Rohan Naidu
rpnaidu.bsky.social
Rohan Naidu
@rpnaidu.bsky.social
Astronomer @ MIT. First graduating class of Yale-NUS College, Singapore. 🇮🇳 →🇸🇬 →🇺🇸 https://rohannaidu.github.io/
The paper: ui.adsabs.harvard.edu/abs/2024ApJ....

A nice article covering the excitement around LRDs: www.quantamagazine.org/the-beautifu...
June 8, 2025 at 3:15 PM
Thanks for maintaining this! I'm an astronomer and would love to join this feed. rohannaidu.github.io
Welcome!
About me
rohannaidu.github.io
May 20, 2025 at 8:43 PM
i am a postdoc and would love to share and discuss latest research on this feed rohannaidu.github.io
Welcome!
About me
rohannaidu.github.io
May 20, 2025 at 8:38 PM
yes
May 20, 2025 at 8:35 PM
May 20, 2025 at 8:33 PM
Reposted by Rohan Naidu
While it is too luminous by pre-JWST standards, it aligns well with the new models of galaxy formation inspired by JWST observations
May 19, 2025 at 9:35 AM
Looking forward! And totally understand!
April 8, 2025 at 9:08 PM
We'll know the fate of our Pop III candidate (and learn a lot about ultra-faint galaxies!) this summer thanks to our recently approved DDT program. Stay tuned!
www.stsci.edu/jwst-program...
www.stsci.edu
March 2, 2025 at 3:07 PM
My favorite quote from the article, courtesy Tim Beers, alluding to the Milky Way's own ultra-faint satellites that seem quite primordial themselves: “I find it exciting that you can draw a straight line from what we see around the Milky Way to this proposed birthplace.”
March 2, 2025 at 3:07 PM
It was an absolute joy working with @sfseiji.bsky.social on this grand adventure that began at this year's Hubble Symposium, with John Chisholm and @dyonysos.bsky.social -- the fearless leaders of GLIMPSE, and with our team mates who put countless hours into making these data science-ready!
January 22, 2025 at 9:04 PM
I'll end this thread with some purple prose that didn't quite make it into the final draft.
January 22, 2025 at 8:58 PM
In the mean time, with the clean selection technique, we can already place strong constraints on the # density of such sources that our theorist friends can match their models against! These #s matter for e.g., LISA black hole merger rates and whether Roman might detect Pop III supernovae!
January 22, 2025 at 8:58 PM