Jessica R. Lu
astro.berkeley.edu
0000-0001-9611-0009
University of California
242 papers found
Refreshing results…
AstroBetter: A Blog and Wiki for Professional Astronomers
Using LGS AO to Measure the Arches Mass Function
A sharper look at the motion of stars in the Arches with Keck-LGS adaptive optics
Clarifying our View of Star Formation in Massive Young Clusters with Adaptive Optics
Towards the Detection of General Relativity and Dark Matter with Stellar Orbits at the Galactic Center: Improving Reference Frame Stability
The Structure and Stellar Population of the Central 0.5 pc of the Milky Way Nuclear Star Cluster
Clarifying Our View of Milky Way Massive Young Star Clusters with Adaptive Optics
ERRATUM: “IMPROVING GALACTIC CENTER ASTROMETRY BY REDUCING THE EFFECTS OF GEOMETRIC DISTORTION” (2010, ApJ, 725, 331)
The Adaptive Optics Summer School Laboratory Activities
Improving Galactic Center Astrometry by Reducing the Effects of Geometric Distortion
Young and Old Stellar Populations in the Central Ten Parsecs of M31
The Infrared Imaging Spectrograph (IRIS) for TMT: the science case
Disks in the Arches Cluster—survival in a Starburst Environment
Clarifying our View of Massive Young Clusters in the Galactic Center and Galactic Disk with Adaptive Optics
DISCOVERY OF PRECURSOR LUMINOUS BLUE VARIABLE OUTBURSTS IN TWO RECENT OPTICAL TRANSIENTS: THE FITFULLY VARIABLE MISSING LINKS UGC 2773-Ot AND SN 2009ip
Discovery of Precursor LBV Outbursts in Two Recent Optical Transients: The Fitfully Variable Missing Links UGC 2773-OT AND SN 2009ip
Testing stellar cusp formation theories with observations of the Milky Way nuclear star cluster
Pushing Orbital Parameter Estimates of the Young Stars at the Galactic Center to Larger Radii by Improving Models of Systematic Errors
Recent results and perspectives for precision astrometry and photometry with adaptive optics
Relative Astrometry with Ground-Based Adaptive Optics Imaging
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