Daniel Stevens on Muck Rack

Daniel Stevens

Washington, D.C.
As seen in: Color Research & Application, Nature, The Washington Post, HKS Misinformation Review, St. Louis Post-Dispatch, Washington Examiner, The Sacramento Bee, The News & Observer, East Bay Times, The Modesto Bee and
Executive Director at @Accountable_Org Formers: @MapLight @CREWcrew @SenatorHarkin. Native of Okoboji, #Iowa dstevens [at] campaignforaccountability [dot] org
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Articles

Conflicts between the DNA replication and repair machineries promote cell death in Gram-positive bacteria

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By Hannah Gaimster, Daniel Stevens, James Grimshaw Verified, Julia Hubbard
| Microbiology Research
Article metrics loading... /content/journal/micro/10.1099/mic.0.001633 Metrics Download as PowerPoint /deliver/fulltext/micro/171/11/mic001633.html?itemId=/content/journal/micro/10.1099/mic.0.001633&mimeType=html&fmt=ahah References Gaimster H, Stevens D, Grimshaw J, Hubbard J, Mickiewicz K et al.Conflicts between the DNA replication and repair machineries promote cell death in gram-positive bacteria Microbiology Society Figshare 2025 [View Article] [Google Scholar] Haeusser DP, Levin PA.
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SA’s Biggest GDP Contributor Battles Climate Change Risk

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By Daniel Stevens
| Cover
By: Daniel Stevens – Head Santam Agriculture Crop Insurance The agriculture sector is vital for economic growth. It contributes 3% to GDP, supports 941,000 jobs, and generated US$13.2 billion in export revenue in 2023 – South Africa produces 10% of the global citrus production.
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A hot-Jupiter progenitor on a super-eccentric retrograde orbit - Nature

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By Arvind Gupta, Sarah Millholland, Jiayin Dong, Jonathan Jackson, Keivan G. Stassun, Diana Dragomir, Suvrath Mahadevan, William Cochran, Bruno Guillet, Sarah Logsdon, Margaret Loose, Grzegorz Nowak, Enric Pallé, Joshua Pepper, Michael Primm, Arpita Roy, Masao Shimizu, Daniel Stevens, Stefan Will, Haedam Im, Ilaria Carleo, Jaime A. Alvarado-Montes, Jessica Klusmeyer, Liouba Leroux, Michael W. McElwain
| Nature Verified
Abstract Giant exoplanets orbiting close to their host stars are unlikely to have formed in their present configurations1. These ‘hot Jupiter’ planets are instead thought to have migrated inward from beyond the ice line and several viable migration channels have been proposed, including eccentricity excitation through angular-momentum exchange with a third body followed by tidally driven orbital circularization2,3.
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