I am a scientist-astronomer at the National Radio Astronomy Observatory (NRAO). During the past years I primarily worked on the scientific-astronomical commissioning of the Expanded Very Large Array (EVLA). As of Fall 2012, the project is officially concluded. The array has been named the Karl G. Jansky Very Large Array (VLA) to honor the founder of Radio Astronomy. The VLA is the world's dominant cm-wavelength radio telescope and most sensitive interferometer operating between 1 and 50 GHz.
Before joining NRAO, I was an astronomer at the world's largest
single dish radio telescope: The
305-m (1000 ft) Arecibo Radio Telescope of the
National Astronomy and Ionosphere Center
My research is focused on high angular resolution radio observations of
extragalactic objects known as
LIRGs (Luminous Infrared Galaxies) and ULIRGs (Ultra Luminous Infrared
Galaxies), to study both the structure and the kinematics of the
central regions in these galaxies. This research includes imaging of
these galaxies in radio continuum, in HI 21 cm absorption, and in
OH 18 cm megamaser emission.
For this research, and in order to study the nuclear active regions of
these galaxies at very high spatial resolution, I mainly use the Very
Long Baseline Array (VLBA)
of the NRAO.
However, the radio emission from these IR galaxies is very weak. So, in
order to have successful
observations, the Very Large Array (VLA)
of the NRAO,
with its twenty seven 25-meter antennas, participates in these
In some of these observations, the giant 305-meter
Arecibo radio telescope has been used along with both the VLBA
and the VLA.
Thanks to the enhanced observational capabilities of the VLA, I have become actively involved in magnetic field studies through Methanol masers. This work has led us to discover the Zeeman effect in two Class I methanol maser transitions. Visit my publications page to read about the discovery and the follow-up papers on this topic.
I am also involved in the COSMOS HI Large Extragalactic Survey (CHILES). This is a blind HI survey to detect 21 cm neutral hydrogen emission up to a redshift of 0.45 using the new capabilities of the VLA, and will require significant amount of telescope time. The pilot for this survey has been concluded successfully, and the results look very promising to carry out the full survey.
I continue to be actively involved in sensitive VLBI imaging of the radio continuum emission from very high redshift
quasars, both radio-loud and radio-quiet. These quasars are believed to be near the epoch of re-ionization,
i. e., when the first stars and galaxies started to form (less than 1 billion years after the Big Bang). We have
recently expanded this work to sub-millimeter galaxies (SMGs) at z~2-3 to study and determine their nuclear power sources (AGN vs. starburst).
If you are interested in history,
then you should read about the history of my
people, the Armenian people, a real but painful example of
a nation's survival for thousands of years (3500 years!). Here are some
a web site by Yuri Babayan.
The Armenian Genocide:
The first genocide of the 20th
century. During the Genocide, 1.5 million armenians perished in the turkish occupied Western Armenia. To read more, visit the
Armenian National Institute
The year 2015 marks the Armenian Genocide Centennial: For news and updates on various activities, visit armeniangenocide100.org
You can also read about the armenian genocide at the following web sites:
Wikipedia on Armenian Genocide
The Armenian alphabet and language
Armeniapedia: the online Armenia Encyclopedia
ArmenianHouse.org: an electronic library featuring a huge collection of documents on Armenian literature, history, religion and anything else Armenia-related
You can reach me by sending an email
updated: Sunday, 15-Mar-2015 12:21:14 MDT