# A common lines approach for ab-initio modeling of cyclically-symmetric   molecules

**Authors:** Gabi Pragier, Yoel Shkolnisky

arXiv: 1901.10888 · 2020-01-08

## TL;DR

This paper introduces a robust angular reconstitution algorithm for cyclically-symmetric molecules in cryo-electron microscopy, leveraging self common lines in Fourier space to accurately determine 3D structures from noisy 2D projections.

## Contribution

It presents a novel method that exploits symmetry and geometrical constraints of self common lines for improved orientation estimation in cryo-EM.

## Key findings

- Effective in high noise conditions
- Works for molecules with high-order rotational symmetry
- Validated on simulated and experimental data

## Abstract

One of the challenges in single particle reconstruction in cryo-electron microscopy is to find a three-dimensional model of a molecule using its two-dimensional noisy projection-images. In this paper, we propose a robust "angular reconstitution" algorithm for molecules with $n$-fold cyclic symmetry, that estimates the orientation parameters of the projections-images. Our suggested method utilizes self common lines which induce identical lines within the Fourier transform of each projection-image. We show that the location of self common lines admits quite a few favorable geometrical constraints, thus allowing to detect them even in a noisy setting. In addition, for molecules with higher order rotational symmetry, our proposed method exploits the fact that there exist numerous common lines between any two Fourier transformed projection-images of such molecules, thus allowing to determine their relative orientation even under high levels of noise. The efficacy of our proposed method is demonstrated using numerical experiments conducted on simulated and experimental data.

## Full text

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## Figures

32 figures with captions in the complete paper: https://tomesphere.com/paper/1901.10888/full.md

## References

24 references — full list in the complete paper: https://tomesphere.com/paper/1901.10888/full.md

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Source: https://tomesphere.com/paper/1901.10888