High-energy transient signals are most often determined to be gamma-ray burst events, but the recently-launched Einstein Probe has expanded astronomers’ ability to quickly respond to similar signals occurring at X-ray wavelengths. Now, a multi-wavelength study of EP240408a concludes that while many of the signal’s characteristics might lead to the conclusion that it is a gamma-ray burst, the non-detection at radio wavelengths precludes that possibility.
Recent News
Students Contribute to New Understanding of ‘Twinkling’ Pulsars
The flexible observing setup of the Green Bank Observatory’s 20-meter telescope enabled frequent, long-duration observations of eight pulsars, spanning two and a half years for a student-driven study carried out by students in the Pulsar Science Collaboratory program.
Double the Disks, Double the Discovery: New Insights into Planet Formation in DF Tau
Tucked away in a star-forming region in the Taurus constellation, a pair of circling stars are displaying some unexpected differences in the circumstellar disks of dust and gas that surround them. A new study led by researchers at Lowell Observatory, combining data from the Atacama Large Millimeter/submillimeter Array (ALMA) and Keck Observatory, has unveiled intriguing findings about planet formation in this binary star system, known as DF Tau, along with other systems in this region.
Physics Inspiring the Next Generation! PING Camp 2018: July 15–21
PING is a STEMtastic summer camp program that actively seeks to increase the diversity of the next generation of scientists, engineers, and technologists. We are seeking current 8th graders (rising 9th-graders), who are interested in science, engineering and math, and a fun, and challenging experience on location at the Green Bank Observatory. While we are especially interested in recruiting youth from under-represented groups, all current 8th graders are encouraged to apply.
Green Bank Observatory is home to the National Science Foundation’s world famous Green Bank Telescope. Students will be immersed in the research activities of this national research center. While in residence, students will work in small teams supported by an undergraduate student mentor and an Observatory staff scientist (astronomer, physicist, engineer, etc.) to conduct research by observing the universe with a 40-foot diameter radio telescope. Supplemental educational activities, including bench experiences building electronic circuits, and coding activities complement the primary research theme. In addition, there is plenty of non-science fun to be had! Whole group seminars can include swimming, hiking, making and dancing – who knows? All activities take place on the Green Bank Observatory campus under the supervision of staff, who include outstanding teachers and STEM undergraduate students.
Space is limited! Please submit all of your application materials by our deadline!
Application Deadline: Wednesday, May 16, 2018
For more information or to apply, please visit http://greenbankobservatory.org/education/student_research/ping/
Recent News
NSF VLA Contributes Crucial Puzzle Piece to ‘Peculiar’ High Energy Transient
High-energy transient signals are most often determined to be gamma-ray burst events, but the recently-launched Einstein Probe has expanded astronomers’ ability to quickly respond to similar signals occurring at X-ray wavelengths. Now, a multi-wavelength study of EP240408a concludes that while many of the signal’s characteristics might lead to the conclusion that it is a gamma-ray burst, the non-detection at radio wavelengths precludes that possibility.
Students Contribute to New Understanding of ‘Twinkling’ Pulsars
The flexible observing setup of the Green Bank Observatory’s 20-meter telescope enabled frequent, long-duration observations of eight pulsars, spanning two and a half years for a student-driven study carried out by students in the Pulsar Science Collaboratory program.
Double the Disks, Double the Discovery: New Insights into Planet Formation in DF Tau
Tucked away in a star-forming region in the Taurus constellation, a pair of circling stars are displaying some unexpected differences in the circumstellar disks of dust and gas that surround them. A new study led by researchers at Lowell Observatory, combining data from the Atacama Large Millimeter/submillimeter Array (ALMA) and Keck Observatory, has unveiled intriguing findings about planet formation in this binary star system, known as DF Tau, along with other systems in this region.