Ji Hoon Kim's Avatar

Ji Hoon Kim

@jhkim.bsky.social

Astronomer@Seoul National University; Project Manager of 7DT/7DS; LSBGs, Star-forming ISM, Late-type galaxy dynamics; He/him/views are own

406 Followers  |  302 Following  |  146 Posts  |  Joined: 03.07.2023  |  1.7589

Latest posts by jhkim.bsky.social on Bluesky

Say hi to @lellifede.bsky.social. ๐Ÿ˜‰

08.09.2025 09:01 โ€” ๐Ÿ‘ 1    ๐Ÿ” 0    ๐Ÿ’ฌ 0    ๐Ÿ“Œ 0

A meeting nearby Firenze?

08.09.2025 01:39 โ€” ๐Ÿ‘ 0    ๐Ÿ” 0    ๐Ÿ’ฌ 1    ๐Ÿ“Œ 0
Merger fraction as a function of distance from the cluster
center, separated by AGN presence. Red circles show galaxies
hosting AGNs, and blue squares show non-AGN galaxies. While
overall merger fractions are similar, AGN-host galaxies exhibit a
mild increase in merger fraction toward the cluster center. Alt text:
The x axes show the R/R200 from 0.0 to 1.0. The y axes show the
merger fraction from 0.22 to 0.6.

Merger fraction as a function of distance from the cluster center, separated by AGN presence. Red circles show galaxies hosting AGNs, and blue squares show non-AGN galaxies. While overall merger fractions are similar, AGN-host galaxies exhibit a mild increase in merger fraction toward the cluster center. Alt text: The x axes show the R/R200 from 0.0 to 1.0. The y axes show the merger fraction from 0.22 to 0.6.

We also present tentative evidence that mergers contribute to AGN triggering in cluster cores.

Anri put a great effort into this work!

This paper is accepted for publication in PASJ.

02.09.2025 02:26 โ€” ๐Ÿ‘ 0    ๐Ÿ” 0    ๐Ÿ’ฌ 0    ๐Ÿ“Œ 0
Merger fraction as a function of redshift, shown for cluster member galaxies (blue circle), galaxy pairs (orange square), and field galaxies (green triangle). All subsamples show a positive correlation with redshift.

Merger fraction as a function of redshift, shown for cluster member galaxies (blue circle), galaxy pairs (orange square), and field galaxies (green triangle). All subsamples show a positive correlation with redshift.

We find that the merger fraction increases with redshift for all environments, showing a strong radial gradient in clusters. This suggests that galaxy merger activity is enhanced both at earlier cosmic times and in dense environments, highlighting the role of groups.

02.09.2025 02:22 โ€” ๐Ÿ‘ 0    ๐Ÿ” 0    ๐Ÿ’ฌ 1    ๐Ÿ“Œ 0
 Distribution of galaxies in the Giniโ€“M20 plane. The solid line (G = โˆ’0.14 M20 + 0.33) indicates the merger/non-merger boundary. The color scale represents shape_asymmetry (Ashape). Galaxies above the line and with high asymmetry tend to be classified as mergers under our criterion. Alt text: A scatter graph, the x axes shows the M20 from -3.0 to 0.0, the y axes shows the Gini coefficient from 0.3 to 0.9.

Distribution of galaxies in the Giniโ€“M20 plane. The solid line (G = โˆ’0.14 M20 + 0.33) indicates the merger/non-merger boundary. The color scale represents shape_asymmetry (Ashape). Galaxies above the line and with high asymmetry tend to be classified as mergers under our criterion. Alt text: A scatter graph, the x axes shows the M20 from -3.0 to 0.0, the y axes shows the Gini coefficient from 0.3 to 0.9.

Using a new non-parametric classification scheme that combines Gini-M20 and shape asymmetry, we identify 12,666 mergers from a sample of 33,320 galaxies, validating our method against GALAXY CRUISE visual classifications.

02.09.2025 02:19 โ€” ๐Ÿ‘ 1    ๐Ÿ” 0    ๐Ÿ’ฌ 1    ๐Ÿ“Œ 0
Merger fraction in galaxy groups and clusters at z < 0.2: A non-parametric morphological study with Subaru Hyper Suprime-Cam We investigate the environmental dependence of galaxy mergers using high-resolution imaging data from the Hyper Suprime-Cam (HSC) Subaru Strategic Program. We focus on galaxy groups and clusters at $z...

It's paper day! ๐Ÿงช๐Ÿ”ญ
Our latest paper investigates galaxy merger rates and their environmental dependence at z<0.2 using high-resolution Hyper Suprime-Cam (HSC) data.
ui.adsabs.harvard.edu/abs/2025arXi...

02.09.2025 02:13 โ€” ๐Ÿ‘ 2    ๐Ÿ” 1    ๐Ÿ’ฌ 2    ๐Ÿ“Œ 0
Preview
Non-equilibrium dynamics in galaxies that appear to lack dark matter: tidal dwarf galaxies There are a number of galaxies that have been reported to lack dark matter. This is weird in a universe made of dark matter. It is also weird in MOND, which (if true) is what causes the inference oโ€ฆ

Tidal dwarfs & non-equilibrium dynamics ๐Ÿ”ญ๐Ÿงช
tritonstation.com/2025/08/20/n...

27.08.2025 02:30 โ€” ๐Ÿ‘ 33    ๐Ÿ” 5    ๐Ÿ’ฌ 1    ๐Ÿ“Œ 0

These bright AGNs fill key gaps in the SDSS and Quaia catalogs and will serve as prime targets for future multi-wavelength studies.

Congratulations, Yunyi!

11.08.2025 09:14 โ€” ๐Ÿ‘ 1    ๐Ÿ” 0    ๐Ÿ’ฌ 0    ๐Ÿ“Œ 0
Distribution of redshift and bolometric luminosity for AllBRICQS quasars in this work (Northern Hemisphere; red circles) and from Onken et al. (2023) (Southern Hemisphere; blue triangles), in comparison to the SDSS DR16 Quasar Catalog (SDSS DR16Q; Lyke et al. 2020), shown as grey contours. The AllBRICQS quasars occupy the bright end of the quasar luminosity distribution, exhibiting significantly higher luminosities than the bulk of the SDSS DR16Q sample.  The grey contours correspond to a two-dimensional histogram constructed using 10,000 bins (100 bins per axis), effectively illustrating the density distribution of the SDSS quasars.

Distribution of redshift and bolometric luminosity for AllBRICQS quasars in this work (Northern Hemisphere; red circles) and from Onken et al. (2023) (Southern Hemisphere; blue triangles), in comparison to the SDSS DR16 Quasar Catalog (SDSS DR16Q; Lyke et al. 2020), shown as grey contours. The AllBRICQS quasars occupy the bright end of the quasar luminosity distribution, exhibiting significantly higher luminosities than the bulk of the SDSS DR16Q sample. The grey contours correspond to a two-dimensional histogram constructed using 10,000 bins (100 bins per axis), effectively illustrating the density distribution of the SDSS quasars.

It's paper day! ๐Ÿงช๐Ÿ”ญ

Our latest ApJS paper presents the second AllBRICQS catalog โ€” 62 newly confirmed luminous quasars in the Northern Hemisphere (0.09 < z < 2.48), selected via WISE + Gaia DR3. Highlights include the most luminous FeLoBAL quasar ever found.

arxiv.org/pdf/2508.06028

11.08.2025 09:12 โ€” ๐Ÿ‘ 6    ๐Ÿ” 2    ๐Ÿ’ฌ 2    ๐Ÿ“Œ 0

What's more?

28.07.2025 08:47 โ€” ๐Ÿ‘ 1    ๐Ÿ” 0    ๐Ÿ’ฌ 1    ๐Ÿ“Œ 0
15.07.2025 00:14 โ€” ๐Ÿ‘ 4    ๐Ÿ” 1    ๐Ÿ’ฌ 1    ๐Ÿ“Œ 0

Post a song from the year you turned 12.

youtu.be/djV11Xbc914?...

14.07.2025 14:20 โ€” ๐Ÿ‘ 1    ๐Ÿ” 0    ๐Ÿ’ฌ 0    ๐Ÿ“Œ 0

I often disagree with him, but Stacyโ€™s physics posts are always thoughtful and informative, and the observational truth of Milgromโ€™s law โ€” which Stacy has been trying to get people to take seriously for decades โ€” really does seem to say something fundamental about the Universe. ๐Ÿงช

13.07.2025 12:58 โ€” ๐Ÿ‘ 14    ๐Ÿ” 2    ๐Ÿ’ฌ 1    ๐Ÿ“Œ 0
Post image Post image

Here's a little side-by-side of a patch of our Virgo imaging (from Mihos+17) compared to today's Rubin release. I knew that Rubin field looked familiar! Nice to see they recover a lot of that low surface brightness structure. ๐Ÿ”ญ

23.06.2025 16:22 โ€” ๐Ÿ‘ 84    ๐Ÿ” 20    ๐Ÿ’ฌ 5    ๐Ÿ“Œ 1
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All this time & Mike Turner still making promises he canโ€™t keep. A quarter century ago it was โ€œwe will detect dark matter in five years.โ€

23.06.2025 21:36 โ€” ๐Ÿ‘ 9    ๐Ÿ” 1    ๐Ÿ’ฌ 1    ๐Ÿ“Œ 0
Preview
โ€˜This is bullโ€”โ€”โ€: National Science Foundation employees protest HUD's takeover Dozens of National Science Foundation employees crowded the agencyโ€™s headquarters in Alexandria, Virginia, Wednesday to protest the news that the Department of Housing and Urban Development, or HUD, w...

Another day testing the limits of resilience.

The Alexandria NSF building was designed for the NSF merit review process (gold standard), complete with a floor devoted to panels.

Now we arenโ€™t allowed to have in person panels.

The loss of US science leadership will haunt this country for decades.

25.06.2025 23:13 โ€” ๐Ÿ‘ 918    ๐Ÿ” 439    ๐Ÿ’ฌ 15    ๐Ÿ“Œ 38

I got to wonder if this is the end of an era for SExtractor. So, be ready for Tractor?

24.06.2025 05:32 โ€” ๐Ÿ‘ 2    ๐Ÿ” 0    ๐Ÿ’ฌ 0    ๐Ÿ“Œ 0
Preview
Ever-changing Universe Revealed in First Imagery From NSFโ€“DOE Vera C. Rubin Observatory From distant stars and galaxies to asteroids whizzing through the Solar System, this next-generation facility unveils its first imagery and brings the night sky to life like never before.

Holy smokes.๐Ÿ”ญ๐Ÿงช
noirlab.edu/public/news/...

24.06.2025 05:31 โ€” ๐Ÿ‘ 22    ๐Ÿ” 0    ๐Ÿ’ฌ 1    ๐Ÿ“Œ 0
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Taeho Ryu is providing a clue on the formation of blue straggler stars via magnetic field amplification. ๐Ÿ”ญ๐Ÿงช

19.06.2025 05:18 โ€” ๐Ÿ‘ 6    ๐Ÿ” 1    ๐Ÿ’ฌ 0    ๐Ÿ“Œ 0
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Eun-jin Shin is giving a talk on IMBH formation in dwarf galaxies during IAUS398/MODEST-25. ๐Ÿ”ญ๐Ÿงช

18.06.2025 02:45 โ€” ๐Ÿ‘ 6    ๐Ÿ” 0    ๐Ÿ’ฌ 0    ๐Ÿ“Œ 0
Post image

Michela Mapelli is starting the very first scientific talk for IAU Symposium 398/MODEST-25 โ€œCompact Stars and Binaries in Dense Stellar Systemsโ€. ๐Ÿ”ญ๐Ÿงช

16.06.2025 02:03 โ€” ๐Ÿ‘ 5    ๐Ÿ” 0    ๐Ÿ’ฌ 0    ๐Ÿ“Œ 0

Exit polls show that the outcome of this election will be what has been obvious. Or, rather what should have been obvious. Whatโ€™s not obvious is how quickly the country will overcome the harms done by the previous president.

03.06.2025 11:13 โ€” ๐Ÿ‘ 0    ๐Ÿ” 0    ๐Ÿ’ฌ 0    ๐Ÿ“Œ 0

After we impeached the president second time in 9 years, we are voting for the 21st president. While the entire globe is slowly turning conservative, we may have someone central. I mean not far right.

03.06.2025 09:54 โ€” ๐Ÿ‘ 2    ๐Ÿ” 0    ๐Ÿ’ฌ 1    ๐Ÿ“Œ 0

Based on my previous skeet five months ago, pot?

25.04.2025 02:13 โ€” ๐Ÿ‘ 2    ๐Ÿ” 0    ๐Ÿ’ฌ 0    ๐Ÿ“Œ 0
Preview
Crisis at NASA It's very bad news all round for NASA science, but the worst hit is Astrophysics (which includes cosmology) where the proposed cut is about two-thirds, which would be devastating.

Crisis at NASA

It's very bad news all round for NASA science, but the worst hit is Astrophysics (which includes cosmology) where the proposed cut is about two-thirds, which would be devastating.

23.04.2025 18:31 โ€” ๐Ÿ‘ 51    ๐Ÿ” 32    ๐Ÿ’ฌ 2    ๐Ÿ“Œ 4
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Woong-seop Jeong is giving a talk on SPHEREx at Seoul National University. ๐Ÿ”ญ๐Ÿงช

24.04.2025 07:37 โ€” ๐Ÿ‘ 4    ๐Ÿ” 0    ๐Ÿ’ฌ 0    ๐Ÿ“Œ 0

This is what we (South-) Koreans should be worried about.

25.02.2025 02:18 โ€” ๐Ÿ‘ 2    ๐Ÿ” 0    ๐Ÿ’ฌ 0    ๐Ÿ“Œ 0

Advertise your sky account in 3 words:

So it goes

19.01.2025 08:58 โ€” ๐Ÿ‘ 0    ๐Ÿ” 0    ๐Ÿ’ฌ 0    ๐Ÿ“Œ 1
Preview
Old galaxies in the early universe Continuing our discussion of galaxy formation and evolution in the age of JWST, we saw previously that there appears to be a population of galaxies that grew rapidly in the early universe, attaininโ€ฆ

New blog post - Old galaxies in the early universe
tritonstation.com/2025/01/14/o...

14.01.2025 17:57 โ€” ๐Ÿ‘ 11    ๐Ÿ” 2    ๐Ÿ’ฌ 1    ๐Ÿ“Œ 1

Sort of an audiobook for a journal article. ๐Ÿ”ญ๐Ÿงช

08.01.2025 22:35 โ€” ๐Ÿ‘ 12    ๐Ÿ” 2    ๐Ÿ’ฌ 0    ๐Ÿ“Œ 0

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