Iβm grateful for the opportunity to join @rescorp.org's #CottrellScholar community. This recognition means a lot to me. Iβm excited to advance our understanding of the cosmos by uncovering hidden low-mass galaxies, and to (re-)humanize our computing education in physics and astronomy for the AI era.
12.02.2026 16:24
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LGBTQIA+ progress flag.
There is no LGB without the TQIA+
We stand together or we fall together.
π³οΈβπ π³οΈββ§οΈ
01.02.2025 00:50
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It was really nice to come back to Pittsburgh to see friends and talk about the SAGA Survey.
23.11.2024 02:36
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Wow that translation was really bad... Here's what it says:
Rich in calcium, protein
Filling contains > 12% imported cheese powder
100% imported cocoa powder
0 trans fat
Where did the iron and turmeric come from?? π€¦
10.11.2024 05:58
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Astronomy and Astrophysics Outlist
Outlist and ally list for LGBTQIA+ members in the astronomy and astrophysics community
(Just realized that I haven't advertized the Astronomy and Astrophysics Outlist on this platform.)
If you are an LGBTQ+ π³οΈβπ astronomers/astrophysicists (or an ally) and are comfortable of being out, you can join the Astro Outlist to help increase LGBTQ+ visibility and connect with local community!
07.11.2024 22:11
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Lovely! Hope it goes well!
24.04.2024 22:04
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Images of 378 SAGA satellites, sorted by r-band absolute magnitude within each of the 101 complete systems that have satellites. Four of the 101 systems have the same level of survey completeness but do not have any confirmed satellites. The images of host galaxies are not included. The colors of the frames are assigned by the number of satellites. Images are taken from DESI Imaging DR9 (Dey et al. 2019). The width and height of each image correspond to 40 arcsec.
I was so lucky to be looped into SAGA Survey when I was still a second-year grad student. This amazing project is such an important part of my professional journey. It is so wonderful to work with this group of people. β€οΈπ§‘ππππ
Now go check out these beautiful satellites in our papers and e-posters!!
24.04.2024 21:16
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Pictures of the SAGA team members: Marla Geha (Yale), Yao-Yuan Mao (U Utah), Risa Wechsler (Stanford), Nitya Kallivayalil (U Virginia), Erik Tollerud (STScI), Ben Weiner (U Arizona), Ethan Nadler (Carnegie/USC), Yunchong (Richie) Wang (Stanford), Yasmeen Asali (Yale), Erin Kado-Fong (Yale), Mia de los Reyes (Amherst College), John F. Wu (Stsci)
It is ONLY through the team effort that the SAGA Survey reaches this major milestone: the fearless Marla Geha and Risa Wechsler, and an amazing team: Nitya, Erik, Ben, Ethan, Richie, Yasmeen, Erin, Mia, and John!
24.04.2024 21:13
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A screenshot of the SAGA Survey website that highlights the three SAGA DR3 papers: PAPER III: 101 SATELLITE SYSTEMS. SAGA DR3 includes 378 satellites identified across 101 MW-mass systems. The number of confirmed satellites per system ranges from 0 to 13, in the stellar mass range 10^6β10 solar masses.
PAPER IV: STAR-FORMING PROPERTIES. SAGA satellites that have lower masses or are closer to the host galaxy are more likely to be quenched. This data enable use to study the environmental processes that suppress or quench star formation.
PAPER V: COMPARING WITH MODELS. Using SAGA DR3 data to constrain an updated version of the Universe Machine model, we can directly test whether environmental quenching can be modeled by halo assembly histories.
Three SAGA Survey DR3 papers on arXiv:
3οΈβ£ 2404.14498 - survey overview & main results
4οΈβ£ 2404.14499 - satellites' star-forming properties
5οΈβ£ 2404.14500 - comparison with theoretical models
We also made "e-posters" that summarize the major points! Find the links on our website.
24.04.2024 21:07
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A screenshot of the homepage of SAGA Survey Data Release 3 website, with background filled with SAGA satellite images.
It's very fitting that my first post here is about this important milestone for the SAGA Survey and for myself personally!
The SAGA Survey characterizes satellite galaxy systems around Milky Way-mass galaxies, and we just posted our major results from our Data Release 3! Check arXiv & our website!
24.04.2024 21:04
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Target Selection and Sample Characterization for the DESI LOW-Z Secondary Target Program
We introduce the DESI LOW-Z Secondary Target Survey, which combines the wide-area capabilities of the Dark Energy Spectroscopic Instrument (DESI) with an efficient, low-redshift target selection metho...
This is a really rich analysis and data set, made possible by Elise Darragh-Ford, @yymao.bsky.social, Risa Wechsler, @jegpeek.bsky.social, and many others!
You can now access some of the data from the the DESI Early Data Release. Stay tuned for even more!
21.09.2023 17:14
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