Last parsec problem – how do smbh binaries cross the last pc to the centi-pc scale where GW emission drives orbit decay?
Last parsec problem – how do smbh binaries cross the last pc to the centi-pc scale where GW emission drives orbit decay?
#AAS245
#AAS245
#AAS245
#AAS245
#AAS245
#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.
Pulsar timing arrays – smbh mergers. NANOGrav currently has monthly obs with GBT and VLA, and daily CHIME. lost Arecibo :(. 2023 detection of GW background.
#AAS245 #RadioAstronomy
#AAS245 #RadioAstronomy
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”!
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”!
*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
*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