CERIN AMROTH · RESEARCH

LRD Watch DR1 · candidate

LRDW J131124.16-012204.4

candidate tableSILVERmain classcolour laneAbell 1689
RA 13:11:24.166 197.8506925°
Dec −01:22:04.49 -1.3679151°

Images

No image stamps: the mosaics this object was measured on are not on disk.

Spectral energy distribution

11.523451310301004000500060008000100001500020000Balmer limitrest frame (Å) at z = 1.200, adopted by vettingobserved wavelength (µm)flux density (nJy)
  • NIRCam wide
  • NIRCam medium
  • 2σ upper limit (S/N < 2)
Aperture fluxes in a 0.16″-radius circle, not corrected to total; the values are in the photometry table below. The gold line marks the Balmer limit (3646 Å rest) at z = 1.200.

At a glance

Tier
SILVER main class
Found by
colour lane
Redshift
1.20 colour-lane fit
Spectral shape
no labelled spectrum
F444W
27.70 AB S/N 10, 0.16″ aperture
F277W − F444W
2.17 mag strict redness
BH* share
not in the BH* channel
Compactness
FWHM 0.166″
Balmer break
not measured
Image vetting
half-stack pass; no flags raised
Literature
no published match within 1″

Vetting

  • Image vettingpassed
  • Half-stack testpass
  • Artifact risknone
  • Neighbournone
  • Extendedno
  • No vetting notes.

Redshifts

Each redshift keeps its own column. Photometric redshifts of little red dots are unreliable: against spectra, about a third of AGN-template redshifts (z_agn; 31 of 95 in the last purity run) and about half of galaxy-template redshifts at z > 3 were catastrophic outliers (methods Section 8).

ColumnWhat it iszSource
z_specSpectroscopic, DJA grade 3——
z_vetAdopted by vetting1.2000z_agn
z_photPhotometric (P(z) peak)9.07468%: 9.002–12.047
z_bhsBH* channel fit——
z_agnColour-lane fit1.20AGN-inclusive templates

Spectral checks

V-shape (spectrum)
no labelled spectrum
Star (spectrum)
no spectrum
V-shape (photometry)
not measurable βUV not measured, βopt not measured at z_agn
Line in F410M
none 0 line-free optical band(s)
Line-ambiguous
no
Settling verdict
not evaluated

Literature

Published objects within 1″ of this position. A match is a positional recovery, not an adopted classification.

  • No published JWST little red dot or broad-line AGN within 1″.

Photometry

Circular aperture of radius 0.16″ at each band's native resolution, background from a 0.40–0.65″ annulus, programmes combined by inverse variance. For a point source multiply by the field's aperture correction (r = 0.16″ → 0.70″). Grey rows are below S/N 2.

BandInstrumentPivot (µm)f (nJy)σ (nJy)AB magS/NAp. corr.
F090WNIRCam wide0.9028.836.6929.041.31.18
F115WNIRCam wide1.1549.143.6729.002.51.16
F150WNIRCam wide1.50153.147.9727.096.71.11–1.14
F182MNIRCam medium1.8450.473.2532.220.11.17
F200WNIRCam wide1.9891.732.8230.810.61.16
F210MNIRCam medium2.09565.178.6426.867.51.12
F277WNIRCam wide2.7624.061.7729.882.31.29
F300MNIRCam medium2.990−0.722.14—−0.31.28
F356WNIRCam wide3.56825.783.6527.877.11.28–1.32
F410MNIRCam medium4.08219.654.5428.174.31.28
F444WNIRCam wide4.40430.093.0927.709.71.34

Provenance

Field
Abell 1689 (a1689)
Programmes
05782, 06882 behind every mosaic the field measured
Pipeline rows merged
2 all at one position
Detection pass
original
Release build
33af9933d1cc 2026-10-17T14:29:44Z

Cite

Anderson, Jordan (2026). LRD Watch DR1: little red dot candidates from an independent search of public JWST imaging (Version DR1) [Data set]. Cerin Amroth Research. Zenodo. https://doi.org/10.5281/zenodo.23062632 Object LRDW J131124.16-012204.4.

CC BY 4.0. Please also acknowledge the JWST programmes that took the data. LRD Watch DR1 is a vetted candidate catalogue, not a complete census: it has no selection function and cannot on its own give number densities. About the release.