YSN |
SN |
SN R.A. |
SN Decl. |
SN Type |
SN Mag |
G/S Redshift |
Disc Date |
GAL name |
GAL R.A. |
GAL Decl. |
Host? |
GAL Type |
GAL Mag |
GAL Incl. |
GAL Log10d |
GAL Logab |
GAL PosAng |
Disc Surveys |
Discoverer(s) |
S? |
SN_comment |
2015 |
PS15cyz |
03 25 10.73 |
-06 10 48.9 |
II |
> 19 |
0.03382 |
2015-11-28 |
PGC012785 |
03 25 11.58 |
-06 10 51.5 |
|
Sbc |
13.97 |
48 |
0.98 |
0.17 |
41.3 |
|
PS1 |
|
|
2015 |
DES15X3mwb |
02 23 45.79 |
-05 03 12.2 |
Ia |
> 23.8 |
|
2015-11-28 |
|
02 23 45.79 |
-05 03 12.2 |
|
|
|
|
|
|
|
Dark_Energy_S |
Dark Energy Survey |
|
|
2015 |
OGLE15vk |
01 24 40.98 |
-74 47 15.3 |
Ic |
> 18.6 |
|
2015-11-28 |
2MASXJ01244101-7447152 |
01 24 41.04 |
-74 47 15.2 |
|
|
16.2 |
|
0.20412 |
0.028029 |
145 |
OGLE |
OGLE Transient Search |
|
|
2015 |
DES15X3naa |
02 26 58.48 |
-04 58 03.8 |
Ia |
> 23.6 |
|
2015-11-29 |
|
02 26 58.48 |
-04 58 03.8 |
? |
|
|
|
|
|
|
Dark_Energy_S |
Dark Energy Survey |
|
Faint objects are near SN posi |
2015 |
DES15E1neh |
00 26 40.77 |
-42 57 50.6 |
Ia: |
> 22.6 |
|
2015-11-29 |
|
00 26 40.77 |
-42 57 50.6 |
|
|
|
|
|
|
|
Dark_Energy_S |
Dark Energy Survey |
|
|
2015 |
DES15C1nfb |
03 37 49.93 |
-27 01 10.6 |
Ia |
> 22.4 |
|
2015-11-29 |
2MASXJ03374970-2701095 |
03 37 49.72 |
-27 01 09.7 |
|
|
18.69 |
|
0.278754 |
0.132626 |
|
Dark_Energy_S |
Dark Energy Survey |
|
|
2015 |
DES15X2nkz |
02 22 13.21 |
-05 52 18.2 |
Ia |
> 24.1 |
0.458814 |
2015-11-29 |
GALEXMSC J022213.32-055218.2 |
02 22 13.28 |
-05 52 18.1 |
|
|
21.4 |
|
|
|
|
Dark_Energy_S |
Dark Energy Survey |
|
|
2015 |
DES15X3nad |
02 23 54.34 |
-04 10 06.6 |
II |
> 24.2 |
|
2015-11-29 |
PGC1061884 |
02 23 53.89 |
-04 10 14.3 |
? |
|
18.43 |
|
0.39 |
0.14 |
116 |
Dark_Energy_S |
Dark Energy Survey |
|
SN is located far from the cen |
2015 |
ASASSN-15tf |
21 29 20.31 |
-23 05 39.5 |
Ia |
> 17.1 |
0.035288 |
2015-11-29 |
PGC134217 |
21 29 19.86 |
-23 05 27.3 |
|
Sc |
15.87 |
57 |
0.88 |
0.25 |
41 |
|
ASAS-SN |
|
|
2015 |
DES15C2nfs |
03 34 29.04 |
-29 10 08.5 |
Ia |
> 23.4 |
|
2015-11-29 |
|
03 34 29.04 |
-29 10 08.5 |
|
|
|
|
|
|
|
Dark_Energy_S |
Dark Energy Survey |
|
|
2015 |
DES15E1nei |
00 32 20.08 |
-43 44 27.0 |
Ia |
> 22.5 |
0.116863 |
2015-11-29 |
ESIS J003220.06-434426.9 |
00 32 20.07 |
-43 44 27.0 |
? |
|
21.9 |
|
|
|
|
Dark_Energy_S |
Dark Energy Survey |
|
In a cluster of galaxies. |
2015 |
DES15E2nlz |
00 35 51.33 |
-44 40 36.1 |
Ia |
> 24 |
|
2015-11-30 |
|
00 35 51.33 |
-44 40 36.1 |
|
|
|
|
|
|
|
Dark_Energy_S |
Dark Energy Survey |
|
|
2015 |
AT2016dsn |
00 20 41.06 |
+25 13 44.6 |
IaPec |
> 19.4 |
0.035615 |
2015-11-30 |
AGC102641 |
00 20 41.60 |
+25 13 40.0 |
|
|
|
|
|
|
|
|
|
|
A 1991T-like type-Ia supernova |
2015 |
DES15C2njv |
03 36 29.87 |
-28 34 11.5 |
Ia |
> 21.8 |
|
2015-11-30 |
SSTSL2 J033629.89-283411.7 |
03 36 29.90 |
-28 34 11.7 |
? |
|
|
|
|
|
|
Dark_Energy_S |
Dark Energy Survey |
|
A faint object is near SN posi |
2015 |
2015az |
03 09 42.51 |
+40 58 29.3 |
Ia |
> 15.9 |
0.020117 |
2015-11-30 |
IC0290 |
03 09 42.74 |
+40 58 27.2 |
|
Sb |
15.43 |
80 |
1.09 |
0.59 |
129.3 |
|
Gagliano et al. |
|
|
2015 |
CSS151130:014258+273410 |
01 42 58.44 |
+27 34 10.5 |
IIb: |
> 17.6 |
|
2015-11-30 |
GALEXASC J014258.21+273356.6 |
01 42 58.14 |
+27 33 55.6 |
? |
|
18 |
|
|
|
|
|
CRTS |
|
In a galaxy system with two bi |
2015 |
DES15X2nkl |
02 23 19.33 |
-06 31 34.7 |
Ia |
> 23.3 |
|
2015-11-30 |
SDSS J022319.37-063135.3 |
02 23 19.37 |
-06 31 35.3 |
? |
|
21.23452 |
|
|
|
|
Dark_Energy_S |
Dark Energy Survey |
|
Faint objects are near SN posi |
2015 |
PS15dbd |
05 56 52.94 |
-22 00 45.9 |
Ia |
> 18.2 |
0.046866 |
2015-12-01 |
PGC178739 |
05 56 53.67 |
-22 00 35.5 |
|
|
15.84 |
|
0.86 |
0.12 |
75.9 |
|
PS1 |
|
|
2015 |
PS15cze |
03 47 23.43 |
+00 52 37.8 |
Ia |
> 18.7 |
0.039335 |
2015-12-01 |
2MASXJ03472342+0052316 |
03 47 23.38 |
+00 52 31.7 |
|
S0-a |
16.21 |
30 |
0.79 |
0.06 |
29.8 |
|
PS1 |
|
|
2015 |
ASASSN-15ti |
03 05 08.62 |
+37 54 00.7 |
Ia |
> 18.7 |
|
2015-12-01 |
PGC2112473 |
03 05 10.61 |
+37 54 00.0 |
? |
|
18.05 |
|
0.31 |
0.06 |
82 |
|
ASAS-SN |
|
Star-like objects are close to |