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.
Now Accepting Applications for 2023 Astronomy in Chile Educator Ambassadors Program
Photo Credit: David Falkner, ACEAP 2020 Ambassador
Applications are now being accepted for the 2023 Astronomy in Chile Educator Ambassadors Program (ACEAP).
This program, in its eighth year, brings amateur astronomers, planetarium personnel, and formal and informal astronomy educators to U.S.-funded astronomy observatories in Chile. While there, ambassadors receive behind-the-scenes tours of some of the world’s most productive and advanced telescopes, including in-depth information on their instruments and discoveries. Prior to the ACEAP Expedition, participants engage in professional development activities designed to improve STEM communication and education.
This unique professional development experience has become known for:
- Providing unique access to facilities and people, and the astronomy ecosystem,
- Bringing together people with diverse backgrounds and skills from both formal and informal education communities,
- Investing in the Ambassadors: activities don’t stop at the end of the expedition or year of involvement,
- Creating a network that continues to branch out and engage in innovative activities,
- Providing a creative space for participants to interact.
Anyone, including international participants, may apply for five positions that are fully supported by their institution and/or personal funding. The remaining slots are restricted to U.S. citizens and permanent residents or Chilean residents who are amateur astronomers, K through college formal and informal educators who teach astronomy as part of their curriculum or program, planetarium educators, or those working in the area of astronomy communications.
Ten ambassadors will be selected for the northern hemisphere summer 2024 Expedition with specific travel dates TBD. This ten-day expedition (not including travel time between the U.S. and Chile) will include stops at the Cerro Tololo Inter-American Observatory (CTIO), Gemini-South Observatory, Rubin Observatory, and the Atacama Large Millimeter/submillimeter Array (ALMA).
In addition to the professional facilities, ACEAP ambassadors will visit smaller amateur/public observatories. Weather permitting, nighttime observing opportunities will be made available.
To learn more about the program and to apply, visit the ACEAP website or Facebook page. The deadline for applications is 11:59 p.m. (applicant’s local time), 30 April 2023.
Contact: Yasmin Catricheo at [email protected] or Tim Spuck at [email protected]
ACEAP is a collaborative project of Associated Universities, Inc., the National Radio Astronomy Observatory, Association of Universities for Research in Astronomy (AURA), and NSF’s National Optical-Infrared Astronomy Research Laboratory including Cerro Tololo Inter-American Observatory, Gemini Observatory, and The NSF Vera C. Rubin Observatory. ACEAP was initially funded in 2015 as a two-year pilot program by the National Science Foundation (NSF). Due to its success, a combination of institution, personal, and NSF funding have allowed the program to continue.
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.