Karl G. Jansky Very Large Array
Observatory in Socorro County, New MexicoWikipedia
44
MENTIONS
13
EPISODES
11
PODCASTS
Search complete. 44 mentions across 13 episodes found for "Karl G. Jansky Very Large Array".
Sep 8, 2026
The Moon in Five Hours
A
16:00AveryHOST
What's in the data set?
A
16:01AnnaHOST
ALMA, the Jansky Very Large Array, and JWST.
A
16:06AnnaHOST
And the picture they build is two massive protostars about 200 astronomical units apart, so five times the Sun to Pluto distance, on a violently eccentric orbit.
A
16:18AveryHOST
And the eccentricity is the evidence.
The Moon in Five Hours
A
15:24AnnaHOST
two separate cores forming independently that happen to fall past each other and don't escape a capture and that's what this team says they're watching the object is iras 07 299-1651 about 1680 parsecs away call it five and a half thousand light years The work is led by Yichen Zhang at Shanghai Jiao Tong University with Guido Garay at the Universidad de Chile, and it's built on eight years of observations from 2016 to 2024.
A
15:56AnnaHOST
Eight years? What's in the data set? ALMA, the Jansky Very Large Array, and JWST.
A
16:06AnnaHOST
And the picture they build is two massive protostars about 200 astronomical units apart, so five times the Sun to Pluto distance, on a violently eccentric orbit.
A
16:18AveryHOST
And the eccentricity is the evidence.
1.5 Hours of History Mysteries and Legends For Sleep | History Compilation
J
78:35JimmyHOST
Robert Dixon, the director of the SETI program at Ohio State, coordinated repeated attempts to find the signal again.
J
78:43JimmyHOST
Other observatories, including the Very Large Array in New Mexico and the Oak Ridge Observatory in Massachusetts, also conducted targeted searches of the area.
J
78:54JimmyHOST
None of them ever detected anything resembling the original signal.
J
78:58JimmyHOST
This failure to replicate is one of the most important and frustrating aspects of the WOW signal.
P
Unknown podcast
The Mysterious Signals Scientists Still Can_t Explain in Deep Space
Sep 4 · 1 Mention
S
54:35speaker_2NARRATOR
Follow-up observations confirmed that GPM J183910 was actively pulsing during the observation campaigns, producing regular radio bursts roughly every 21 minutes, with a pulse width of approximately 30 to 60 seconds per cycle.
S
54:52speaker_2NARRATOR
More remarkably, when the team searched archival data from the Very Large Array and the Giant Metrowave Radio Telescope, they found that this source had been detectable in observations dating back over 30 years.
S
55:04speaker_2NARRATOR
This was not a brief flare-up.
S
55:05speaker_2NARRATOR
This was a persistent radio emitter that had been pulsing for at least three decades, possibly much longer, sitting far below the conventional death line for radio pulsars, and apparently unconcerned with the theoretical rules that said it should have gone silent long ago.
Fall Asleep to The Signals We've Never Been Able to Explain
S
17:41speaker_0NARRATOR
The signal was not there.
S
17:44speaker_0NARRATOR
Robert Gray, an independent researcher who became obsessed with the WOW signal, conducted dedicated searches using the Very Large Array in New Mexico and the University of Tasmania's radio telescope.
S
18:01speaker_0NARRATOR
He observed the same coordinates for hours at a time, on multiple occasions over a period of years.
S
18:09speaker_0NARRATOR
Nothing.
Hyphenate Wavley Groves
W
31:30Waverly GrovesGUEST
At first, I was just building amps for...
W
31:33Waverly GrovesGUEST
The main project was the Very Large Array out in New Mexico.
W
31:38Waverly GrovesGUEST
If you've ever seen Contact, it's like where Jodie Foster is out in the desert.
W
31:42Waverly GrovesGUEST
And the Green Bank Telescope, not far from here in West Virginia.
Marcus Amerman (Choctaw): Multimedia Artist - Epi. 411, Host Dr. Mark Sublette
M
34:02Marcus AmermanGUEST
They all hang separately.
M
34:03Marcus AmermanGUEST
They could be sold separately or exhibited in a line, but they're made to be formed like that as like a giant shield themselves, kind of like the very large array, you know, that like there's power inside.
M
34:17Marcus AmermanGUEST
in each individual one like combined like a net when they're together or something like that but they're supposed to represent uh lifetimes as a warrior you know which was the main job yeah so the lifetimes yeah you know and i think i also worked for royalty sometime like the mound builders you know making yeah working for a ruling class you know but still it's a job
M
34:44Mark SubletteHOST
yeah well those so they're actual hubcaps right yeah and then you must have collected those over many many yeah yeah
Seeing the Entire Sky at Once in Radio Waves with Dr Jayce Dowell
J
2:37Jace DowellGUEST
So we're at the Sevilleta National Wildlife Refuge where we have built our second LWA station.
J
2:44Jace DowellGUEST
So the first one we built was around in 2010 and we did that out at the VLA.
J
2:49Jace DowellGUEST
And that was a lot of fun.
J
2:51Jace DowellGUEST
So we decided to build this one and we built this one in like 2015, 2016.
J
3:24Jace DowellGUEST
Yeah, and they're all about five feet tall-ish.
E
3:31Eric LloydHOST
So the antennas are just in the two spots, or the arrays rather?
J
3:36Jace DowellGUEST
We have a third one that's at the end of the VLA's north arm, which is a quarter this size.
J
3:41Jace DowellGUEST
So it has like the same physical footprint, but it has a quarter number of the elements.
P
Unknown podcast
The Mysterious Signals Scientists Still Can_t Explain in Deep Space
Aug 31 · 1 Mention
S
52:45speaker_4NARRATOR
Follow-up observations confirmed that GPM J183910 was actively pulsing during the observation campaigns, producing regular radio bursts roughly every 21 minutes, with a pulse width of approximately 30 to 60 seconds per cycle.
S
53:01speaker_4NARRATOR
More remarkably, when the team searched archival data from the Very Large Array and the Giant Metrowave Radio Telescope, They found that this source had been detectable in observations dating back over 30 years.
S
53:13speaker_4NARRATOR
This was not a brief flare-up.
S
53:15speaker_4NARRATOR
This was a persistent radio emitter that had been pulsing for at least three decades, possibly much longer, sitting far below the conventional death line for radio pulsars, and apparently unconcerned with the theoretical rules that said it should have gone silent long ago.
P
Unknown podcast
The Biggest Secrets Of Milky Ways Dark Heart
Aug 24 · 1 Mention
K
65:50KeithNARRATOR
So radio telescopes have been essential for studying Sagittarius A* since the beginning.
K
65:56KeithNARRATOR
The Very Large Array in New Mexico, the Atacama Large Millimeter Array in Chile, and many other radio observatories around the world regularly observe the galactic center.
K
66:08KeithNARRATOR
They map the structure of the gas, detect flares in emission, and contribute to efforts like the Event Horizon Telescope.
K
66:16KeithNARRATOR
Then there's infrared astronomy.
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