alphaFeedback
FM

Fergal Mullally

astro-ph.EPastro-ph.SRastro-phastro-ph.IMastro-ph.GAastro-ph.HEcatalogsplanetary systemsPlanetsplanets and satellites: detection

On Valency

published · living versions
W_wsmk4geh·v1 · currentpublished
ExoVetter and a TESS Exoplanet Transit Search of Kepler Stars as Ground Truth
with Matthew M. Dallas, Susan E. Mullally, Michelle Kunimoto, Te Han +1
1 version

Preprints & journals

63 papers in the corpus · 2005–2026
ExoVetter and a TESS Exoplanet Transit Search of Kepler Stars as Ground Truth2610.32949v1 · Matthew M. Dallas, Susan E. Mullally, Fergal Mullally et al.2026 · 0 citationsPublications of the Astronomical Society of the Pacific, 2026, Volume 138, Issue 10, id.104504, 13 ppon Valency
Follow-up Observations of Candidate White Dwarf Planets with MIRI2512.08191v1 · Fergal Mullally, Susan E. Mullally, Misty Cracraft et al.2025 · 1 citationarXiv
Composition of planetary debris around the white dwarf GD 3622510.07595v1 · William T. Reach, Mukremin Kilic, Carey M. Lisse et al.2025 · 4 citationsarXiv
Metal Polluted White Dwarfs with 21 {\mu}m IR excesses from JWST/MIRI: Planets or Dust?2506.21224v1 · John H. Debes, Sabrina Poulsen, Ashley Messier et al.2025 · 5 citationsarXiv
JWST Directly Images Giant Planet Candidates Around Two Metal-Polluted White Dwarf Stars2401.13153v1 · Susan E. Mullally, John Debes, Misty Cracraft et al.2024 · 38 citationsarXiv
A MIRI Search for Planets and Dust Around WD 2149+022311.14165v1 · Sabrina Poulsen, John Debes, Misty Cracraft et al.2023 · 0 citationsarXiv
Kepler K2 Campaign 9: II. First space-based discovery of an exoplanet using microlensing2203.16959v2 · D. Specht, R. Poleski, M. T. Penny et al.2022 · 5 citationsarXiv
The Occurrence of Rocky Habitable Zone Planets Around Solar-Like Stars from Kepler Data2010.14812v2 · Steve Bryson, Michelle Kunimoto, Ravi K. Kopparapu et al.2020 · 183 citationsarXivon Valency
The pulsating white dwarf G117-B15A: still the most stable optical clock known2010.16062v2 · S.O. Kepler, D.E. Winget, Zachary P. Vanderbosch et al.2020 · 23 citationsarXiv
The First Habitable Zone Earth-sized Planet from TESS. I: Validation of the TOI-700 System2001.00952v2 · Emily A. Gilbert, Thomas Barclay, Joshua E. Schlieder et al.2020 · 107 citationsarXiv
The L 98-59 System: Three Transiting, Terrestrial-Sized Planets Orbiting a Nearby M-dwarf1903.08017v2 · Veselin B. Kostov, Joshua E. Schlieder, Thomas Barclay et al.2019 · 135 citationsarXiv
Discovery and Vetting of Exoplanets I: Benchmarking K2 Vetting Tools1901.07459v1 · Veselin B. Kostov, Susan E. Mullally, Elisa V. Quintana et al.2019 · 61 citationsarXiv
Re-Evaluating Small Long-Period Confirmed Planets From Kepler1901.00506v1 · Christopher J. Burke, F. Mullally, Susan E. Thompson et al.2019 · 24 citationsarXiv
PLANETARY CANDIDATES OBSERVED BY Kepler. VIII. A FULLY AUTOMATED CATALOG WITH MEASURED COMPLETENESS AND RELIABILITY BASED ON DATA RELEASE 25.32908325 · Thompson, Susan E, Coughlin, Jeffrey L, Hoffman, Kelsey et al.2023 · 431 citationsThe Astrophysical journal. Supplement series. 2018;235(2)
Kepler's Earth-like Planets Should Not Be Confirmed Without Independent Detection: The Case of Kepler-452b1803.11307v1 · Fergal Mullally, Susan E. Thompson, Jeffery L. Coughlin et al.2018 · 29 citationsarXiv
Periodic optical variability and debris accretion in white dwarfs: a test for a causal connection1711.10488v2 · Na'ama Hallakoun, Dan Maoz, Eric Agol et al.2017 · 11 citationsarXiv
The Pseudosynchronization of Binary Stars Undergoing Strong Tidal Interactions1706.05434v1 · Mara Zimmerman, Susan Thompson, Fergal Mullally et al.2017 · 25 citationsarXiv
Three's Company: An additional non-transiting super-Earth in the bright HD 3167 system, and masses for all three planets1706.01892v1 · Jessie L. Christiansen, Andrew Vanderburg, Jennifer Burt et al.2017 · 84 citationsarXiv
Identifying False Alarms in the Kepler Planet Candidate Catalog1602.03204v1 · F. Mullally, Jeffery L. Coughlin, Susan E. Thompson et al.2016 · 38 citationsarXiv
A Machine Learning Technique to Identify Transit Shaped Signals1509.00041v1 · Susan E. Thompson, Fergal Mullally, Jeff Coughlin et al.2015 · 65 citationsarXiv
SDSS J1152+0248: An eclipsing double white dwarf from the Kepler K2 campaign1507.06311v2 · N. Hallakoun, D. Maoz, M. Kilic et al.2015 · 42 citationsarXiv
Terrestrial Planet Occurrence Rates for the Kepler GK Dwarf Sample1506.04175v1 · Christopher J. Burke, Jessie L. Christiansen, F. Mullally et al.2015 · 360 citationsarXivon Valency
A double white dwarf with a paradoxical origin?1505.05144v1 · M.C.P. Bours, T.R. Marsh, B.T. Gaensicke et al.2015 · 25 citationsarXiv
Planetary Candidates Observed by Kepler VI: Planet Sample from Q1-Q16 (47 Months)1502.02038v1 · F. Mullally, Jeffrey L. Coughlin, Susan E. Thompson et al.2015 · 253 citationsarXiv
Planetary Candidates Observed by Kepler V: Planet Sample from Q1-Q12 (36 Months)1501.07286v2 · Jason F. Rowe, Jeffrey L. Coughlin, Victoria Antoci et al.2015 · 180 citationsarXiv
The K2 Mission: Characterization and Early results1402.5163v2 · Steve B. Howell, Charlie Sobeck, Michael Haas et al.2014 · 1,702 citationsarXiv
Masses, Radii, and Orbits of Small Kepler Planets: The Transition from Gaseous to Rocky Planets1401.4195v1 · Geoffrey W. Marcy, Howard Isaacson, Andrew W. Howard et al.2014 · 489 citationsGeoffrey W. Marcy et al. 2014 ApJS 210 20on Valency
Contamination in the Kepler Field. Identification of 685 KOIs as False Positives Via Ephemeris Matching Based On Q1-Q12 Data1401.1240v2 · Jeffrey L. Coughlin, Susan E. Thompson, Stephen T. Bryson et al.2014 · 127 citationsarXiv
Planetary Candidates Observed by Kepler IV: Planet Sample From Q1-Q8 (22 Months)1312.5358v1 · Christopher J. Burke, Stephen T. Bryson, F. Mullally et al.2013 · 228 citationsarXiv
Kepler-62: a five-planet system with planets of 1.4 and 1.6 Earth radii in the habitable zone.23599262 · Borucki, William J, Agol, Eric, Fressin, Francois et al.2013 · 250 citationsScience (New York, N.Y.). 2013;340(6132):587-90
A super-Earth-sized planet orbiting in or near the habitable zone around Sun-like star1304.4941v1 · Thomas Barclay, Christopher J. Burke, Steve B. Howell et al.2013 · 76 citationsarXiv
A sub-Mercury-sized exoplanet.23426260 · Barclay, Thomas, Rowe, Jason F, Lissauer, Jack J et al.2013 · 216 citationsNature. 2013;494(7438):452-4
Fundamental Properties of Kepler Planet-Candidate Host Stars using Asteroseismology1302.2624v2 · Daniel Huber, William J. Chaplin, J\orgen Christensen-Dalsgaard et al.2013 · 329 citationsarXiv
A New Timescale for Period Change in the Pulsating DA White Dwarf WD 0111+00181302.1875v1 · J. J. Hermes, M. H. Montgomery, Fergal Mullally et al.2013 · 25 citationsarXiv
SDSS 1355+0856: A detached white dwarf + M star binary in the period gap discovered by the SWARMS survey1210.6532v1 · Carles Badenes, Marten H. van Kerkwijk, Mukremin Kilic et al.2012 · 9 citationsarXiv
Photometrically derived masses and radii of the planet and star in the TrES-2 system1210.4592v2 · Thomas Barclay, Daniel Huber, Jason F. Rowe et al.2012 · 104 citationsarXivon Valency
Alignment of the stellar spin with the orbits of a three-planet system.22836999 · Sanchis-Ojeda, Roberto, Fabrycky, Daniel C, Winn, Joshua N et al.2012 · 222 citationsNature. 2012;487(7408):449-53
Three ways to solve the orbit of KIC11558725: a 10 day beaming sdB+WD binary with a pulsating subdwarf1206.3872v1 · J. H. Telting, R. H. \Ostensen, A. S. Baran et al.2012 · 68 citationsarXiv
Planetary Candidates Observed by Kepler, III: Analysis of the First 16 Months of Data1202.5852v1 · Natalie M. Batalha, Jason F. Rowe, Stephen T. Bryson et al.2012 · 1,042 citationsarXivon Valency
Seismic evidence for non-synchronization in two close sdB+dM binaries from Kepler photometry1202.3649v1 · Herbert Pablo, Steven D. Kawaler, M. D. Reed et al.2012 · 57 citationsarXiv
Two Earth-sized planets orbiting Kepler-20.22186831 · Fressin, Francois, Torres, Guillermo, Rowe, Jason F et al.2012 · 183 citationsNature. 2011;482(7384):195-8
Career total: 164 works. 63 are in this corpus.Showing the 50 most recent.

Profile built from the corpus for this byline.

Author records are still filling in while the Hub is in alpha. If this is your page, you'll be able to claim it soon. Spot a mistake? Tell us.