Transient Yield Report ======================= .. note:: This page is generated automatically from the latest published release, **v0.0.7alpha**, of UVEX Transients -- specifically its ``yield_summary.ecsv`` and ``detection_counts.ecsv`` data products (see :doc:`../user_guide`). It is regenerated on every documentation build, so it may lag between releases. Summary ======= .. list-table:: :header-rows: 1 :widths: 26 37 37 * - Transient Type - Detection Probability - Expected Detections * - Ia Sne - :math:`0.0189^{+0.000356}_{-0.000351}\,{}^{+0}_{-0}` - :math:`152,458^{+2,876}_{-2,834}\,{}^{+11,728}_{-11,728}` * - Type Ib SNe - :math:`0.0212^{+0.00157}_{-0.00149}\,{}^{+0}_{-0}` - :math:`10,423^{+773}_{-731}\,{}^{+4,690}_{-4,940}` * - Type Ic SNe - :math:`0.0296^{+0.00238}_{-0.00224}\,{}^{+0}_{-0}` - :math:`8,791^{+707}_{-667}\,{}^{+4,482}_{-4,669}` * - Icbl Sne - :math:`0.00367^{+0.000806}_{-0.000690}\,{}^{+0}_{-0}` - :math:`1,394^{+306}_{-262}\,{}^{+1,178}_{-1,476}` * - Type IIb SNe - :math:`0.00274^{+0.000519}_{-0.000453}\,{}^{+0}_{-0}` - :math:`1,834^{+347}_{-302}\,{}^{+834}_{-877}` * - Type IIP SNe (Excess) - :math:`0.0252^{+0.000413}_{-0.000408}\,{}^{+0}_{-0}` - :math:`200,609^{+3,284}_{-3,243}\,{}^{+59,338}_{-67,212}` * - Type IIP SNe - :math:`0.00698^{+0.000210}_{-0.000205}\,{}^{+0}_{-0}` - :math:`61,597^{+1,851}_{-1,808}\,{}^{+18,220}_{-20,637}` * - Kilonova - :math:`0^{+0.0392}_{-0}\,{}^{+0}_{-0}` - :math:`0^{+4.09}_{-0}\,{}^{+0}_{-0}` * - LFBOT - :math:`0.0888^{+0.0347}_{-0.0273}\,{}^{+0}_{-0}` - :math:`323^{+126}_{-99.6}\,{}^{+80.8}_{-294}` * - SLSNe (Magnetar) - :math:`0.0895^{+0.00540}_{-0.00518}\,{}^{+0}_{-0}` - :math:`14,260^{+860}_{-825}\,{}^{+5,335}_{-7,727}` * - Tidal Disruption Event - :math:`0.124^{+0.00771}_{-0.00740}\,{}^{+0}_{-0}` - :math:`12,966^{+806}_{-774}\,{}^{+2,510}_{-4,183}` Detections vs. Threshold ========================= For each transient type, the expected number of UVEX events detected in at least :math:`k` SNR-qualifying epochs, as :math:`k` increases. The narrow, black-capped bars are 90% Clopper-Pearson simulation-only uncertainty; the wide, pale bands are the event-rate uncertainty. .. tab-set:: .. tab-item:: Ia Sne .. image:: _images/ia_sne.png :width: 100% :align: center .. tab-item:: Type Ib SNe .. image:: _images/ib_sne.png :width: 100% :align: center .. tab-item:: Type Ic SNe .. image:: _images/ic_sne.png :width: 100% :align: center .. tab-item:: Icbl Sne .. image:: _images/icbl_sne.png :width: 100% :align: center .. tab-item:: Type IIb SNe .. image:: _images/iib_sne.png :width: 100% :align: center .. tab-item:: Type IIP SNe (Excess) .. image:: _images/iip_excess_sne.png :width: 100% :align: center .. tab-item:: Type IIP SNe .. image:: _images/iip_sne.png :width: 100% :align: center .. tab-item:: LFBOT .. image:: _images/lfbot.png :width: 100% :align: center .. tab-item:: SLSNe (Magnetar) .. image:: _images/slsne.png :width: 100% :align: center .. tab-item:: Tidal Disruption Event .. image:: _images/tde.png :width: 100% :align: center