Year |
Citation |
Score |
2024 |
Poggiali V, Brighi G, Hayes AG, Nicholson PD, MacKenzie S, Lalich DE, Bonnefoy LE, Oudrhiri K, Lorenz RD, Soderblom JM, Tortora P, Zannoni M. Surface properties of the seas of Titan as revealed by Cassini mission bistatic radar experiments. Nature Communications. 15: 5454. PMID 39013844 DOI: 10.1038/s41467-024-49837-2 |
0.368 |
|
2022 |
Neveu M, Coker RF, Lorenz RD, MacKenzie SM, Lunine JI, Davila AF. Planetary Protection Assessment of Radioisotope Thermoelectric Generator (RTG)-Powered Landed Missions to Ocean Worlds: Application to Enceladus. Astrobiology. PMID 35972349 DOI: 10.1089/ast.2020.2432 |
0.326 |
|
2020 |
Hofgartner JD, Hayes AG, Campbell DB, Lunine JI, Black GJ, MacKenzie SM, Birch SPD, Elachi C, Kirk RD, Le Gall A, Lorenz RD, Wall SD. The root of anomalously specular reflections from solid surfaces on Saturn's moon Titan. Nature Communications. 11: 2829. PMID 32546817 DOI: 10.1038/S41467-020-16663-1 |
0.527 |
|
2019 |
Martin KP, MacKenzie SM, Barnes JW, Ytreberg FM. Protein Stability in Titan's Subsurface Water Ocean. Astrobiology. PMID 31730377 DOI: 10.1089/Ast.2018.1972 |
0.609 |
|
2019 |
MacKenzie SM, Barnes JW, Hofgartner JD, Birch SPD, Hedman MM, Lucas A, Rodriguez S, Turtle EP, Sotin C. The case for seasonal surface changes at Titan’s lake district Nature Astronomy. 3: 506-510. DOI: 10.1038/S41550-018-0687-6 |
0.663 |
|
2019 |
Lucas A, Rodriguez S, Lemonnier F, Gall AL, MacKenzie S, Ferrari C, Paillou P, Narteau C. Texture and composition of Titan's equatorial sand seas inferred from Cassini SAR data: Implications for aeolian transport and dune morphodynamics Journal of Geophysical Research. 124: 3140-3163. DOI: 10.1029/2019Je005965 |
0.44 |
|
2018 |
Barnes JW, MacKenzie SM, Lorenz RD, Turtle EP. Titan’s Twilight and Sunset Solar Illumination The Astronomical Journal. 156: 247. DOI: 10.3847/1538-3881/Aae519 |
0.552 |
|
2018 |
Barnes JW, MacKenzie SM, Young EF, Trouille LE, Rodriguez S, Cornet T, Jackson BK, Ádámkovics M, Sotin C, Soderblom JM. Spherical Radiative Transfer in C++ (SRTC++): A Parallel Monte Carlo Radiative Transfer Model for Titan The Astronomical Journal. 155: 264. DOI: 10.3847/1538-3881/Aac2Db |
0.509 |
|
2018 |
Hatchett WT, Barnes JW, Ahlers JP, MacKenzie SM, Hedman MM. A pilot investigation to constrain the presence of ring systems around transiting exoplanets New Astronomy. 60: 88-94. DOI: 10.1016/J.Newast.2017.11.001 |
0.541 |
|
2018 |
Martin K, MacKenzie S, Barnes J, Ytreberg FM. Comparing Structure Stability between Earth and Subsurface Ocean on Titan using Molecular Dynamics Simulation Biophysical Journal. 114: 528a. DOI: 10.1016/J.Bpj.2017.11.2885 |
0.554 |
|
2017 |
Birch SPD, Hayes AG, Corlies P, Stofan ER, Hofgartner JD, Lopes RMC, Lorenz RD, Lunine JI, MacKenzie SM, Malaska MJ, Wood CA. Morphological evidence that Titan’s southern hemisphere basins are paleoseas Icarus. 310: 140-148. DOI: 10.1016/J.Icarus.2017.12.016 |
0.446 |
|
2016 |
MacKenzie SM, Barnes JW. Compositional Similarities And Distinctions Between Titan’S Evaporitic Terrains The Astrophysical Journal. 821: 17. DOI: 10.3847/0004-637X/821/1/17 |
0.633 |
|
2016 |
MacKenzie SM, Caswell TE, Phillips-Lander CM, Stavros EN, Hofgartner JD, Sun VZ, Powell KE, Steuer CJ, O'Rourke JG, Dhaliwal JK, Leung CWS, Petro EM, Wynne JJ, Phan S, Crismani M, et al. THEO concept mission: Testing the Habitability of Enceladus's Ocean Advances in Space Research. 58: 1117-1137. DOI: 10.1016/J.Asr.2016.05.037 |
0.447 |
|
2015 |
Cordier D, Cornet T, Barnes JW, MacKenzie SM, Le Bahers T, Nna-Mvondo D, Rannou P, Ferreira AG. Structure of Titan's evaporites Icarus. DOI: 10.1016/J.Icarus.2015.12.034 |
0.619 |
|
2015 |
Vixie G, Barnes JW, Jackson B, Rodriguez S, Le Mouélic S, Sotin C, MacKenzie S, Wilson P. Possible temperate lakes on Titan Icarus. 257: 313-323. DOI: 10.1016/J.Icarus.2015.05.009 |
0.581 |
|
2015 |
Neish CD, Barnes JW, Sotin C, Mackenzie S, Soderblom JM, Le Mouélic S, Kirk RL, Stiles BW, Malaska MJ, Le Gall A, Brown RH, Baines KH, Buratti B, Clark RN, Nicholson PD. Spectral properties of Titan's impact craters imply chemical weathering of its surface Geophysical Research Letters. 42: 3746-3754. DOI: 10.1002/2015Gl063824 |
0.657 |
|
2014 |
MacKenzie SM, Barnes JW, Sotin C, Soderblom JM, Le Mouélic S, Rodriguez S, Baines KH, Buratti BJ, Clark RN, Nicholson PD, McCord TB. Evidence of Titan's climate history from evaporite distribution Icarus. 243: 191-207. DOI: 10.1016/J.Icarus.2014.08.022 |
0.656 |
|
Show low-probability matches. |