The cosipy library: COSI’s high-level analysis software

Authors

Israel Martinez-Castellanos, NASA Goddard Space Flight Center
Savitri Gallego, Johannes Gutenberg-Universität Mainz
Chien You Huang, National Tsing Hua University
Chris Karwin, NASA Goddard Space Flight Center
Carolyn Kierans, NASA Goddard Space Flight Center
Jan Peter Lommler, Johannes Gutenberg-Universität Mainz
Saurabh Mittal, Julius-Maximilians-Universität Würzburg
Michela Negro, Louisiana State University
Eliza Neights, NASA Goddard Space Flight Center
Sean N. Pike, University of California, San Diego
Yong Sheng, Clemson University
Thomas Siegert, Julius-Maximilians-Universität Würzburg
Hiroki Yoneda, Julius-Maximilians-Universität Würzburg
Andreas Zoglauer, Space Sciences Laboratory
John A. Tomsick, Space Sciences Laboratory
Steven E. Boggs, Space Sciences Laboratory
Dieter Hartmann, Clemson University
Marco Ajello, Clemson University
Eric Burns, Louisiana State University
Chris Fryer, Los Alamos National Laboratory
Alexander Lowell, Space Sciences Laboratory
Julien Malzac, Institut de Recherche en Astrophysique et Planétologie (IRAP)
Jarred Roberts, University of California, San Diego
Pascal Saint-Hilaire, Space Sciences Laboratory
Albert Shih, NASA Goddard Space Flight Center
Clio Sleator, U.S. Naval Research Laboratory
Tadayuki Takahashi, The University of Tokyo
Fabrizio Tavecchio, Istituto Nazionale Di Astrofisica, Rome
Eric Wulf, U.S. Naval Research Laboratory
Jacqueline Beechert, Space Sciences Laboratory
Hannah Gulick, Space Sciences Laboratory
Alyson Joens, Space Sciences Laboratory
Hadar Lazar, Space Sciences Laboratory

Document Type

Conference Proceeding

Publication Date

9-27-2024

Abstract

The Compton Spectrometer and Imager (COSI) is a selected Small Explorer (SMEX) mission launching in 2027. It consists of a large field-of-view Compton telescope that will probe with increased sensitivity the under-explored MeV gamma-ray sky (0.2-5 MeV). We will present the current status of cosipy, a Python library that will perform spectral and polarization fits, image deconvolution, and all high-level analysis tasks required by COSI’s broad science goals: uncovering the origin of the Galactic positrons, mapping the sites of Galactic nucleosynthesis, improving our models of the jet and emission mechanism of gamma-ray bursts (GRBs) and active galactic nuclei (AGNs), and detecting and localizing gravitational wave and neutrino sources. The cosipy library builds on the experience gained during the COSI balloon campaigns and will bring the analysis of data in the Compton regime to a modern open-source likelihood-based code, capable of performing coherent joint fits with other instruments using the Multi-Mission Maximum Likelihood framework (3ML). In this contribution, we will also discuss our plans to receive feedback from the community by having yearly software releases accompanied by publicly-available data challenges.

Publication Source (Journal or Book title)

Proceedings of Science

This document is currently not available here.

Share

COinS