Two Years in the Tenure Track
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Reflecting on my journey towards becoming a tenure-track astronomer
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Reflecting on my journey towards becoming a tenure-track astronomer
Published:
Reflecting on my journey towards becoming a tenure-track astronomer
Published:
Writing these posts is fun but time-consuming. How can I stay motivated enough to post consistently? To sustain a habit of writing, I’ll need to create an easier path for my future self.
Published:
Oh hey, it’s me again. Yes, I’m going to try to write more blog posts. Yes, I’ve promised that before. Sorry. This time it’ll be different.
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Generative adversarial networks are magical… when they work.
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Training a U-Net to enhance images of galaxies.
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Exploring the latent space of galaxy images with autoencoders.
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Let’s explore the morphological feature space of galaxies represented by a trained CNN. We will use PCA to reduce the dimensionality of the neural network’s latent features, and then visualize these features with matplotlib.
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Let’s train a deep neural network from scratch! In this post, I provide a demonstration of how to optimize a model in order to predict galaxy metallicities using images, and I discuss some tricks for speeding up training and obtaining better results.
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Welcome! In this first post to my blog, we will take a deeper look at galaxy images. Why should we bother measuring the metallicities, or elemental abundances, of other galaxies? And why would we use convolutional neural networks? Read more to find out!
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We are becoming more and more reliant on machine learning algorithms in our everyday lives. But what if these algorithms aren’t fair? In this exploratory data analysis of Obermeyer et al. 2019, we look at how racial biases can creep in to an algorithm’s decision-making process.
Published:
Generative adversarial networks are magical… when they work.
Published:
Training a U-Net to enhance images of galaxies.
Published:
Exploring the latent space of galaxy images with autoencoders.
Published:
In the previous post, we examined the feature space of galaxy morphological features. Now, we will use the Grad-CAM algorithm to visualize the parts of a galaxy image that are most strongly associated with certain classifications. This will allows us to identify exactly which morphological features are correlated with low- and high-metallicity predictions.
Published:
Let’s explore the morphological feature space of galaxies represented by a trained CNN. We will use PCA to reduce the dimensionality of the neural network’s latent features, and then visualize these features with matplotlib.
Published:
Let’s train a deep neural network from scratch! In this post, I provide a demonstration of how to optimize a model in order to predict galaxy metallicities using images, and I discuss some tricks for speeding up training and obtaining better results.
Published:
Welcome! In this first post to my blog, we will take a deeper look at galaxy images. Why should we bother measuring the metallicities, or elemental abundances, of other galaxies? And why would we use convolutional neural networks? Read more to find out!
Published:
Writing these posts is fun but time-consuming. How can I stay motivated enough to post consistently? To sustain a habit of writing, I’ll need to create an easier path for my future self.
Published:
In the previous post, we examined the feature space of galaxy morphological features. Now, we will use the Grad-CAM algorithm to visualize the parts of a galaxy image that are most strongly associated with certain classifications. This will allows us to identify exactly which morphological features are correlated with low- and high-metallicity predictions.
Published:
Let’s explore the morphological feature space of galaxies represented by a trained CNN. We will use PCA to reduce the dimensionality of the neural network’s latent features, and then visualize these features with matplotlib.
Published:
We are becoming more and more reliant on machine learning algorithms in our everyday lives. But what if these algorithms aren’t fair? In this exploratory data analysis of Obermeyer et al. 2019, we look at how racial biases can creep in to an algorithm’s decision-making process.
Published:
Let’s train a deep neural network from scratch! In this post, I provide a demonstration of how to optimize a model in order to predict galaxy metallicities using images, and I discuss some tricks for speeding up training and obtaining better results.
Published:
Welcome! In this first post to my blog, we will take a deeper look at galaxy images. Why should we bother measuring the metallicities, or elemental abundances, of other galaxies? And why would we use convolutional neural networks? Read more to find out!
Published:
Oh hey, it’s me again. Yes, I’m going to try to write more blog posts. Yes, I’ve promised that before. Sorry. This time it’ll be different.
Published:
Reflecting on my journey towards becoming a tenure-track astronomer
Published:
Writing these posts is fun but time-consuming. How can I stay motivated enough to post consistently? To sustain a habit of writing, I’ll need to create an easier path for my future self.
Published:
Reflecting on my journey towards becoming a tenure-track astronomer
Published:
Generative adversarial networks are magical… when they work.
Published:
Training a U-Net to enhance images of galaxies.
Published:
Exploring the latent space of galaxy images with autoencoders.
Published:
Generative adversarial networks are magical… when they work.
Published:
Training a U-Net to enhance images of galaxies.
Published:
Exploring the latent space of galaxy images with autoencoders.
Published:
In the previous post, we examined the feature space of galaxy morphological features. Now, we will use the Grad-CAM algorithm to visualize the parts of a galaxy image that are most strongly associated with certain classifications. This will allows us to identify exactly which morphological features are correlated with low- and high-metallicity predictions.
Published:
Let’s explore the morphological feature space of galaxies represented by a trained CNN. We will use PCA to reduce the dimensionality of the neural network’s latent features, and then visualize these features with matplotlib.
Published:
We are becoming more and more reliant on machine learning algorithms in our everyday lives. But what if these algorithms aren’t fair? In this exploratory data analysis of Obermeyer et al. 2019, we look at how racial biases can creep in to an algorithm’s decision-making process.
Published:
Let’s train a deep neural network from scratch! In this post, I provide a demonstration of how to optimize a model in order to predict galaxy metallicities using images, and I discuss some tricks for speeding up training and obtaining better results.
Published:
In the previous post, we examined the feature space of galaxy morphological features. Now, we will use the Grad-CAM algorithm to visualize the parts of a galaxy image that are most strongly associated with certain classifications. This will allows us to identify exactly which morphological features are correlated with low- and high-metallicity predictions.
Published:
Let’s explore the morphological feature space of galaxies represented by a trained CNN. We will use PCA to reduce the dimensionality of the neural network’s latent features, and then visualize these features with matplotlib.