DRAFT
2023-06-29 23:27:20
Type: Object/s-Data/Analysis
Photometric Follow-Up observations of specific optical transients from DAO
Authors: D. D. Balam (Dominion Astrophysical Observatory, National Research Council of Canada), M. R. Kendurkar (GSNST)
Source Group: GSNST
Abstract:
We have obtained SDSS u, g and r filter observations of specific optical transients discovered by ZTF (Fremling, C., et al.), Pan-STARRS (Chambers, K.C., et al.), ATLAS (Tonry, J., et al), A. Horti-David, et al and K.Itagaki. The photometric observations and colour index were done using 1.8-m Plaskett Telescope (E2V, 4K x 2K CCD) at the Dominion Astrophysical Observatory of the National Research Council of Canada.
Name          UTC       u   (error)      g      (error)     r       (error)    u-g      g-r
2022wsu 2022-10-05.369    ------------    16.76 (0.01)    16.26 (0.01)     +0.50
2022yax 2022-10-20.191

   ------------

   20.20 (0.01)   18.95 (0.01)    

 +1.25

2022yax 2022-10-25.206    ------------    20.85 (0.01)   ------------  -----    -----
2023ixf 2023-06-23.316    ------------    11.93 (0.01)    11.61 (0.01)     +0.20
2023lhb 2023-06-23.446    ------------    17.14 (0.01)    ------------  -----   -----
2023lhy 2023-06-23.446    ------------    17.10 (0.02)    ------------   -----   -----
2023lgz 2023-06-23.379    ------------    17.21 (0.02)    ------------  -----   -----
2023lkw 2023-06-24.259    ------------    17.55 (0.01)    ------------  -----   -----
2023ixf 2023-06-27.253    12.53 (0.01)    ------------      11.85 (0.01)  -----   -----
2023lpa 2023-06-27.360    ------------    18.20 (0.01)    ------------  -----   ------
2023lya 2023-06-28.374    ------------    17.40 (0.01)    ------------  -----   ------

 

 *secondary standards are as follows; 2MASS 14040276+5418180, 2MASS J23270681+4135467, SDSS  J164845.48+413436.5, SDSS  J160953.21+153528.9, SDSS  J164733.01+521940.5, 2MASS J18415625+4956224, SDSS  J172844.13+582236.9 and 2MASS 00433834+4115321.
 
 
 Several different secondary standards were used from SDSS DR16 (Ahumada+, 2020), LAMOST DR7 catalogs (Luo+, 2019), All-sky spectrally matched Tycho2 stars (Pickles+, 2010) and PS1 Survey DR1 (Chambers+, 2016) to perform differential photometry using Image Reduction and Analysis Facility (IRAF) (Tody, D. 1986, "The IRAF Data Reduction and Analysis System").

 

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 2022wsu 02:16:11.652 +17:58:15.44 SN Ia 0.027 02:16:11.652 +17:58:15.44 SN Ia 0.027
TNS 2022yax 00:43:45.854 +41:15:58.61 M31 00:43:45.854 +41:15:58.61
TNS 2023ixf 14:03:38.562 +54:18:41.94 SN II 0.000804 M101 14:03:38.562 +54:18:41.94 SN II 0.0008
TNS 2023lhb 23:27:11.590 +41:36:32.45 23:27:11.599 +41:36:32.45 SN Ia 0.049
TNS 2023lhy 16:09:50.314 +15:35:54.91 SN Ia 0.046 2MASX J16095004+1535552 0.04612 16:09:50.314 +15:35:54.91 SN Ia 0.046
TNS 2023lgz 16:47:40.382 +52:20:12.21 SN II 0.029 16:47:40.384 +52:20:12.09 SN II 0.029
TNS 2023lkw 16:48:36.214 +41:36:02.68 SN II 0.031 16:48:36.210 +41:36:02.59 SN II 0.031
TNS 2023lpa 18:41:53.728 +49:55:04.63 SN Ia 0.045 18:41:53.727 +49:55:04.54 SN Ia 0.045
TNS 2023lya 17:28:53.264 +58:22:41.62 17:28:53.215 +58:22:41.53 SN II 0.03

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