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Paper Citation Record · LEDGER

The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology

As of 7 August 2026, this Paper Citation Record lists 50 of 50 outbound references and 0 inbound Pith citation observations for arXiv:2507.11400.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2507.11400 v1

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Pith citing papers itemized under the disclosed page cap.

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Outbound references

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The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology Unresolved cited work

Reference 1

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This paper cites The code utilizes the common libraries: cv2, tensorflow, and keras (see Github project page for associated code, https://github.com/caleb-nasa/gt-CAE).

The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology The code utilizes the common libraries: cv2, tensorflow, and keras (see Github project page for associated code, https://github.com/caleb-nasa/gt-CAE)

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The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology Unresolved cited work

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This paper cites in-painting.

The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology in-painting

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This paper cites Error bars correspond to 1-sigma errors on the mean.

The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology Error bars correspond to 1-sigma errors on the mean

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The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology out of bounds

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The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology best-guess

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The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology best possible

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The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology MultiMAE: Multi-modal Multi-task Masked Autoencoders

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This paper cites Machine Learning with Applications 6, 100134.

The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology Machine Learning with Applications 6, 100134

Reference 16

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This paper cites JGR Solid Earth 126, e2020JB021589.

The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology JGR Solid Earth 126, e2020JB021589

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This paper cites A guide to convolution arithmetic for deep learning.

The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology A guide to convolution arithmetic for deep learning

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The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology Masked Autoencoders As Spatiotemporal Learners

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The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology ConvMAE: Masked Convolution Meets Masked Autoencoders

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This paper cites IEEE, New Orleans, LA, USA, pp.

The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology IEEE, New Orleans, LA, USA, pp

Reference 25

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The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology Using Pre-Training Can Improve Model Robustness and Uncertainty

Reference 26

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The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology Denoising Diffusion Probabilistic Models

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The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology SpectralGPT: Spectral Remote Sensing Foundation Model

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The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology Conv2Former: A Simple Transformer-Style ConvNet for Visual Recognition

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The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology IEEE Transactions on Pattern Analysis and Machine Intelligence 46, 2506–2517

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The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology Computer Vision and Image Understanding 203, 103147

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The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology IEEE Journal of Selected Topics in Applied Earth Observations and Remote Sensing 12, 3900–3918

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The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology Adam: A Method for Stochastic Optimization

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The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology Earth and Space Science 10, e2022EA002278

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The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology Nat Astron 8, 8–9

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The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology Icarus 419, 115612

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The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology Attention Is All You Need

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The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology Monthly Notices of the Royal Astronomical Society 513, 1581–1599

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The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology Diffusion Models as Masked Autoencoders

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The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology Revealing the Dark Secrets of Masked Image Modeling

Reference 49

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The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology latent”, features in data as multi-dimensional vectors (a “latent representation

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The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology Monthly Notices of the Royal Astronomical Society 211, 111–124

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This paper cites Proceedings of the IEEE 86, 2278–2324.

The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology Proceedings of the IEEE 86, 2278–2324

Reference 1998

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This paper cites Proceedings of the IEEE 88, 569–587.

The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology Proceedings of the IEEE 88, 569–587

Reference 2000

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Reference 2011

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Reference 2014

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Reference 2015

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The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology up sampling

Reference 2016

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The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology Unresolved cited work

Reference 2017

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Observation cdeb3009-fc2f-4223-b2c0-89be4f910a4f · outbound

This paper cites 2022, Xie et al.

The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology 2022, Xie et al

Reference 2018

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Observation 67615f3f-e8f7-498b-ab70-941ccbc678be · outbound

This paper cites BERT: Pre-training of Deep Bidirectional Transformers for Language Understanding.

The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology BERT: Pre-training of Deep Bidirectional Transformers for Language Understanding

Reference 2019

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The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology EPSC2020-773)

Reference 2020

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Observation 4b6c5f52-b4b4-4507-9c84-45d090748a91 · outbound

This paper cites Maximum Entropy Auto-Encoding.

The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology Maximum Entropy Auto-Encoding

Reference 2021

Resolution
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Observation 6c1c1bf0-f4b8-4738-b50d-16257c6914af · outbound

This paper cites 2022, Huang et al.

The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology 2022, Huang et al

Reference 2022

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Observation 18e9537b-76d8-43ea-ad43-3ffe4f32266f · outbound

This paper cites MGMAE: Motion Guided Masking for Video Masked Autoencoding.

The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology MGMAE: Motion Guided Masking for Video Masked Autoencoding

Reference 2023

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Observation a7e46725-e6b9-436b-a6e1-7863cd6274db · outbound

This paper cites Monthly Notices of the Royal Astronomical Society 529, 732–747.

The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology Monthly Notices of the Royal Astronomical Society 529, 732–747

Reference 2024

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Observation 4e5115f8-dbfd-4fa3-be47-d6daa87e0c69 · outbound

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The model is the message: Lightweight convolutional autoencoders applied to noisy imaging data for planetary science and astrobiology Unresolved cited work

Reference 5607

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Pith citing papers

No inbound Pith citation observations are available.