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Finding Planet Nine: apsidal anti-alignment Monte Carlo results

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Monthly Notices of the Royal Astronomical Society 462 (2) 1972 (2016)
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BLACKBODY RADIATION FROM ISOLATED NEPTUNES

Sivan Ginzburg, Re’em Sari and Abraham Loeb
The Astrophysical Journal 822 (1) L11 (2017)
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Evaluating the Dynamical Stability of Outer Solar System Objects in the Presence of Planet Nine

Juliette C. Becker, Fred C. Adams, Tali Khain, Stephanie J. Hamilton and David Gerdes
The Astronomical Journal 154 (2) 61 (2017)
DOI: 10.3847/1538-3881/aa7aa2
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Numerical Solutions for the Orbital Motion of the Solar System over the Past 100 Myr: Limits and New Results

Richard E. Zeebe
The Astronomical Journal 154 (5) 193 (2017)
DOI: 10.3847/1538-3881/aa8cce
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Non-resonant secular dynamics of trans-Neptunian objects perturbed by a distant super-Earth

Melaine Saillenfest, Marc Fouchard, Giacomo Tommei and Giovanni B. Valsecchi
Celestial Mechanics and Dynamical Astronomy 129 (3) 329 (2017)
DOI: 10.1007/s10569-017-9775-7
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Measuring the Radius and Mass of Planet Nine

J. Schneider
Publications of the Astronomical Society of the Pacific 129 (980) 104401 (2017)
DOI: 10.1088/1538-3873/aa79fd
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Is the Recently Proposed Mars-Sized Perturber at 65–80 AU Ruled Out by the Cassini Ranging Data?

Lorenzo Iorio
Frontiers in Astronomy and Space Sciences 4 (2017)
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Planetary science: Cassini aids hunt for Planet Nine

Nature 531 (7595) 417 (2016)
DOI: 10.1038/531417e
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Binary stripping as a plausible origin of correlated pairs of extreme trans-Neptunian objects

C. de la Fuente Marcos, R. de la Fuente Marcos and S. J. Aarseth
Astrophysics and Space Science 362 (11) (2017)
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Producing Distant Planets by Mutual Scattering of Planetary Embryos

Kedron Silsbee and Scott Tremaine
The Astronomical Journal 155 (2) 75 (2018)
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Constraints on Planet Nine’s Orbit and Sky Position within a Framework of Mean-motion Resonances

Sarah Millholland and Gregory Laughlin
The Astronomical Journal 153 (3) 91 (2017)
DOI: 10.3847/1538-3881/153/3/91
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Is there an exoplanet in the Solar system?

Alexander J. Mustill, Sean N. Raymond and Melvyn B. Davies
Monthly Notices of the Royal Astronomical Society: Letters 460 (1) L109 (2016)
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Mass of the Kuiper belt

E. V. Pitjeva and N. P. Pitjev
Celestial Mechanics and Dynamical Astronomy 130 (9) (2018)
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The Influence of Planet Nine on the Orbits of Distant TNOs: The Case for a Low-perihelion Planet

Jessica Cáceres and Rodney Gomes
The Astronomical Journal 156 (4) 157 (2018)
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Comprehensive wide-band magnitudes and albedos for the planets, with applications to exo-planets and Planet Nine

Anthony Mallama, Bruce Krobusek and Hristo Pavlov
Icarus 282 19 (2017)
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SEARCHING FOR PLANET NINE WITH COADDEDWISEANDNEOWISE-REACTIVATION IMAGES

Aaron M. Meisner, Benjamin C. Bromley, Peter E. Nugent, et al.
The Astronomical Journal 153 (2) 65 (2017)
DOI: 10.3847/1538-3881/153/2/65
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The fates of Solar system analogues with one additional distant planet

Dimitri Veras
Monthly Notices of the Royal Astronomical Society 463 (3) 2958 (2016)
DOI: 10.1093/mnras/stw2170
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OBSERVATIONAL CONSTRAINTS ON PLANET NINE:CASSINIRANGE OBSERVATIONS

Matthew J. Holman and Matthew J. Payne
The Astronomical Journal 152 (4) 94 (2016)
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NEW EXTREME TRANS-NEPTUNIAN OBJECTS: TOWARD A SUPER-EARTH IN THE OUTER SOLAR SYSTEM

Scott S. Sheppard and Chadwick Trujillo
The Astronomical Journal 152 (6) 221 (2016)
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THE HUNT FOR PLANET NINE: ATMOSPHERE, SPECTRA, EVOLUTION, AND DETECTABILITY

Jonathan J. Fortney, Mark S. Marley, Gregory Laughlin, et al.
The Astrophysical Journal 824 (2) L25 (2016)
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OBSERVATIONAL CONSTRAINTS ON PLANET NINE: ASTROMETRY OF PLUTO AND OTHER TRANS-NEPTUNIAN OBJECTS

Matthew J. Holman and Matthew J. Payne
The Astronomical Journal 152 (4) 80 (2016)
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CORRALLING A DISTANT PLANET WITH EXTREME RESONANT KUIPER BELT OBJECTS

Renu Malhotra, Kathryn Volk and Xianyu Wang
The Astrophysical Journal 824 (2) L22 (2016)
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COSMOLOGISTS IN SEARCH OF PLANET NINE: THE CASE FOR CMB EXPERIMENTS

Nicolas B. Cowan, Gil Holder and Nathan A. Kaib
The Astrophysical Journal 822 (1) L2 (2016)
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A new approach to distant solar system object detection in large survey data sets

V. Perdelwitz, M. Völschow and H. M. Müller
Astronomy & Astrophysics 615 A159 (2018)
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Orbital clustering of distant Kuiper belt objects by hypothetical Planet 9. Secular or resonant?

H. Beust
Astronomy & Astrophysics 590 L2 (2016)
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Towards an explanation of orbits in the extreme trans-Neptunian region: The effect of Milgromian dynamics

R. Paučo
Astronomy & Astrophysics 603 A11 (2017)
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Dynamical impact of the Planet Nine scenario:N-body experiments

Carlos de la Fuente Marcos, Raúl de la Fuente Marcos and Sverre J. Aarseth
Monthly Notices of the Royal Astronomical Society: Letters 460 (1) L123 (2016)
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Nemesis, Tyche, Planet Nine Hypotheses. I. Can We Detect the Bodies Using Gravitational Lensing?

J. P. Philippov and M. I. Chobanu
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CONSEQUENCES OF A DISTANT MASSIVE PLANET ON THE LARGE SEMIMAJOR AXIS TRANS-NEPTUNIAN OBJECTS

C. Shankman, J. J. Kavelaars, S. M. Lawler, B. J. Gladman and M. T. Bannister
The Astronomical Journal 153 (2) 63 (2017)
DOI: 10.3847/1538-3881/153/2/63
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OBSERVATIONAL CONSTRAINTS ON THE ORBIT AND LOCATION OF PLANET NINE IN THE OUTER SOLAR SYSTEM

Michael E. Brown and Konstantin Batygin
The Astrophysical Journal 824 (2) L23 (2016)
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Finding Planet Nine: a Monte Carlo approach

C. de la Fuente Marcos and R. de la Fuente Marcos
Monthly Notices of the Royal Astronomical Society: Letters 459 (1) L66 (2016)
DOI: 10.1093/mnrasl/slw049
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Some physical properties predicted for the putative Planet Nine of the solar system

I. Toth
Astronomy & Astrophysics 592 A86 (2016)
DOI: 10.1051/0004-6361/201628444
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THE INCLINATION OF THE PLANETARY SYSTEM RELATIVE TO THE SOLAR EQUATOR MAY BE EXPLAINED BY THE PRESENCE OF PLANET 9

Rodney Gomes, Rogerio Deienno and Alessandro Morbidelli
The Astronomical Journal 153 (1) 27 (2016)
DOI: 10.3847/1538-3881/153/1/27
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Improvement of the position of planet X based on the motion of nearly parabolic comets

Yu. D. Medvedev, D. E. Vavilov, Yu. S. Bondarenko, D. A. Bulekbaev and N. B. Kunturova
Astronomy Letters 43 (2) 120 (2017)
DOI: 10.1134/S1063773717020037
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