Production of ammonia makes Venusian clouds habitable and explains observed cloud-level chemical anomalies by Bains, William, Petkowski, Janusz J, Rimmer, Paul B, Seager, Sara

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Constraints on the Production of Phosphine by Venusian Volcanoes by Bains, William, Shorttle, Oliver, Ranjan, Sukrit, Rimmer, Paul B., Petkowski, Janusz J., Greaves, Jane S., Seager, Sara

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Only extraordinary volcanism can explain the presence of parts per billion phosphine on Venus by Bains, William, Shorttle, Oliver, Ranjan, Sukrit, Rimmer, Paul B, Petkowski, Janusz J, Greaves, Jane S, Seager, Sara

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Phosphine on Venus Cannot Be Explained by Conventional Processes by Bains, William, Petkowski, Janusz J, Seager, Sara, Ranjan, Sukrit, Sousa-Silva, Clara, Rimmer, Paul B, Zhan, Zhuchang, Greaves, Jane S, Richards, Anita MS

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Venusian phosphine: a ‘wow!’ signal in chemistry? by Bains, William, Petkowski, Janusz J, Seager, Sara, Ranjan, Sukrit, Sousa-Silva, Clara, Rimmer, Paul B, Zhan, Zhuchang, Greaves, Jane S, Richards, Anita MS

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Phosphine gas in the cloud decks of Venus by Greaves, Jane S, Richards, Anita MS, Bains, William, Rimmer, Paul B, Sagawa, Hideo, Clements, David L, Seager, Sara, Petkowski, Janusz J, Sousa-Silva, Clara, Ranjan, Sukrit, Drabek-Maunder, Emily, Fraser, Helen J, Cartwright, Annabel, Mueller-Wodarg, Ingo, Zhan, Zhuchang, Friberg, Per, Coulson, Iain, Lee, E’lisa, Hoge, Jim

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Stellar Flares from the First TESS Data Release: Exploring a New Sample of M Dwarfs by Günther, Maximilian N, Zhan, Zhuchang, Seager, Sara, Rimmer, Paul B, Ranjan, Sukrit, Stassun, Keivan G, Oelkers, Ryan J, Daylan, Tansu, Newton, Elisabeth, Kristiansen, Martti H, Olah, Katalin, Gillen, Edward, Rappaport, Saul, Ricker, George R, Vanderspek, Roland K, Latham, David W, Winn, Joshua N, Jenkins, Jon M, Glidden, Ana, Fausnaugh, Michael, Levine, Alan M, Dittmann, Jason A, Quinn, Samuel N, Krishnamurthy, Akshata, Ting, Eric B

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