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pith:CIZNZNW5

pith:2026:CIZNZNW55475DQDQO26J3XEUCQ
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JWST high-contrast spectroscopy with speckle modelling: Atmospheric retrievals of the T dwarf companion HD 19467 B

Dar\'io Gonz\'alez Picos, Ignas Snellen, Jean-Baptiste Ruffio, Natalie Grasser, Sam de Regt, Tessa van der Post

Jointly fitting speckle contamination with the atmospheric model enables native-resolution retrievals of HD 19467 B from JWST/NIRSpec without continuum subtraction.

arxiv:2605.02769 v1 · 2026-05-04 · astro-ph.EP · astro-ph.SR

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Claims

C1strongest claim

Joint fitting of the atmospheric spectrum and the speckle contamination enables native-resolution retrievals of the high-contrast companion HD 19467 B with JWST/NIRSpec without continuum subtraction. Over 2.87--5.2 μm, medium-resolution spectroscopy constrains elemental and isotopic composition; both objects exhibit near-solar metallicity and subsolar C/O ratios.

C2weakest assumption

The assumption that a linear combination of integral-field-unit speckle spectra fully captures the wavelength-dependent residual stellar contamination without residual biases that propagate into the retrieved molecular abundances or isotopic ratios.

C3one line summary

Joint speckle-atmosphere retrievals on JWST spectra of HD 19467 B and a field T dwarf detect H2O, CH4, CO, CO2 and NH3, yield carbon isotopic ratios of 154 and 85 respectively, and show near-solar metallicity with subsolar C/O.

References

297 extracted · 297 resolved · 5 Pith anchors

[1] The Astrophysical Journal Supplement Series , keywords = · doi:10.3847/1538-4365/ac4414
[2] Abel, Martin and Frommhold, Lothar and Li, Xiaoping and Hunt, Katharine L. C. , doi =. Collision-. J. Phys. Chem. A , month =
[3] Accretion in Brown Dwarfs:
[4] doi:10.1086/321540 , eprint = · doi:10.1086/321540
[5] Zh and Sousa, S · doi:10.1051/0004-6361/201219401
Receipt and verification
First computed 2026-06-24T14:15:59.113826Z
Builder pith-number-builder-2026-05-17-v1
Signature Pith Ed25519 (pith-v1-2026-05) · public key
Schema pith-number/v1.0

Canonical hash

1232dcb6ddef3fd1c07076bc9ddc94141599b12664a3a5d1bba7e1704681a507

Aliases

arxiv: 2605.02769 · arxiv_version: 2605.02769v1 · doi: 10.48550/arxiv.2605.02769 · pith_short_12: CIZNZNW55475 · pith_short_16: CIZNZNW55475DQDQ · pith_short_8: CIZNZNW5
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Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/CIZNZNW55475DQDQO26J3XEUCQ \
  | 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: 1232dcb6ddef3fd1c07076bc9ddc94141599b12664a3a5d1bba7e1704681a507
Canonical record JSON
{
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    "license": "http://creativecommons.org/licenses/by/4.0/",
    "primary_cat": "astro-ph.EP",
    "submitted_at": "2026-05-04T16:09:12Z",
    "title_canon_sha256": "d601686794cc3c8558f2dfda739690f96bf7c8a1cda4732489fc82fec5fe654d"
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  "source": {
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    "kind": "arxiv",
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