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Fink filters

Each night, telescopes are sending raw alerts and the broker enriches these alerts by adding new information to identify interesting candidates for follow-up observations or further scientific processing. The raw incoming stream volume is huge, and each user might want to focus only on a subset of the stream. Hence the output of the broker contains filters that flag only particular parts of the stream to be distributed. Criteria are based on the alert entries: position, flux, properties, ... and Fink added values as filters act after science modules are applied.

Screenshot

Note that if the filters reduce the size of the stream, they do not filter the content of alerts, i.e. you will receive the full information of alerts distributed.

Available topics

Each stream subset from a particular filter is identified by a topic name. This stream can be accessed outside via its topic, and several users can poll the data from the same topic (see fink-client).

Below we summarise the default Fink topics:

Name Link Contents Status
fink_early_sn_candidates_ztf early_sn_candidates Return alerts considered as Early SN-Ia candidates. The data from this topic is pushed to TNS every night. deployed
fink_sn_candidates_ztf sn_candidates Return alerts considered as SN candidates deployed
fink_sso_ztf_candidates_ztf sso_ztf_candidates Return alerts with a counterpart in the Minor Planet Center database (Solar System Objects) deployed
fink_sso_fink_candidates_ztf sso_fink_candidates Return alerts considered as new Solar System Object candidates deployed
fink_kn_candidates_ztf kn_candidates Return alerts considered as Kilonova candidates based on Machine Learning deployed
fink_early_kn_candidates_ztf early_kn_candidates Return alerts considered as Kilonova candidates based on crossmatch and property cuts deployed
fink_rate_based_kn_candidates_ztf rate_based_kn_candidates Return alerts considered as Kilonova candidates following Andreoni et al. 2021 (https://arxiv.org/abs/2104.06352) deployed
fink_microlensing_candidates_ztf microlensing_candidates Return alerts considered as microlensing candidates deployed
fink_blazar_ztf blazar Return alerts flagged as Blazar, Blazar_Candidate, BLLac, or BLLac_Candidate in the SIMBAD database. deployed
fink_simbad_ztf simbad Return all alerts with a counterpart in the SIMBAD database. See left column of http://simbad.u-strasbg.fr/simbad/sim-display?data=otypes for more information available on demand
fink_<single-simbad-type>_ztf Example rrlyr Return alerts matching one specific type in the SIMBAD database. See left column of http://simbad.u-strasbg.fr/simbad/sim-display?data=otypes for more information available on demand
fink_grb_bronze MM module Alerts with a real bogus (rb) above 0.7, classified by Fink as an extragalactic event within the error location of a GRB event.
fink_grb_silver MM module Alerts satisfying the bronze filter with a grb_proba above 5 sigma.
fink_grb_gold MM module Alerts satisfying the silver filter with a mag_rate above 0.3 mag/day and a rb above 0.9.
fink_gw_bronze MM module Alerts with a real bogus (rb) above 0.7, classified by Fink as an extragalactic event within the error location of a GW event.

We also have many internal ones focusing on specific parts of the stream. Feel free also to propose new topics! The topic data is stored for 4 days after creation (i.e. you can access alert data up to 4 days after it has been emitted).

Create your filter for ZTF

This tutorial goes step-by-step for creating a filters used to define which information will be sent to you by the broker. Running entirely Fink just for testing a filter might be an overwhelming task. Fink can be a complex system, but hopefully it is highly modular such that you do not need all the parts to test one part in particular. In principle, to test a filter you only need Apache Spark installed, and processed data by Fink. Spark API exposes nearly the same methods for static or streaming DataFrame. Hence, to avoid complication due to streaming (e.g. creating streams with Kafka, reading streams, managing offsets, etc...), it is always best to prototype on static DataFrame. If the logic works for static, it will work for streaming.

Set up your development environment

First make sure you are working in the correct environment. You can either use the Fink Docker images:

# pull and run the image used for ZTF processing
docker run -t -i --rm julienpeloton/fink-ci:latest bash

The advantage of this method is that you have everything installed in it (Python and various frameworks).

Alternatively, you can install everything on your machine. For Python packages, just use a virtual environment:

conda create -n fink-env python=3.9
BASEURL=https://raw.githubusercontent.com/astrolabsoftware/fink-broker/master/deps
pip install -r $BASEURL/requirements.txt
pip install -r $BASEURL/requirements-science.txt
pip install -r $BASEURL/requirements-science-no-deps.txt

Then you need to install Apache Spark. If you opted for the Docker version, it is already installed for you. Otherwise just execute:

SPARK_VERSION=3.1.3
wget --quiet https://archive.apache.org/dist/spark/spark-${SPARK_VERSION}/spark-${SPARK_VERSION}-bin-${HADOOP_VERSION}.tgz
tar -xf spark-${SPARK_VERSION}-bin-${HADOOP_VERSION}.tgz
rm spark-${SPARK_VERSION}-bin-${HADOOP_VERSION}.tgz

and put these lines in your ~/.bash_profile:

export SPARK_HOME=/path/to/spark-${SPARK_VERSION}-bin-${HADOOP_VERSION}
export PATH=$PATH:$SPARK_HOME/bin
export PYTHONPATH=$PYTHONPATH:$SPARK_HOME/python

Fork and clone the fink-filters repository, and create a new folder in fink_filters. The name of the new folder does not matter much, but try to make it meaningful as much as possible!

Define your filter

A filter is typically a Python routine that selects which alerts need to be sent based on user-defined criteria. Criteria are based on the alert entries: position, flux, properties, ... plus all the added-values from the Fink science modules. A full example can be found at https://github.com/astrolabsoftware/fink-filters/tree/master/tutorial where we focus on alerts with a counterpart in the SIMBAD database and a magnitude above 20.5.

To test your filter, you need some real data to play with. For this, you can use the Data Transfer service (a few nights are usually enough to prototype): https://fink-portal.org/download.

Submit your science module

Once your filter is done, open a Pull Request on the fink-filters repository on GitHub, and we will review it and test it extensively before deployment. The criteria for acceptance are:

  • The filter works ;-)
  • The volume of data to be transferred is tractable on our side.

Keep in mind, LSST incoming stream is 10 million alerts per night, or ~1TB/night. Hence your filter must focus on a specific aspect of the stream, to reduce the outgoing volume of alerts. Based on your submission, we will also provide estimate of the volume to be transferred.

Step 4: Play!

If your filter is accepted, it will be plugged in the broker, and you will be able to receive your alerts in real-time using the fink-client.