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Karl G. Jansky Very Large Array

Karl G. Jansky Very Large Array

Observatory in Socorro County, New MexicoWikipedia

Search complete. 44 mentions across 13 episodes found for "Karl G. Jansky Very Large Array".

Sep 8, 2026

AveryHOST
16:00
What's in the data set?
AnnaHOST
16:01
ALMA, the Jansky Very Large Array, and JWST.
AnnaHOST
16:06
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.
AveryHOST
16:18
And the eccentricity is the evidence.
AnnaHOST
15:24
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.
AnnaHOST
15:56
Eight years? What's in the data set? ALMA, the Jansky Very Large Array, and JWST.
AnnaHOST
16:06
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.
AveryHOST
16:18
And the eccentricity is the evidence.
JimmyHOST
78:35
Robert Dixon, the director of the SETI program at Ohio State, coordinated repeated attempts to find the signal again.
JimmyHOST
78:43
Other observatories, including the Very Large Array in New Mexico and the Oak Ridge Observatory in Massachusetts, also conducted targeted searches of the area.
JimmyHOST
78:54
None of them ever detected anything resembling the original signal.
JimmyHOST
78:58
This failure to replicate is one of the most important and frustrating aspects of the WOW signal.

Unknown podcast

The Mysterious Signals Scientists Still Can_t Explain in Deep Space

Sep 4 · 1 Mention

speaker_2NARRATOR
54:35
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.
speaker_2NARRATOR
54:52
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.
speaker_2NARRATOR
55:04
This was not a brief flare-up.
speaker_2NARRATOR
55:05
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.
speaker_0NARRATOR
17:41
The signal was not there.
speaker_0NARRATOR
17:44
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.
speaker_0NARRATOR
18:01
He observed the same coordinates for hours at a time, on multiple occasions over a period of years.
speaker_0NARRATOR
18:09
Nothing.
Waverly GrovesGUEST
31:30
At first, I was just building amps for...
Waverly GrovesGUEST
31:33
The main project was the Very Large Array out in New Mexico.
Waverly GrovesGUEST
31:38
If you've ever seen Contact, it's like where Jodie Foster is out in the desert.
Waverly GrovesGUEST
31:42
And the Green Bank Telescope, not far from here in West Virginia.
Marcus AmermanGUEST
34:02
They all hang separately.
Marcus AmermanGUEST
34:03
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.
Marcus AmermanGUEST
34:17
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
Mark SubletteHOST
34:44
yeah well those so they're actual hubcaps right yeah and then you must have collected those over many many yeah yeah
Jace DowellGUEST
2:37
So we're at the Sevilleta National Wildlife Refuge where we have built our second LWA station.
Jace DowellGUEST
2:44
So the first one we built was around in 2010 and we did that out at the VLA.
Jace DowellGUEST
2:49
And that was a lot of fun.
Jace DowellGUEST
2:51
So we decided to build this one and we built this one in like 2015, 2016.
Jace DowellGUEST
3:24
Yeah, and they're all about five feet tall-ish.
Eric LloydHOST
3:31
So the antennas are just in the two spots, or the arrays rather?
Jace DowellGUEST
3:36
We have a third one that's at the end of the VLA's north arm, which is a quarter this size.
Jace DowellGUEST
3:41
So it has like the same physical footprint, but it has a quarter number of the elements.

Unknown podcast

The Mysterious Signals Scientists Still Can_t Explain in Deep Space

Aug 31 · 1 Mention

speaker_4NARRATOR
52:45
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.
speaker_4NARRATOR
53:01
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.
speaker_4NARRATOR
53:13
This was not a brief flare-up.
speaker_4NARRATOR
53:15
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.

Unknown podcast

The Biggest Secrets Of Milky Ways Dark Heart

Aug 24 · 1 Mention

KeithNARRATOR
65:50
So radio telescopes have been essential for studying Sagittarius A* since the beginning.
KeithNARRATOR
65:56
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.
KeithNARRATOR
66:08
They map the structure of the gas, detect flares in emission, and contribute to efforts like the Event Horizon Telescope.
KeithNARRATOR
66:16
Then there's infrared astronomy.

3 more episodes mention Karl G. Jansky Very Large Array.

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