PolarLight: a CubeSat X-ray Polarimeter based on the Gas Pixel Detector
Abstract
The gas pixel detector (GPD) is designed and developed for high-sensitivity astronomical X-ray polarimetry, which is a new window about to open in a few years. Due to the small mass, low power, and compact geometry of the GPD, we propose a CubeSat mission Polarimeter Light (PolarLight) to demonstrate and test the technology directly in space. There is no optics but a collimator to constrain the field of view to 2.3 degrees. Filled with pure dimethyl ether (DME) at 0.8 atm and sealed by a beryllium window of 100 micron thick, with a sensitive area of about 1.4 mm by 1.4 mm, PolarLight allows us to observe the brightest X-ray sources on the sky, with a count rate of, e.g., ~0.2 counts/s from the Crab nebula. The PolarLight is 1U in size and mounted in a 6U CubeSat, which was launched into a low Earth Sun-synchronous orbit on October 29, 2018, and is currently under test. More launches with improved designs are planned in 2019. These tests will help increase the technology readiness for future missions such as the enhanced X-ray Timing and Polarimetry (eXTP), better understand the orbital background, and may help constrain the physics with observations of the brightest objects.
Keywords
Cite
@article{arxiv.1903.01619,
title = {PolarLight: a CubeSat X-ray Polarimeter based on the Gas Pixel Detector},
author = {Hua Feng and Weichun Jiang and Massimo Minuti and Qiong Wu and Aera Jung and Dongxin Yang and Saverio Citraro and Hikmat Nasimi and Jiandong Yu and Ge Jin and Jiahui Huang and Ming Zeng and Peng An and Luca Baldini and Ronaldo Bellazzini and Alessandro Brez and Luca Latronico and Carmelo Sgrò and Gloria Spandre and Michele Pinchera and Fabio Muleri and Paolo Soffitta and Enrico Costa},
journal= {arXiv preprint arXiv:1903.01619},
year = {2019}
}
Comments
Accepted for publication in Experimental Astronomy