Tidal Dissipation Regimes among the Short-period Exoplanets by Louden, Emma M., Laughlin, Gregory P., Millholland, Sarah C.

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A Larger Sample Confirms Small Planets around Hot Stars Are Misaligned by Louden, Emma M, Wang, Songhu, Winn, Joshua N, Petigura, Erik A, Isaacson, Howard, Handley, Luke, Yee, Samuel W, Beard, Corey, Akana Murphy, Joseph M, Laughlin, Gregory

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HATS-34b and HATS-46b: re-characterization using TESS and Gaia by Louden, Emma M, Hartman, Joel D

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Hot Stars with Kepler Planets Have High Obliquities by Louden, Emma M., Winn, Joshua N., Petigura, Erik A., Isaacson, Howard, Howard, Andrew W., Masuda, Kento, Albrecht, Simon, Kosiarek, Molly R.

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TESS Giants Transiting Giants. VI. Newly Discovered Hot Jupiters Provide Evidence for Efficient Obliquity Damping after the Main Sequence by Saunders, Nicholas, Grunblatt, Samuel K., Chontos, Ashley, Dai, Fei, Huber, Daniel, Zhang, Jingwen, Stefánsson, Guđmundur, van Saders, Jennifer L., Winn, Joshua N., Hey, Daniel, Howard, Andrew W., Fulton, Benjamin, Isaacson, Howard, Beard, Corey, Giacalone, Steven, Van Zandt, Judah, Murphey, Joseph M. Akana, Rice, Malena, Blunt, Sarah, Turtelboom, Emma, Dalba, Paul A., Lubin, Jack, Brinkman, Casey, Louden, Emma M., Page, Emma, Watkins, Cristilyn N., Collins, Karen A., Stockdale, Chris, Tan, Thiam-Guan, Schwarz, Richard P., Massey, Bob, Howell, Steve B., Vanderburg, Andrew, Ricker, George R., Jenkins, Jon M., Seager, Sara, Christiansen, Jessie L., Daylan, Tansu, Falk, Ben, Brodheim, Max, Gibson, Steven R., Hill, Grant M., Holden, Bradford, Householder, Aaron, Kaye, Stephen, Laher, Russ R., Lanclos, Kyle, Petigura, Erik A., Roy, Arpita, Rubenzahl, Ryan A., Schwab, Christian, Shaum, Abby P., Sirk, Martin M., Smith, Christopher L., Walawender, Josh, Yeh, Sherry

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The TESS-Keck Survey. XVI. Mass Measurements for 12 Planets in Eight Systems by Akana Murphy, Joseph M., Batalha, Natalie M., Scarsdale, Nicholas, Isaacson, Howard, Ciardi, David R., Gonzales, Erica J., Giacalone, Steven, Twicken, Joseph D., Dattilo, Anne, Fetherolf, Tara, Rubenzahl, Ryan A., Crossfield, Ian J. M., Dressing, Courtney D., Fulton, Benjamin, Howard, Andrew W., Huber, Daniel, Kane, Stephen R., Petigura, Erik A., Robertson, Paul, Roy, Arpita, Weiss, Lauren M., Beard, Corey, Chontos, Ashley, Dai, Fei, Rice, Malena, Van Zandt, Judah, Lubin, Jack, Blunt, Sarah, Polanski, Alex S., Behmard, Aida, Dalba, Paul A., Hill, Michelle L., Rosenthal, Lee J., Brinkman, Casey L., Mayo, Andrew W., Turtelboom, Emma V., Angelo, Isabel, Močnik, Teo, MacDougall, Mason G., Pidhorodetska, Daria, Tyler, Dakotah, Kosiarek, Molly R., Holcomb, Rae, Louden, Emma M., Hirsch, Lea A., Gilbert, Emily A., Anderson, Jay, Valenti, Jeff A.

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A Larger Sample Confirms Small Planets around Hot Stars Are Misaligned ∗ ∗ The data presented herein were obtained at the W. M. Keck Observatory, operated as a scientific partnersh... by Louden, Emma M., Wang, Songhu, Winn, Joshua N., Petigura, Erik A., Isaacson, Howard, Handley, Luke, Yee, Samuel W., Beard, Corey, Murphy, Joseph M. Akana, Laughlin, Gregory

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The TESS-Keck Survey. XX. 15 New TESS Planets and a Uniform RV Analysis of All Survey Targets by Polanski, Alex S., Lubin, Jack, Beard, Corey, Akana Murphy, Joseph M., Rubenzahl, Ryan, Hill, Michelle L., Crossfield, Ian J. M., Chontos, Ashley, Robertson, Paul, Isaacson, Howard, Kane, Stephen R., Ciardi, David R., Batalha, Natalie M., Dressing, Courtney, Fulton, Benjamin, Howard, Andrew W., Huber, Daniel, Petigura, Erik A., Weiss, Lauren M., Angelo, Isabel, Behmard, Aida, Blunt, Sarah, Brinkman, Casey L., Dai, Fei, Dalba, Paul A., Fetherolf, Tara, Giacalone, Steven, Hirsch, Lea A., Holcomb, Rae, Kosiarek, Molly R., Mayo, Andrew W., MacDougall, Mason G., Močnik, Teo, Pidhorodetska, Daria, Rice, Malena, Rosenthal, Lee J., Scarsdale, Nicholas, Turtelboom, Emma V., Tyler, Dakotah, Van Zandt, Judah, Yee, Samuel W., Coria, David R., Dulz, Shannon D., Hartman, Joel D., Householder, Aaron, Lange, Sarah, Langford, Andrew, Louden, Emma M., Siegel, Jared C., Gilbert, Emily A., Gonzales, Erica J., Schlieder, Joshua E., Boyle, Andrew W., Christiansen, Jessie L., Clark, Catherine A., Fernandes, Rachel B., Lund, Michael B., Savel, Arjun B., Gill, Holden, Beichman, Charles, Matson, Rachel, Matthews, Elisabeth C., Furlan, E., Howell, Steve B., Scott, Nicholas J., Everett, Mark E., Livingston, John H., Ershova, Irina O., Cheryasov, Dmitry V., Safonov, Boris, Lillo-Box, Jorge, Barrado, David, Morales-Calderón, María

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NGTS-6b: an ultrashort period hot-Jupiter orbiting an old K dwarf by Vines, Jose I, Jenkins, James S, Acton, Jack S, Briegal, Joshua, Bayliss, Daniel, Bouchy, François, Belardi, Claudia, Bryant, Edward M, Burleigh, Matthew R, Cabrera, Juan, Casewell, Sarah L, Chaushev, Alexander, Cooke, Benjamin F, Csizmadia, Szilárd, Eigmüller, Philipp, Erikson, Anders, Foxell, Emma, Gill, Samuel, Gillen, Edward, Goad, Michael R, Jackman, James A G, King, George W, Louden, Tom, McCormac, James, Moyano, Maximiliano, Nielsen, Louise D, Pollacco, Don, Queloz, Didier, Rauer, Heike, Raynard, Liam, Smith, Alexis M S, Soto, Maritza G, Tilbrook, Rosanna H, Titz-Weider, Ruth, Turner, Oliver, Udry, Stéphane, Walker, Simon R, Watson, Christopher A, West, Richard G, Wheatley, Peter J

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NGTS-10b: the shortest period hot Jupiter yet discovered by McCormac, James, Gillen, Edward, Jackman, James A G, Brown, David J A, Bayliss, Daniel, Wheatley, Peter J, Anderson, David R, Armstrong, David J, Bouchy, François, Briegal, Joshua T, Burleigh, Matthew R, Cabrera, Juan, Casewell, Sarah L, Chaushev, Alexander, Chazelas, Bruno, Chote, Paul, Cooke, Benjamin F, Costes, Jean C, Csizmadia, Szilárd, Eigmüller, Philipp, Erikson, Anders, Foxell, Emma, Gänsicke, Boris T, Goad, Michael R, Günther, Maximilian N, Hodgkin, Simon T, Hooton, Matthew J, Jenkins, James S, Lambert, Gregory, Lendl, Monika, Longstaff, Emma, Louden, Tom, Moyano, Maximiliano, Nielsen, Louise D, Pollacco, Don, Queloz, Didier, Rauer, Heike, Raynard, Liam, Smith, Alexis M S, Smalley, Barry, Soto, Maritza, Turner, Oliver, Udry, Stéphane, Vines, Jose I, Walker, Simon R, Watson, Christopher A, West, Richard G

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