| Year |
Name |
School |
Project |
|
2007 |
|
Troy
High School, Troy, Michigan
|
Period
Analysis of Cataclysmic Variable X10 and Its Implications on
the Origin of Low States |
| Emily
Brook Petroff, 16 |
Oregon
Episcopal School, Portland, Oregon |
Variation
in Star Formation Rate from Galaxy Cluster Center for cl1037 |
| 2006 |
|
Taipei
First Girl High School
|
Magic
Mirror for Galaxy Clusters |
| Philip
Mocz, 16 |
Mililani
High School, Mililani, HI |
Group
Analysis to Pattern Discovery in Stellar and Galactic Distributions |
| 2005 |
Gabrielle
Alyce Gianelli, 17
|
Lake
Highland Preparatory School, Orlando, FL
|
Fractal
Dimension Analysis of Putative Martian Coastlines |
| Anand
M. Palaniappan, 17 |
David
H. Hickman High School, Columbia, MO |
A
New Algorithm for Multiple Hypothesis-based Tracking and Discovery
of Potentially Hazardous Near Earth Objects |
| 2004 |
|
Hempfield
High School, Landisville, PA
|
Relationship
Between Sunspots and Solar Flares |
| Julie
Ann Krugler, 18 |
Grosse
Pointe North High School, Grosse Pointe, MI |
In
Pursuit of Population III |
| |
|
New
Milford High School, New Milford, Connecticut
|
A
Rapid, Accurate Method of Determining the Distance to Near-Earth
Asteroids |
| Jonathan
Nicholas Sick |
Queen
Elizbeth High School, Calgary, Alberta |
Development
of an Adaptively Controlled Telescope |
| |
Matthew
Douglas Apau Jachowski, 16
|
Maui
High School, Kahului, Hawaii
|
Effect
of Observation Timing on Initial Orbit Determination Accuracy |
| Harish
Gautam Khandrika, 14 |
La
Jolla High School, La Jolla, California |
Evidence
for Decay of 44Titanium to 44Calcium in Supernova Remnant Cassiopeia
A. |
| 2001 |
|
School
Without Walls, Washington, District of Columbia
|
The
Optical Divide |
Michael
Barynov, 18
Aliaksei Akulionak, 16 |
Lyceum
#2, Minsk, Belarus |
Improved
System of Radio Observations of Meteors |
| 2000 |
|
College
Jean-de-Brebeuf, Montreal, Quebec, Canada
|
Cosmic
Bubbles Improving Hi Shell Detection Around Massive Stars |
| Daniel
Alan Perley, 17 |
Socorro
High School, Socorro, New Mexico |
Dynamic
Formation of Tidal Structure in Interacting Galaxies as Determined
by Newtonian Model Computer Simulations: Phase II |
