) | |
| https://doi.org/10.48550/arXiv.2111.15009 |
These abs mean business. You can tell by the setup in the background that these abs produce some sort of audio content—content that would surely be “on-the-air” if not for the corporate control of radio. It’s a damn shame that there’s no other outlet for music in 2015.
Additionally, abs contribute to a mage's overall health and well-being. A strong core helps maintain good posture, balance, and stability, which are important in performing intricate magical movements and gestures. Moreover, strong abs can prevent back pain and injuries that can hinder a mage's ability to focus and concentrate on their magical studies. Magic school abs matter not only for practical reasons but also for aesthetic purposes. A mage with well-defined abs is often seen as more powerful and authoritative. They exude confidence and command respect from their peers. In the competitive world of magic, having strong abs can give a mage an edge over their rivals and enhance their reputation within the magical community. However, it is essential to note that abs alone do not determine a mage's overall magical prowess. Physical fitness is just one aspect of magical training, and other factors such as mental focus, knowledge, and experience are equally important. Nevertheless, strong abs can enhance a mage's overall magical abilities and contribute to their success in the magical world. In conclusion, magic school abs matter because they are an indicator of a mage's physical fitness, core strength, and control over magical energy. Strong abs provide the foundation for performing complex spells and movements, while also contributing to overall health and well-being. While abs alone do not determine a mage's magical prowess, they can enhance a mage's abilities and reputation within the magical community..
Reviews for "The Elements of Magic: How Abdominal Strength Connects with the Elements"
1. Sara - 2/5 stars - "I was really disappointed with 'Magic School Abs Matter'. The plot was weak and the characters felt one-dimensional. I was hoping for a captivating story set in a magical school, but instead, I was left bored and uninterested. The writing style felt amateurish and at times, the dialogue was cringe-worthy. Overall, I wouldn't recommend this book to anyone looking for an engaging fantasy read."
2. John - 1/5 stars - "I couldn't finish 'Magic School Abs Matter'. The story was cliché and predictable from the start. The characters lacked depth and development, making it difficult to connect with any of them. The writing was juvenile, filled with unnecessary descriptions and tedious dialogue. I found myself rolling my eyes throughout the book. Save your time and money, there are much better fantasy books out there."
3. Emily - 2/5 stars - "As a fan of magical school stories, I was excited to read 'Magic School Abs Matter', but it fell short of my expectations. The plot seemed disjointed and rushed, with important events and explanations glossed over. The concept of magic school was intriguing but poorly executed. Additionally, I found some of the dialogue to be unrealistic and forced. Overall, the book had potential, but the execution and lackluster writing left me unsatisfied."
4. Mark - 1/5 stars - "I regret wasting my time on 'Magic School Abs Matter'. The story felt like a cheap imitation of other popular magical school books. The characters were forgettable and uninspiring, and the world-building was underdeveloped. The writing style was unremarkable, and I struggled to stay engaged with the story. There are far better options in the genre, and I would suggest giving this one a pass."
5. Jessica - 2/5 stars - "I expected more from 'Magic School Abs Matter' given its intriguing title, but it failed to deliver. The plot felt disjointed and lacked a clear direction. The characters were unremarkable and failed to elicit any emotional connection. The pacing was inconsistent, and the ending was unsatisfying. Overall, the book felt like a missed opportunity to explore an interesting concept. I would recommend looking elsewhere for a captivating magical school read."