2.1k citations · 4.3k across the 14 of their papers we have counts for
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AMPEL workflows for LSST: Modular and reproducible real-time photometric classification
Jakob Nordin, Valery Brinnel, Jakob van Santen +2
Modern time-domain astronomical surveys produce high throughput data streams which require tools for processing and analysis. This will be critical for programs making full use of…
SNGuess: A method for the selection of young extragalactic transients
N. Miranda, J. C. Freytag, J. Nordin +7
With a rapidly rising number of transients detected in astronomy, classification methods based on machine learning are increasingly being employed. Their goals are typically to obt…
Transient processing and analysis using : Alert Management, Photometry and Evaluation of Lightcurves
J. Nordin, V. Brinnel, J. van Santen +18
Both multi-messenger astronomy and new high-throughput wide-field surveys require flexible tools for the selection and analysis of astrophysical transients. We here introduce the A…
A Fully Automated Integral Field Spectrograph Pipeline for the SEDMachine: pysedm
M. Rigault, J. D. Neill, N. Blagorodnova +8
Current time domain facilities are discovering hundreds of new galactic and extra-galactic transients every week. Classifying the ever-increasing number of transients is challengin…
The Zwicky Transient Facility: Science Objectives
Matthew J. Graham, S. R. Kulkarni, Eric C. Bellm +114
The Zwicky Transient Facility (ZTF), a public-private enterprise, is a new time domain survey employing a dedicated camera on the Palomar 48-inch Schmidt telescope with a 47 deg$^2…
The Zwicky Transient Facility: System Overview, Performance, and First Results
Eric C. Bellm, Shrinivas R. Kulkarni, Matthew J. Graham +112
The Zwicky Transient Facility (ZTF) is a new optical time-domain survey that uses the Palomar 48-inch Schmidt telescope. A custom-built wide-field camera provides a 47 deg fiel…
: Estimating Transient Discovery Rates for the Zwicky Transient Facility
Ulrich Feindt, Jakob Nordin, Mickael Rigault +4
When planning a survey for astronomical transients, many factors such as cadence, filter choice, sky coverage, and depth of observations need to be balanced in order to optimize th…