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The Zwicky Transient Facility Alert Distribution System

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arxiv 1902.02227 v1 pith:PFHMZR27 submitted 2019-02-06 astro-ph.IM

classification astro-ph.IM
keywords systemalertdistributionstreamalertsprocessingproductionsurvey
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The Zwicky Transient Facility (ZTF) survey generates real-time alerts for optical transients, variables, and moving objects discovered in its wide-field survey. We describe the ZTF alert stream distribution and processing (filtering) system. The system uses existing open-source technologies developed in industry: Kafka, a real-time streaming platform, and Avro, a binary serialization format. The technologies used in this system provide a number of advantages for the ZTF use case, including (1) built-in replication, scalability, and stream rewind for the distribution mechanism; (2) structured messages with strictly enforced schemas and dynamic typing for fast parsing; and (3) a Python-based stream processing interface that is similar to batch for a familiar and user-friendly plug-in filter system, all in a modular, primarily containerized system. The production deployment has successfully supported streaming up to 1.2 million alerts or roughly 70 GB of data per night, with each alert available to a consumer within about 10 s of alert candidate production. Data transfer rates of about 80,000 alerts/minute have been observed. In this paper, we discuss this alert distribution and processing system, the design motivations for the technology choices for the framework, performance in production, and how this system may be generally suitable for other alert stream use cases, including the upcoming Large Synoptic Survey Telescope.

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Forward citations

Cited by 4 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. SN 2023uqf: An Interacting Supernova Coincident with a High-Energy Neutrino

    astro-ph.HE 2025-08 conditional novelty 7.0 of 10

    SN 2023uqf, a rare interacting Type Ibn supernova found coincident with neutrino IC231004A, is the first observational evidence that interacting supernovae are hadronic accelerators.

  2. AT 2024qfm: a luminous fast blue optical transient at a redshift of z = 0.2267 identified by Lasair-ZTF

    astro-ph.HE 2026-08 accept novelty 6.0 of 10

    A new luminous fast blue optical transient, AT 2024qfm, was discovered at z=0.2267 with a Lasair broker filter and matches AT 2018cow in luminosity and 13 day fade.

  3. ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo

    astro-ph.HE 2026-08 conditional novelty 6.0 of 10

    The tidal disruption event ATLAS22kjn shows a resolved 9-day pre-peak bump, coronal lines that imply a stable ~1e6 K ionising source, and a dust echo whose covering fraction is much higher than typical TDEs.

  4. AT2021yky: A Fast-Rising Optical Transient with Evolving Broad Hydrogen Emission Consistent with an Ambiguous Nuclear Transient

    astro-ph.HE 2026-08 accept novelty 5.0 of 10

    AT2021yky is a fast-rising, cool nuclear flare with only broad H-alpha emission, best classified as an ambiguous nuclear transient rather than a typical TDE, AGN flare, supernova, or LFBOT.

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