DRAFT
2025-01-30 23:42:19
Type: Object/s-Discovery/Classification
Classification of Bright, Nearby Transients During Jan 23 - 27 2025
Authors: S. Karthik Yadavalli (Harvard/CfA), Yize Dong (Harvard/CfA), Kaylee de Soto (Harvard/CfA), V. Ashley Villar (Harvard/CfA), Matthew Grayling (Cambridge), Erin Hayes (Cambridge), Kaisey S. Mandel (Cambridge), Diego Farias (DARK/NBI), Christa Gall (DARK/NBI), Aprajita Hajela (DARK/NBI), Jens Hjorth (DARK/NBI), Luca Izzo (DARK/NBI), Danial Langeroodi (DARK/NBI), Aidan Sedgewick (DARK/NBI), Radek Wojtak, Sandra Raimundo (DARK/NBI+ U. Southampton), Charlie Kilpatrick (Northwestern), Steven Smartt (QUB/Oxford), Ken W. Smith (QUB/Oxford), Charlotte Angus (QUB), David Coulter (STScI), Justin Pierel (STScI), Armin Rest (STScI), Matthew Seibert (STScI), Prasiddha Arunachalam (UC Santa Cruz), Kyle W. Davis (UC Santa Cruz), Ryan J. Foley (UC Santa Cruz), Rav Kaur (UC Santa Cruz), Phillip Macias (UC Santa Cruz), Kishore Patra (UC Santa Cruz), César Rojas-Bravo (UC Santa Cruz), Enrico Ramirez-Ruiz (UC Santa Cruz), Kirsty Taggart (UC Santa Cruz), Ken C. Chambers (U Hawaii), David Jones (U Hawaii), Mark E. Huber (U Hawaii), Eugene A. Magnier (U Hawaii), R. J. Wainscoat (U Hawaii), Henna Abunemeh (UIUC), Nicholas Earl (UIUC), K. Decker French (UIUC), Ayan Mitra (UIUC), Tanner Murphey (UIUC), Jack O’Brien (UIUC), Haille Perkins (UIUC), Gautham Narayan (UIUC), Margaret Shepherd (UIUC), Margaret Verrico (UIUC), Amanda Wasserman (UIUC), Maria Drout (U. Toronto), Vivienne Baldasarre (Washington State University), Alexander Messick (Washington State University), Sandra Raimundo (U. Southampton), Katie Auchettl (University of Melbourne), Stephen Thorpe (Stockholm University), Yen-Chen Pan (National Central University)
Source Group: YSE
Abstract:
We report the classifications of 4 Type Ia's and 1 Type II.

Here we report on the classifications of 5 transients, triggered on Superphot+ (de Soto et. al, 2024, ApJ, 974, 169) candidates with >50% core-collapse probabilities and a latest ZTF observation brighter than 18.5 magnitudes in either the r- or g-band. We list the transients by name, newly found classifications, and time of spectroscopic observation below. All classifications are performed using SNID (Blondin & Tonry, 2007, ApJ, 666, 1024) and confirmed using Astrodash (Muthukrishna, Parkinson, and Tucker. ApJ 885.1: 85.). 

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 2025gp 16:32:13.314 +44:24:10.38 SN Ia 0.03 16:32:13.314 +44:24:10.38 SN Ia 0.03
TNS 2025nn 07:17:39.340 +43:49:03.12 SN Ia-91bg-like 0.05 07:17:39.340 +43:49:03.12 SN Ia-91bg-like 0.05
TNS 2025nz 17:01:09.870 +20:40:17.45 SN II 0.03 Z 110-23 0.03138 17:01:09.867 +20:40:17.61 SN II 0.03
TNS 2025xj 11:42:09.251 -18:41:04.81 SN Ia 0.05 11:42:09.241 -18:41:04.66 SN Ia 0.05
TNS 2025kx 02:50:36.157 +07:27:59.53 SN Ia 0.06 02:50:36.160 +07:27:59.53 SN Ia 0.06

Comments

Yize
Dong