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.. _ztf figures: | ||
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ZTF Figures Tutorial | ||
============================== | ||
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.. contents:: Table of Contents | ||
:depth: 1 | ||
:local: | ||
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This tutorial demonstrates plotting ZTF cutouts and light curves. | ||
It is based heavily on https://github.com/ZwickyTransientFacility/ztf-avro-alert/blob/master/notebooks/Filtering_alerts.ipynb. | ||
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Prerequisites | ||
------------- | ||
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1. Load a ZTF alert to a dict or a pandas DataFrame. For examples, see: | ||
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- :ref:`cloud storage` | ||
- :ref:`bigquery` | ||
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Imports | ||
--------- | ||
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.. code:: python | ||
import gzip | ||
import io | ||
from typing import Optional | ||
import aplpy | ||
import matplotlib as mpl | ||
import numpy as np | ||
import pandas as pd | ||
from astropy.io import fits | ||
from astropy.time import Time | ||
from matplotlib import pyplot as plt | ||
import pittgoogle | ||
Plot a Light Curve | ||
------------------ | ||
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.. code:: python | ||
def plot_lightcurve(lightcurve_df: pd.DataFrame, days_ago: bool = True): | ||
"""Plot the per-band light curve of a single ZTF object. | ||
Adapted from: | ||
https://github.com/ZwickyTransientFacility/ztf-avro-alert/blob/master/notebooks/Filtering_alerts.ipynb | ||
Parameters | ||
---------- | ||
lightcurve_df | ||
Lightcurve history of a ZTF object. Must contain columns | ||
['jd','fid','magpsf','sigmapsf','diffmaglim'] | ||
days_ago | ||
If True, x-axis will be number of days in the past. | ||
Else x-axis will be Julian date. | ||
""" | ||
filter_code = pittgoogle.utils.ztf_fid_names() # dict | ||
filter_color = {1: "green", 2: "red", 3: "pink"} | ||
# set the x-axis (time) details | ||
if days_ago: | ||
now = Time.now().jd | ||
t = lightcurve_df.jd - now | ||
xlabel = "Days Ago" | ||
else: | ||
t = lightcurve_df.jd | ||
xlabel = "Time (JD)" | ||
# plot lightcurves by band | ||
for fid, color in filter_color.items(): | ||
# plot detections in this filter: | ||
w = (lightcurve_df.fid == fid) & ~lightcurve_df.magpsf.isnull() | ||
if np.sum(w): | ||
label = f"{fid}: {filter_code[fid]}" | ||
kwargs = {"fmt": ".", "color": color, "label": label} | ||
plt.errorbar(t[w], lightcurve_df.loc[w, "magpsf"], lightcurve_df.loc[w, "sigmapsf"], **kwargs) | ||
# plot nondetections in this filter | ||
wnodet = (lightcurve_df.fid == fid) & lightcurve_df.magpsf.isnull() | ||
if np.sum(wnodet): | ||
plt.scatter( | ||
t[wnodet], | ||
lightcurve_df.loc[wnodet, "diffmaglim"], | ||
marker="v", | ||
color=color, | ||
alpha=0.25, | ||
) | ||
plt.gca().invert_yaxis() | ||
plt.xlabel(xlabel) | ||
plt.ylabel("Magnitude") | ||
plt.legend() | ||
.. code:: python | ||
plot_lightcurve(lightcurve_df) | ||
Plot Cutouts | ||
------------ | ||
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.. code:: python | ||
def plot_stamp(stamp, fig=None, subplot=None, **kwargs): | ||
"""Adapted from: | ||
https://github.com/ZwickyTransientFacility/ztf-avro-alert/blob/master/notebooks/Filtering_alerts.ipynb | ||
""" | ||
with gzip.open(io.BytesIO(stamp), "rb") as f: | ||
with fits.open(io.BytesIO(f.read())) as hdul: | ||
if fig is None: | ||
fig = plt.figure(figsize=(4, 4)) | ||
if subplot is None: | ||
subplot = (1, 1, 1) | ||
ffig = aplpy.FITSFigure(hdul[0], figure=fig, subplot=subplot, **kwargs) | ||
ffig.show_grayscale(stretch="arcsinh") | ||
return ffig | ||
def plot_cutouts(alert_dict): | ||
"""Adapted from: | ||
https://github.com/ZwickyTransientFacility/ztf-avro-alert/blob/master/notebooks/Filtering_alerts.ipynb | ||
""" | ||
# fig, axes = plt.subplots(1,3, figsize=(12,4)) | ||
fig = plt.figure(figsize=(12, 4)) | ||
for i, cutout in enumerate(["Science", "Template", "Difference"]): | ||
stamp = alert_dict["cutout{}".format(cutout)]["stampData"] | ||
ffig = plot_stamp(stamp, fig=fig, subplot=(1, 3, i + 1)) | ||
ffig.set_title(cutout) | ||
.. code:: python | ||
plot_cutouts(alert_dict) | ||
plt.show(block=False) |