TNS Classification Report No. 20629 [ 2025TNSCR1136....1C ]
Date Received (UTC): 2025-03-25 11:02:24 Sender: Geza Csornyei
Group: adH0cc
G. Csoernyei, B. Leibundgut, J. Spyromilio (ESO), S. Taubenberger (TUM / MPA), W. Hillebrandt (MPA), S. Blondin (CNRS, LAM / ESO) report/s a classification of object: SN 2025dyr
Type: SN IIRedshift: 0.03426
Remarks: The SN shows broad P Cygni lines of H and He, indicating it is a Type II supernova. GELATO (Harutyunyan et al. 2008, 2008A&A...488..383H) found good matches with canonical SN II spectra two weeks after explosion. We adopted the redshift of the host for the supernova.
The following Classification spectrum was provided:
Obsdate: 2025-03-22 07:52:40
Instrument: FORS1
Telescope: The Very Large Telescope - UT1
Remarks: Quick-reduction spectrum
Details of the object and its spectra can be viewed here: https://www.wis-tns.org/object/2025dyr
Date Received (UTC): 2025-03-25 11:02:24 Sender: Geza Csornyei
Group: adH0cc
G. Csoernyei, B. Leibundgut, J. Spyromilio (ESO), S. Taubenberger (TUM / MPA), W. Hillebrandt (MPA), S. Blondin (CNRS, LAM / ESO) report/s a classification of object: SN 2025dyr
Type: SN IIRedshift: 0.03426
Remarks: The SN shows broad P Cygni lines of H and He, indicating it is a Type II supernova. GELATO (Harutyunyan et al. 2008, 2008A&A...488..383H) found good matches with canonical SN II spectra two weeks after explosion. We adopted the redshift of the host for the supernova.
The following Classification spectrum was provided:
Obsdate: 2025-03-22 07:52:40
Instrument: FORS1
Telescope: The Very Large Telescope - UT1
Remarks: Quick-reduction spectrum
Details of the object and its spectra can be viewed here: https://www.wis-tns.org/object/2025dyr