Strongly lensed candidates from the HSC transient survey
Autor: | Anton T. Jaelani, Tomoki Morokuma, Cristian E. Rusu, Naoki Yasuda, Tohru Nagao, Sherry H. Suyu, James H. H. Chan, D. C. Y. Chao |
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Jazyk: | angličtina |
Rok vydání: | 2020 |
Předmět: |
Brightness
gravitational lensing data analysis quasar lenses selection FOS: Physical sciences Astrophysics Astrophysics::Cosmology and Extragalactic Astrophysics strong 01 natural sciences methods black-holes law.invention Search algorithm Observatory law 0103 physical sciences Instrumentation and Methods for Astrophysics (astro-ph.IM) 010303 astronomy & astrophysics cosmic evolution search Physics 010308 nuclear & particles physics space warps Astronomy and Astrophysics Quasar Astrophysics - Astrophysics of Galaxies Galaxy image processing Lens (optics) imaging sugohi Photometry (astronomy) Space and Planetary Science Feature (computer vision) Astrophysics of Galaxies (astro-ph.GA) gaia digital sky survey techniques Astrophysics - Instrumentation and Methods for Astrophysics discovery |
Popis: | We present a lensed quasar search based on the variability of lens systems in the HSC transient survey. Starting from 101,353 variable objects with i-band photometry in the HSC transient survey, we used a variability-based lens search method measuring the spatial extent in difference images to select potential lensed quasar candidates. We adopted conservative constraints in this variability selection and obtained 83,657 variable objects as possible lens candidates. We then ran CHITAH, a lens search algorithm based on the image configuration, on those 83,657 variable objects, and 2,130 variable objects were identified as potential lensed objects. We visually inspected the 2,130 variable objects, and seven of them are our final lensed quasar candidates. Additionally, we found one lensed galaxy candidate as a serendipitous discovery. Among the eight final lensed candidates, one is the only known quadruply lensed quasar in the survey field, HSCJ095921+020638. None of the other seven lensed candidates have been previously classified as a lens nor a lensed candidate. Three of the five final candidates with available HST images, including HSCJ095921+020638, show clues of a lensed feature in the HST images. A tightening of variability selection criteria might result in the loss of possible lensed quasar candidates, especially the lensed quasars with faint brightness or narrow separation, without efficiently eliminating the non-lensed objects; CHITAH is therefore important as an advanced examination to improve the lens search efficiency through the object configuration. The recovery of HSCJ095921+020638 proves the effectiveness of the variability-based lens search method, and this lens search method can be used in other cadenced imaging surveys, such as the upcoming Rubin Observatory Legacy Survey of Space and Time. 12 pages, 6 figures, accepted for publication in A&A |
Databáze: | OpenAIRE |
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