Leveraging SN Ia spectroscopic similarity to improve the measurement of H0 von Murakami, Yukei S, Riess, Adam G, Stahl, Benjamin E, W D'Arcy Kenworthy, Pluck, Dahne-More A, Macoretta, Antonella, Dillon Brout, Jones, David O, Scolnic, Dan M, Filippenko, Alexei V

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Leveraging SN Ia spectroscopic similarity to improve the measurement of H 0 von Murakami, Yukei S., Riess, Adam G., Stahl, Benjamin E., D'Arcy Kenworthy, W., Pluck, Dahne-More A., Macoretta, Antonella, Brout, Dillon, Jones, David O., Scolnic, Dan M., Filippenko, Alexei V.

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Leveraging SN Ia spectroscopic similarity to improve the measurement of $H_0 von Murakami, Yukei S, Riess, Adam G, Stahl, Benjamin E, Kenworthy, W. D'Arcy, Pluck, Dahne-More A, Macoretta, Antonella, Brout, Dillon, Jones, David O, Scolnic, Dan M, Filippenko, Alexei V

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Leveraging SN Ia spectroscopic similarity to improve the measurement of \(H_0\) von Murakami, Yukei S, Riess, Adam G, Stahl, Benjamin E, W D'Arcy Kenworthy, Pluck, Dahne-More A, Macoretta, Antonella, Dillon Brout, Jones, David O, Scolnic, Dan M, Filippenko, Alexei V

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Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics beyond ΛCDM von Riess, Adam G., Casertano, Stefano, Yuan, Wenlong, Macri, Lucas M., Scolnic, Dan

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A 2.4% DETERMINATION OF THE LOCAL VALUE OF THE HUBBLE CONSTANT von Riess, Adam G, Macri, Lucas M, Hoffmann, Samantha L, Scolnic, Dan, Casertano, Stefano, Filippenko, Alexei V, Tucker, Brad E, Reid, Mark J, Jones, David O, Silverman, Jeffrey M, Chornock, Ryan, Challis, Peter, Yuan, Wenlong, Brown, Peter J, Foley, Ryan J

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Type Ia Supernova Distances at Redshift >1.5 from the Hubble Space Telescope Multi-cycle Treasury Programs: The Early Expansion Rate von Riess, Adam G., Rodney, Steven A., Scolnic, Daniel M., Shafer, Daniel L., Strolger, Louis-Gregory, Ferguson, Henry C., Postman, Marc, Graur, Or, Maoz, Dan, Jha, Saurabh W., Mobasher, Bahram, Casertano, Stefano, Hayden, Brian, Molino, Alberto, Hjorth, Jens, Garnavich, Peter M., Jones, David O., Kirshner, Robert P., Koekemoer, Anton M., Grogin, Norman A., Brammer, Gabriel, Hemmati, Shoubaneh, Dickinson, Mark, Challis, Peter M., Wolff, Schuyler, Clubb, Kelsey I., Filippenko, Alexei V., Nayyeri, Hooshang, Vivian, U, Koo, David C., Faber, Sandra M., Kocevski, Dale, Bradley, Larry, Coe, Dan

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The Pantheon+ Analysis: SuperCal-fragilistic Cross Calibration, Retrained SALT2 Light-curve Model, and Calibration Systematic Uncertainty von Brout, Dillon, Taylor, Georgie, Scolnic, Dan, Wood, Charlotte M., Rose, Benjamin M., Vincenzi, Maria, Dwomoh, Arianna, Lidman, Christopher, Riess, Adam, Ali, Noor, Qu, Helen, Dai, Mi

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JWST Observations Reject Unrecognized Crowding of Cepheid Photometry as an Explanation for the Hubble Tension at 8σ Confidence von Riess, Adam G., Anand, Gagandeep S., Yuan, Wenlong, Casertano, Stefano, Dolphin, Andrew, Macri, Lucas M., Breuval, Louise, Scolnic, Dan, Perrin, Marshall, Anderson, Richard I.

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Crowded No More: The Accuracy of the Hubble Constant Tested with High-resolution Observations of Cepheids by JWST von Riess, Adam G., Anand, Gagandeep S., Yuan, Wenlong, Casertano, Stefano, Dolphin, Andrew, Macri, Lucas M., Breuval, Louise, Scolnic, Dan, Perrin, Marshall, Anderson, Richard I.

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The Accuracy of the Hubble Constant Measurement Verified through Cepheid Amplitudes von Riess, Adam G., Yuan, Wenlong, Casertano, Stefano, Macri, Lucas M., Scolnic, Dan

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The Pantheon+ analysis: Improving the redshifts and peculiar velocities of Type Ia supernovae used in cosmological analyses von Carr, Anthony, Davis, Tamara M., Scolnic, Dan, Said, Khaled, Brout, Dillon, Peterson, Erik R., Kessler, Richard

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SuperRAENN: A Semisupervised Supernova Photometric Classification Pipeline Trained on Pan-STARRS1 Medium-Deep Survey Supernovae von Villar, V. Ashley, Hosseinzadeh, Griffin, Berger, Edo, Ntampaka, Michelle, Jones, David O., Challis, Peter, Chornock, Ryan, Drout, Maria R., Foley, Ryan J., Kirshner, Robert P., Lunnan, Ragnhild, Margutti, Raffaella, Milisavljevic, Dan, Sanders, Nathan, Pan, Yen-Chen, Rest, Armin, Scolnic, Daniel M., Magnier, Eugene, Metcalfe, Nigel, Wainscoat, Richard, Waters, Christopher

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Prospects for Resolving the Hubble Constant Tension with Standard Sirens von Feeney, Stephen M, Peiris, Hiranya V, Williamson, Andrew R, Nissanke, Samaya M, Mortlock, Daniel J, Alsing, Justin, Scolnic, Dan

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Cluster Cepheids with High Precision Gaia Parallaxes, Low Zero-point Uncertainties, and Hubble Space Telescope Photometry von Riess, Adam G., Breuval, Louise, Yuan, Wenlong, Casertano, Stefano, Macri, Lucas M., Bowers, J. Bradley, Scolnic, Dan, Cantat-Gaudin, Tristan, Anderson, Richard I., Reyes, Mauricio Cruz

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The Pantheon+ Analysis: Cosmological Constraints von Brout, Dillon, Scolnic, Dan, Popovic, Brodie, Riess, Adam G., Carr, Anthony, Zuntz, Joe, Kessler, Rick, Davis, Tamara M., Hinton, Samuel, Jones, David, Kenworthy, W. D’Arcy, Peterson, Erik R., Said, Khaled, Taylor, Georgie, Ali, Noor, Armstrong, Patrick, Charvu, Pranav, Dwomoh, Arianna, Meldorf, Cole, Palmese, Antonella, Qu, Helen, Rose, Benjamin M., Sanchez, Bruno, Stubbs, Christopher W., Vincenzi, Maria, Wood, Charlotte M., Brown, Peter J., Chen, Rebecca, Chambers, Ken, Coulter, David A., Dai, Mi, Dimitriadis, Georgios, Filippenko, Alexei V., Foley, Ryan J., Jha, Saurabh W., Kelsey, Lisa, Kirshner, Robert P., Möller, Anais, Muir, Jessie, Nadathur, Seshadri, Pan, Yen-Chen, Rest, Armin, Rojas-Bravo, Cesar, Sako, Masao, Siebert, Matthew R., Smith, Mat, Stahl, Benjamin E., Wiseman, Phil

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The Pantheon+ Analysis: The Full Data Set and Light-curve Release von Scolnic, Dan, Brout, Dillon, Carr, Anthony, Riess, Adam G., Davis, Tamara M., Dwomoh, Arianna, Jones, David O., Ali, Noor, Charvu, Pranav, Chen, Rebecca, Peterson, Erik R., Popovic, Brodie, Rose, Benjamin M., Wood, Charlotte M., Brown, Peter J., Chambers, Ken, Coulter, David A., Dettman, Kyle G., Dimitriadis, Georgios, Filippenko, Alexei V., Foley, Ryan J., Jha, Saurabh W., Kilpatrick, Charles D., Kirshner, Robert P., Pan, Yen-Chen, Rest, Armin, Rojas-Bravo, Cesar, Siebert, Matthew R., Stahl, Benjamin E., Zheng, WeiKang

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JWST Validates HST Distance Measurements: Selection of Supernova Subsample Explains Differences in JWST Estimates of Local H 0 von Riess, Adam G., Scolnic, Dan, Anand, Gagandeep S., Breuval, Louise, Casertano, Stefano, Macri, Lucas M., Li, Siyang, Yuan, Wenlong, Huang, Caroline D., Jha, Saurabh, Murakami, Yukei S., Beaton, Rachael, Brout, Dillon, Wu, Tianrui, Addison, Graeme E., Bennett, Charles, Anderson, Richard I., Filippenko, Alexei V., Carr, Anthony

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Photometric Classification of 2315 Pan-STARRS1 Supernovae with Superphot von Hosseinzadeh, Griffin, Dauphin, Frederick, Villar, V. Ashley, Berger, Edo, Jones, David O., Challis, Peter, Chornock, Ryan, Drout, Maria R., Foley, Ryan J., Kirshner, Robert P., Lunnan, Ragnhild, Margutti, Raffaella, Milisavljevic, Dan, Pan, Yen-Chen, Rest, Armin, Scolnic, Daniel M., Magnier, Eugene, Metcalfe, Nigel, Wainscoat, Richard, Waters, Christopher

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ILLUMINATING A DARK LENS: A TYPE Ia SUPERNOVA MAGNIFIED BY THE FRONTIER FIELDS GALAXY CLUSTER ABELL 2744 von Rodney, Steven A., Patel, Brandon, Scolnic, Daniel, Foley, Ryan J., Molino, Alberto, Brammer, Gabriel, Jauzac, Mathilde, Brada, Maruša, Broadhurst, Tom, Coe, Dan, Diego, Jose M., Graur, Or, Hjorth, Jens, Hoag, Austin, W. Jha, Saurabh, Johnson, Traci L., Kelly, Patrick, Lam, Daniel, McCully, Curtis, Medezinski, Elinor, Meneghetti, Massimo, Merten, Julian, Richard, Johan, Riess, Adam, Sharon, Keren, Strolger, Louis-Gregory, Treu, Tommaso, Wang, Xin, Williams, Liliya L. R., Zitrin, Adi

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