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NASA Exoplanet Science Institute (NExScI)

Known as: NExScI 
The NASA Exoplanet Science Institute (NExScI) is part of the Infrared Processing and Analysis Center (IPAC) and is on the campus of the California… 
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NASA Exoplanet Archive

Papers overview

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Highly Cited
2017
Highly Cited
2017
Discovery of Water at High Spectral Resolution in the Atmosphere of 51 Peg b
We report the detection of water absorption features in the day side spectrum of the first-known hot Jupiter, 51 Peg b… 
Highly Cited
2016
Highly Cited
2016
A CANDIDATE YOUNG MASSIVE PLANET IN ORBIT AROUND THE CLASSICAL T TAURI STAR CI TAU
The ∼2 Myr old classical T Tauri star CI Tau shows periodic variability in its radial velocity (RV) variations measured at… 
2016
2016
KIC 3749404: a heartbeat star with rapid apsidal advance indicative of a tertiary component
Heartbeat stars are eccentric (e> 0.2) ellipsoidal variables whose light curves resemble a cardiogram. We present the… 
Review
2015
Review
2015
CRITERIA FOR SAMPLE SELECTION TO MAXIMIZE PLANET SENSITIVITY AND YIELD FROM SPACE-BASED MICROLENS PARALLAX SURVEYS
Space-based microlens parallax measurements are a powerful tool for understanding planet populations, especially their… 
2015
2015
CHARACTERIZATION OF THE K2-19 MULTIPLE-TRANSITING PLANETARY SYSTEM VIA HIGH-DISPERSION SPECTROSCOPY, AO IMAGING, AND TRANSIT TIMING VARIATIONS
K2-19 (EPIC201505350) is an interesting planetary system in which two transiting planets with radii ∼7 R⊕ (inner planet b) and ∼4… 
Highly Cited
2014
Highly Cited
2014
FIRST SPACE-BASED MICROLENS PARALLAX MEASUREMENT OF AN ISOLATED STAR: SPITZER OBSERVATIONS OF OGLE-2014-BLG-0939
We present the first space-based microlens parallax measurement of an isolated star. From the striking differences in the… 
Highly Cited
2014
Highly Cited
2014
SPITZER AS A MICROLENS PARALLAX SATELLITE: MASS MEASUREMENT FOR THE OGLE-2014-BLG-0124L PLANET AND ITS HOST STAR
We combine Spitzer and ground-based observations to measure the microlens parallax vector , and thus the mass and distance of… 
Review
2012
Review
2012
A T8.5 BROWN DWARF MEMBER OF THE ξ URSAE MAJORIS SYSTEM
The Wide-field Infrared Survey Explorer has revealed a T8.5 brown dwarf (WISE J111838.70+312537.9) that exhibits common proper… 
Review
2010
Review
2010
The NASA Exoplanet Science Institute Archives: KOA and NStED
The NASA Exoplanet Science Institute (NExScI) maintains a series of archival services in support of NASA’s planet finding and… 
Highly Cited
1996
Highly Cited
1996
Constraints on Stellar Grain Formation from Presolar Graphite in the Murchison Meteorite
We report the results of isotopic, chemical, structural, and crystallographic microanalyses of graphitic spherules (0.3-9 μm… 
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