HIDE & SEEK: End-to-end packages to simulate and process radio survey data

被引:24
作者
Akeret, J. [1 ]
Seehars, S. [1 ]
Chang, C. [1 ]
Monstein, C. [1 ]
Amara, A. [1 ]
Refregier, A. [1 ]
机构
[1] Swiss Fed Inst Technol, Inst Astron, Dept Phys, Wolfgang Pauli Str 27, CH-8093 Zurich, Switzerland
关键词
Radio cosmology; Forward modeling; RFI mitigation; HIDE; SEEK; PIPELINE;
D O I
10.1016/j.ascom.2016.11.001
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
As several large single-dish radio surveys begin operation within the coming decade, a wealth of radio data will become available and provide a new window to the Universe. In order to fully exploit the potential of these datasets, it is important to understand the systematic effects associated with the instrument and the analysis pipeline. A common approach to tackle this is to forward-model the entire system from the hardware to the analysis of the data products. For this purpose, we introduce two newly developed, open-source Python packages: the HI Data Emulator (HIDE) and the Signal Extraction and Emission Kartographer (SEEK) for simulating and,processing single-dish radio survey data. HIDE forward models the process of collecting astronomical radio signals in a single-dish radio telescope instrument and outputs pixel-level time-ordered-data. SEEK processes the time-ordered-data, removes artifacts from Radio Frequency Interference (RFI), automatically applies flux calibration, and aims to recover the astronomical radio signal. The two packages can be used separately or together depending on the application. Their modular and flexible nature allows easy adaptation to other instruments and datasets. We describe the basic architecture of the two packages and examine in detail the noise and RFI modeling in HIDE, as well as the implementation of gain calibration and RH mitigation in SEEK. We then apply HIDE & SEEK to forward-model a Galactic survey in the frequency range 990-1260 MHz based on data taken at the Bleien Observatory. For this survey, we expect to cover 70% of the full sky and achieve a median signal-to-noise ratio of approximately 5-6 in the cleanest channels including systematic uncertainties. However, we also point out the potential challenges of high RFI contamination and baseline removal when examining the early data from the Bleien Observatory. The fully documented HIDE & SEEK packages are available at http://hideseek.phys.ethz.ch/ and are published under the GPLv3 license on-GitHub. (C)2016 Elsevier B.V. All rights reserved.
引用
收藏
页码:8 / 17
页数:10
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