Dr Robert Minchin
banner
robminchin.bsky.social
Dr Robert Minchin
@robminchin.bsky.social
Radio astronomer at NRAO, posting on a personal basis. Affirming Christian (Episcopalian). Alumnus of Durham (MSci) & Cardiff (PhD). He/him.
High altitude balloon seen to the north of #Socorro this evening. Without the telephoto lens it was just a bright object hovering high in the sky at dusk.
September 15, 2025 at 1:26 AM
It was our annual picnic/mass at a campground in a local National Forest. I played guitar (with others, not pictured). The question was raised as to whether barbecue smoke counts as incense.
September 8, 2025 at 3:25 AM
Great Horned Owl at the Bosque del Apache this evening #Socorro
August 23, 2025 at 3:18 AM
Led MP for the first time … and the second time (two churches a 45 minute dash apart). I think it went okay, despite being stopped on the way up the aisle at the second church and told the lectionary book hadn’t been put out – I was able to deploy it before the end of the opening hymn!
June 30, 2025 at 12:51 AM
Bosque fire in #Socorro! 🔥 #nmwx
April 28, 2025 at 2:47 AM
The first bats of summer. #Socorro
March 25, 2025 at 5:38 AM
Remember that you are dust, and to dust you shall return.
March 5, 2025 at 8:08 PM
My REU student, Yulián Humaran of UPR Mayagüez, did a great job presenting his poster on signs of ram pressure in ionized-carbon rich dwarfs in the Virgo cluster today at #AAS245 #RadioAstronomy #ExtragalacticAstronomy
January 16, 2025 at 8:50 PM
Final talk for the session is Jessie Runnoe, on “Nanohertz Gravitational Waves and Their Electromagnetic Counterparts”.
Last parsec problem – how do smbh binaries cross the last pc to the centi-pc scale where GW emission drives orbit decay?
January 15, 2025 at 8:14 PM
ngVLA will contribute by resolving GW emitting smbh binaries and their progenitors. Can resolve smbh binaries in nearby clusters like Virgo and Fornax. Further away, use ngVLA + space VLBI. To resolve 3,000 au separation at 100 Mpc – separation 30 μas, so need 70,000 km baseline at 3mm!
#AAS245
January 15, 2025 at 8:05 PM
Next up is Joe Lazio, talking about “Ground- and Space-Based Long Baseline Interferometry” – in particular its relationship to pulsar timing arrays and merging black holes.
January 15, 2025 at 7:54 PM
After Paul telling us how ngVLA will find and measure Galactic centre pulsars, next is Thankful Cromartie on “Probing the Extremes of Physical Laws with Pulsars” – and how ngVLA will make this possible. Not just sensitivity but also sub-arrays, beam forming and high freq capability.
#AAS245
January 15, 2025 at 7:34 PM
First speaker is Paul Demorest, talking about “Sgr A* and Its Neighbors: Fundamental Physics with Galactic Center Pulsars”. Pulsars around Sgr A* would measure the gravitational field around the smbh, testing GR predictions such as “cosmic censorship” and the “no hair theorem”.
January 15, 2025 at 7:16 PM
If you looking for the #AAS245 session “Fundamental Physics and New Messengers”, it’s in Maryland Ballroom B, on the left of a narrow corridor between ballrooms A & C!
January 15, 2025 at 7:12 PM
More DSA-2000 with Gregg Hallinan speaking again in the Exhibit Hall theatre #AAS245 is just full of #RadioAstronomy!
January 15, 2025 at 4:37 PM
Closing out the session, Liam Connor talking about strong lensing synergies. Fewer than 100 currently known in the radio. Want fast survey speed, deep redshift distribution, and sub-arcsec resolution. DSA-2000 expected to find 50-100k sources. Science needs resolution – ngVLA delivers this.
#AAS245
January 15, 2025 at 3:47 PM
Science continues with Thankful Cromartie talking about synergies in pulsar science. #RadioAstronomy #AAS245
Pulsar timing arrays – smbh mergers. NANOGrav currently has monthly obs with GBT and VLA, and daily CHIME. lost Arecibo :(. 2023 detection of GW background.
January 15, 2025 at 3:32 PM
Now moving to science synergy with Alessandra Corsi talking about multi-messenger interfacing. Timescales from a few seconds to a few years. LIGO/Virgo/KAGRA O5 run (gravitational waves) well aligned with DSA-2000 start of operations. Following run likely to be aligned with ngVLA early science.
January 15, 2025 at 3:16 PM
Rachel Akeson talking about archiving: “DSA-2000, ngVLA and the era of surveys and big data”. Something the optical community has got used to – data sets to big to work with. Many other big surveys across multiple wavelengths. Interoperability – IVOA standards.
January 15, 2025 at 3:06 PM
Eric Murphy next with a summary of the ngVLA project. Fills gap in frequency between SKA and ALMA. Synergy with DSA-2000 in studies of galaxies, pulsars and the dynamic radio sky.
#AAS245 #RadioAstronomy
January 15, 2025 at 2:51 PM
Gregg Hallinan starts the splinter with a summary of DSA-2000. Survey-optimised telescope near the Nevada–Utah border. “Cake pan” feed actually made from cake pans from Fat Daddio!
January 15, 2025 at 2:41 PM
“Our friendly astronomers are waiting to answer your questions”.
I’m right at the back of the #AAS245 hall, in the middle (straight down from the AAS 125 years pillar). Come hear about my latest #RadioAstronomy results on possible “dark galaxies”!
January 14, 2025 at 10:09 PM
After the #AAS245 poster session today, there’s a Christian Astronomers dinner - meet at 18:30 at the noticeboard (by the registration desk).
January 14, 2025 at 8:35 PM
Recommendations:
*VLBA Unchanged*
VLA should maintain at least L, S, C, X, K bands. Fixed configuration, if done, should be only for a couple of years.
Conclusion: Any reduction In capability to the VLA or VLBA will reduce science return
#AAS245 #RadioAstronomy
January 14, 2025 at 8:03 PM
Next up – Joe Lazio presenting the transition concept. Draft report from the transition advisory group posted on Astro-ph this morning.
January 14, 2025 at 7:48 PM