Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- D. Stern3 profiles493 · h 97
- F. Harrison2 profiles182 · h 58
- P. Eisenhardt3 profiles168 · h 59
- S. Boggs124 · h 60
- F. Christensen123 · h 58
- C. Hailey120 · h 59
- W. Craig2 profiles120 · h 49
- S. Stanford2 profiles117 · h 75
- S. Turyshev116 · h 38
- D. Walton2 profiles108 · h 53
- K. Stapelfeldt104 · h 70
- D. Mawet98 · h 53
- California Institute of TechnologyUS4.7k papers
- Centre National de la Recherche ScientifiqueFR2k papers
- Center for Astrophysics Harvard & SmithsonianUS1.3k papers
- Goddard Space Flight CenterUS1.2k papers
- University of California, BerkeleyUS1.2k papers
- University of ArizonaUS1k papers
- Infrared Processing and Analysis CenterUS1k papers
- University College LondonGB984 papers
- Princeton UniversityUS925 papers
- University of CambridgeGB871 papers
- Institut d'Astrophysique de ParisFR858 papers
- Space Telescope Science InstituteUS808 papers
48 papers · 2 filters
Near Earth Asteroids with measurable Yarkovsky effect
D. Farnocchia, S. R. Chesley, D. Vokrouhlicky +2
We seek evidence of the Yarkovsky effect among Near Earth Asteroids (NEAs) by measuring the Yarkovsky-related orbital drift from the orbital fit. To prevent the occurrence of unrel…
On The Relative Sizes of Planets Within Kepler Multiple Candidate Systems
David R. Ciardi, Daniel C. Fabrycky, Eric B. Ford +5
We present a study of the relative sizes of planets within the multiple candidate systems discovered with the mission. We have compared the size of each planet to the size…
Ground-based near-infrared observations of water vapour in the Venus troposphere
S. Chamberlain, J. A. Bailey, D. Crisp +1
We present a study of water vapour in the Venus troposphere obtained by modelling specific water vapour absorption bands within the 1.18 μm window. We compare the results with the…
A DEBRIS Disk Around The Planet Hosting M-star GJ581 Spatially Resolved with Herschel
J. -F. Lestrade, B. C. Matthews, B. Sibthorpe +17
Debris disks have been found primarily around intermediate and solar mass stars (spectral types A-K) but rarely around low mass M-type stars. We have spatially resolved a debris di…
A Search for Giant Planet Companions to T Tauri Stars
Christopher J. Crockett, Naved I. Mahmud, L. Prato +4
We present results from an ongoing multiwavelength radial velocity (RV) survey of the Taurus-Auriga star forming region as part of our effort to identify pre--main sequence giant p…
Looking for a Pulse: A search for Rotationally Modulated Radio Emission from the Hot Jupiter, Tau Bootis b
G. Hallinan, S. K. Sirothia, A. Antonova +5
Hot Jupiters have been proposed as a likely population of low frequency radio sources due to electron cyclotron maser emission of similar nature to that detected from the auroral r…
The Structure of Pre-transitional Protoplanetary Disks I: Radiative Transfer Modeling of the Disk+Cavity in the PDS 70 system
Ruobing Dong, Jun Hashimoto, Roman Rafikov +49
Through detailed radiative transfer modeling, we present a disk+cavity model to simultaneously explain both the SED and Subaru H-band polarized light imaging for the pre-transition…
Bodily tides near the 1:1 spin-orbit resonance. Correction to Goldreich's dynamical model
James G. Williams, Michael Efroimsky
Spin-orbit coupling is often described in the "MacDonald torque" approach which has become the textbook standard. Within this method, a concise expression for the additional tidal…
Physical Parameters of Asteroids Estimated from the WISE 3 Band Data and NEOWISE Post-Cryogenic Survey
A. Mainzer, T. Grav, J. Masiero +7
Enhancements to the science data processing pipeline of NASA's Wide-field Infrared Explorer (WISE) mission, collectively known as NEOWISE, resulted in the detection of 158,000 m…
Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-Cryogenic Observations of Main Belt Asteroids
Joseph R. Masiero, A. K. Mainzer, T. Grav +4
We present preliminary diameters and albedos for 13511 MBAs that were observed during the 3-Band Cryo phase of the WISE survey (after the outer cryogen tank was exhausted) and as p…
Characterization of Active Main Belt Object P/2012 F5 (Gibbs): A Possible Impacted Asteroid
R. Stevenson, E. A. Kramer, J. M. Bauer +2
In this work we characterize the recently discovered active main belt object P/2012 F5 (Gibbs), which was discovered with a dust trail > 7' in length in the outer main belt, 7 mont…
A Common Proper Motion Stellar Companion to HAT-P-7
Norio Narita, Yasuhiro H. Takahashi, Masayuki Kuzuhara +51
We report that HAT-P-7 has a common proper motion stellar companion. The companion is located at arcsec to the east and estimated as an M5.5V dwarf based on its colors. W…
Regolith grain sizes of Saturn's rings inferred from Cassini-CIRS far-infrared spectra
Ryuji Morishima, Scott G. Edgington, Linda Spilker
We analyze far-infrared (10-650 cm) emissivity spectra of Saturn's main rings obtained by the Cassini Composite Infrared Spectrometer (CIRS). In modeling of the spectra, the…
A multilayer model for thermal infrared emission of Saturn's rings. III: Thermal inertia inferred from Cassini CIRS
Ryuji Morishima, Linda Spilker, Keiji Ohtsuki
The thermal inertia values of Saturn's main rings (the A, B, and C rings and the Cassini division) are derived by applying our thermal model to azimuthally scanned spectra taken by…
WISE/NEOWISE Preliminary Analysis and Highlights of the 67P/Churyumov-Gerasimenko Near Nucleus Environs
James M. Bauer, Emily Kramer, A. K. Mainzer +15
On January 18-19 and June 28-29 of 2010, the Wide-field Infrared Survey Explorer (WISE) spacecraft imaged the Rosetta mission target, comet 67P/Churyumov-Gerasimenko. We present a…
Near-Nucleus Photometry of Outbursting Comet 17P/Holmes
Rachel Stevenson, David Jewitt
Comet 17P/Holmes underwent the largest cometary outburst in recorded history on UT 2007 Oct. 23, releasing massive quantities of dust and gas. We used the Canada-France-Hawaii tele…
WISE/NEOWISE Observations of the Jovian Trojan Population: Taxonomy
Tommy Grav, Amy K. Mainzer, James M. Bauer +2
We present updated/new thermal model fits for 478 Jovian Trojan asteroids observed with the Wide-field Infrared Survey Explorer (WISE). Using the fact that the two shortest bands u…
Revising the age for the Baptistina asteroid family using WISE/NEOWISE data
Joseph R. Masiero, A. K. Mainzer, T. Grav +2
We have used numerical routines to model the evolution of a simulated Baptistina family to constrain its age in light of new measurements of the diameters and albedos of family mem…
Composition of Near-Earth Asteroid 2008 EV5: Potential target for Robotic and Human Exploration
Vishnu Reddy, Lucille Le Corre, Michael Hicks +5
We observed potentially hazardous asteroid (PHA) 2008 EV5 in the visible (0.30-0.92 microns) and near-IR (0.75-2.5 microns) wavelengths to determine its surface composition. This a…
Planetesimal Compositions in Exoplanet Systems
Torrence V. Johnson, Olivier Mousis, Jonathan I. Lunine +1
We have used recent surveys of the composition of exoplanet host stars to investigate the expected composition of condensed material in planetesimals formed beyond the snow line in…
Direct imaging of extra-solar planets in star forming regions: Lessons learned from a false positive around IM Lup
Dimitri Mawet, Olivier Absil, Guillaume Montagnier +8
Most exoplanet imagers consist of ground-based adaptive optics coronagraphic cameras which are currently limited in contrast, sensitivity and astrometric precision, but advantageou…
Precision Near Infrared Photometry For Exoplanet Transit Observations - I : Ensemble Spot Photometry for An All-Sky Survey
C. Clanton, C. Beichman, G. Vasisht +2
Near-IR observations are important for the detection and characterization of exoplanets using the transit technique, either in surveys of large numbers of stars or for follow-up sp…
The Yarkovsky Drift's Influence on NEAs: Trends and Predictions with NEOWISE Measurements
C. R. Nugent, A. Mainzer, J. Masiero +2
We used WISE-derived geometric albedos (p_V) and diameters, as well as geometric albedos and diameters from the literature, to produce more accurate diurnal Yarkovsky drift predict…
Herschel imaging of 61 Vir: implications for the prevalence of debris in low-mass planetary systems
M. C. Wyatt, G. Kennedy, B. Sibthorpe +15
This paper describes Herschel observations of the nearby (8.5pc) G5V multi-exoplanet host star 61 Vir at 70-500micron carried out by the DEBRIS survey. These reveal emission that i…