{ "id": "2409.16236", "version": "v1", "published": "2024-09-24T16:52:41.000Z", "updated": "2024-09-24T16:52:41.000Z", "title": "Discover high-$z$ BL Lacs by {\\it Swift} and SARA observations with the dropout technique", "authors": [ "Y. Sheng", "K. Imam", "A. Kaur", "M. Ajello", "A. DomĂ­nguez", "A. Rau", "S. B. Cenko", "J. Greiner", "D. H. Hartmann", "I. Cox", "S. Joffre", "A. Mcdaniel", "R. Silver", "N. Torres-AlbĂ " ], "comment": "Updated the CGRH plot", "categories": [ "astro-ph.HE" ], "abstract": "The spectroscopic redshift measurement of BL Lac, a class of blazar, is challenging because its spectrum has no or weak emission lines ($\\leqslant5\\AA$). We estimate the redshift by the photometric dropout technique for a sample of 64 blazars (59 BL Lacs and five blazar candidates of uncertainty type). Two telescopes are utilized to observe the sample: the {\\it Swift} space telescope observes sources in $uvw2,\\ uvm2,\\ uvw1,\\ u,\\ b,\\ v$ filters, while the ground-based telescopes SARA-CT/RM observed sources in $g',\\ r,' \\ i',\\ z'$ filters. The photometric data are obtained using the {\\it photozpy} package. We fit the photometric data by the LePhare package and report four new high-$z$ ($z>1.3$) BL Lacs at $2.03^{+0.07}_{-0.05}$, $1.84^{+0.10}_{-0.03}$, $2.04^{+0.16}_{-0.14}$, $2.93^{+0.01}_{-0.04}$ as well as upper limits for 50 sources. The work increased the number of high-$z$ BL Lacs found by this method up to 23. The high-$z$ sources are discussed in the context of the cosmic gamma-ray horizon, blazar sequence, Fermi blazar divide, and masquerading BL Lacs.", "revisions": [ { "version": "v1", "updated": "2024-09-24T16:52:41.000Z" } ], "analyses": { "keywords": [ "bl lac", "sara observations", "photometric data", "cosmic gamma-ray horizon", "spectroscopic redshift measurement" ], "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable" } } }