NRAO, EVLA, VLBA, ALMA, AIPS, CASA

NRAO, EVLA, VLBA, ALMA, AIPS, CASA

Along with several other graduate students from Harvard University, I attended the first EVLA data reduction workshop in Socorro, New Mexico. Around 25 graduate students and researchers were present, along with many post-doctoral fellows and NRAO staff that devoted their time to help us learn how to use CASA, or Common Astronomy Software Applications.

An Excess of Positivity

An Excess of Positivity

The Fermi Large Area Telescope used a clever method of splitting electrons and positrons via the Earth’s magnetic field to show that there’s a significant excess of cosmic ray positrons at high energies – much more than can be explained using known cosmic ray processes.

Quakes on Jupiter: a new look at a familiar object

Quakes on Jupiter: a new look at a familiar object

In this paper, techniques from helioseismology – using waves to learn about the interior of the Sun – are applied to yet another object: Jupiter. Because Jupiter is largely a fluid, like the Sun, astronomers have expected it to show global seismic behavior since the mid-1970s; the signal was even theorized to be about the same magnitude as solar oscillations. However, attempts to detect Jupiter’s global oscillations in the 80s and 90s were largely unsuccessful.

EMU: A Radio Survey of the Southern Sky

EMU: A Radio Survey of the Southern Sky

EMU will contribute to many different areas of astrophysics from stars to galaxies to cosmology; it will find interesting objects that can be followed up with other observatories designed for deep observations such as ALMA. ASKAP will also provide an excellent testbed for the new phased array detector technology expected to be used in the Square Kilometre Array in the next decade.