DRAFT
2024-09-11 15:45:18
Type: Object/s-Discovery/Classification
SLSN and TDE candidates from NEEDLE on Lasair
Authors: A. Aamer, C. R. Angus, X. Sheng, M. Nicholl, K. W. Smith, M. Fulton, T. Moore, J. Weston, D. R. Young (QUB), P. Ramsden (Birmingham/QUB), S. J. Smartt (Oxford/QUB), S. Srivastav, H. Stevance (Oxford), A. Sankar. K (NCU)
Source Group: OxQUB
Abstract:
We report 7 SLSN and 2 TDE candidates from the ZTF public alert stream, identified by the NEEDLE classifier running on the Lasair alert broker. We encourage spectroscopic classification of these events.

The Neural Engine for Discovering Luminous Events (NEEDLE) classifier (Sheng et al. 2024) is a machine-learning tool for identifying rare astronomical transients from real-time alerts. NEEDLE is trained to identify Superluminous Supernova (SLSN) and Tidal Disruption Events (TDE) candidates in data from the Zwicky Transient Facility (ZTF; Bellm et al. 2019; Graham et al. 2019). We are running NEEDLE daily on public ZTF alerts, streamed via the Lasair alert broker (Williams et al. 2024), and publicly providing classification predictions as annotations on Lasair.

We provide three SQL filters on Lasair with our candidates (also output as Kafka streams): NEEDLE SLSN candidates, NEEDLE TDE candidates, and all NEEDLE annotations. Lasair users can also incorporate NEEDLE outputs into their own custom SQL filters.

We manually vet all alerts with a SLSN or TDE score > 0.5, and will highlight the most promising candidates in these AstroNotes. A complete set of candidates can be found in the Lasair streams. This report includes recent SLSN and TDE candidates, shown below. We encourage spectroscopic classification and follow-up.

Show current TNS values
Catalog Name Reported RA Reported DEC Reported Obj-Type Reported Redshift Host Name Host Redshift Candidate type Latest magnitude Remarks TNS RA TNS DEC TNS Obj-Type TNS Redshift
TNS 2024uql [ZTF24abfduvm] 00:30:17.972 +46:22:08.50 SLSN r = 19.77±0.14 https://lasair-ztf.lsst.ac.uk/objects/ZTF24abfduvm/ 00:30:17.978 +46:22:08.63
TNS 2024twp [ZTF24abdlusb] 22:52:49.842 +32:02:55.04 SLSN r = 19.00±0.09 https://lasair-ztf.lsst.ac.uk/objects/ZTF24abdlusb/ 22:52:49.836 +32:02:54.96
TNS 2024uap [ZTF24abdjezn] 00:19:24.295 +39:29:33.53 SLSN r = 18.70±0.06 https://lasair-ztf.lsst.ac.uk/objects/ZTF24abdjezn/ 00:19:24.295 +39:29:33.53 SN Ia 0.085
TNS 2024szv [ZTF24abcyoby] 21:10:45.315 +17:57:26.12 SDSS J211045.43+175723.7 SLSN r = 19.72±0.15 https://lasair-ztf.lsst.ac.uk/objects/ZTF24abcyoby/ 21:10:45.312 +17:57:26.05
TNS 2024sll [ZTF24abccufc] 16:32:18.119 +49:50:56.04 SLSN g = 18.87±0.11 https://lasair-ztf.lsst.ac.uk/objects/ZTF24abccufc/ - Blue transient with a rise time of >30 days. The host is a massive spiral galaxy, which is very unusual for SLSNe but not unprecedented 16:32:18.119 +49:50:56.04
TNS 2024syk [ZTF24abcwfbp] 01:05:39.540 +35:03:52.50 SLSN g = 20.11±0.17 https://lasair-ztf.lsst.ac.uk/objects/ZTF24abcwfbp/ 01:05:39.540 +35:03:52.50
TNS 2024uez [ZTF24abempjh] 21:51:10.866 +31:09:33.30 PS1 145393277952332063 SLSN r = 20.14±0.19 https://lasair-ztf.lsst.ac.uk/objects/ZTF24abempjh/ 21:51:10.866 +31:09:33.30
TNS 2024uip [PS24ikt] 00:17:48.939 +21:42:05.64 TDE r = 20.39±0.19 https://lasair-ztf.lsst.ac.uk/objects/ZTF24aaxzvia/ 00:17:48.939 +21:42:05.64
TNS 2024uqm [ZTF24abfhjot] 15:45:53.957 +12:12:06.53 TDE r = 19.22±0.12 https://lasair-ztf.lsst.ac.uk/objects/ZTF24abfhjot/ 15:45:53.957 +12:12:06.53

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