Erin Kado-Fong's Avatar

Erin Kado-Fong

@kadofong

YCAA prize fellow at Yale. PhD from Princeton; headed to Stanford in 2025 as a Kavli fellow. I use large surveys of dwarf galaxies to disentangle the roles that star formation, stellar pop. assembly, and DM structure play in governing galaxy evolution.

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Latest posts by Erin Kado-Fong @kadofong

Around one week left to register for Galactic Frontiers II -- looking forward to discussing low-mass galaxies with a great group this June!

#astro #extragalactic

23.02.2025 23:55 ๐Ÿ‘ 14 ๐Ÿ” 4 ๐Ÿ’ฌ 1 ๐Ÿ“Œ 0
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Saw this cool work on the arxiv today from Blake Keith & @ferahm.bsky.social!

A demonstration of how the 3D shapes of stars trace that of DM in cosmologically simulated dwarfs, including a comparison to observed stellar shapes from my previous work.

arxiv.org/abs/2501.16317

๐Ÿ”ญ #extragalactic

28.01.2025 16:52 ๐Ÿ‘ 15 ๐Ÿ” 1 ๐Ÿ’ฌ 1 ๐Ÿ“Œ 0
Mass-size relation of LG/LV/LF dwarfs

Mass-size relation of LG/LV/LF dwarfs

Was psyched that Andrew Pace's Local Volume Database of dwarfs & star clusters was on ArXiV the other day! The push for community-facing collation is great to see in the #extragalactic space. (๐Ÿ”ญ)

๐Ÿ“ arxiv.org/abs/2411.07424
๐Ÿ’ป github.com/apace7/local...

22.11.2024 14:49 ๐Ÿ‘ 18 ๐Ÿ” 2 ๐Ÿ’ฌ 0 ๐Ÿ“Œ 0
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On ApJ now so technically an #extragalactic #astro #paperday!

We deconvolve survey selection from evolution of the low-mass SFS at z<0.2. This constrains models of dwarf assembly, and signals how care is needed to use low-z galaxies to contextualize the LV/LG.

ui.adsabs.harvard.edu/abs/2024ApJ....

19.11.2024 17:27 ๐Ÿ‘ 18 ๐Ÿ” 2 ๐Ÿ’ฌ 1 ๐Ÿ“Œ 1
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For the dwarf galaxy enthusiasts in #astro & #extragalactic! Excited to share the conference we'll be hosting June 2025:

๐Ÿ”Ž Galactic Frontiers II: Dwarfs in the LV & Beyond
๐Ÿ”Ž 6/23-6/25 at Dartmouth

Note that the conference is NOT region-specific!
Register at: sites.dartmouth.edu/galactic-fro...

15.11.2024 17:54 ๐Ÿ‘ 13 ๐Ÿ” 4 ๐Ÿ’ฌ 0 ๐Ÿ“Œ 1

I am an astronomer, focusing on extragalactic astrophysics and galaxy evolution (postdoc at Yale).

15.11.2024 16:49 ๐Ÿ‘ 0 ๐Ÿ” 0 ๐Ÿ’ฌ 1 ๐Ÿ“Œ 0

yes

15.11.2024 16:48 ๐Ÿ‘ 0 ๐Ÿ” 0 ๐Ÿ’ฌ 1 ๐Ÿ“Œ 0

@bot.astronomy.blue signup

15.11.2024 14:56 ๐Ÿ‘ 0 ๐Ÿ” 0 ๐Ÿ’ฌ 1 ๐Ÿ“Œ 0
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And in the second Merian ๐Ÿฆ‹ paper out today:

Princeton student Abby Mintz develops methods to turn medium-band imaging into Hฮฑ maps, and shows that low-mass starbursts tend to be more compact than their more massive counterparts.

Read the paper here! arxiv.org/abs/2410.01886

04.10.2024 16:39 ๐Ÿ‘ 0 ๐Ÿ” 0 ๐Ÿ’ฌ 0 ๐Ÿ“Œ 0
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So excited to share the first two science papers of the Merian medium-band survey! ๐Ÿฆ‹

We image Hฮฑ and [OIII] to measure weak lensing and resolved star formation in low-z dwarfs over ~750 deg^2.

Check out the survey paper led by Shany Danieli at: arxiv.org/abs/2410.01884 !

04.10.2024 16:38 ๐Ÿ‘ 0 ๐Ÿ” 0 ๐Ÿ’ฌ 0 ๐Ÿ“Œ 0
Preview
The SAGA Survey. V. Modeling Satellite Systems around Milky... Environment plays a critical role in shaping the assembly of low-mass galaxies. Here, we use the UniverseMachine (UM) galaxy-halo connection framework and the Data Release 3 of the Satellites...

It's DR3 Paper Day for the SAGA Survey!! ๐ŸŽ‰
๐ŸŒŸMao+ gives a satellite census of 101 MW-like hosts arxiv.org/abs/2404.14498
๐ŸŒŸGeha+ surveys the link btwn environment & star formation arxiv.org/abs/2404.14499
๐ŸŒŸ Wang+ models dwarf quenching with the UniverseMachine arxiv.org/abs/2404.14500

24.04.2024 14:59 ๐Ÿ‘ 2 ๐Ÿ” 1 ๐Ÿ’ฌ 0 ๐Ÿ“Œ 0

Excited to see this very nice research highlight of our recent quenched field dwarf paper by @aasnova.bsky.social !

08.03.2024 17:32 ๐Ÿ‘ 0 ๐Ÿ” 0 ๐Ÿ’ฌ 0 ๐Ÿ“Œ 0
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Paper day! arxiv.org/abs/2401.16469
We use the background galaxies in the SAGA survey to infer the efficiency of winds driven by star formation in low-mass galaxies. We find a mass-loading factor of ~1: consistent with direct observations, but smaller than what some sims predict at these masses.

31.01.2024 14:02 ๐Ÿ‘ 6 ๐Ÿ” 2 ๐Ÿ’ฌ 1 ๐Ÿ“Œ 0
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A late ArXiV post since I wasnโ€™t active here โ€” we present a field dwarf pair where one is starbursting and the other is *quenched*! VLA data reveal that the non-SF dwarf's HI is in large tidal tails, showing that field dwarfs can temporarily quench even as non-satellites. arxiv.org/abs/2311.09280

30.11.2023 19:19 ๐Ÿ‘ 12 ๐Ÿ” 2 ๐Ÿ’ฌ 0 ๐Ÿ“Œ 0