2026A&A...706A.364G


Query : 2026A&A...706A.364G

2026A&A...706A.364G - Astronomy and Astrophysics, volume 706A364 (2026/2-1)

Mysteries of Capotauro: Investigating the puzzling nature of an extreme F356W-dropout.

GANDOLFI G., RODIGHIERO G., CASTELLANO M., FONTANA A., SANTINI P., DICKINSON M., FINKELSTEIN S., CATONE M., CALABRO A., MERLIN E., PENTERICCI L., BISIGELLO L., GRAZIAN A., NAPOLITANO L., VULCANI B., TAYLOR A.J., ARRABAL HARO P., KIRKPATRICK A., BACKHAUS B.E., HOLWERDA B.W., GIULIETTI M., BIANCHETTI A., CASSATA P., CLERI N.J., DADDI E., FERGUSON H.C., GIRARDI G., HIRSCHMANN M., KOEKEMOER A.M., LAPI A., PACUCCI F., PEREZ-GONZALEZ P.G., DE LA VEGA A., VIETRI A., WILKINS S., YUNG L.Y.A., BAGLEY M., BHATAWDEKAR R., KARTALTEPE J., PAPOVICH C. and PIRZKAL N.

Abstract (from CDS):

Context. The James Webb Space Telescope (JWST) has uncovered a diverse population of extreme near-infrared dropouts, including ultra-high-redshift (z > 15) galaxy candidates, dust-obscured galaxies challenging theories of dust production, sources with strong Balmer breaks (possibly compact active galactic nuclei in dense gas-rich environments), and cold, substellar Galactic objects.
Aims. This work presents Capotauro, a F356W-dropout identified in the CEERS survey with a F444W AB magnitude of ∼27.68 and exhibiting a sharp flux drop by > 3 mag between 3.5 and 4.5 μm, being nondetected below 3.5 μm. We investigated its nature and constrained its properties, paving the way for follow-up observations.
Methods. We combined JWST/NIRCam, MIRI, and NIRSpec/MSA data with HST/ACS and WFC3 observations to perform a spectrophotometric analysis of Capotauro using multiple SED-fitting codes. Our setup is tailored to test z ≥ 15 as well as z < 10 dusty, Balmer-break or strong-line emitter galaxy solutions, and the possibility of Capotauro being a Milky Way substellar object.
Results. Among extragalactic options, our analysis favors interpreting the sharp flux drop of Capotauro as a bright (MUV ∼ -21.5) Lyman break at z ∼ 32, consistent with the formation epoch of the first stars and black holes, with only ∼0.5% of the redshift posterior volume lying at z < 25. Lower-redshift solutions struggle to reproduce the extreme break, suggesting that if Capotauro resides at z < 10, it must show a nonstandard combination of high dust attenuation and/or prominent Balmer breaks, making it a peculiar interloper. Finally, our analysis indicates that Capotauro's properties could be consistent with it being a very cold (i.e., Y2-Y3 type) brown dwarf or a free-floating exoplanet with a record-breaking combination of low temperature and large distance (Teff ≤ 300 K; d ≳ 130 pc, up to ∼2 kpc).
Conclusions. While present observations cannot determine Capotauro's nature, our analysis points to a remarkably unique object in all plausible scenarios. This makes Capotauro stand out as a compelling target for follow-up observations.

Abstract Copyright: © The Authors 2026

Journal keyword(s): brown dwarfs - galaxies: evolution - galaxies: formation - galaxies: high-redshift

Status at CDS : Acronym for new objects described in the dictionary of nomenclature and being created in SIMBAD.

Simbad objects: 10

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Number of rows : 10
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NAME SMC G 00 52 38.0 -72 48 01   2.79 2.2     ~ 12317 1
2 NGC 1333 OpC 03 29 09.2 +31 20 59           ~ 1575 1
3 WISE J035934.06-540154.6 BD* 03 59 34.24998 -54 01 46.4287           Y0 43 0
4 ClG J0647+7015 ClG 06 47 50.0 +70 14 55           ~ 177 0
5 WISEA J085510.74-071442.5 BD* 08 55 16.53798 -07 14 49.3728           Y2 124 0
6 NAME COSMOS Field reg 10 00 28.60 +02 12 21.0           ~ 3639 0
7 NAME CAPERS-LRD-z9 AGN 10 00 32.7008 +02 18 28.907           ~ 8 0
8 NAME Extended Groth Strip reg 14 19 +52.8           ~ 1023 0
9 [ADF2023b] MSA ID 0 G 14 19 39.490 +52 56 34.94           ~ 28 0
10 Z 49-122 G 15 19 05.7764474544 +03 22 01.709925708   15.89       ~ 17 0

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