DRAFT
2023-05-21 20:21:42
Type: Object/s-Data/Analysis
Bibcode: 2023TNSAN.129....1K
Multi-Band Photometric Follow-up of SN 2023ixf
Authors: M. R. Kendurkar (PGAO) and D. D. Balam (Dominion Astrophysical Observatory, National Research Council of Canada, 5071 West Saanich Road, Victoria, BC V9E 2E7, Canada)
Source Group: GSNST
Keywords: Transient, Supernova, Optical, Photometry
Abstract:
Photometric follow-up observations of SN 2023ixf

We have obtained SDSS g,r and i filter observations of SN 2023ixf in M101 using 1.8-m Plaskett Telescope (E2V, 4K x 2K CCD) at the (Dominion Astrophysical Observatory) of the National Research Council of Canada.

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Transient        UT                           g     error         r      error        i     error      host
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SN2023ixf     2023-05-20.407     12.95 (0.01)    13.34 (0.01)   13.50 (0.01)   M101
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The secondary standard was used from LAMOST DR7 catalogs (Luo+, 2019) 

The differential photometry was performed using Image Reduction and Analysis Facility (IRAF) (Tody, D. 1986, "The IRAF Data Reduction and Analysis System").

We thank the Royal Astronomical Society of Canada (Victoria Centre) and Friends of Dominion Astrophysical Observatory for their kind donation of telescope time on their public outreach night for target of opportunity.

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 2023ixf 14:03:38.564 +54:18:42.02 SN II 0.000804 M101 14:03:38.562 +54:18:41.94 SN II 0.0008

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