The SNAD Viewer: Everything You Want to Know about Your Favorite ZTF Object

被引:5
|
作者
Malanchev, Konstantin [1 ,2 ]
Kornilov, Matwey V. [2 ,3 ]
Pruzhinskaya, Maria V. [2 ,4 ]
Ishida, Emille E. O. [4 ]
Aleo, Patrick D. [1 ,5 ]
Korolev, Vladimir S.
Lavrukhina, Anastasia [6 ]
Russeil, Etienne [4 ]
Sreejith, Sreevarsha [7 ]
Volnova, Alina A. [8 ]
Voloshina, Anastasiya [4 ]
Krone-Martins, Alberto [9 ,10 ]
机构
[1] Univ Illinois, Dept Astron, 1002 W Green St, Urbana, IL 61801 USA
[2] Lomonosov Moscow State Univ, Sternberg Astron Inst, Univ Sky Pr 13, Moscow 119234, Russia
[3] Natl Res Univ Higher Sch Econ, 21-4 Staraya Basmannaya Ulitsa, Moscow 105066, Russia
[4] Univ Clermont Auvergne, CNRS, LPC, IN2P3, F-63000 Clermont Ferrand, France
[5] Natl Ctr Supercomp Applicat, Ctr Astro Phys Surveys, Urbana, IL 61801 USA
[6] Lomonosov Moscow State Univ, Fac Space Res, Leninsky Gori 1 bld 52, Moscow 119234, Russia
[7] Phys Dept, Brookhaven Natl Lab, Upton, NY 11973 USA
[8] Russian Acad Sci IKI, Space Res Inst, 84-32 Profsoyuznaya St, Moscow 117997, Russia
[9] Univ Calif Irvine, Donald Bren Sch Informat & Comp Sci, Irvine, CA 92697 USA
[10] Univ Lisbon, Fac Ciencias, CENTRA, SIM, Ed C8, P-1749016 Lisbon, Portugal
基金
美国国家航空航天局;
关键词
VARIABLE-STARS; ANOMALY-DETECTION; GENERAL CATALOG; TRANSIENT; DATABASE; CLASSIFICATION; PACKAGE; VERSION; EVENTS; GOALS;
D O I
10.1088/1538-3873/acb292
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We describe the SNAD Viewer, a web portal for astronomers which presents a centralized view of individual objects from the Zwicky Transient Facility's (ZTF) data releases, including data gathered from multiple publicly available astronomical archives and data sources. Initially built to enable efficient expert feedback in the context of adaptive machine learning applications, it has evolved into a full-fledged community asset that centralizes public information and provides a multi-dimensional view of ZTF sources. For users, we provide detailed descriptions of the data sources and choices underlying the information displayed in the portal. For developers, we describe our architectural choices and their consequences such that our experience can help others engaged in similar endeavors or in adapting our publicly released code to their requirements. The infrastructure we describe here is scalable and flexible and can be personalized and used by other surveys and for other science goals. The Viewer has been instrumental in highlighting the crucial roles domain experts retain in the era of big data in astronomy. Given the arrival of the upcoming generation of large-scale surveys, we believe similar systems will be paramount in enabling an optimal exploitation of the scientific potential enclosed in current terabyte and future petabyte-scale data sets. The Viewer is publicly available online at https://ztf.snad.space.
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页数:18
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