Shashank Dholakia
astroshashank.bsky.social
Shashank Dholakia
@astroshashank.bsky.social
Astrophysics PhD candidate at University of Queensland | UC Berkeley '21 | Exoplanets and Stars | @astrosoundbites.bsky.social co-host | Astrophotographer

shashankdholakia.github.io
I think he refers to her at his Fuhi which (in gujarati) is part of a whole vocabulary of extended family relations that doesn't translate well and gets compressed into aunt/uncle

I'm still confused by the cousin-x-removed in English tbh
October 29, 2025 at 9:58 AM
Just after sunset to the west! The star Alphecca (alpha CrB) is in this photo, so it's quite close to the constellation corona borealis
October 27, 2025 at 9:18 PM
Forgot the astrophoto tag!
#astrophotography
October 27, 2025 at 1:40 AM
I took this w a monochrome camera & refractor w H-alpha etalon (Daystar Quark). 800 frames every 30s, best 5% stacked. Autostakkert, ImPPG for alignment, Wavesharp for sharpening and final warp stabilizer in Premiere. Humans have poor acuity in the real deep red H-alpha so colored orange instead.
October 19, 2025 at 9:01 PM
Reposted by Shashank Dholakia
In a companion paper, PhD student @maxecharles.bsky.social applies this to reconstructing complex images, not just fields of dots. We apply a regularised maximum likelihood method to restore clean, diffraction limited imaging by fitting directly to pixel level data.
Image reconstruction with the JWST Interferometer
Flying on board the James Webb Space Telescope (JWST) above Earth's turbulent atmosphere, the Aperture Masking Interferometer (AMI) on the NIRISS instrument is the highest-resolution infrared interfer...
arxiv.org
October 14, 2025 at 3:35 AM
Reposted by Shashank Dholakia
In the first paper Louis Desdoigts (ex PhD in my group, now Leiden postdoc) learns a model for the entire AMI system's optical physics together with a neural network 'effective detector model' the sensor, which suffers from a serious 'brighter-fatter effect' that blurs images at the pixel level.
AMIGO: a Data-Driven Calibration of the JWST Interferometer
The James Webb Space Telescope (JWST) hosts a non-redundant Aperture Masking Interferometer (AMI) in its Near Infrared Imager and Slitless Spectrograph (NIRISS) instrument, providing the only dedicate...
arxiv.org
October 14, 2025 at 3:35 AM
Yeah, it was labor intensive for sure. 15 mins for each video plus >100gb, but I'm a grad student so I've got time 😆
October 6, 2025 at 6:17 PM
It's all hand-tracked! I aligned the long axis of the camera in the direction of the drift and would recenter it every few seconds.
October 6, 2025 at 5:30 PM
Reposted by Shashank Dholakia
Research also shows that spreading smaller amounts of funding out over more researchers generally delivers better scientific outcomes per dollar spent than focusing bigger grants on fewer researchers.

journals.plos.org/plosone/arti...
Big Science vs. Little Science: How Scientific Impact Scales with Funding
Agencies that fund scientific research must choose: is it more effective to give large grants to a few elite researchers, or small grants to many researchers? Large grants would be more effective only...
journals.plos.org
October 4, 2025 at 5:50 PM
FFTs are pretty hard to beat in speed but restricting to the surface of a sphere and the analytic solution certainly helps! The goal is to do HMC on the surface map coefficients
October 2, 2025 at 1:58 AM
I believe @astromonnier.bsky.social has work on interferometrically detecting hot Jupiters from closure phases, maybe he'd have more to add about this
October 2, 2025 at 1:51 AM