DRAFT
2025-01-07 20:40:15
Type: Object/s-Discovery/Classification
Hostless candidates detected by ELEPHANT
Authors: R. Durgesh (independent), P. Pessi (OKC), E. E. O. Ishida (CNRS), E. E. Hayes (KIC), L. Nakazono (USP), R. A. P. Oliveira (UW), A. Moitinho (CENTRA), A. Krone-Martins (UC), B. Moews (UE), R. S. de Souza (UH), R. Beck (independent), M. A. Kuhn (UH), K. Nowak (UH), and S. Vaughan (MU), for the COIN collaboration.
Source Group: COIN
Abstract:
We report 12 hostless candidates selected by the ELEPHANT pipeline.

Transient astronomical events that exhibit no evident association with a host galaxy are rare phenomena associated with extremely energetic events. They can offer unique insights into the properties and evolution of stars and galaxies. In this context, we developed the ELEPHANT pipeline (Pessi et al. 2024) to process alerts from the Zwicky Transient Facility (ZTF; Bellm et al. 2019; Graham et al. 2019) ingested by the Fink broker (Möller et al. 2021) and automatically find hostless candidates. 

This report includes recent hostless candidates, summarized below. We encourage classification and follow up of these targets.

These candidates were found through a dedicated Telegram bot, publicly available at https://t.me/fink_hostless .  This is part of a series of public bots made available by Fink. The full list can be found here.

Show current TNS values
Catalog Name Reported RA Reported DEC Reported Obj-Type Reported Redshift Host Name Host Redshift Remarks TNS RA TNS DEC TNS Obj-Type TNS Redshift
TNS 2024aemi [ZTF24abybmsk] 03:51:39.167 -16:24:30.58 Supernova candidate. Just past peak. 03:51:39.167 -16:24:30.58
TNS 2024aeon [ZTF24abyjjjt] 04:04:25.356 -10:07:31.34 Supernova candidate. Around peak. 04:04:25.356 -10:07:31.34
TNS 2024adge [ZTF24abvkybi] 00:39:31.433 +70:43:33.45 Flagged as a SLSN candidate by NEEDLE (Astronote 2024-378, Aamer et al. 2024) 00:39:31.433 +70:43:33.45
TNS 2024aenw [ZTF24abyiwzh] 05:17:08.075 -14:58:46.26 Supernova candidate. Around peak. 05:17:08.075 -14:58:46.26
TNS 2024aeev [ZTF24abydgdk] 23:12:11.741 +11:54:38.53 Supernova candidate. Light curve shows a possible 2 week long plateau. 23:12:11.741 +11:54:38.53
TNS 2024aezo [ZTF24abwsvtj] 13:24:17.079 +27:43:01.10 Supernova candidate. Light curve seems to have been slowly rising for the last 30 days. 13:24:17.079 +27:43:01.10
TNS 2024afro [ZTF24abzjfdz] 11:04:54.303 +78:55:38.84 Supernova candidate. Reported as an early SN Ia candidate by Fink. 11:04:54.303 +78:55:38.84
TNS 2024aefk [ZTF24abwmcrv] 23:50:26.836 +37:10:24.04 Supernova candidate. Reported as a SN Ia candidate by Fink. 23:50:26.836 +37:10:24.04
TNS 2017edo [Gaia17bgw] 23:09:29.950 +43:55:21.32 This source has been recently detected as ZTF24abxhdum. It has declined ~0.8mag in around 2 weeks. This decline is consistent with the transient being a CV. This source was first discovered by Gaia in 2017. Pre-outburst activity can be found on the ZTF DR from 2018 until 2023. 23:09:29.950 +43:55:21.32
TNS 2024adxt [ZTF24abwzbei] 15:15:10.232 +10:26:57.78 Supernova candidate. Slowly rising for ~20days. It seems to be declining fast now. 15:15:10.232 +10:26:57.78
TNS 2024aetw [ZTF24abydfcn] 00:19:53.353 -22:07:39.29 Supernova candidate. Just past peak. 00:19:53.353 -22:07:39.29
TNS 2024agid [ZTF24abzvwfa] 09:33:04.831 +56:39:32.96 Supernova candidate. Rising or around peak. 09:33:04.831 +56:39:32.96

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