ASIVA – Platform for observational and computational analysis of stellar variables

IF 1.9 4区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Parvej Reja Saleh , Tanveer Singh , Debasish Hazarika , Surabhi Rajkumari , Saurabh Rajkumar , Pritam Das , Padmakar Singh Parihar , Eeshankur Saikia
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引用次数: 0

Abstract

The astronomical data analysis consists of two crucial process; data reduction of the captured images and data analysis of the derived magnitudes. We present the platform ASIVA, a data analysis platform which comes along with a data reduction pipeline. The data reduction pipeline gives flexibility to analyse the FITS images and also perform image alignment for detecting the correct image coordinates for required objects. It can be custom scheduled with cron jobs so that it picks the latest data and appends the results accordingly. The data analysis platform allows user to effectively analyse the ensemble data and perform accurate data processing and grouping with ease. It is integrated with a custom algorithm to detect the variable stars from an ensemble with its relative standard deviations. The statistical, spectral and non-linear dynamics features can be extracted from time series data which can be eventually used for in-depth analysis. To validate the capability, we have analysed 15 nights of Orion Nebula Cluster field in I filter which had 1585 images. ASIVA reduces manual effort to a great extent thus saves analysis time and excludes human errors.

Abstract Image

ASIVA - 恒星变量观测和计算分析平台
天文数据分析包括两个关键过程:对拍摄到的图像进行数据还原和对得出的星等进行数据分析。我们介绍的 ASIVA 平台是一个数据分析平台,它配备了数据还原管道。数据还原流水线可以灵活地分析 FITS 图像,还可以执行图像配准,为所需的天体检测正确的图像坐标。它可以通过 cron 作业进行自定义调度,以便选取最新数据并相应地添加结果。数据分析平台可让用户有效地分析集合数据,并轻松执行精确的数据处理和分组。它集成了一种定制算法,可以从集合中检测出变星及其相对标准偏差。可以从时间序列数据中提取统计、光谱和非线性动力学特征,最终用于深入分析。为了验证其能力,我们分析了猎户座星云星团15个夜晚的I滤光片,共1585幅图像。ASIVA 在很大程度上减少了人工操作,从而节省了分析时间并避免了人为错误。
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来源期刊
New Astronomy
New Astronomy 地学天文-天文与天体物理
CiteScore
4.00
自引率
10.00%
发文量
109
审稿时长
13.6 weeks
期刊介绍: New Astronomy publishes articles in all fields of astronomy and astrophysics, with a particular focus on computational astronomy: mathematical and astronomy techniques and methodology, simulations, modelling and numerical results and computational techniques in instrumentation. New Astronomy includes full length research articles and review articles. The journal covers solar, stellar, galactic and extragalactic astronomy and astrophysics. It reports on original research in all wavelength bands, ranging from radio to gamma-ray.
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