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

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arxiv 2211.07605 v2 pith:VQUMYMWT submitted 2022-11-14 astro-ph.IM

classification astro-ph.IM
keywords dataviewerdescribepubliclysnadsourcesavailablechoices
verification ladder T0 review T1 audit T2 compute T3 formal
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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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Cited by 1 Pith paper

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  1. XMM-Newton follow-up of two eROSITA X-ray binary candidates

    astro-ph.HE 2025-07 conditional novelty 4.0 of 10

    Two eROSITA X-ray binary candidates are reclassified: J061331 as a chromospherically active M-type subgiant and J161201 as a novalike cataclysmic variable with a tentative 4.802-hour orbital period.

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