Amaro-Seoane, P., Andrews, J., Arca Sedda, M., Askar, A., Baghi, Q., Balasov, R., . . . Vigna-Gómez, A. (2023). Astrophysics with the Laser Interferometer Space Antenna. Living Reviews in Relativity, 26, 2. doi:10.1007/s41114-022-00041-y

Shields, D., Boe, B., Pfountz, C., Davis, B. L., Hartley, M., Miller, R., . . . Kennefick, J. (2022). Spirality: A Novel Way to Measure Spiral Arm Pitch Angle. Galaxies, 10, 100. doi:10.3390/galaxies10050100

Sahu, N., Graham, A. W., & Davis, B. L. (2022). The (Black Hole Mass)-(Spheroid Stellar Density) Relations: M <SUB>BH</SUB>-μ (and M <SUB>BH</SUB>-Σ) and M <SUB>BH</SUB>-ρ. The Astrophysical Journal, 927, 67. doi:10.3847/1538-4357/ac4251

Sahu, N., Graham, A., & Davis, B. (2022). The Morphology-dependent Black Hole - Host Galaxy Correlations: A Consequence of Physical Formation Processes. Acta Astrophysica Taurica, 3, 39-43. doi:10.31059/aat.vol3.iss1.pp39-43

Hon, D. S.-H., Graham, A. W., Davis, B. L., & Marconi, A. (2022). Disc cloaking: Establishing a lower limit to the number density of local compact massive spheroids/bulges and the potential fate of some high-z red nuggets. Monthly Notices of the Royal Astronomical Society, 514(3), 3410-3451. doi:10.1093/mnras/stac1171

Fusco, M. S., Davis, B. L., Kennefick, J., Kennefick, D., & Seigar, M. S. (2022). Probing the Low-Mass End of the Black Hole Mass Function via a Study of Faint Local Spiral Galaxies. Universe, 8(12), 649. Retrieved from https://www.mdpi.com/2218-1997/8/12/649

Abdeen, S., Davis, B. L., Eufrasio, R., Kennefick, D., Kennefick, J., Miller, R., . . . O'Mara, H. (2022). Evidence in favour of density wave theory through age gradients observed in star formation history maps and spatially resolved stellar clusters. Monthly Notices of the Royal Astronomical Society, 512, 366-377. doi:10.1093/mnras/stac459

Graham, A. W., Soria, R., Davis, B. L., Kolehmainen, M., Maccarone, T., Miller-Jones, J., . . . Swartz, D. A. (2021). Central X-Ray Point Sources Found to Be Abundant in Low-mass, Late-type Galaxies Predicted to Contain an Intermediate-mass Black Hole. The Astrophysical Journal, 923, 246. doi:10.3847/1538-4357/ac34f4

Graham, A. W., Soria, R., Ciambur, B. C., Davis, B. L., & Swartz, D. A. (2021). Potential Black Hole Seeding of the Spiral Galaxy NGC 4424 via an Infalling Star Cluster. The Astrophysical Journal, 923, 146. doi:10.3847/1538-4357/ac235b

Davis, B. L., & Graham, A. W. (2021). Refining the mass estimate for the intermediate-mass black hole candidate in NGC 3319. Publications of the Astronomical Society of Australia, 38, e030. doi:10.1017/pasa.2021.23

Sahu, N., Graham, A. W., & Davis, B. L. (2020). Defining the (Black Hole)–Spheroid Connection with the Discovery of Morphology-dependent Substructure in the M BH–n sph and M BH–R e,sph Diagrams: New Tests for Advanced Theories and Realistic Simulations. The Astrophysical Journal, 903(2), 97. doi:10.3847/1538-4357/abb675

Abdeen, S., Kennefick, D., Kennefick, J., Miller, R., Shields, D. W., Monson, E. B., & Davis, B. L. (2020). Determining the co-rotation radii of spiral galaxies using spiral arm pitch angle measurements at multiple wavelengths. Monthly Notices of the Royal Astronomical Society, 496(2), 1610-1619. doi:10.1093/mnras/staa1596

Sahu, N., Graham, A. W., & Davis, B. L. (2019). Black Hole Mass Scaling Relations for Early-type Galaxies. I. M BH–M *, sph and M BH–M *,gal. The Astrophysical Journal, 876(2), 155. doi:10.3847/1538-4357/ab0f32

Sahu, N., Graham, A. W., & Davis, B. L. (2019). Revealing Hidden Substructures in the M BH–σ Diagram, and Refining the Bend in the L–σ Relation. The Astrophysical Journal, 887(1), 10. doi:10.3847/1538-4357/ab50b7

Miller, R., Kennefick, D., Kennefick, J., Abdeen, M. S., Monson, E., Eufrasio, R. T., . . . Davis, B. L. (2019). Investigating the Origins of Spiral Structure in Disk Galaxies through a Multiwavelength Study. The Astrophysical Journal, 874(2), 177. doi:10.3847/1538-4357/ab0d26

Davis, B. L., Graham, A. W., & Combes, F. (2019). A Consistent Set of Empirical Scaling Relations for Spiral Galaxies: The (v max, M oM)–(σ 0, M BH, ϕ) Relations. The Astrophysical Journal, 877(1), 64. doi:10.3847/1538-4357/ab1aa4

Davis, B. L., Graham, A. W., & Cameron, E. (2019). Black Hole Mass Scaling Relations for Spiral Galaxies. I. M BH–M *,sph. The Astrophysical Journal, 873(1), 85. doi:10.3847/1538-4357/aaf3b8

Graham, A. W., Soria, R., & Davis, B. L. (2018). Expected intermediate mass black holes in the Virgo cluster. II. Late-type galaxies. Monthly Notices of the Royal Astronomical Society, 484, 814. doi:10.1093/mnras/sty3068

Davis, B. L., Graham, A. W., & Cameron, E. (2018). Black Hole Mass Scaling Relations for Spiral Galaxies. II. M BH–M *,tot and M BH–M *,disk. The Astrophysical Journal, 869(2), 113. doi:10.3847/1538-4357/aae820

Koliopanos, F., Ciambur, B. C., Graham, A. W., Webb, N. A., Coriat, M., Mutlu-Pakdil, B., . . . Seigar, M. S. (2017). Searching for intermediate-mass black holes in galaxies with low-luminosity AGN: a multiple-method approach. Astronomy & Astrophysics, 601, A20. doi:10.1051/0004-6361/201630061

Davis, B. L., Graham, A. W., & Seigar, M. S. (2017). Updating the (supermassive black hole mass)–(spiral arm pitch angle) relation: a strong correlation for galaxies with pseudobulges. Monthly Notices of the Royal Astronomical Society, 471(2), 2187-2203. doi:10.1093/mnras/stx1794

Pour-Imani, H., Kennefick, D., Kennefick, J., Davis, B. L., Shields, D. W., & Abdeen, M. S. (2016). Strong Evidence for the Density-Wave Theory of Spiral Structure in Disk Galaxies. The Astrophysical Journal, 827(1), L2. doi:10.3847/2041-8205/827/1/l2

Mutlu-Pakdil, B., Seigar, M. S., & Davis, B. L. (2016). THE LOCAL BLACK HOLE MASS FUNCTION DERIVED FROM THEMBH–PAND THEMBH–nRELATIONS. The Astrophysical Journal, 830(2), 117. doi:10.3847/0004-637x/830/2/117

Davis, B. L., Kennefick, D., Kennefick, J., Westfall, K. B., Shields, D. W., Flatman, R., . . . Swaters, R. A. (2015). A Fundamental Plane of Spiral Structure in Disk Galaxies. The Astrophysical Journal, 802(1), L13. doi:10.1088/2041-8205/802/1/l13

Davis, B. (2015). Logarithmic Spiral Arm Pitch Angle of Spiral Galaxies: Measurement and Relationship to Galactic Structure and Nuclear Supermassive Black Hole Mass. Retrieved from https://ui.adsabs.harvard.edu/abs/2015PhDT........14D

Seigar, M. S., Davis, B. L., Berrier, J., & Kennefick, D. (2014). Constraining Dark Matter Halo Profiles and Galaxy Formation Models Using Spiral Arm Morphology. Ii. Dark and Stellar Mass Concentrations for 13 Nearby Face-on Galaxies. The Astrophysical Journal, 795(1), 90. doi:10.1088/0004-637x/795/1/90

Davis, B. L., Berrier, J. C., Johns, L., Shields, D. W., Hartley, M. T., Kennefick, D., . . . Lacy, C. H. S. (2014). The Black Hole Mass Function Derived from Local Spiral Galaxies. The Astrophysical Journal, 789(2), 124. doi:10.1088/0004-637x/789/2/124

Berrier, J. C., Davis, B. L., Kennefick, D., Kennefick, J. D., Seigar, M. S., Barrows, R. S., . . . Lacy, C. H. S. (2013). Further Evidence for a Supermassive Black Hole Mass-Pitch Angle Relation. The Astrophysical Journal, 769(2), 132. doi:10.1088/0004-637x/769/2/132

Davis, B. L., Berrier, J. C., Shields, D. W., Kennefick, J., Kennefick, D., Seigar, M. S., . . . Puerari, I. (2012). Measurement of Galactic Logarithmic Spiral Arm Pitch Angle Using Two-Dimensional Fast Fourier Transform Decomposition. The Astrophysical Journal Supplement Series, 199(2), 33. doi:10.1088/0067-0049/199/2/33