000064666 001__ 64666 000064666 005__ 20180207125353.0 000064666 037__ $$aTAZ-TFM-2017-658 000064666 041__ $$aeng 000064666 1001_ $$aGonzález San Emeterio, Miguel 000064666 24200 $$aRadioPy: a synchrotron radio package in Python 000064666 24500 $$aRadioPy: un paquete en Python para analizar emisión radio sincrotrón 000064666 260__ $$aZaragoza$$bUniversidad de Zaragoza$$c2017 000064666 506__ $$aby-nc-sa$$bCreative Commons$$c3.0$$uhttp://creativecommons.org/licenses/by-nc-sa/3.0/ 000064666 520__ $$aRadioPy is an open source Python package for radio astrophysics capable of fitting spectra of synchrotron radio emission. Adapted for supernovae in its first version, one of its main features is that it can perform a complete an automatic analysis for a sequence of supernova spectra and calculate the shockwave radius (R), the intensity of the magnetic field (B) and the circumstellar density (A) and their evolution over time. Its other main feature is its object-oriented architecture that sets a standard on how to record the data regarding the non-thermal emission of radio sources and at the same time provides an easily extendible structure designed to evolve. The design of the architecture makes it easy to use and to extend, allowing researchers all over the world to download RadioPy and implement their own models and methods easily. The first version of this package contains 15 classes and 126 methods (version: June 2017) and provides robust algorithms for fitting spectra to an approximation of the Synchrotron Self-Absorption (SSA) model. The development of those algorithms and the goodness of the approximation are reasonable and they are discussed in the present document. A comparison between the results in the literature and those obtained with RadioPy for a case study of the radio evolution of supernova SN2011dh proved the capabilities of the software tool. 000064666 521__ $$aMáster Universitario en Física y Tecnologías Físicas 000064666 540__ $$aDerechos regulados por licencia Creative Commons 000064666 700__ $$aPérez Torres, Miguel$$edir. 000064666 7102_ $$aUniversidad de Zaragoza$$bFísica Teórica$$cAstronomía y astrofísica 000064666 8560_ $$f723701@celes.unizar.es 000064666 8564_ $$s1837547$$uhttps://zaguan.unizar.es/record/64666/files/TAZ-TFM-2017-658.pdf$$yMemoria (eng) 000064666 8564_ $$s386561$$uhttps://zaguan.unizar.es/record/64666/files/TAZ-TFM-2017-658_ANE.pdf$$yAnexos (eng) 000064666 909CO $$ooai:zaguan.unizar.es:64666$$pdriver$$ptrabajos-fin-master 000064666 950__ $$a 000064666 951__ $$adeposita:2018-02-07 000064666 980__ $$aTAZ$$bTFM$$cCIEN