Euclid Quick Data Release (Q1) The Strong Lensing Discovery Engine B -- Early strong lens candidates from visual inspection of high velocity dispersion galaxies

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Mar 19, 2025
18 pages
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Abstract: (arXiv)
We present a search for strong gravitational lenses in Euclid imaging with high stellar velocity dispersion (σν>180\sigma_\nu > 180 km/s) reported by SDSS and DESI. We performed expert visual inspection and classification of 1166011\,660\Euclid images. We discovered 38 grade A and 40 grade B candidate lenses, consistent with an expected sample of \sim32. Palomar spectroscopy confirmed 5 lens systems, while DESI spectra confirmed one, provided ambiguous results for another, and help to discard one. The \Euclid automated lens modeler modelled 53 candidates, confirming 38 as lenses, failing to model 9, and ruling out 6 grade B candidates. For the remaining 25 candidates we could not gather additional information. More importantly, our expert-classified non-lenses provide an excellent training set for machine learning lens classifiers. We create high-fidelity simulations of \Euclid lenses by painting realistic lensed sources behind the expert tagged (non-lens) luminous red galaxies. This training set is the foundation stone for the \Euclid galaxy-galaxy strong lensing discovery engine.
Note:
  • Paper submitted as part of the A&A Special Issue `Euclid Quick Data Release (Q1)', 18 pages, 9 figures
  • All the lensing galaxies proved to be early-type galaxies with
    • Ca ii H & K absorption and, generally, strong 4000 Å breaks
      • We obtained quality A redshifts for four lensed sources, all at z ∼ 2, as well as one quality B redshift at z = 2.316 (Fig. 6)
        • In most cases, the lensed background source was revealed as a slightly offset or extended blue emission line coincident with the early-type lensing galaxy. Since the emission features did not correspond to any strong, redshifted spectral features in earlytype galaxies (which generally do not have emission lines), the most plausible identifications were lensed Lyα at z ∼ 2. One lensed source, EUCL J175555.21+635718.7, does not show Lyα emission but instead shows the classic spectrum of a Lymanbreak galaxy with multiple absorption lines due to the interstellar medium. A detailed analysis and further follow-up of this target and EUCL J174907.29+645946.3, a possible double source plane candidate, will be presented in
          • Moustakas
          • 4.2. Additional available spectra
            • We visually inspected the available DESI and SDSS spectra for all 78 targets. We found that all ten redshift for the lens galaxies obtained from Palomar are in agreement with the redshifts previously reported. Regarding the source detections made by
              • Palomar, in most of the cases, the Lyα emission line is out of the
                • DESI spectra coverage or very near to the edge making its detection in DESI data impossible or unreliable. Additional spectral features were identified in only four targets, including the
                  • EUCL J175555.21+635718.7, the Lyman-break galaxy previously mentioned. Based on insights from Palomar spectroscopic data, we believe that in many cases, the emission or absorption lines may fall outside the observed spectral range or near the edges, where noise levels are high, making detection challenging. Additionally, the integration time may not have been sufficient to capture the often faint signals from the sources. The
                    • Table 2. Lens candidates in category B
                      • Name RA Dec zLens σv [km s-1
                        • VI score Modela
                          • θE[′′
                            • Discovery
                              • EUCL J174557.20+655632.7 266.488341 65.942430 0.60 218 1.15 N/- - This work
                                • EUCL J180007.48+631553.4 270.031189 63.264859 0.29 316 1.15 NM - This work
                                  • EUCL J180330.53+631941.8 270.877209 63.328302 0.92 236 1.10 NM - This work
                                    • EUCL J175605.62+635749.9 269.023418 63.963877 0.70 283 1.10 N/- - This work
                                      • EUCL J175149.82+635445.1 267.957618 63.912530 0.33 191 1.05 N/- - This work
                                        • EUCL J180621.71+663023.3 271.590471 66.506485 0.85 280 1.00 Y/Y 1.43 This work
                                          • EUCL J175633.58+662304.9 269.139948 66.384706 0.39 230 1.00 Y/Y 0.99 This work
                                            • EUCL J174704.75+655341.9 266.769824 65.894996 0.77 236 1.00 Y/Y 0.54 This work
                                              • EUCL J100130.52+021903.1 150.377170 2.317550 0.70 271 1.00 NM - [1]
                                                • EUCL J175943.34+642612.6 269.930605 64.436846 0.65 253 0.95 Y/Y 0.75 This work
                                                  • EUCL J180843.14+660735.6 272.179785 66.126567 0.22 292 0.95 Y/N - This work