Arecibo-related presentations at AAS 209

* (017.24) Hydrogen-Dating Molecular Clouds
* (025.04) Correlating Arecibo Radar and IRTF Near-Infrared Spectral Observations of 105 Artemis
* (029.14) Fast-Drifting Radio Bursts Seen on the Flare Star AD Leo with the Arecibo Observatory
* (053.01) Discovery of Faint Radio Structures over 50 Square Degrees Down to 3 arcmin Scales near the NGP
* (075.02) The Arecibo Remote Command Center: Involving Students in Major Astronomical Research
* (078.10) Arecibo Observatory and the National Virtual Observatory
* (084.10) OH Study of the Massive Star-Forming Region IRAS 19111+1048
* (091.01) Measurement of Orbital Decay in the Double Neutron Star Binary PSR B2127+11C
* (094.12) Arecibo Observatory for All
* (095.01) The Arecibo Legacy Fast ALFA Survey: HI Sources in the Northern Virgo Cluster Region
* (095.02) The Arecibo Legacy Fast ALFA HI Survey: The Rich Galaxy Group Zwicky 1400+0949
* (095.03) A Neutral Hydrogen Survey of the NGC 7332 Region with the Arecibo L-band Feed Array
* (095.04) The ALFA Zone of Avoidance Survey: Results from the Precursor Observations
* (097.06) Arecibo Survey of HI Emission from Disk Galaxies at Intermediate Redshift
* (101.01) The dM/dt of O-rich OH/IR Stars is Strongly Modulated
* (104.02) Radio Emission Signatures of the Crab Pulsar's High Frequency Interpulse
* (115.06) Big, Smart Dishes to Find Thousands of New Radio Pulsars
* (131.07) Pulsar Timing and Gravitational Wave Detection: Current Status and Future Prospects
* (159.02) New Pulsars in the Globular Cluster M28
* (159.03) Discovery and Timing of Eight New Millisecond Pulsars in NGC 6440 and NGC 6441
* (159.09) Updated Timing Parameters of two Massive Binary Pulsars: J0621+1002 and J0751+1807
* (172.19) An Arecibo HI 21-cm Absorption Survey of X-ray Rich Clusters
* (198.06) The Discovery of Extragalactic Magnetic Fields in OH Megamasers
* (211.03) The Angular Momentum of Disk Galaxies: A Multi-Wavelength Study Using the Virtual Observatory
* (217.05) A Radio Spectral Line Study of the 2-Jy IRAS-NVSS Sample