The HST/WFC3 Quicklook Project: A User Interface to Hubble Space Telescope Wide Field Camera 3 Data

被引：0
|
作者：
Bourque, Matthew [1 ]
Bajaj, Varun [1 ]
Bowers, Ariel [1 ]
Dulude, Michael [1 ]
Durbin, Meredith [2 ]
Gosmeyer, Catherine [1 ]
Gunning, Heather [1 ]
Khandrika, Harish [1 ]
Martlin, Catherine [1 ]
Sunnquist, Ben [1 ]
Viana, Alex [3 ]
机构：
[1] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA
[2] Univ Washington, Dept Astron, Box 351580, Uw Seattle, WA 98195 USA
[3] Terbium Labs, Baltimore, MD USA
来源：
ASTROINFORMATICS | 2017年 / 12卷 / S325期
关键词：
Hubble Space Telescope; HST; Wide Field Camera 3; WFC3; Automation; Database; Filesystem; Website; !text type='Python']Python[!/text; Quicklook;
D O I：
10.1017/S174392131601276X
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The Hubble Space Telescope's Wide Field Camera 3 (WFC3) instrument, comprised of two detectors, UVIS (Ultraviolet-Visible) and IR (Infrared), has been acquiring similar to 50-100 images daily since its installation in 2009. The WFC3 Quicklook project provides a means for instrument analysts to store, calibrate, monitor, and interact with these data through the various Quicklook systems: (1) a similar to 175 TB filesystem, which stores the entire WFC3 archive on disk, (2) a MySQL database, which stores image header data, (3) a Python-based automation platform, which currently executes 22 unique calibration/ monitoring scripts, (4) a Python-based code library, which provides system functionality such as logging, downloading tools, database connection objects, and filesystem management, and (5) a Python/Flask-based web interface to the Quicklook system. The Quicklook project has enabled large-scale WFC3 analyses and calibrations, such as the monitoring of the health and stability of the WFC3 instrument, the measurement of similar to 20 million WFC3/ UVIS Point Spread Functions (PSFs), the creation of WFC3/IR persistence calibration products, and many others.
引用
收藏
页码：397 / 400
页数：4
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