<h1>Hansen, Bradley Miles Stougaard</h1>
<h2>Combined from <a href="https://authors.library.caltech.edu">CaltechAUTHORS</a></h2>
<ul>
<li>Richer, Harvey B. and Cohen, Roger E., el al. (2022) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20220531-844238000">When Do Stars Go Boom?</a>; Astrophysical Journal Letters; Vol. 931; No. 2; Art. No. L20; <a href="https://doi.org/10.3847/2041-8213/ac6585">10.3847/2041-8213/ac6585</a></li>
<li>Zink, Jon K. and Hansen, Bradley M. S. (2019) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20190725-125944308">Accounting for multiplicity in calculating eta Earth</a>; Monthly Notices of the Royal Astronomical Society; Vol. 487; No. 1; 246-252; <a href="https://doi.org/10.1093/mnras/stz1246">10.1093/mnras/stz1246</a></li>
<li>Vinson, Alec M. and Tamayo, Daniel, el al. (2019) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20190726-093513125">The Chaotic Nature of TRAPPIST-1 Planetary Spin States</a>; <a href="https://doi.org/10.48550/arXiv.1905.11419">10.48550/arXiv.1905.11419</a></li>
<li>Zink, Jon K. and Christiansen, Jessie L., el al. (2019) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20190415-130416951">Accounting for incompleteness due to transit multiplicity in Kepler planet occurrence rates</a>; Monthly Notices of the Royal Astronomical Society; Vol. 483; No. 4; 4479-4494; <a href="https://doi.org/10.1093/mnras/sty3463">10.1093/mnras/sty3463</a></li>
<li>Livingston, John H. and Crossfield, Ian J. M., el al. (2019) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20190124-122559376">Spitzer transit follow-up of planet candidates from the K2 mission</a>; Astronomical Journal; Vol. 157; No. 3; Art. No. 102; <a href="https://doi.org/10.3847/1538-3881/aaff69">10.3847/1538-3881/aaff69</a></li>
<li>Sinukoff, Evan and Howard, Andrew W., el al. (2017) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20170601-135603463">K2-66b and K2-106b: Two Extremely Hot Sub-Neptune-size Planets with High Densities</a>; Astronomical Journal; Vol. 153; No. 6; Art. No. 271; <a href="https://doi.org/10.3847/1538-3881/aa725f">10.3847/1538-3881/aa725f</a></li>
<li>Sinukoff, Evan and Howard, Andrew W., el al. (2017) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20170120-132220743">Mass Constraints of the WASP-47 Planetary System from Radial Velocities</a>; Astronomical Journal; Vol. 153; No. 2; Art. No. 70; <a href="https://doi.org/10.3847/1538-3881/153/2/70">10.3847/1538-3881/153/2/70</a></li>
<li>Sinukoff, Evan and Howard, Andrew W., el al. (2016) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20160810-152533844">Eleven Multiplanet Systems from K2 Campaigns 1 and 2 and the Masses of Two Hot Super-Earths</a>; Astrophysical Journal; Vol. 827; No. 1; Art. No. 78; <a href="https://doi.org/10.3847/0004-637X/827/1/78">10.3847/0004-637X/827/1/78</a></li>
<li>Ngo, Henry and Knutson, Heather A., el al. (2016) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20160707-153537679">Friends of Hot Jupiters. IV. Stellar companions beyond 50 AU might facilitate giant planet formation, but most are unlikely to cause Kozai-Lidov migration</a>; Astrophysical Journal; Vol. 827; No. 1; Art. No. 8; <a href="https://doi.org/10.3847/0004-637X/827/1/8">10.3847/0004-637X/827/1/8</a></li>
<li>Petigura, Erik A. and Howard, Andrew W., el al. (2016) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20160311-123435885">Two Transiting Low Density Sub-Saturns from K2</a>; Astrophysical Journal; Vol. 818; No. 1; Art. No. 36; <a href="https://doi.org/10.3847/0004-637X/818/1/36">10.3847/0004-637X/818/1/36</a></li>
<li>Crossfield, Ian J. M. and Barman, Travis, el al. (2013) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20170623-154020107">Warm ice giant GJ 3470b. I. A flat transmission spectrum indicates a hazy, low-methane, and/or metal-rich atmosphere</a>; Astronomy and Astrophysics; Vol. 559; Art. No. A33; <a href="https://doi.org/10.1051/0004-6361/201322278">10.1051/0004-6361/201322278</a></li>
<li>Salim, Samir and Rich, R. Michael, el al. (2004) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20170408-172900790">Cool White Dwarfs Revisited: New Spectroscopy and Photometry</a>; Astrophysical Journal; Vol. 601; No. 2; 1075-1087; <a href="https://doi.org/10.1086/380581">10.1086/380581</a></li>
<li>Hansen, Brad M. S. and Phinney, E. Sterl (1998) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20190205-142100141">Stellar forensics — I. Cooling curves</a>; Monthly Notices of the Royal Astronomical Society; Vol. 294; No. 4; 557-568; <a href="https://doi.org/10.1111/j.1365-8711.1998.01232.x">10.1111/j.1365-8711.1998.01232.x</a></li>
<li>Hansen, Brad M. S. and Phinney, E. Sterl (1998) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20190205-142100054">Stellar forensics — II. Millisecond pulsar binaries</a>; Monthly Notices of the Royal Astronomical Society; Vol. 294; No. 4; 569-581; <a href="https://doi.org/10.1111/j.1365-8711.1998.01233.x">10.1111/j.1365-8711.1998.01233.x</a></li>
<li>Hansen, Brad M. S. and Phinney, E. Sterl (1997) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20190205-142100363">The pulsar kick velocity distribution</a>; Monthly Notices of the Royal Astronomical Society; Vol. 291; No. 3; 569-577; <a href="https://doi.org/10.1093/mnras/291.3.569">10.1093/mnras/291.3.569</a></li>
</ul>