# $\texttt{simsurvey}$: Estimating Transient Discovery Rates for the   Zwicky Transient Facility

**Authors:** Ulrich Feindt, Jakob Nordin, Mickael Rigault, Val\'ery Brinnel, Suhail, Dhawan, Ariel Goobar, and Marek Kowalski

arXiv: 1902.03923 · 2019-10-09

## TL;DR

This paper introduces 'simsurvey', a flexible software tool for simulating supernova lightcurves based on survey strategies, aiding in optimizing transient discovery plans like those for ZTF.

## Contribution

The paper presents 'simsurvey', a modular software package that allows customizable simulations of transient lightcurves for survey planning and analysis.

## Key findings

- ZTF will discover thousands of bright supernovae annually.
- Approximately 10 supernovae could be detected within two days of explosion.
- Simulations align well with actual early ZTF detection data.

## Abstract

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 the scientific gain of the survey. Here we present a software package called $\texttt{simsurvey}$ for simulating the supernova lightcurves that are expected based on a survey strategy, which can then be used to determine the potential for discoveries of each strategy in question. The code is set up in a modular fashion that allows easy modification of small details of the survey and enables the user to adapt it to any survey design and transient template that they wish to use in planning their survey. As an example of its utility, we use $\texttt{simsurvey}$ to simulate the lightcurve of several types of supernovae that the recently started Zwicky Transient Facility (ZTF) is expected to find and compare the results to the discoveries made during its early operations. We conclude that ZTF will find thousands of bright supernovae per year, of which about 10 could potentially be found with two days of explosion. Over the course of three years the survey will obtain lightcurves of about 1800 type Ia supernovae with $z < 0.1$ that can be used as distance indicators in cosmology if they are spectroscopically classified using additional telescopes. In a comparison to detections from the ZTF public survey, we found good agreement with the numbers of detections expected from the simulations.

## Full text

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## Figures

15 figures with captions in the complete paper: https://tomesphere.com/paper/1902.03923/full.md

## References

50 references — full list in the complete paper: https://tomesphere.com/paper/1902.03923/full.md

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Source: https://tomesphere.com/paper/1902.03923