Publications by Year: 2017

Lund MB, Rodriguez JE, Zhou G, Gaudi BS, Stassun KG, Johnson MC, Bieryla A, Oelkers RJ, Stevens DJ, Collins KA, et al. KELT-20b: A Giant Planet with a Period of P ̃ 3.5 days Transiting the V ̃ 7.6 Early A Star HD 185603. \aj. 2017;154 (5) :194.
Giles HA C, Collier Cameron A, Haywood RD. A Kepler study of starspot lifetimes with respect to light-curve amplitude and spectral type. \mnras. 2017;472 (2) :1618-1627.
Moschou S-P, Drake JJ, Cohen O, Alvarado-Gomez JD, Garraffo C. A Monster CME Obscuring a Demon Star Flare. \apj. 2017;850 (2) :191.
Bouchy F, Doyon R, Artigau É, Melo C, Hernandez O, Wildi F, Delfosse X, Lovis C, Figueira P, Canto Martins B L, et al. Near-InfraRed Planet Searcher to Join HARPS on the ESO 3.6-metre Telescope. The Messenger. 2017;169 :21-27.
Dupree A K, Dotter A, Johnson C I, Marino A F, Milone A P, Bailey, J. I. III, Crane J D, Mateo M, Olszewski E W. NGC 1866: First Spectroscopic Detection of Fast-rotating Stars in a Young LMC Cluster. \apjl. 2017;846 (1) :L1.
Kenyon SJ, Bromley BC. Numerical Simulations of Gaseous Disks Generated from Collisional Cascades at the Roche Limits of White Dwarf Stars. \apj. 2017;850 (1) :50.
Morley CV, Kreidberg L, Rustamkulov Z, Robinson T, Fortney JJ. Observing the Atmospheres of Known Temperate Earth-sized Planets with JWST. \apj. 2017;850 (2) :121.
Shin I-G, Udalski A, Yee J C, Calchi Novati S, Han C, Skowron J, Mróz P, Soszyński I, Poleski R, Szymański M K, et al. OGLE-2016-BLG-0168 Binary Microlensing Event: Prediction and Confirmation of the Microlens Parallax Effect from Space-based Observations. \aj. 2017;154 (5) :176.
Han C, Udalski A, Gould A, Bond I A, and, Albrow M D, Chung S-J, Jung Y K, Ryu Y-H, Shin I-G, et al. OGLE-2016-BLG-0263Lb: Microlensing Detection of a Very Low-mass Binary Companion through a Repeating Event Channel. \aj. 2017;154 (4) :133.
Han C, Udalski A, Gould A, Lee C-U, Shvartzvald Y, Zang W C, Mao S, Kozłowski S, Albrow M D, Chung S-J, et al. OGLE-2016-BLG-0613LABb: A Microlensing Planet in a Binary System. \aj. 2017;154 (6) :223.
Ryu Y-H, Udalski A, Yee J C, Albrow M D, Chung S-J, Gould A, Han C, Hwang K-H, Jung Y K, Shin I-G, et al. OGLE-2016-BLG-0693LB: Probing the Brown Dwarf Desert with Microlensing. \aj. 2017;154 (6) :247.
Le Gal R, Xie C, Herbst E, Talbi D, Guo H, Muller S. The ortho-to-para ratio of H₂Cl$^+$: Quasi-classical trajectory calculations and new simulations in light of new observations. \aap. 2017;608 :A96.
Alam M, Abramczyk J, Manyam U, Farroni J, Guertin D. Performance of optical fibers in space radiation environment, in \procspie. Vol 10567. ; 2017 :105672M.
Sirorattanakul K, Engle S, Pepper J, Wells M, Laney CD, Rodriguez JE, Stassun KG. Period Variations for the Cepheid VZ Cyg. \aj. 2017;154 (6) :217.
Osborn H P, Rodriguez J E, Kenworthy M A, Kennedy G M, Mamajek E E, Robinson C E, Espaillat C C, Armstrong D J, Shappee B J, Bieryla A, et al. Periodic eclipses of the young star PDS 110 discovered with WASP and KELT photometry. \mnras. 2017;471 (1) :740-749.
Vanderburg A, Becker JC, Buchhave LA, Mortier A, Lopez E, Malavolta L, Haywood RD, Latham DW, Charbonneau D, López-Morales M, et al. Precise Masses in the WASP-47 System. \aj. 2017;154 (6) :237.
Louden T, Wheatley PJ, Irwin PG J, Kirk J, Skillen I. A precise optical transmission spectrum of the inflated exoplanet WASP-52b. \mnras. 2017;470 (1) :742-754.
Fayolle EC, Öberg KI, Jørgensen JK, Altwegg K, Calcutt H, Müller HS P, Rubin M, van der Wiel MH D, Bjerkeli P, Bourke TL, et al. Protostellar and cometary detections of organohalogens. Nature Astronomy. 2017;1 :703-708.
Chapman JW, Zellem RT, Line MR, Vasisht G, Bryden G, Willacy K, Iyer AR, Bean J, Cowan NB, Fortney JJ, et al. Quantifying the Impact of Spectral Coverage on the Retrieval of Molecular Abundances from Exoplanet Transmission Spectra. \pasp. 2017;129 (980) :104402.
Dittmann JA, Irwin JM, Charbonneau D, Berta-Thompson ZK, Newton ER. A Search for Additional Bodies in the GJ 1132 Planetary System from 21 Ground-based Transits and a 100-hr Spitzer Campaign. \aj. 2017;154 (4) :142.