Imad Pasha
@prappleizer.bsky.social
280 followers 88 following 37 posts
BA UC Berkeley, PhD Yale. Currently working on CGM observations with the Dragonfly FRO. Interested in galaxy evolution and statistical methods! Author of Astronomical Python and the pysersic code.
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prappleizer.bsky.social
Supporting that this evolutionary pathway is possible. For the dynamics-minded, this system will also allow for really strong constraints on the DM halo shape and DM distribution, as the rings are clean tracers of the potential out to large radii, something we’re following up with!
prappleizer.bsky.social
Some simulations have suggested that these ring galaxies can evolve into giant low surface brightness galaxies, another enigmatic population. Here we find faded rings in the distant outskirts of the system that rival the size of such galaxies, making this the first observational evidence…
prappleizer.bsky.social
These rings formed in the aftermath of the smaller blue galaxy flying through the center of a massive spiral. We were able to measure the ring positions and spacing, and it turns out to match predictions from analytic theory extremely well over a wide range. But there’s more…
prappleizer.bsky.social
Happy to share my latest paper, characterizing a rare-to-catch post collision galaxy with nine rings! Nice write up from stsci hubblesite.org/contents/new...
Straight Shot: Hubble Investigates Galaxy with Nine Rings
hubblesite.org
Reposted by Imad Pasha
stsci.edu
Bullseye! Researchers using Hubble found a massive galaxy rippling with nine star-filled rings after an “arrow,” the blue dwarf galaxy to its center-left, plunged through its core 50 million years ago. A thin trail of gas still links the pair: bit.ly/4hcX52n 🔭 🧪
A large galaxy is at center, and a significantly smaller galaxy is to its left. The large galaxy, nicknamed the Bullseye, is mostly face-on, but the top appears slightly tilted away. It has several rings. Its circular core is bright white at the very center, but light yellow overall. Going outward, there are gaps between the rings. The core is surrounded by two slightly lighter yellow rings, which also appear to be overlapping. The next ring is slightly more transparent and yellow. The two or three rings that are farther out are bluer, sometimes with blue clumps. The widest ring is also blue, but also the most transparent. At 9 o’clock is a small dwarf galaxy. It is about the same size as the yellow core of the Bullseye. The dwarf galaxy is blue, with many dots. It looks like the edge of the Bullseye might touch the dwarf galaxy. Both galaxies are set on the black background of space, which is dotted with a range of galaxies in different shapes, colors, and sizes.
Reposted by Imad Pasha
malenarice.bsky.social
Applications are open for the 2025 Dorrit Hoffleit Research Fellowship program for current undergraduate students to conduct summer research in the Yale Department of Astronomy!

Open to 2nd/3rd year undergrads of any nationality — due February 15th 🪐🧪🚀 astronomy.yale.edu/undergraduat...
Dorrit Hoffleit Undergraduate Research Scholarship | Department of Astronomy
astronomy.yale.edu
Reposted by Imad Pasha
jwuphysics.bsky.social
Awesome job opportunity for PhDs with observational astronomy and software engineering skills!

🔭
dokkum.bsky.social
This little movie illustrates the "filter tilter" concept of the 1000-lens array we're building in Chile. This is a single telephoto lens, raw 5 minute exposures. We're looking for a new team member to help turn such data into 3D images of cosmic flows!
aas.org/jobregister/...
Reposted by Imad Pasha
chloeneufeld.bsky.social
Looking for speakers for Yale's Galaxy Lunch! If you're a grad student or postdoc working on galaxy formation/evolution research, we'd love to have you present at our seminar. Reach out to me ([email protected]) or find more information about the seminar here:
yalegalaxylunch.github.io/about/
Seminar Overview · Yale Galaxy Lunch
yalegalaxylunch.github.io
prappleizer.bsky.social
Can I be added if I defended this week? I’m clinging on to the grad status for at least a month…
prappleizer.bsky.social
Feel free to reach out to me if you have questions or want to chat about the position!
prappleizer.bsky.social
Interested in working on the development of novel data analysis techniques? Our team at Dragonfly is hiring for a data algorithms position for a forthcoming 1000 lens array observatory in Chile! 5 year position w/great benefits and location flexibility: aas.org/jobregister/...
Software Developer for the Dragonfly FRO | American Astronomical Society
Dragonfly is a Convergent Research Focused Research Organization (FRO). Our mission is to capture the faint cosmic web of gas that connects galaxies across the universe, using a groundbreaking distrib...
aas.org
prappleizer.bsky.social
I hear i'm supposed to add a 🔭
prappleizer.bsky.social
We hope to create an "amortized" version of this framework, which would require many more simulations (think millions or more), but which then for a given survey, could produce inferences for new input galaxies in a matter of seconds. A challenge, but super useful in the upcoming era of surveys.
prappleizer.bsky.social
So what's next? At the moment, the training/fitting process is "bespoke" to every galaxy, because we fix things like sersic index/PA and survey depth/noise based on the appropriate values for every input galaxy. This takes time (~12 hr) and resources (GPU access). But...
prappleizer.bsky.social
In this paper we focus on distances, as there is a ground truth measurement of comparison. But there are some early signs that we are getting reasonable estimates for, e.g., stellar mass here as well (below: an injection/recovery test placing a logM=7.4 galaxy at many distances).
prappleizer.bsky.social
The method actually appears to be working rather well! Below is an example of one real input galaxy and three random draws from the posterior. On a sample of ~20 nearby galaxies with literature distances from TRGB/SBF, silkscreen almost always recovers the distance within the 5-95% posterior.
prappleizer.bsky.social
To do this we created Silkscreen, a code which uses neural posterior estimation and rounds of simulation and training to fit a set of galaxy properties given input images. In short, we simulate galaxy images with artpop, and use a ResNet to extract summary statistics before passing to the sbi code.
prappleizer.bsky.social
Given this fidelity, we wondered if one could "fit" the basic properties (distance/mass especially) using artpop as a simulator. Such a method would be dramatically cheaper than the gold-standard of TRGB, and might be able to marginalize over some of the uncertainties in SBF from Z/stellar pops
prappleizer.bsky.social
Our idea stems from the ability for the Artpop code to make realistic galaxy images from first principles -- i.e., create stellar populations sampling IMFs and place them "star by star" in some distribution (e.g., Sérsic), while also simulating survey depths and noise properties.
prappleizer.bsky.social
New Paper! With tim miller, @avapolzin.bsky.social, and pieter van dokkum, we explore whether forward modeling+simulation based inference can provide a robust, likelihood-free way to estimate galaxy distances in the distance range of 2-20 Mpc (too close for hubble-flow)🧵 arxiv.org/abs/2407.04091
Silkscreen: Direct Measurements of Galaxy Distances from Survey...
With upcoming wide field surveys from the ground and space the number of known dwarf galaxies at $\lesssim 25$ Mpc is expected to dramatically increase. Insight into their nature and analyses of...
arxiv.org
prappleizer.bsky.social
Also, I have a new textbook coming out with IOP/AAS later this year expanding on the above! You may also check out astro-330.github.io, which is the course site for a slightly higher level astro coding class I ran at Yale. Also, astro-rps.github.io has resources we're using for an intro seminar
astro-330.github.io
prappleizer.bsky.social
Definitely! The exercises in the astrocodex will be open source and available publicly; the solution sets repository will be available to registered instructors.
prappleizer.bsky.social
And so I would hope the materials end up being complementary! I took part in carpentries as part of the LSST DSFP and think they're doing great work, particularly around the concepts of bootcamps and workshops. Our focus is on the "exercise"/materials portion for a classroom setting. 2/2
prappleizer.bsky.social
good q: i think the key diffs are: 1) focus on standalone exercises/materials more at the assignment level rather than workshop-style walkthroughs 2) much expanded focus on various astronomy topics 3) no (public/immediate) solutions 4) interoperability for inserting into existing curricula 1/2