ZTF runs its signature summer school for a fifth year

For a fifth consecutive year, we hosted the ZTF summer school from July 21 to 25 at the University of Minnesota, where senior undergraduates, graduate students, and postdocs learned about "Data Science in the Rubin Era." We welcomed 75 attendees from nearly 50 different institutions to the hybrid workshop. The format of the school focused on the delivery of engaging Jupyter notebook-based talks and tutorials covering a variety of science cases and technical topics.

Highlights included hands-on tutorials covering the development of fast transient metrics for Rubin Observatory, demonstration of our new broker BOOM (the Burst and Outburst Observations Monitor), and applications of our multi-modal classification pipeline, AppleCiDEr (Applying Multimodal Learning to Classify Transient Detections Early), making detection and simulating the evolution of light echoes from historical transients. The school ended with a hackathon on Friday, where the students applied what they had learned to a sample survey data set from ZTF and built a multi-modal classifier.

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Mansi Kasliwal appointed as the next director of Palomar Observatory

Mansi Kasliwal, the principal investigator of the Zwicky Transient Facility and a professor of astronomy at Caltech was appointed as the new Palomar Observatory Director, making her the first woman to lead the historic facility. Mansi's research career has been deeply connected to the observatory from her PhD days to today when she is an internationally recognized leader in time-domain and multi-messenger astrophysics. She has been central to building and leading discovery engines at Palomar, including the Zwicky Transient Facility (ZTF), the pioneering infrared surveys Palomar Gattini-IR (PGIR) and WINTER, and the newly-commissioned Next Generation Palomar Spectrograph (NGPS). Mansi's appointment marks a historic milestone and an exciting new chapter for the Observatory as she takes on the mission to harnessing Palomar’s unique capabilities to explore the dynamic universe.

Sky & Telescope

The ZTF Scientific Steering Committee invites proposals to the “ZTF Experiments” program, designed to explore one or more novel aspects of ZTF scientific/technical capabilities by employing non-standard field selection, cadence, and filter choice to pursue specific scientific questions. Non-standard in this context refers to ZTF observing configurations that are distinct from those in the standard survey, which observes the joint ZTF+LSST footprint at 1-day cadence in g-band, r-band, and i-band for 30s each.

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Public Data Releases in ZTF3

ZTF continues science observations in 2025 and 2026 thanks to extended funding by the National Science Foundation. There will be two yearly public releases that will become available in the January 2026 and 2027. Public releases are announced on our website and soial media X account @ztfsurvey.

Data Access via IRSA

Science Highlights

Black Hole Flare is Biggest and Most Distant Seen

Graham, J Matthew et al

ZTF has co-discovered the most distant and brightest flare from a black hole eating away a massive star. The event has taken place in the distant universe 10 billion light years away and at its brightest, it release the energy equivalent to 100 trillion suns.

Press Release

ZTF catches a never-before-seen flare of a supernova

Schulze, Steve et al.; Nature

A large team of astronomers, led by ZTF partners at the Northwestern university stumbled upon a unique explosion of a supernova from a massive star back in Sept 2021. After extensive analysis of the supernova using data from multiple telescopes around the world, the astronomers believe they have seen for the first time the inner layers of a dying star.

Press Release

Prediscovery activity of a new interstellar object

Quanzhi Ye et al.,

The authors report on the prediscovery observations and constraints of the new interstellar comet 3I/2025 N1 (ATLAS), made by the Zwicky Transient Facility (ZTF), for the inbound leg of the comet out to a heliocentric distance of rh=17au, or approximately a year before its discovery.

Interacting supernova coincident with a high energy neutrino

Stein, Robert et al.,

Astrophysical high-energy (TeV-PeV) neutrinos were first discovered in 2013, but their origin remains largely unknown. In this paper, authors present SN 2023uqf, a supernova found in coincidence with high-energy neutrino IC231004A, as part of a systematic optical follow-up program with the Zwicky Transient Facility.

A machine learning tool to predict kilonova light curves

Plestkova, Natalya, et al.,

The authors have developed a public tool to predict kilonova light curves using simulated low-latency alert data from the International Gravitational Wave Network during observing runs 4 (O4) and 5 (O5). It uses a bidirectional long-short-term memory (LSTM) model to forecast kilonova light curves from binary neutron star and neutron star-black hole mergers in ZTF and Rubin's LSST filters. The models are publicly available and can help plan follow-up of candidate events discovered by current and next-generation public surveys.


ZTF search for circumstellar debris transits in white dwarfs

Bhattacharjee, Soumyadeep et al.,

White dwarfs (WDs) showing transits from orbiting planetary debris provide significant insights into the structure and dynamics of debris disks, which are eventually accreted to produce metal pollution. This is a rare class of objects with only eight such reported systems. In this work, the authors perform a systematic search for such systems within 500 pc in the Gaia-eDR3 catalog of WDs using the light curves from the Zwicky Transient Facility (ZTF) and present six new candidates.

Studying ice water in 243P/NEAT and other comets

Kelley, Michael et al.,

ZTF partners from the University of Maryland who study solar system bodies have observed several comet outbursts which provide scientists with the opportunity to study the properties of water ice - a fundamental building block in solar system objects.

ZTF observetions of a neutron star merger candidate

Ahumada, Tomas et al.,

Authors present the ZTF search in response to S250206dm, a bona fide event with a false alarm rate of one in 25 years, detected by the International Gravitational Wave Network (IGWN). Although the event was significant, the nature of the compact objects involved remains unclear, with at least one likely neutron star. ZTF covered 68% of the localization region and no likely optical counterpart was identified. The paper provides details about the ZTF strategy, potential candidates, and the observations that helped rule out candidates, including sources circulated by other collaborations.

 

ZTF Faces

Every summer we welcome a number of undergraduate students who carry out a summer research project with members of our team.

Shreyashi Manna
(Shiv Nadar Uni)

Summer project: Photometric and morphological behavior of near-Sun asteroids
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Samridh Tiwari
(IIT-Bombay)

Summer project: Studying lightcurves of fast moving near-Earth asteroids with ZTF
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Amaliya Atamalibekova
(Cornell University)

Summer project: Search for gamma-ray emission from broad-lined Ic supernovae
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Nat Sutton
(CWU)

Summer project: Searching for exclipsing white dwarf binaries with SCoPe
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Community science with ZTF

We highlight scientific publications from individuals and groups outside of the ZTF partnership that use ZTF public data

Multi-year stacking searches for solar system bodies

Geringer-Sameth, Alex ; Golovich, Nathan ; Iwabuchi, Keita

[Abstract]
Digital tracking detects faint solar system bodies by stacking many images along hypothesized orbits, revealing objects that are undetectable in every individual exposure. Previous searches have been restricted to small areas and short time baselines. We present a general framework to quantify both sensitivity and computational requirements for digital tracking of nonlinear motion across the full sky over multi-year baselines. We start from matched-filter stacking and derive how signal-to-noise ratio (SNR) degrades with trial orbit mismatch, which leads to a metric tensor on orbital parameter space. The metric defines local Euclidean coordinates in which SNR loss is isotropic, and a covariant density that specifies the exact number of trial orbits needed for a chosen SNR tolerance. We validate the approach with Zwicky Transient Facility (ZTF) data, recovering known objects in blind searches that stack thousands of images over six years along billions of trial orbits. We quantify ZTF’s sensitivity to populations beyond 5 au and show that stacking reaches most of the remaining Planet 9 parameter space. The computational demands of all-sky, multi-year tracking are extreme, but we demonstrate that time segmentation and image blurring greatly reduce orbit density at modest sensitivity cost. Stacking effectively boosts medium-aperture surveys to the Rubin Observatory single-exposure depth across the northern sky. Digital tracking in dense Rubin observations of a 10 sq. deg field is tractable and could detect trans-Neptunian objects to 27th magnitude in a single night, with deep drilling fields reaching fainter still.

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ZTF is supported by the National Science Foundation and a collaboration including the following universities : University of Maryland, College Park, USA; Drexel University, USA; Cornell University, USA; University of California, Berkeley; University of North Caroline Chapel Hill, USA; Institute of Science and Technology, Austria;National Central University, Taiwan; German Center for Astrophysics (DZA), Germany; IPAC/Caltech, USA; Caltech, USA. Operations are conducted by COO, IPAC and University of Washington.
Any opinions, findings, and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily reflect the views of the National Science Foundation.