dc.date.accessioned | 2022-12-13T16:11:59Z | |
dc.date.available | 2022-12-13T16:11:59Z | |
dc.date.created | 2022-12-07T13:35:30Z | |
dc.date.issued | 2022 | |
dc.identifier.citation | Sukay, Ezra Khullar, Gourav Gladders, Michael D. Sharon, Keren Mahler, Guillaume Napier, Kate Bleem, Lindsey E. Dahle, Håkon Florian, Michael K. Gozman, Katya Lin, Jason J. Martinez, Michael N. Matthews Acuña, Owen S. Medina, Elisabeth Merz, Kaiya Sanchez, Jorge A. Sisco, Emily E. Stein, Daniel J. Kavin Tavangar, Kiyan Whitaker, Katherine E. . COOL-LAMPS. II. Characterizing the Size and Star Formation History of a Bright Strongly Lensed Early-type Galaxy at Redshift 1.02. The Astrophysical Journal (ApJ). 2022, 940(1) | |
dc.identifier.uri | http://hdl.handle.net/10852/98153 | |
dc.description.abstract | We present COOL J1323+0343, an early-type galaxy at z = 1.0153 ± 0.0006, strongly lensed by a cluster of galaxies at z = 0.353 ± 0.001. This object was originally imaged by DECaLS and noted as a gravitational lens by COOL-LAMPS, a collaboration initiated to find strong-lensing systems in recent public optical imaging data, and confirmed with follow-up data. With ground-based grzH imaging and optical spectroscopy from the Las Campanas Observatory and the Nordic Optical Telescope, we derive a stellar mass, metallicity, and star formation history from stellar-population synthesis modeling. The lens modeling implies a total magnification, summed over the three images in the arc, of μ ∼ 113. The stellar mass in the source plane is M* ∼ 10.64 M⊙ and the 1σ upper limit on the star formation rate (SFR) in the source plane is SFR ∼ 3.75 × 10−2 M⊙ yr−1 (log sSFR = −12.1 yr−1) in the youngest two age bins (0–100 Myr), closest to the epoch of observation. Our measurements place COOL J1323+0343 below the characteristic mass of the stellar mass function, making it an especially compelling target that could help clarify how intermediate-mass quiescent galaxies evolve. We reconstruct COOL J1323+0343 in the source plane and fit its light profile. This object is below the expected size evolution of an early-type galaxy at this mass with an effective radius re ∼ 0.5 kpc. This extraordinarily magnified and bright lensed early-type galaxy offers an exciting opportunity to study the morphology and star formation history of an intermediate-mass early-type galaxy in detail at z ∼ 1. | |
dc.language | EN | |
dc.rights | Attribution 4.0 International | |
dc.rights.uri | https://creativecommons.org/licenses/by/4.0/ | |
dc.title | COOL-LAMPS. II. Characterizing the Size and Star Formation History of a Bright Strongly Lensed Early-type Galaxy at Redshift 1.02 | |
dc.title.alternative | ENEngelskEnglishCOOL-LAMPS. II. Characterizing the Size and Star Formation History of a Bright Strongly Lensed Early-type Galaxy at Redshift 1.02 | |
dc.type | Journal article | |
dc.creator.author | Sukay, Ezra | |
dc.creator.author | Khullar, Gourav | |
dc.creator.author | Gladders, Michael D. | |
dc.creator.author | Sharon, Keren | |
dc.creator.author | Mahler, Guillaume | |
dc.creator.author | Napier, Kate | |
dc.creator.author | Bleem, Lindsey E. | |
dc.creator.author | Dahle, Håkon | |
dc.creator.author | Florian, Michael K. | |
dc.creator.author | Gozman, Katya | |
dc.creator.author | Lin, Jason J. | |
dc.creator.author | Martinez, Michael N. | |
dc.creator.author | Matthews Acuña, Owen S. | |
dc.creator.author | Medina, Elisabeth | |
dc.creator.author | Merz, Kaiya | |
dc.creator.author | Sanchez, Jorge A. | |
dc.creator.author | Sisco, Emily E. | |
dc.creator.author | Stein, Daniel J. Kavin | |
dc.creator.author | Tavangar, Kiyan | |
dc.creator.author | Whitaker, Katherine E. | |
cristin.unitcode | 185,15,3,0 | |
cristin.unitname | Institutt for teoretisk astrofysikk | |
cristin.ispublished | true | |
cristin.fulltext | original | |
cristin.qualitycode | 2 | |
dc.identifier.cristin | 2090092 | |
dc.identifier.bibliographiccitation | info:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=The Astrophysical Journal (ApJ)&rft.volume=940&rft.spage=&rft.date=2022 | |
dc.identifier.jtitle | The Astrophysical Journal (ApJ) | |
dc.identifier.volume | 940 | |
dc.identifier.issue | 1 | |
dc.identifier.pagecount | 9 | |
dc.identifier.doi | https://doi.org/10.3847/1538-4357/ac9974 | |
dc.subject.nvi | VDP::Astrofysikk, astronomi: 438 | |
dc.type.document | Tidsskriftartikkel | |
dc.type.peerreviewed | Peer reviewed | |
dc.source.issn | 0004-637X | |
dc.type.version | PublishedVersion | |
cristin.articleid | 42 | |