Responses are due no later than 5:00 pm ET on 30 November 2026.
Responses are due no later than 5:00 pm ET on 30 November 2026.
I suspect (with lots of confidence) we are going to start seeing more profile events with much more sensitive new instruments coming online (SKA, DSA, ngVLA), so fingers crossed at one point new X-ray instruments catch them too!
I suspect (with lots of confidence) we are going to start seeing more profile events with much more sensitive new instruments coming online (SKA, DSA, ngVLA), so fingers crossed at one point new X-ray instruments catch them too!
https://arxiv.org/pdf/2610.41071
T. K. Sridharan.
https://arxiv.org/pdf/2610.41071
T. K. Sridharan.
🗓️ Saturday, October 10 ⤵️
#astronomy #radioastro #verylargearray #nrao
🗓️ Saturday, October 10 ⤵️
#astronomy #radioastro #verylargearray #nrao
10 AM MDT - Ylva Pihlstrom, Deputy Assistant Director, New Mexico Operations – “Radio Astronomy in New Mexico”
11 AM MDT - Jill Malusky, News Manager – “NRAO Telescopes On Screen”
12 PM MDT - Rob Selina, Project Engineer for ngVLA – "The next generation Very Large Array"
10 AM MDT - Ylva Pihlstrom, Deputy Assistant Director, New Mexico Operations – “Radio Astronomy in New Mexico”
11 AM MDT - Jill Malusky, News Manager – “NRAO Telescopes On Screen”
12 PM MDT - Rob Selina, Project Engineer for ngVLA – "The next generation Very Large Array"
11 AM MDT - Jill Malusky, News Manager – “NRAO Telescopes On Screen”
12 PM MDT - Rob Selina, Project Engineer for ngVLA – "The next generation Very Large Array"
11 AM MDT - Jill Malusky, News Manager – “NRAO Telescopes On Screen”
12 PM MDT - Rob Selina, Project Engineer for ngVLA – "The next generation Very Large Array"
We’ve recently reached some milestones for “first fringes” – meaning successful correlation, combining signals from 2+ separate antennas.
📸 Credit: Scott Broadwell
More ⤵️
#ngVLA #Astronomy #RadioAstronomy
We’ve recently reached some milestones for “first fringes” – meaning successful correlation, combining signals from 2+ separate antennas.
📸 Credit: Scott Broadwell
More ⤵️
#ngVLA #Astronomy #RadioAstronomy
2️⃣ ngVLA prototype ↔ NSF Very Large Array (NSF VLA): detections at Q-band (45 GHz)
2️⃣ ngVLA prototype ↔ NSF Very Large Array (NSF VLA): detections at Q-band (45 GHz)
SKA, ngVLA, Deep Synoptic Array which also compliment instruments like FAST and MeerKAT.
My prediction is we are about to see MANY more profile change events in the MSP population, and use these to probe magnetosphere physics.
SKA, ngVLA, Deep Synoptic Array which also compliment instruments like FAST and MeerKAT.
My prediction is we are about to see MANY more profile change events in the MSP population, and use these to probe magnetosphere physics.
Corder’s extensive experience and deep understanding of large-scale astronomical facilities will be significant assets as the ngVLA advances toward the next stage of development.
Corder’s extensive experience and deep understanding of large-scale astronomical facilities will be significant assets as the ngVLA advances toward the next stage of development.
He will be based in Albuquerque, beginning January 2027.
📸 Credit: NSF/AUI/NSF NRAO/M.Weiss, A.Sosnovic
He will be based in Albuquerque, beginning January 2027.
📸 Credit: NSF/AUI/NSF NRAO/M.Weiss, A.Sosnovic
Listen now ⤵️
YouTube: https://bit.ly/4hZc8Qt
Spotify: https://bit.ly/4zJlqqf
PodBean: https://bit.ly/4zGdl5B
Listen now ⤵️
YouTube: https://bit.ly/4hZc8Qt
Spotify: https://bit.ly/4zJlqqf
PodBean: https://bit.ly/4zGdl5B
U.S. National Science Foundation (NSF), NSF National Radio Astronomy Observatory, and U.S. Naval Observatory (USNO) Partner on Pathfinder for Next Generation Very Large Array #ngVLA
https://public.nrao.edu/news/ngvla-pathfinder/
U.S. National Science Foundation (NSF), NSF National Radio Astronomy Observatory, and U.S. Naval Observatory (USNO) Partner on Pathfinder for Next Generation Very Large Array #ngVLA
https://public.nrao.edu/news/ngvla-pathfinder/
ngvla.nrao.edu/page/technol...
ngvla.nrao.edu/page/technol...
The next-gen Array will have 263 dishes in core, spiral, and long-baseline arrangement, more than 5000 miles wide. It will be a powerful compound radio eye. 🔭🧪
ngvla.nrao.edu/page/array-c...
The next-gen Array will have 263 dishes in core, spiral, and long-baseline arrangement, more than 5000 miles wide. It will be a powerful compound radio eye. 🔭🧪
ngvla.nrao.edu/page/array-c...
If its funding survives (far from certain, sadly), the ngVLA will be 10x as sensitive and 10x as sharp. 🧪🔭
public.nrao.edu/news/nsf-nra...
If its funding survives (far from certain, sadly), the ngVLA will be 10x as sensitive and 10x as sharp. 🧪🔭
public.nrao.edu/news/nsf-nra...
#BlueSkyArtShow #Photography #Monochrome #NM
#BlueSkyArtShow #Photography #Monochrome #NM