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pith:IWEL75IG

pith:2026:IWEL75IGLGIT2AAT5JKYT444BU
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Revisiting the 2021 Outburst of the BHC MAXI J1803-298 Using NICER, NuSTAR, and Insight-HXMT Data

Kaushik Chatterjee, Sujoy K. Nath

LFQPOs in MAXI J1803-298 arise from the dynamically evolving inner accretion flow.

arxiv:2605.13232 v1 · 2026-05-13 · astro-ph.HE

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2 Internet Archive
3 Author claim open · sign in to claim
4 Citations open
5 Replications open
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Claims

C1strongest claim

The combined spectral and timing results support a scenario in which LFQPOs in MAXI J1803-298 arise from the dynamically evolving inner accretion flow.

C2weakest assumption

That the two-component advective flow (TCAF) model accurately captures the accretion geometry and yields an unbiased independent black hole mass estimate from the fitted shock location and flow parameters.

C3one line summary

Multi-instrument observations of MAXI J1803-298 link LFQPOs to the evolving inner Comptonizing accretion flow in the hard state, with TCAF modeling yielding a black hole mass estimate.

References

3 extracted · 3 resolved · 0 Pith anchors

[1] A., Cook, R., et al 2015
[2] A., Cook, R., et al 2022 · doi:10.1088/0004-637x/800/2/109
[3] 1989, in Timing Neutron Stars: proceedings of the NA TO Advanced Study Institute on Timing Neutron Stars held April 4-15, 27 Xu, Y ., & Harrison, F 2018

Formal links

2 machine-checked theorem links

Receipt and verification
First computed 2026-05-18T02:44:49.578344Z
Builder pith-number-builder-2026-05-17-v1
Signature Pith Ed25519 (pith-v1-2026-05) · public key
Schema pith-number/v1.0

Canonical hash

4588bff50659913d0013ea5589f39c0d3265ec314502f8ab3c86202cd9649eea

Aliases

arxiv: 2605.13232 · arxiv_version: 2605.13232v1 · doi: 10.48550/arxiv.2605.13232 · pith_short_12: IWEL75IGLGIT · pith_short_16: IWEL75IGLGIT2AAT · pith_short_8: IWEL75IG
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curl -sH 'Accept: application/ld+json' https://pith.science/pith/IWEL75IGLGIT2AAT5JKYT444BU \
  | 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: 4588bff50659913d0013ea5589f39c0d3265ec314502f8ab3c86202cd9649eea
Canonical record JSON
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    "primary_cat": "astro-ph.HE",
    "submitted_at": "2026-05-13T09:20:37Z",
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