AstroNote 2024-231

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DRAFT
2024-08-28 16:07:38
Type: Object/s-Discovery/Classification
SLSN and TDE candidates from NEEDLE on Lasair
Authors: X. Sheng, M. Nicholl, K. W. Smith, C. R. Angus, A. Aamer, 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 2 SLSN and 2 TDE candidates and 1 red, long-rising transient 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 2 SLSN and 2 TDE candidates, and one ambiguous object.

2024sbm [ZTF24aaybwcs] shows a slow rise similar to SLSNe, but is quite red (g-r~0.3). Its host galaxy shows an irregular morphology but may be blended with a foreground star.

2024rny[ZTF24aazlori] was initially suggested as a SLSN candidate by NEEDLE (AstroNote 2024-222), however, given its location at the centre of its host and persistent blue colour, it is now more confidently predicted as a TDE candidate.

2023aclf [ZTF23abscfuu] was first discovered on 2023-11-10, and has been rising for over 290 days. Its smooth rise and lack of previous variability are unlike AGN activity. 

 We encourage spectroscopic classification and follow-up.

Show current TNS values
CatalogNameReported RAReported DECReported Obj-TypeReported RedshiftHost NameHost RedshiftCandidate typeLatest magnitudeRemarksTNS RATNS DECTNS Obj-TypeTNS Redshift
TNS2024rrk [ZTF24aaxucpk]17:10:52.671+39:07:57.03SLSNr = 19.88±0.14https://lasair-ztf.lsst.ac.uk/objects/ZTF24aaxucpk/17:10:52.671+39:07:57.03
TNS2024qkt [ZTF24aaxavnf]15:57:36.654+45:28:41.23SDSS J155736.60+452841.0SLSNr = 19.02±0.13https://lasair-ztf.lsst.ac.uk/objects/ZTF24aaxavnf/15:57:36.654+45:28:41.23
TNS2024sbm [ZTF24aaybwcs]16:13:34.030+28:34:08.06Ambiguousr = 19.66±0.21https://lasair-ztf.lsst.ac.uk/objects/ZTF24aaybwcs/16:13:34.030+28:34:08.06
TNS2024rny [ZTF24aazlori]22:57:28.808+39:25:44.37PS1 155313443699515427TDEr = 19.69±0.12https://lasair-ztf.lsst.ac.uk/objects/ZTF24aazlori/ - This object was previously predicted as SLSN, however, it is re-classified as TDE with photometric evolution.22:57:28.808+39:25:44.37TDE0.1055
TNS2023aclf [ZTF23abscfuu]07:48:19.591+28:15:53.88TDEr = 18.57±0.15https://lasair-ztf.lsst.ac.uk/objects/ZTF23abscfuu/ - This object has been rising for over 290 days. From PanSTARRS survey, its variability before MJD 60259.42 is much lower than current growing, therefore it is less likely to be a normal AGN variability.07:48:19.591+28:15:53.88