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[READ-ONLY] Mirror of https://github.com/emilyhunt/ocelot. A toolbox for working with observations of star clusters. ocelot-docs.org
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<nav class="md-nav md-nav--secondary" aria-label="Table of contents"> <label class="md-nav__title" for="__toc"> <span class="md-nav__icon md-icon"></span> Table of contents </label> <ul class="md-nav__list" data-md-component="toc" data-md-scrollfix> <li class="md-nav__item"> <a href="#ocelot.simulate.SimulatedCluster" class="md-nav__link"> <span class="md-ellipsis"> SimulatedCluster </span> </a> <nav class="md-nav" aria-label="SimulatedCluster"> <ul class="md-nav__list"> <li class="md-nav__item"> <a href="#ocelot.simulate.SimulatedCluster.make" class="md-nav__link"> <span class="md-ellipsis"> make </span> </a> </li> <li class="md-nav__item"> <a href="#ocelot.simulate.SimulatedCluster.make_cluster" class="md-nav__link"> <span class="md-ellipsis"> make_cluster </span> </a> </li> <li class="md-nav__item"> <a href="#ocelot.simulate.SimulatedCluster.make_observations" class="md-nav__link"> <span class="md-ellipsis"> make_observations </span> </a> </li> <li class="md-nav__item"> <a href="#ocelot.simulate.SimulatedCluster.make_observation" class="md-nav__link"> <span class="md-ellipsis"> make_observation </span> </a> </li> </ul> </nav> </li> <li class="md-nav__item"> <a href="#ocelot.simulate.SimulatedClusterParameters" class="md-nav__link"> <span class="md-ellipsis"> SimulatedClusterParameters </span> </a> <nav class="md-nav" aria-label="SimulatedClusterParameters"> <ul class="md-nav__list"> <li class="md-nav__item"> <a href="#ocelot.simulate.SimulatedClusterParameters.get_position_as_skycoord" class="md-nav__link"> <span class="md-ellipsis"> get_position_as_skycoord </span> </a> </li> <li class="md-nav__item"> <a href="#ocelot.simulate.SimulatedClusterParameters.to_dict" class="md-nav__link"> <span class="md-ellipsis"> to_dict </span> </a> </li> </ul> </nav> </li> <li class="md-nav__item"> <a href="#ocelot.simulate.SimulatedClusterModels" class="md-nav__link"> <span class="md-ellipsis"> SimulatedClusterModels </span> </a> <nav class="md-nav" aria-label="SimulatedClusterModels"> <ul class="md-nav__list"> <li class="md-nav__item"> <a href="#ocelot.simulate.SimulatedClusterModels.initialise_defaults" class="md-nav__link"> <span class="md-ellipsis"> initialise_defaults </span> </a> </li> <li class="md-nav__item"> <a href="#ocelot.simulate.SimulatedClusterModels.with_default_options" class="md-nav__link"> <span class="md-ellipsis"> with_default_options </span> </a> </li> </ul> </nav> </li> <li class="md-nav__item"> <a href="#ocelot.simulate.cluster.SimulatedClusterFeatures" class="md-nav__link"> <span class="md-ellipsis"> SimulatedClusterFeatures </span> </a> </li> </ul> </nav> </div> </div> </div> <div class="md-content" data-md-component="content"> <article class="md-content__inner md-typeset">
<h1>SimulatedCluster</h1>
<p>See also: introductory tutorial on <a href="../../tutorials/simulate_a_cluster/">how to simulate a cluster</a>.</p>
<div class="doc doc-object doc-class">
<h2 id="ocelot.simulate.SimulatedCluster" class="doc doc-heading"> <code>ocelot.simulate.SimulatedCluster</code>
<a href="#ocelot.simulate.SimulatedCluster" class="headerlink" title="Permanent link">¤</a></h2>
<div class="doc doc-contents first">
<p>A class for simulating and keeping track of a simulated cluster - including itsoriginal membership list and any observations simulated from it.</p><p>This class is the main entry point in ocelot for simulating star clusters.</p>
<p><span class="doc-section-title">Parameters:</span></p> <table> <thead> <tr> <th>Name</th> <th>Type</th> <th>Description</th> <th>Default</th> </tr> </thead> <tbody> <tr class="doc-section-item"> <td> <code>parameters</code> </td> <td> <code><a class="autorefs autorefs-internal" title="ocelot.simulate.SimulatedClusterParameters
dataclass (ocelot.simulate.cluster.SimulatedClusterParameters)" href="#ocelot.simulate.SimulatedClusterParameters">SimulatedClusterParameters</a> or <span title="dict">dict</span></code> </td> <td> <div class="doc-md-description"> <p>Parameters of the simulated cluster to generate. Should be aSimulatedClusterParameters object, but may also be a dict with keys for requiredparameters such as position, etc.</p> </div> </td> <td> <em>required</em> </td> </tr> <tr class="doc-section-item"> <td> <code>models</code> </td> <td> <code>(<a class="autorefs autorefs-internal" title="ocelot.simulate.SimulatedClusterModels
dataclass (ocelot.simulate.cluster.SimulatedClusterModels)" href="#ocelot.simulate.SimulatedClusterModels">SimulatedClusterModels</a>, <span title="dict">dict</span> or None)</code> </td> <td> <div class="doc-md-description"> <p>SimulatedClusterModels object or dict containing models used to overwrite oraugment certain simulation features. Default: None</p> </div> </td> <td> <code>None</code> </td> </tr> <tr class="doc-section-item"> <td> <code>prune_simulated_cluster</code> </td> <td> <code><span title="str">str</span></code> </td> <td> <div class="doc-md-description"> <p>Optional string used early during cluster simulation to prune a simulatedcluster. Will be passed to pandas.DataFrame.query(). It can access parametersread directly from cluster isochrones, including magnitude, temperature,and luminosity. Default: ""</p> </div> </td> <td> <code>''</code> </td> </tr> <tr class="doc-section-item"> <td> <code>random_seed</code> </td> <td> <code><span title="int">int</span> or None</code> </td> <td> <div class="doc-md-description"> <p>Random seed to use for cluster generation. When set, cluster generation with thesame seed should be identical. Default: None</p> </div> </td> <td> <code>None</code> </td> </tr> <tr class="doc-section-item"> <td> <code>features</code> </td> <td> <code><a class="autorefs autorefs-internal" title="ocelot.simulate.cluster.SimulatedClusterFeatures
dataclass " href="#ocelot.simulate.cluster.SimulatedClusterFeatures">SimulatedClusterFeatures</a> or <span title="dict">dict</span> or None</code> </td> <td> <div class="doc-md-description"> <p>A SimulatedClusterFeatures or dict object specifying features of clustergeneration to turn off. Mostly intended to aid with testing. Default: None</p> </div> </td> <td> <code>None</code> </td> </tr> <tr class="doc-section-item"> <td> <code>observations</code> </td> <td> <code>list of str or None</code> </td> <td> <div class="doc-md-description"> <p>List of observations to generate. Soon to be deprecated; do not use.</p> </div> </td> <td> <code>None</code> </td> </tr> </tbody> </table>
<p><span class="doc-section-title">Attributes:</span></p> <table> <thead> <tr> <th>Name</th> <th>Type</th> <th>Description</th> </tr> </thead> <tbody> <tr class="doc-section-item"> <td><code><span title="ocelot.simulate.SimulatedCluster.isochrone">isochrone</span></code></td> <td> <code><span title="pandas.DataFrame">DataFrame</span></code> </td> <td> <div class="doc-md-description"> <p>Dataframe containing the isochrone used to simulate this cluster.</p> </div> </td> </tr> <tr class="doc-section-item"> <td><code><span title="ocelot.simulate.SimulatedCluster.cluster">cluster</span></code></td> <td> <code><span title="pandas.DataFrame">DataFrame</span></code> </td> <td> <div class="doc-md-description"> <p>Dataframe containing the true members of the cluster.</p> </div> </td> </tr> <tr class="doc-section-item"> <td><code><span title="ocelot.simulate.SimulatedCluster.observations">observations</span></code></td> <td> <code>dict of pd.DataFrame</code> </td> <td> <div class="doc-md-description"> <p>Dict of dataframes, with each one containing a different observation of thesame cluster.</p> </div> </td> </tr> </tbody> </table>
<div class="doc doc-children">
<div class="doc doc-object doc-function">
<h3 id="ocelot.simulate.SimulatedCluster.make" class="doc doc-heading"> <code class="highlight language-python"><span class="n">make</span><span class="p">()</span></code>
<a href="#ocelot.simulate.SimulatedCluster.make" class="headerlink" title="Permanent link">¤</a></h3>
<div class="doc doc-contents ">
<p>Makes entire cluster according to specification set at initialization.</p><p>This is the main function that should be used to simulate a cluster.</p>
<p><span class="doc-section-title">Returns:</span></p> <table> <thead> <tr> <th>Type</th> <th>Description</th> </tr> </thead> <tbody> <tr class="doc-section-item"> <td> <code><a class="autorefs autorefs-internal" title="ocelot.simulate.SimulatedCluster (ocelot.simulate.cluster.SimulatedCluster)" href="#ocelot.simulate.SimulatedCluster">SimulatedCluster</a></code> </td> <td> <div class="doc-md-description"> <p>A reference to the SimulatedCluster object.</p> </div> </td> </tr> </tbody> </table>
</div>
</div>
<div class="doc doc-object doc-function">
<h3 id="ocelot.simulate.SimulatedCluster.make_cluster" class="doc doc-heading"> <code class="highlight language-python"><span class="n">make_cluster</span><span class="p">()</span></code>
<a href="#ocelot.simulate.SimulatedCluster.make_cluster" class="headerlink" title="Permanent link">¤</a></h3>
<div class="doc doc-contents ">
<p>Creates the true stars and positions in a cluster.</p><p>In general, just calling .make() is the recommended method for most users.</p>
<p><span class="doc-section-title">Returns:</span></p> <table> <thead> <tr> <th>Type</th> <th>Description</th> </tr> </thead> <tbody> <tr class="doc-section-item"> <td> <code><a class="autorefs autorefs-internal" title="ocelot.simulate.SimulatedCluster (ocelot.simulate.cluster.SimulatedCluster)" href="#ocelot.simulate.SimulatedCluster">SimulatedCluster</a></code> </td> <td> <div class="doc-md-description"> <p>A reference to the SimulatedCluster object.</p> </div> </td> </tr> </tbody> </table>
</div>
</div>
<div class="doc doc-object doc-function">
<h3 id="ocelot.simulate.SimulatedCluster.make_observations" class="doc doc-heading"> <code class="highlight language-python"><span class="n">make_observations</span><span class="p">()</span></code>
<a href="#ocelot.simulate.SimulatedCluster.make_observations" class="headerlink" title="Permanent link">¤</a></h3>
<div class="doc doc-contents ">
<p>Makes all observations of the cluster.</p><p>In general, just calling .make() is the recommended method for most users.</p>
<p><span class="doc-section-title">Returns:</span></p> <table> <thead> <tr> <th>Type</th> <th>Description</th> </tr> </thead> <tbody> <tr class="doc-section-item"> <td> <code><a class="autorefs autorefs-internal" title="ocelot.simulate.SimulatedCluster (ocelot.simulate.cluster.SimulatedCluster)" href="#ocelot.simulate.SimulatedCluster">SimulatedCluster</a></code> </td> <td> <div class="doc-md-description"> <p>A reference to the SimulatedCluster object.</p> </div> </td> </tr> </tbody> </table>
</div>
</div>
<div class="doc doc-object doc-function">
<h3 id="ocelot.simulate.SimulatedCluster.make_observation" class="doc doc-heading"> <code class="highlight language-python"><span class="n">make_observation</span><span class="p">(</span><span class="n">survey</span><span class="p">,</span> <span class="n">seed</span><span class="o">=</span><span class="kc">None</span><span class="p">)</span></code>
<a href="#ocelot.simulate.SimulatedCluster.make_observation" class="headerlink" title="Permanent link">¤</a></h3>
<div class="doc doc-contents ">
<p>Makes one observation of the cluster.</p><p>In general, just calling .make() is the recommended method for most users.</p>
<p><span class="doc-section-title">Parameters:</span></p> <table> <thead> <tr> <th>Name</th> <th>Type</th> <th>Description</th> <th>Default</th> </tr> </thead> <tbody> <tr class="doc-section-item"> <td> <code>survey</code> </td> <td> <code><span title="str">str</span></code> </td> <td> <div class="doc-md-description"> <p>Name of the survey (i.e. name in self.observations) to make.</p> </div> </td> <td> <em>required</em> </td> </tr> <tr class="doc-section-item"> <td> <code>seed</code> </td> <td> <code>None</code> </td> <td> <div class="doc-md-description"> <p>Seed used to reseed the random generator. Useful for doing multipledifferent simulated observations of the same cluster. May not be supportedby all cluster observation models. Default: None, meaning that the currentcluster random number generator generated from the seed specified duringclass initialization is used.</p> </div> </td> <td> <code>None</code> </td> </tr> </tbody> </table>
<p><span class="doc-section-title">Returns:</span></p> <table> <thead> <tr> <th>Type</th> <th>Description</th> </tr> </thead> <tbody> <tr class="doc-section-item"> <td> <code><span title="pandas.DataFrame">DataFrame</span></code> </td> <td> <div class="doc-md-description"> <p>The simulated cluster observation made by this method.</p> </div> </td> </tr> </tbody> </table>
</div>
</div>
</div>
</div>
</div>
<div class="doc doc-object doc-class">
<h2 id="ocelot.simulate.SimulatedClusterParameters" class="doc doc-heading"> <code>ocelot.simulate.SimulatedClusterParameters</code>
<span class="doc doc-labels"> <small class="doc doc-label doc-label-dataclass"><code>dataclass</code></small> </span>
<a href="#ocelot.simulate.SimulatedClusterParameters" class="headerlink" title="Permanent link">¤</a></h2>
<div class="doc doc-contents first">
<p>Class for keeping track of parameters specified for a cluster to simulate.</p>
<p><span class="doc-section-title">Parameters:</span></p> <table> <thead> <tr> <th>Name</th> <th>Type</th> <th>Description</th> <th>Default</th> </tr> </thead> <tbody> <tr class="doc-section-item"> <td> <code>position</code> </td> <td> <code><span title="astropy.coordinates.SkyCoord">SkyCoord</span></code> </td> <td> <div class="doc-md-description"> <p>Position of the cluster as an astropy SkyCoord. Must have full 3D distance and3D velocity information.</p> </div> </td> <td> <em>required</em> </td> </tr> <tr class="doc-section-item"> <td> <code>mass</code> </td> <td> <code><span title="float">float</span></code> </td> <td> <div class="doc-md-description"> <p>Mass of the cluster in solar masses.</p> </div> </td> <td> <em>required</em> </td> </tr> <tr class="doc-section-item"> <td> <code>log_age</code> </td> <td> <code><span title="float">float</span></code> </td> <td> <div class="doc-md-description"> <p>Age of the cluster in log (base 10) years.</p> </div> </td> <td> <em>required</em> </td> </tr> <tr class="doc-section-item"> <td> <code>metallicity</code> </td> <td> <code><span title="float">float</span></code> </td> <td> <div class="doc-md-description"> <p>The metallicity of the cluster, [Fe/H].</p> </div> </td> <td> <em>required</em> </td> </tr> <tr class="doc-section-item"> <td> <code>r_core</code> </td> <td> <code><span title="float">float</span></code> </td> <td> <div class="doc-md-description"> <p>The core radius of the cluster, in parsecs.</p> </div> </td> <td> <em>required</em> </td> </tr> <tr class="doc-section-item"> <td> <code>r_tidal</code> </td> <td> <code><span title="float">float</span></code> </td> <td> <div class="doc-md-description"> <p>The tidal radius of the cluster, in parsecs.</p> </div> </td> <td> <em>required</em> </td> </tr> <tr class="doc-section-item"> <td> <code>extinction</code> </td> <td> <code><span title="float">float</span></code> </td> <td> <div class="doc-md-description"> <p>The extinction (A_V / A_0) of the cluster in magnitudes.</p> </div> </td> <td> <em>required</em> </td> </tr> <tr class="doc-section-item"> <td> <code>differential_extinction</code> </td> <td> <code><span title="float">float</span></code> </td> <td> <div class="doc-md-description"> <p>Amount of differential extinction to apply to the cluster, also in magnitudes.Default: 0.</p> </div> </td> <td> <code>0.0</code> </td> </tr> <tr class="doc-section-item"> <td> <code>minimum_stars</code> </td> <td> <code><span title="int">int</span></code> </td> <td> <div class="doc-md-description"> <p>Specify the minimum number of stars the cluster can have. Default: 0</p> </div> </td> <td> <code>1</code> </td> </tr> <tr class="doc-section-item"> <td> <code>virial_ratio</code> </td> <td> <code><span title="float">float</span></code> </td> <td> <div class="doc-md-description"> <p>Virial ratio of the cluster. Acts as a square-root scale factor to the cluster'svelocity dispersion. Default: 0.5, meaning that the cluster is virialized.</p> </div> </td> <td> <code>0.5</code> </td> </tr> <tr class="doc-section-item"> <td> <code>eta_virial_ratio</code> </td> <td> <code><span title="float">float</span></code> </td> <td> <div class="doc-md-description"> <p>Scale factor of the 1D velocity dispersion equation. Default: 10, which is agood approximation for most clusters.</p> </div> </td> <td> <code>10.0</code> </td> </tr> <tr class="doc-section-item"> <td> <code>id</code> </td> <td> <code><span title="int">int</span></code> </td> <td> <div class="doc-md-description"> <p>ID of the simulated cluster. When set, this allows for unique identification ofdifferent simulated clusters. Default: 0.</p> </div> </td> <td> <code>0</code> </td> </tr> </tbody> </table>
<p><span class="doc-section-title">Attributes:</span></p> <table> <thead> <tr> <th>Name</th> <th>Type</th> <th>Description</th> </tr> </thead> <tbody> <tr class="doc-section-item"> <td><code><span title="ocelot.simulate.SimulatedClusterParameters.r_50">r_50</span></code></td> <td> <code><span title="float">float</span></code> </td> <td> <div class="doc-md-description"> <p>The half-light radius of the cluster in parsecs.</p> </div> </td> </tr> <tr class="doc-section-item"> <td><code><span title="ocelot.simulate.SimulatedClusterParameters.velocity_dispersion_1d">velocity_dispersion_1d</span></code></td> <td> <code><span title="float">float</span></code> </td> <td> <div class="doc-md-description"> <p>The 1D velocity dispersion of the cluster in metres per second.</p> </div> </td> </tr> </tbody> </table>
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<div class="doc doc-object doc-function">
<h3 id="ocelot.simulate.SimulatedClusterParameters.get_position_as_skycoord" class="doc doc-heading"> <code class="highlight language-python"><span class="n">get_position_as_skycoord</span><span class="p">(</span><span class="n">frame</span><span class="o">=</span><span class="s1">'icrs'</span><span class="p">,</span> <span class="n">with_zeroed_proper_motions</span><span class="o">=</span><span class="kc">False</span><span class="p">)</span></code>
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<p>Returns the position of the cluster as a SkyCoord.</p>
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<h3 id="ocelot.simulate.SimulatedClusterParameters.to_dict" class="doc doc-heading"> <code class="highlight language-python"><span class="n">to_dict</span><span class="p">()</span></code>
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<p>Converts class (and all fields) to dict. Useful for saving information.</p>
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<h2 id="ocelot.simulate.SimulatedClusterModels" class="doc doc-heading"> <code>ocelot.simulate.SimulatedClusterModels</code>
<span class="doc doc-labels"> <small class="doc doc-label doc-label-dataclass"><code>dataclass</code></small> </span>
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<p>Class for keeping track of all models that a generated SimulatedCluster will use.</p>
<p><span class="doc-section-title">Parameters:</span></p> <table> <thead> <tr> <th>Name</th> <th>Type</th> <th>Description</th> <th>Default</th> </tr> </thead> <tbody> <tr class="doc-section-item"> <td> <code>distribution</code> </td> <td> <code><a class="autorefs autorefs-internal" title="ocelot.model.distribution.BaseClusterDistributionModel" href="../model/distribution/#ocelot.model.distribution.BaseClusterDistributionModel">BaseClusterDistributionModel</a> or None</code> </td> <td> <div class="doc-md-description"> <p>The distribution model for the cluster. Must be an instance ofBaseClusterDistributionModel. Default: None, meaning that a King62 model is used</p> </div> </td> <td> <code>None</code> </td> </tr> <tr class="doc-section-item"> <td> <code>binaries</code> </td> <td> <code><a class="autorefs autorefs-internal" title="ocelot.model.binaries.BaseBinaryStarModel" href="../model/binaries/#ocelot.model.binaries.BaseBinaryStarModel">BaseBinaryStarModel</a> or None</code> </td> <td> <div class="doc-md-description"> <p>The binary star model for the cluster. Must be an instance ofBaseBinaryStarModel. Default: None, meaning that aMoeDiStefanoMultiplicityRelation (with Duchene-Kraus+13 below 1 MSun) is used.</p> </div> </td> <td> <code>None</code> </td> </tr> <tr class="doc-section-item"> <td> <code>differential_reddening</code> </td> <td> <code><a class="autorefs autorefs-internal" title="ocelot.model.differential_reddening.BaseDifferentialReddeningModel" href="../model/differential_reddening/#ocelot.model.differential_reddening.BaseDifferentialReddeningModel">BaseDifferentialReddeningModel</a> or None</code> </td> <td> <div class="doc-md-description"> <p>The differential reddening model for the cluster. Must be an instance ofBaseDifferentialReddeningModel. Default: None, meaning that aFractalDifferentialReddening model is used.</p> </div> </td> <td> <code>None</code> </td> </tr> <tr class="doc-section-item"> <td> <code>observations</code> </td> <td> <code>list or tuple of BaseObservation</code> </td> <td> <div class="doc-md-description"> <p>A list or tuple of observation models for the cluster. Each model must be aninstance of a BaseObservation. These observation models will be iterated throughwhen generating cluster observations to generate as many (or few) observationsimulations of a cluster as you'd like. Observation models must be unique.Default: None, meaning that no cluster observation simulation will be generated.</p> </div> </td> <td> <code><span title="tuple">tuple</span>()</code> </td> </tr> </tbody> </table>
<p><span class="doc-section-title">Attributes:</span></p> <table> <thead> <tr> <th>Name</th> <th>Type</th> <th>Description</th> </tr> </thead> <tbody> <tr class="doc-section-item"> <td><code><span title="ocelot.simulate.SimulatedClusterModels.observations_dict">observations_dict</span></code></td> <td> <code>dict of BaseObservation models</code> </td> <td> <div class="doc-md-description"> <p>Same as the observations parameter, but with observations instead organized intoa dictionary.</p> </div> </td> </tr> </tbody> </table>
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<h3 id="ocelot.simulate.SimulatedClusterModels.initialise_defaults" class="doc doc-heading"> <code class="highlight language-python"><span class="n">initialise_defaults</span><span class="p">(</span><span class="n">parameters</span><span class="p">,</span> <span class="n">seed</span><span class="p">)</span></code>
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<p>For all class attributes, replace None values with sensible default models.</p><p>This method is called during simulated cluster generation and should not needto be used by users.</p>
<p><span class="doc-section-title">Parameters:</span></p> <table> <thead> <tr> <th>Name</th> <th>Type</th> <th>Description</th> <th>Default</th> </tr> </thead> <tbody> <tr class="doc-section-item"> <td> <code>parameters</code> </td> <td> <code><a class="autorefs autorefs-internal" title="ocelot.simulate.SimulatedClusterParameters
dataclass (ocelot.simulate.cluster.SimulatedClusterParameters)" href="#ocelot.simulate.SimulatedClusterParameters">SimulatedClusterParameters</a></code> </td> <td> <div class="doc-md-description"> <p>The parameters of the cluster to simulate.</p> </div> </td> <td> <em>required</em> </td> </tr> <tr class="doc-section-item"> <td> <code>seed</code> </td> <td> <code><span title="int">int</span></code> </td> <td> <div class="doc-md-description"> <p>Random seed to use for default models that incorporate randomness.</p> </div> </td> <td> <em>required</em> </td> </tr> </tbody> </table>
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<h3 id="ocelot.simulate.SimulatedClusterModels.with_default_options" class="doc doc-heading"> <code class="highlight language-python"><span class="n">with_default_options</span><span class="p">(</span><span class="n">parameters</span><span class="p">,</span> <span class="n">seed</span><span class="p">)</span></code>
<span class="doc doc-labels"> <small class="doc doc-label doc-label-staticmethod"><code>staticmethod</code></small> </span>
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<p>Return an instance of a SimulatedClusterModels model with default options.</p>
<p><span class="doc-section-title">Parameters:</span></p> <table> <thead> <tr> <th>Name</th> <th>Type</th> <th>Description</th> <th>Default</th> </tr> </thead> <tbody> <tr class="doc-section-item"> <td> <code>parameters</code> </td> <td> <code><a class="autorefs autorefs-internal" title="ocelot.simulate.SimulatedClusterParameters
dataclass (ocelot.simulate.cluster.SimulatedClusterParameters)" href="#ocelot.simulate.SimulatedClusterParameters">SimulatedClusterParameters</a></code> </td> <td> <div class="doc-md-description"> <p>The parameters of the cluster to simulate.</p> </div> </td> <td> <em>required</em> </td> </tr> <tr class="doc-section-item"> <td> <code>seed</code> </td> <td> <code><span title="int">int</span></code> </td> <td> <div class="doc-md-description"> <p>Random seed to use for default models that incorporate randomness.</p> </div> </td> <td> <em>required</em> </td> </tr> </tbody> </table>
<p><span class="doc-section-title">Returns:</span></p> <table> <thead> <tr> <th>Type</th> <th>Description</th> </tr> </thead> <tbody> <tr class="doc-section-item"> <td> <code><a class="autorefs autorefs-internal" title="ocelot.simulate.SimulatedClusterModels
dataclass (ocelot.simulate.cluster.SimulatedClusterModels)" href="#ocelot.simulate.SimulatedClusterModels">SimulatedClusterModels</a></code> </td> <td> <div class="doc-md-description"> <p>An instance of SimulatedClusterModels with default options already set up.</p> </div> </td> </tr> </tbody> </table>
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<h2 id="ocelot.simulate.cluster.SimulatedClusterFeatures" class="doc doc-heading"> <code>ocelot.simulate.cluster.SimulatedClusterFeatures</code>
<span class="doc doc-labels"> <small class="doc doc-label doc-label-dataclass"><code>dataclass</code></small> </span>
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<p>Class for keeping track of all features used to simulate a cluster.</p><p>This class mostly exists to aid in testing parts of ocelot.simulate with certainphysical effects turned on or off.</p>
<p><span class="doc-section-title">Parameters:</span></p> <table> <thead> <tr> <th>Name</th> <th>Type</th> <th>Description</th> <th>Default</th> </tr> </thead> <tbody> <tr class="doc-section-item"> <td> <code>binary_stars</code> </td> <td> <code><span title="bool">bool</span></code> </td> <td> <div class="doc-md-description"> <p>Whether or not to simulate binary stars in the cluster. Default: True</p> </div> </td> <td> <code>True</code> </td> </tr> <tr class="doc-section-item"> <td> <code>differential_extinction</code> </td> <td> <code><span title="bool">bool</span></code> </td> <td> <div class="doc-md-description"> <p>Whether or not to simulate differential extinction of the cluster. Default: True</p> </div> </td> <td> <code>True</code> </td> </tr> <tr class="doc-section-item"> <td> <code>selection_effects</code> </td> <td> <code><span title="bool">bool</span></code> </td> <td> <div class="doc-md-description"> <p>Whether or not to simulate selection effects in simulated observations of thecluster. Default: True</p> </div> </td> <td> <code>True</code> </td> </tr> <tr class="doc-section-item"> <td> <code>astrometric_uncertainties</code> </td> <td> <code><span title="bool">bool</span></code> </td> <td> <div class="doc-md-description"> <p>Whether or not to apply astrometric uncertainties to observations of thecluster. Default: True</p> </div> </td> <td> <code>True</code> </td> </tr> <tr class="doc-section-item"> <td> <code>photometric_uncertainties</code> </td> <td> <code><span title="bool">bool</span></code> </td> <td> <div class="doc-md-description"> <p>Whether or not to apply photometric uncertainties to observations of thecluster. Default: True</p> </div> </td> <td> <code>True</code> </td> </tr> </tbody> </table>
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