Pith Number

pith:5GGEKKBP

pith:2026:5GGEKKBP4RZF34W3KPFU5SLVNB

not attested not anchored not stored refs resolved

Clusters Hiding Under Millimeter Sources (CHUMS) I: Extreme CHUMS

Adam B. Mantz, Denise G. Yudovich, Harshda Saxena, Jack Sayers, Steve W. Allen

Subtracting central AGN emission from millimeter maps reveals previously hidden galaxy clusters.

arxiv:2605.15444 v1 · 2026-05-14 · astro-ph.CO · astro-ph.GA

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\usepackage{pith}
\pithnumber{5GGEKKBP4RZF34W3KPFU5SLVNB}

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Record completeness

1 Bitcoin timestamp

2 Internet Archive

3 Author claim open · sign in to claim

4 Citations open

5 Replications open

✓ Portable graph bundle live · download bundle · merged state

The bundle contains the canonical record plus signed events. A mirror can host it anywhere and recompute the same current state with the deterministic merge algorithm.

Claims

C1strongest claim

We present signal to noise ratio (SNR) estimates for the clusters after subtracting the AGN signal from 90 GHz ACT maps using the CARMA measurements, demonstrating high SNR cluster detections once this contaminating emission is removed.

C2weakest assumption

The AGN flux measured by CARMA at one epoch can be directly subtracted from ACT maps taken at different times, with the low observed variability justifying the assumption that the AGN emission level is stable enough for accurate subtraction.

C3one line summary

AGN emission from central galaxies hides galaxy clusters in SZ surveys; CARMA-based subtraction recovers high-SNR detections in ACT maps for three specific clusters.

References

79 extracted · 79 resolved · 4 Pith anchors

[1] doi:10.1103/PhysRevD.102.023509 , keywords = 2020 · doi:10.1103/physrevd.102.023509

[2] Ade, P. A. R., Aghanim, N., Armitage-Caplan, C., et al. 2014, Astronomy & Astrophysics, 571, A8, doi: 10.1051/0004-6361/201321538 10 T able 3.List of targets with details of the archival CARMA dat 2014 · doi:10.1051/0004-6361/201321538

[3] The Open Journal of Astrophysics , keywords = 2026 · doi:10.33232/001c.155863

[4] 2017, Astronomy & Astrophysics, 607, A122, doi: 10.1051/0004-6361/201630311 2017 · doi:10.1051/0004-6361/201630311

[5] W., Evrard , A 2011 · doi:10.1146/annurev-astro-081710-102514

Receipt and verification

First computed	2026-05-20T00:00:58.932258Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

e98c45282fe4725df2db53cb4ec9756879746e9114689c72793e4ebdb8697bde

Aliases

arxiv: 2605.15444 · arxiv_version: 2605.15444v1 · doi: 10.48550/arxiv.2605.15444 · pith_short_12: 5GGEKKBP4RZF · pith_short_16: 5GGEKKBP4RZF34W3 · pith_short_8: 5GGEKKBP

Agent API

Resolver JSON Graph JSON Events JSON Schema Signing key

Verify this Pith Number yourself

curl -sH 'Accept: application/ld+json' https://pith.science/pith/5GGEKKBP4RZF34W3KPFU5SLVNB \
  | jq -c '.canonical_record' \
  | python3 -c "import sys,json,hashlib; b=json.dumps(json.loads(sys.stdin.read()), sort_keys=True, separators=(',',':'), ensure_ascii=False).encode(); print(hashlib.sha256(b).hexdigest())"
# expect: e98c45282fe4725df2db53cb4ec9756879746e9114689c72793e4ebdb8697bde

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "148017d07505ef99117e96d3b198e438e04d2910e683bf762e8fbd84c7c12b00",
    "cross_cats_sorted": [
      "astro-ph.GA"
    ],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "primary_cat": "astro-ph.CO",
    "submitted_at": "2026-05-14T21:58:46Z",
    "title_canon_sha256": "6138990454cd09b2769135d29e12650bf492278f75663d7ff98c69096820fe72"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2605.15444",
    "kind": "arxiv",
    "version": 1
  }
}