Euclid Quick Data Release (Q1). The Strong Lensing Discovery Engine F -- Bright and low-redshift strong lenses
Abstrak
We present 72 additional galaxy-galaxy strong lenses that complement the sample discovered in the Euclid Quick Release 1 data (63.1 deg^2) of the Strong Lens Discovery Engine (SLDE) papers A-E. It is shown that previous pre-selection of potential lenses, which excluded objects from the Gaia catalogue, led to missing several bright and low-redshift strong lenses, adding more than 10% new strong lens candidates compared to the previous search. In total, the catalogue includes 38"grade A"(confident) and 34"grade B"(probable) candidates. These lenses are identified through a combination of two independent searches for bright nearby objects: one based on machine-learning models followed by expert visual inspection, and the other based solely on expert visual inspection, targeting objects not included in the initial machine-learning selection (a limitation identified only after extensive visual inspection). With these additional strong lens candidates, we augment the expected number of high-confidence candidates in the Euclid Wide Survey from previous forecasts to 120000. Detailed semi-automated lens modelling confirms at least 41 systems out of 72, a fraction consistent with that found in SLDE A (315 out of 488). These include: multiple edge-on disc lenses; sources with arcs near the lens centre;"red sources"; and an edge-on disk galaxy lensing a galaxy merger, producing two sets of lensed features, an Einstein ring and a doubly imaged component. The median redshift of these systems is $\Delta$ z ~ 0.3 lower than that of the SLDE A sample.
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Penulis (500)
Euclid Collaboration L. R. Ecker
M. Fabricius
S. Seitz
R. Saglia
N. Lines
P. Holloway
T. Li
A. Verma
F. Balzer
Q. Jin
A. Manj'on-Garc'ia
S. H. Vincken
J. Wilde
J. Barroso
J. Nightingale
K. Rojas
S. Schuldt
M. Walmsley
T. Collett
G. Despali
A. Sonnenfeld
C. Tortora
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C. Saulder
E. Baeten
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K. Finner
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R. Gavazzi
L. C. Johnson
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A. More
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J. Pearson
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C. Scarlata
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Han Wang
X. Xu
F. Courbin
M. Meneghetti
N. Aghanim
B. Altieri
S. Andreon
N. Auricchio
C. Baccigalupi
M. Baldi
A. Balestra
S. Bardelli
P. Battaglia
A. Biviano
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