Search Publications

Ultra-short-period Planets in K2 with Companions: A Double Transiting System for EPIC 220674823
DOI: 10.3847/1538-3881/153/2/82 Bibcode: 2017AJ....153...82A

Baranec, Christoph; Cochran, William D.; Duev, Dmitry A. +10 more

Two transiting planets have been identified orbiting K2 target EPIC 220674823. One object is an ultra-short-period planet (USP) with a period of just 0.57 days (13.7 hr), while the other has a period of 13.3 days. Both planets are small, with the former having a radius of {R}{{p}1}=1.5 {R}\oplus and the latter {R}{{p

2017 The Astronomical Journal
Gaia 30
Near-IR Transmission Spectrum of HAT-P-32b using HST/WFC3
DOI: 10.3847/1538-3881/aa738b Bibcode: 2017AJ....154...39D

Tsiaras, A.; Morello, G.; Damiano, M. +2 more

We report here the analysis of the near-infrared transit spectrum of the hot Jupiter HAT-P-32b, which was recorded with the Wide Field Camera 3 (WFC3) on board the Hubble Space Telescope. HAT-P-32b is one of the most inflated exoplanets discovered, making it an excellent candidate for transit spectroscopic measurements. To obtain the transit spect…

2017 The Astronomical Journal
eHST 28
A Survey for Planetary-mass Brown Dwarfs in the Chamaeleon I Star-forming Region
DOI: 10.3847/1538-3881/aa74e2 Bibcode: 2017AJ....154...46E

Luhman, K. L.; Faherty, J. K.; Esplin, T. L. +2 more

We have performed a search for planetary-mass brown dwarfs in the Chamaeleon I star-forming region using proper motions and photometry measured from optical and infrared images from the Spitzer Space Telescope, the Hubble Space Telescope, and ground-based facilities. Through near-IR spectroscopy at Gemini Observatory, we have confirmed six of the …

2017 The Astronomical Journal
Gaia eHST 28
Simultaneous Mass Determination for Gravitationally Coupled Asteroids
DOI: 10.3847/1538-3881/aa7de8 Bibcode: 2017AJ....154...76B

Chesley, Steven R.; Baer, James

The conventional least-squares asteroid mass determination algorithm allows us to solve for the mass of a large subject asteroid that is perturbing the trajectory of a smaller test asteroid. However, this algorithm is necessarily a first approximation, ignoring the possibility that the subject asteroid may itself be perturbed by the test asteroid,…

2017 The Astronomical Journal
Gaia 28
Improved Point-source Detection in Crowded Fields Using Probabilistic Cataloging
DOI: 10.3847/1538-3881/aa8565 Bibcode: 2017AJ....154..132P

Finkbeiner, Douglas P.; Daylan, Tansu; Portillo, Stephen K. N. +1 more

Cataloging is challenging in crowded fields because sources are extremely covariant with their neighbors and blending makes even the number of sources ambiguous. We present the first optical probabilistic catalog, cataloging a crowded (∼0.1 sources per pixel brighter than 22nd mag in F606W) Sloan Digital Sky Survey r-band image from M2. Probabilis…

2017 The Astronomical Journal
eHST 28
Infrared Photometric Properties of 709 Candidate Stellar Bowshock Nebulae
DOI: 10.3847/1538-3881/aa90ba Bibcode: 2017AJ....154..201K

Kobulnicky, Henry A.; Dixon, Don M.; Schurhammer, Danielle P. +4 more

Arcuate infrared nebulae are ubiquitous throughout the Galactic Plane and are candidates for partial shells, bubbles, or bowshocks produced by massive runaway stars. We tabulate infrared photometry for 709 such objects using images from the Spitzer Space Telescope, the Wide-field Infrared Explorer, and the Herschel Space Observatory (HSO). Of the …

2017 The Astronomical Journal
Herschel 28
Scattering Properties of the Venusian Clouds Observed by the UV Imager on board Akatsuki
DOI: 10.3847/1538-3881/aa78a5 Bibcode: 2017AJ....154...44L

Yamada, M.; Imamura, T.; Murakami, S. +6 more

We analyze the albedo of Venus obtained from the UV Imager on board Akatsuki. A relative global mean albedo over phase angle is used in this study, and we confirm the glory feature at 283 and 365 nm in the data acquired in 2016 May. We successfully simulate the observation using a radiative transfer model. Our results show that cloud aerosols of {…

2017 The Astronomical Journal
VenusExpress 27
Plasma Environment around Comet 67P/Churyumov-Gerasimenko at Perihelion: Model Comparison with Rosetta Data
DOI: 10.3847/1538-3881/153/1/30 Bibcode: 2017AJ....153...30M

Altwegg, K.; Goetz, C.; Goldstein, R. +6 more

The plasma environment near comet 67P/Churyumov-Gerasimenko (67P/CG) is dynamically affected by various factors, including the incident solar wind and outgassing from the nucleus. The Rosetta spacecraft MAGnetometer (MAG) instrument observations near perihelion showed crossing events into a magnetic field-free region at about 170 km from the nucle…

2017 The Astronomical Journal
Rosetta 24
Revision of Stellar Intrinsic Colors in the Infrared by Spectroscopic Surveys
DOI: 10.3847/1538-3881/153/1/5 Bibcode: 2017AJ....153....5J

Jiang, Biwei; Zhao, He; Gao, Shuang +1 more

Intrinsic colors of normal stars are derived in the popularly used infrared bands involving the Two Micron All-Sky Survey/JHKS, Wide-field Infrared Survey Explorer, Spitzer/IRAC, and AKARI/S9W filters. Based on three spectroscopic surveys—LAMOST, RAVE, and APOGEE, stars are classified into groups of giants and dwarfs, as well as metal-n…

2017 The Astronomical Journal
AKARI 24
Optimized Trajectories to the Nearest Stars Using Lightweight High-velocity Photon Sails
DOI: 10.3847/1538-3881/aa813f Bibcode: 2017AJ....154..115H

Heller, René; Hippke, Michael; Kervella, Pierre

New means of interstellar travel are now being considered by various research teams, assuming lightweight spaceships to be accelerated via either laser or solar radiation to a significant fraction of the speed of light (c). We recently showed that gravitational assists can be combined with the stellar photon pressure to decelerate an incoming ligh…

2017 The Astronomical Journal
Gaia 24