DRAFT
2023-06-08 10:44:56
Type: Object/s-Discovery/Classification
ZTF superluminous supernova candidates
Authors: Jacob Wise (LJMU), Daniel Perley (LJMU), Ragnhild Lunnan (OKC), Lin Yan (Caltech), Priscila Pessi, Jesper Sollerman, Steve Schulze, Anamaria Gkini, Sean Brennan (OKC)
Source Group: ZTF
Abstract:
We report 11 candidate ZTF superluminous supernova candidates from our scanning efforts. In this sample, a typical rise time is about 40 days and a typical peak r-band magnitude is 19. We encourage spectroscopic classifications.

The Zwicky Transient Facility (ZTF; Bellm et al. 2019; Graham et al. 2019) Superluminous Supernova Science Program (Lunnan et al. 2020; Yan et al. 2020; Chen et al. 2022a,b) reports 11 candidate SLSNe, following the methodology outlined by Perley et al. (in prep.)  We selected transients that have a long rise time (>20 days) and a faint or high-z host galaxy.

We summarise properties of the candidates in the Related Objects Table. These include coordinates, current magnitudes, approximate rise times, photometric redshifts of potential host galaxies (taken from the SDSS DR16 or the Legacy Survey DR9) and special remarks.

We will distribute alerts on such SLSN candidates via AstroNotes periodically; spectroscopic classifications and additional follow-up observations of these transients are encouraged.

This report is based on observations obtained with the Samuel Oschin Telescope 48-inch and the 60-inch Telescope at the Palomar Observatory as part of the Zwicky Transient Facility project. ZTF is supported by the National Science Foundation under Grant No. AST-2034437 and a collaboration including Caltech, IPAC, the Weizmann Institute for Science, the Oskar Klein Center at Stockholm University, the University of Maryland, Deutsches Elektronen-Synchrotron and Humboldt University, the TANGO Consortium of Taiwan, the University of Wisconsin at Milwaukee, Trinity College Dublin, Lawrence Livermore National Laboratories, and IN2P3, France. Operations are conducted by COO, IPAC, and UW.

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 2023fzh [ZTF23aagjjbn] 15:38:35.540 +25:13:29.38 SDSS J153836.39+251329.7 r~19.4. Light curve shows a 25 day rise to r~g~19.0 mag, then a slow decay, remaining blue after peak. Counterpart has r = 23.7 in LS and 22.33 in SDSS. First reported to TNS by Pan-STARRS as PS23bwh. 15:38:35.588 +25:13:29.34
TNS 2023hxm [ZTF23aahgpbd] 15:17:27.751 +10:39:09.70 SDSS J151727.73+103909.8 r~19.4. Light curve shows a rise of 20 days, then plateau, and possibly now a second rise as of one week ago. Counterpart in SDSS/LS with r=22.9. 15:17:27.751 +10:39:09.70
TNS 2023gpp [ZTF23aahjdxa] 16:44:02.551 +16:16:18.69 SDSS J164402.56+161617.6 r~19.8, g~20.2. Offset from a red, extended source with photo-z from SDSS/LS/PS1 of z~0.25, indicating M~-20.5 (accounting for Galactic extinction). Rise of 40 days (possibly on plateau for the past 20). 16:44:02.546 +16:16:18.62
TNS 2023gqz [ZTF23aafsqod] 12:05:19.232 +00:34:25.01 r~g~19.7. Light curve shows a rise over the first ~20 days and little fading over the following 30 days, with a persistent blue colour. A red, extended source is located 1.6 arcsec from the transient position in PS1 reference imaging. 12:05:19.232 +00:34:25.01
TNS 2023gbo [ZTF23aafrlmy] 23:41:42.345 +34:13:46.06 SDSS J234142.31+341345.9 i~19.1. Post-peak, emerging from morning twilight, was r ~ 18.5 when observations began and now fading slowly. In a very faint host (r~22.4 mag) with SDSS photo-z = 0.667 ± 0.187 23:41:42.345 +34:13:46.06
TNS 2023eqz [ZTF23aaekmhr] 22:29:46.648 +25:28:25.02 i~19. Emerging from morning twilight, probably currently at or near peak. No bright host counterpart, but there is a r~24 mag source ~1 arcsecond away and a r~22 mag source 4 arcseconds away in LS. 22:29:46.642 +25:28:25.00
TNS 2023dgd [ZTF23aadjnac] 14:19:47.391 +57:56:18.76 SDSS J141947.38+575618.0 r~19.6, g~20.2. The light curve is very flat and slow, with less than 0.5 mag of variation in any band over the past 80 days. Coincident with a faint (r~22.7 mag) and extended source with SDSS photo-z = 0.432 ± 0.100 14:19:47.391 +57:56:18.76
TNS 2023emk [ZTF23aadujra] 13:49:36.611 -00:57:44.17 SDSS J134936.49-005744.3 r~19.7. Very slow evolution (a few tenths of a mag of fading over the past 60 days). Offset by 1.5 arcsec from a high photo-z host (0.41 ± 0.14 in SDSS). 13:49:36.611 -00:57:44.17
TNS 2023gvn [ZTF23aadgqbi] 08:46:57.688 +30:49:22.22 SDSS J084657.69+304922.1 r~18.7. So far rising for almost 60 days with little colour evolution. Coincident with a pointlike SDSS/PS1/LS source with r=21.81 and an LS photo z = 0.313 +/- 0.160, but the amplitude of the ongoing rise is much larger than expected for normal QSO variability. 08:46:57.688 +30:49:22.22
TNS 2023ekh [ZTF23aadqcvq] 16:07:00.306 +05:05:45.01 SDSS J160700.26+050542.2 r~19.8. Slow-evolving, post-peak transient with a red colour (g-r ~ 0.5) and only slight fading over the past 80 days. On the outskirts of an red r = 18.88 galaxy with LS photo z = 0.192 +/- 0.023 and SDSS photo z = 0.189 ± 0.029, implying M < -20 for the transient. 16:07:00.306 +05:05:45.01
TNS 2023isu [ZTF23aajdusw] 11:54:35.317 +58:36:48.32 SDSS J115435.57+583647.1 g~r~19.6. Lightcurve shows a rise over the first 20 days, followed by a possible plateau over the following 20 days. Offset by 2.3 arcsec from a red r = 18.71 galaxy with LS photo z = 0.212 +/- 0.094 and SDSS photo z = 0.192 ± 0.0286, implying M < -20 for the transient. 11:54:35.317 +58:36:48.32

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