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DECam Multimessenger Astrophysics Pipeline. I. From Raw Data to Single-exposure Candidates

  • Authors: Shenming Fu, Thomas Matheson, Aaron Meisner, Yuanyuan Zhang, Sebastián Vicencio, Destry Saul

Shenming Fu et al 2024 The Astronomical Journal 168 .

  • Provider: AAS Journals

Caption: Figure 3.

HiTS SN (both in the g band). Top panels: Blind15A_07_N2_1215_3860 (SNHiTS15H). Bottom panels: Blind15A_12_S28_0091_2772 (SNHiTS15bd). The blank regions are caused by CCD edges. Even though there is a bias artifact in the template, the pipeline still produces clean light curves. These two objects are both from the HiTS labeled set for ML training and thus have high credibility. We titled them with their names in HiTS (year, field, CCD, and pixel coordinates). The presentation and format here (and in the following Figures) are the same as in Figure 2.

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