Minami Takano, a senior at the Faculty of Knowledge Engineering, Tokyo City University won the Tokyo City University Alumni Association Award for her remarkable graduation research work using
ALMA observation data.
Not exact matches
The
data for the more than 1000 calibration sources stored in the ALMA Data Archive are publicly available, and ALMA continues to take calibration data as part of normal observati
data for the more than 1000 calibration sources stored in the
ALMA Data Archive are publicly available, and ALMA continues to take calibration data as part of normal observati
Data Archive are publicly available, and
ALMA continues to take calibration
data as part of normal observati
data as part of normal
observations.
«Eventually, we hope to combine the exquisite
ALMA data with future infrared
observations with NASA's James Webb Space Telescope.
Pablo Pérez - González, an astrophysics professor at the Complutense University of Madrid in Spain and one of several co-investigators on Nørgaard - Nielsen's proposed
observation, said they will use Webb to observe about 40 percent of the HUDF area with MIRI, in roughly the same location that ground - based telescopes like the Atacama Large Millimeter Array (
ALMA) and the Very Large Telescope array (VLT) obtained ultra-deep field
data.
In the majority of cases, the
ALMA observations alone could pinpoint the distances, but for a few galaxies the team combined the
ALMA data with measurements from other telescopes such as the Atacama Pathfinder Experiment (APEX) and the ESO Very Large Telescope.
But, unlike the new
ALMA observations, these
data did not allow the full three - dimensional structure to be studied.
By collecting statistical
data of this kind of galaxies and continuing in more follow - up
observations using
ALMA, we hope to reveal the truth.»
ALMA produces huge amounts of
observation data from gigantic hardware systems.
We use $ ^ -LCB- 12 -RCB- $ CO, $ ^ -LCB- 13 -RCB- $ CO and C$ ^ -LCB- 18 -RCB- $ O spectral line
data to independently describe the outflow and envelope structures associated with HBC... ▽ More We present Atacama Large Millimeter / sub-millimeter Array (
ALMA) Cycle - 2
observations of the HBC 494 molecular outflow and envelope.
In the majority of cases, the
ALMA observations alone could pinpoint the distances, but for a few galaxies the team combined the
ALMA data with measurements from other telescopes, including the Atacama Pathfinder Experiment (APEX) and ESO's Very Large Telescope [1].
The
observation data is made available only to the researcher group that submitted the proposal for a year and thereafter the
data is stored in the
ALMA data archive and becomes accessible and downloadable to everyone who wants to use it for his / her research.
However, the
data size for an
ALMA observation reaches tens of gigabits and it would be difficult for researchers to find and download their intended
data from such a huge amount of
data in a short time.
In
ALMA observations, observers do not have to go to the site and operate the system for themselves because operations are carried out by specialized operators and the obtained
data are processed by another expert team.
Obtained
observation data is firstly sent to a researcher who submitted the proposal, and after a proprietary period of one year, the
data will be stored in the
ALMA archive that is accessible from all over the world.
The
observation data obtained with
ALMA is kept in the
ALMA data archive, which is open to anyone and free to download for research purpose.