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CURRICULUM VITAE Stacy S. Mcgaugh

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CURRICULUM VITAE Stacy S. Mcgaugh CURRICULUM VITAE Stacy S. McGaugh Department of Astronomy phone: (216) 368-1808 Case Western Reserve University fax: (216) 368-5406 Cleveland, OH 44106 cell: (216) 214-0686 http://astroweb.case.edu/ssm/ e-mail: [email protected] Education University of Michigan Ph.D. 1992 Astronomy 1987 { 1992 Princeton University Physics 1985 { 1986 Massachusetts Institute of Technology S.B. 1985 Physics 1981 { 1985 Employment Professor Departments of Astronomy & Physics 2012 { Chair Department of Astronomy 2015 { Director Warner & Swasey Observatory 2015 { Case Western Reserve University Professor Department of Astronomy 2009 { 2012 Associate Professor University of Maryland 2003 { 2009 Assistant Professor College Park 1998 { 2003 Research Fellow Department of Physics and Astronomy 1997 { 1998 Rutgers University Carnegie Fellow Department of Terrestrial Magnetism 1995 { 1997 Carnegie Institution of Washington Research Associate Institute of Astronomy 1992 { 1995 University of Cambridge Research Interests Galaxy formation and evolution, LSB galaxies, the missing mass problem, and cosmology Professional Societies | IAU, AAS, DDA Honors | Distinguished Alumnus, Flint Northern (2001); University of Michigan (2013) Publications in Refereed Journals The order of authors in Astronomy & Astrophysics reflects the degree of contribution. The names of directly supervised students and postdocs are italicized; McGaugh is listed in bold. Citation Statistics (as of 5 February 2020 from the NASA Astrophysical Data System): Total citations: 11,455; Normalized citations per author: 5,743 H-index: 57; riq index: 333; i100-index: 37 (papers with over 100 citations) 120. \A comprehensive catalog of dark matter halo models for SPARC galaxies" Li, P., Lelli, F., McGaugh, S.S., & Schombert, J.M. 2020, ApJS, in press 119. \Tracing the Dynamical Mass in Galaxy Disks Using HI Velocity Dispersion and its Implications for the Dark Matter Distribution in Galaxies" Das, M., McGaugh, S.S., Ianjamasimanana, R., Schombert, J.M., & Dwarakanath, K.S. 2020, ApJ, 889, 10 118. \The Halo Mass Function of Late-Type Galaxies from HI Kinematics" Li, P., Lelli, F., McGaugh, S.S., Pawlowski, M.S., Zwaan, M.A., & Schombert, J.M. 2019, ApJ, 886, L11 117. \The Imprint of Spiral Arms on the Galactic Rotation Curve" McGaugh, S.S. 2019, ApJ, 885, 87 116. \The baryonic Tully-Fisher relation for different velocity definitions and implications for galaxy angular momentum" Lelli, F., McGaugh, S.S., Schombert, J.M., Desmond, H., & Katz, H. 2019, MNRAS, 484, 3267{3278 115. \Uncorrelated velocity and size residuals across galaxy rotation curves" Desmond, H., Katz, H., Lelli, F., & McGaugh, S.S. 2019, MNRAS, 484, 239{244 114. \The Mass-to-light Ratios and the Star Formation Histories of Disk Galaxies" Schombert, J.M., McGaugh, S.S., & Lelli, F. 2019, MNRAS, 483, 1496{1512 113. \The Tight Empirical Relation between Dark Matter Halo Mass and Flat Rotation Velocity for Late-Type Galaxies" Katz, H., Desmond, H., McGaugh, S.S., & Lelli, F. 2019, MNRAS, 483, L98{L103 112. \A constant characteristic volume density of dark matter haloes from SPARC rotation curve fits” Li, P., Lelli, F., McGaugh, S.S., Starkman, N. & Schombert, J.M. 2019, MNRAS, 482, 5106{5124 111. \Presence of a fundamental acceleration scale in galaxies" McGaugh, S.S., Li, P., Lelli, F., & Schombert, J.M. 2018, Nature Astronomy, 2, 924 110. \Predictions for the sky-averaged depth of the 21cm absorption signal at high redshift in cosmologies with and without non-baryonic cold dark matter" McGaugh, S.S. 2018, PRL, 121, 081305 109. \Stellar Feedback and the Energy Budget of Late-Type Galaxies: Missing Baryons and Core Creation" Katz, H., Desmond, H., Lelli, F., McGaugh, S.S., Di Cintio, A., Brook, C.B., & Schombert, J.M. 2018, MNRAS, 480, 4287{4301 108. \A New Algorithm to Quantify Maximum Discs in Galaxies" Starkman, N., McGaugh, S.S., Lelli, F., & Schombert, J.M. 2018, MNRAS, 480, 2292{2301 107. \MOND and the dynamics of NGC1052-DF2" Famaey, B., McGaugh, S.S., & Milgrom, M. 2018, MNRAS, 480, 473{476 106. \Fitting the Radial Acceleration Relation to Individual SPARC Galaxies" Li, P., Lelli, F., McGaugh, S.S., & Schombert, J.M. 2018, A&A, 615, A3 105. \The Star Forming Main Sequence of Dwarf Low Surface Brightness Galaxies" McGaugh, S.S., Schombert, J.M., & Lelli, F. 2017, ApJ, 851, 22 104. \Considerations on how to investigate planes of satellite galaxies" Pawlowski, M.S., Dabringhausen, J., Famaey, B., Flores, H., Hammer, F., Ibata, R.A., Kroupa, P., Lewis, G.F., Libeskind, N.I., McGaugh, S.S., Merritt, D., Puech, M., & Yang, Y. 2017, Astronomische Nachrichten, 338, 854 103. \Testing Verlinde's Emergent Gravity with the Radial Acceleration Relation" Lelli, F., McGaugh, S.S., & Schombert, J.M. 2017, MNRAS, 468, L68{L71 102. \One Law To Rule Them All: The Radial Acceleration Relation of Galaxies" Lelli, F., McGaugh, S.S., Schombert, J.M., & Pawlowski, M.S. 2017, ApJ, 836, 152 101. \Spitzer's View of the Candidate Cluster and Protocluster Catalog (CCPC)" Franck, J.R.,& McGaugh, S.S. 2017, ApJ, 836, 136 100. \Testing Feedback-Modified Dark Matter Haloes with Galaxy Rotation Curves: Esti- mation of Halo Parameters and Consistency with ΛCDM” Katz, H., Lelli, F., McGaugh, S.S., Di Cintio, A., Brook, C.B., & Schombert, J.M. 2017, MNRAS, 466, 1648{1668 99. \The candidate Cluster and Protocluster Catalog (CCPC) II: Spectroscopically iden- tified structures spanning 2 < z < 6:6" Franck, J.R.,& McGaugh, S.S. 2016, ApJ, 833, 15 98. \MOND Prediction for the Velocity Dispersion of the `Feeble Giant' Crater II" McGaugh, S.S. 2016, ApJ, 832, L8 97. \Radial Acceleration Relation in Rotationally Supported Galaxies" McGaugh, S.S., Lelli, F., & Schombert, J.M. 2016, Phys. Rev. Lett., 117, 201101 96. \SPARC: Mass Models for 175 Disk Galaxies with Spitzer Photometry and Accurate Rotation Curves" Lelli, F., McGaugh, S.S., & Schombert, J.M. 2016, AJ, 152, 157 95. \The Relation between Stellar and Dynamical Surface Densities in the Central Regions of Disk Galaxies" Lelli, F., McGaugh, S.S., Schombert, J.M. & Pawlowski, M.S. 2016, ApJ, 827, L19 94. \The Candidate Cluster and Protocluster Catalog (CCPC) of Spectroscopically Iden- tified Structures Spanning 2:74 < z < 3:71" Franck, J.R.,& McGaugh, S.S. 2016, ApJ, 817, 158 93. \The Small Scatter of the Baryonic Tully-Fisher Relation" Lelli, F., McGaugh, S.S., & Schombert, J.M. 2016, ApJ, 816, L14 92. \The Surface Density Profile of the Galactic Disk from the Terminal Velocity Curve" McGaugh, S.S. 2016, ApJ, 816, 42 91. \Gas dynamics in tidal dwarf galaxies: disc formation at z=0" Lelli, F., Duc, P.-A., Brinks, E., Bournaud, F., McGaugh, S.S., Lisenfeld, U., Weil- bacher, P.M., Boquien, M., Revaz, Y., Braine, J., Koribalski, B.S., Belles, P.-E. 2015, A&A, 584, A113 90. \Stellar Populations and the Star Formation Histories of LSB Galaxies: V. WFC3 Color-Magnitude Diagrams" Schombert, J.M., & McGaugh, S.S. 2015, AJ, 150, 72 89. \The new Milky Way satellites: alignment with the VPOS and predictions for proper motions and velocity dispersions" Pawlowski, M.S., McGaugh, S.S., & Jerjen, H. 2015, MNRAS, 453, 1047 88. \Three candidate clusters around high redshift radio-loud sources: MG1 J04426+0202, 3C 068.2, MS 1426.9+1052" Franck, J.R., McGaugh, S.S., & Schombert, J.M. 2015, AJ, 150, 46 87. \Mass models of disk galaxies from the DiskMass Survey in MOND" Angus, G.W., Gentile, G., Swaters, R.A., Famaey, B., Diaferio, A., McGaugh, S.S., & van der Heyden, K.J., 2015, MNRAS, 451, 3551{3580 86. \The link between mass distribution and starbursts in dwarf galaxies" McQuinn, K.B.W., Lelli, F., Skillman, E.D., Dolphin, A.E., McGaugh, S.S.,& Williams, B.F. 2015, MNRAS, 450, 3886{3892 85. \Weighing Galaxy Disks with the Baryonic Tully-Fisher Relation" McGaugh, S.S., & Schombert, J.M. 2015, ApJ, 802, 18 84. \The Third Law of Galactic Rotation" McGaugh, S.S. 2014, Galaxies, 2, 601{622 [invited review] 83. \Stellar Populations and the Star Formation Histories of LSB Galaxies: III. Stellar Population Models" Schombert, J.M., & McGaugh, S.S. 2014, PASA, 31, e036 82. \Color{Mass-to-Light Ratio Relations for Disk Galaxies" McGaugh, S.S., & Schombert, J.M. 2014, AJ, 148, 77 81. \Co-orbiting Planes of Sub-halos are Similarly Unlikely around Paired and Isolated Hosts" Pawlowski, M.S.,& McGaugh, S.S. 2014, ApJ, 789, L24 80. \A Tale of Two Paradigms: the Mutual Incommensurability of ΛCDM and MOND" McGaugh, S.S. 2014, Canadian Journal of Physics, 2014{0203 [invited review] 79. \Perseus I and the NGC 3109 association in the context of the Local Group dwarf galaxy structures" Pawlowski, M.S.,& McGaugh, S.S. 2014, MNRAS, 440, 908 78. \The Inner Dynamical Mass Across Galaxy Morphology: A Weak Scaling with Total Stellar Mass" Kuzio de Naray, R.,& McGaugh, S.S. 2014 ApJ, 782, L12 77. \The Formation of Spiral Galaxies: Adiabatic Compression with Young's Algorithm and the Relation of Dark Matter Haloes to Their Primordial Antecedents" Katz, H., McGaugh, S.S., Sellwood, J.A., & de Blok, W.J.G. 2014, MNRAS, 439, 1897 76. \Stellar Populations and the Star Formation Histories of LSB Galaxies: IV Spitzer Surface Photometry of LSB Galaxies" Schombert, J.M., & McGaugh, S.S. 2014, PASA, 31, e011 75. \Andromeda Dwarfs in Light of MOND. II. Testing Prior Predictions" McGaugh, S.S., & Milgrom, M. 2013, ApJ, 775, 139 74. \Stellar Populations and the Star Formation Histories of LSB Galaxies: II. HII Re- gions" Schombert, J.M., McGaugh, S.S., & Maciel, T. 2013, AJ, 146, 41 73. \Galaxy Cluster Bulk Flows and Collision Velocities in QUMOND" Katz, H., McGaugh, S.S., Teuben, P., & Angus, G.W. 2013, ApJ, 772, 10 72. \Discrete clouds of neutral gas between the galaxies M31 and M33" Wolfe, S.A., Pisano, D.J., Lockman, F.J., McGaugh, S.S., & Shaya, E.J.
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