AstroNote 2024-220

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DRAFT
2024-08-14 06:16:51
Type: Object/s-Discovery/Classification
Hostless candidates detected by ELEPHANT
Authors: E. E. Hayes (KIC), R. Durgesh (independent), P. Pessi (OKC), E. E. O. Ishida (CNRS), 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 4 hostless candidates selected by the ELEPHANT pipeline.

Transient astronomical events that exhibit no evident association with a host galaxy are rare phenomena associated with 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, sumarized below. We encourage classification and follow up of these targets.

 
 
 
Show current TNS values
CatalogNameReported RAReported DECReported Obj-TypeReported RedshiftHost NameHost RedshiftRemarksTNS RATNS DECTNS Obj-TypeTNS Redshift
TNS2024rue [ZTF24abaalzx]21:30:35.302+19:40:27.94Supernova candidate. Light curve seems to be starting to decline.21:30:35.291+19:40:27.90
TNS2024rws [ZTF24aaywynf]21:50:40.105+07:07:06.68Supernova candidate. Light curve is around peak.21:50:40.104+07:07:06.45
TNS2024qxg [ZTF24aavxdpn]21:44:28.309+01:33:52.80Flagged as a SLSN I by NEEDLE (Astronote 2024-217, Sheng et al. 2024)21:44:28.309+01:33:52.80SLSN-I0.45
TNS2024rwv [ZTF24aazaydb]15:02:55.124+45:37:02.89Supernova candidate. Rising15:02:55.124+45:37:02.89