2019MNRAS.490.2799D

Query : 2019MNRAS.490.2799D

2019MNRAS.490.2799D - Mon. Not. R. Astron. Soc., 490, 2799-2821 (2019/December-1)

The Berkeley sample of Type II supernovae: BVRI light curves and spectroscopy of 55 SNe II.

DE JAEGER T., ZHENG W., STAHL B.E., FILIPPENKO A.V., BRINK T.G., BIGLEY A., BLANCHARD K., BLANCHARD P.K., BRADLEY J., CARGILL S.K., CASPER C., CENKO S.B., CHANNA S., CHOI B.Y., CLUBB K.I., COBB B.E., COHEN D., DE KOUCHKOVSKY M., ELLISON M., FALCON E., FOX O.D., FULLER K., GANESHALINGAM M., GOULD C., GRAHAM M.L., HALEVI G., HAYAKAWA K.T., HESTENES J., HYLAND M.P., JEFFERS B., JOUBERT N., KANDRASHOFF M.T., KELLY P.L., KIM H., KIM M., KUMAR S., LEONARD E.J., LI G.Z., LOWE T.B., LU P., MASON M., McALLISTER K.J., MAUERHAN J.C., MODJAZ M., MOLLOY J., PERLEY D.A., PINA K., POZNANSKI D., ROSS T.W., SHIVVERS I., SILVERMAN J.M., SOLER C., STEGMAN S., TAYLOR S., TANG K., WILKINS A., WANG X., WANG X., YUK H., YUNUS S. and ZHANG K.D.

Abstract (from CDS):

In this work, BVRI light curves of 55 Type II supernovae (SNe II) from the Lick Observatory Supernova Search programme obtained with the Katzman Automatic Imaging Telescope and the 1 m Nickel telescope from 2006 to 2018 are presented. Additionally, more than 150 spectra gathered with the 3 m Shane telescope are published. We conduct an analyse of the peak absolute magnitudes, decline rates, and time durations of different phases of the light and colour curves. Typically, our light curves are sampled with a median cadence of 5.5 d for a total of 5093 photometric points. In average, V-band plateau declines with a rate of 1.29 mag (100 d)–1, which is consistent with previously published samples. For each band, the plateau slope correlates with the plateau length and the absolute peak magnitude: SNe II with steeper decline have shorter plateau duration and are brighter. A time-evolution analysis of spectral lines in term of velocities and pseudo-equivalent widths is also presented in this paper. Our spectroscopic sample ranges between 1 and 200 d post-explosion and has a median ejecta expansion velocity at 50 d post-explosion of 6500 km s–1 (H α line) and a standard dispersion of 2000 km s–1. Nebular spectra are in good agreement with theoretical models using a progenitor star having a mass <16M☉. All the data are available to the community and will help to understand SN II diversity better, and therefore to improve their utility as cosmological distance indicators.

Abstract Copyright: © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): techniques: photometric - techniques: spectroscopic - surveys - supernovae: general

Simbad objects: 109

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Number of rows : 109
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 NGC 259 Sy2 00 48 03.281 -02 46 31.01   13.4   13.4 13.2 ~ 62 0
2 SN 2017jbj SN* 00 48 05.420 -02 47 22.40           SNIc 8 0
3 IC 1704 GiG 01 27 09.5314788936 +14 46 34.605545232   14.2       ~ 57 0
4 SN 2007il SN* 01 27 09.75 +14 46 46.5     18.4     SNII 29 1
5 M 74 G 01 36 41.7451236624 +15 47 01.107512304 10.52 10.00 9.46 9.16   ~ 1934 1
6 SN 2013ej SN* 01 36 48.16 +15 45 31.0           SNIIP 248 0
7 NGC 774 LIN 01 59 34.7353817064 +14 00 29.546396964   13.97       ~ 85 1
8 SN 2006ee SN* 01 59 35.40 +14 00 19.6     17.6     SNII 32 1
9 SN 2016cyx SN* 02 21 22.767 +16 33 54.56           SNIIb 10 0
10 Z 462-3 GiG 02 21 23.7101681160 +16 33 59.125103208   14.0       ~ 55 0
11 SN 2009js SN* 02 25 48.28 +18 29 25.8           SNIIP 36 1
12 NGC 918 AGN 02 25 50.7899313312 +18 29 46.358860992   16.00 15.01     ~ 157 0
13 SN 2008gi SN* 02 44 00.33 +05 25 42.8           SNII 24 1
14 Z 415-4 GiP 02 44 00.3856362024 +05 25 47.366846076   14.9       ~ 27 0
15 SN 2012ec SN* 02 45 59.89 -07 34 25.0         22.32 SNIIP 92 3
16 NGC 1084 EmG 02 45 59.926 -07 34 43.10 11.22 11.59 10.73 10.55 11.1 ~ 386 2
17 SN 2016fqr SN* 02 52 51.03 +42 12 25.7           SNII 4 0
18 NGC 1122 GiG 02 52 51.0789378240 +42 12 19.719761688   13.0       ~ 40 0
19 SN 2017hta SN* 03 39 47.580 +66 43 05.99           SNII 3 0
20 UGCA 81 GiG 03 40 07.690 +66 42 47.04           ~ 23 0
21 MCG-01-10-039 EmG 03 49 05.4869956920 -03 03 37.692668916   15   13.31   ~ 29 0
22 SN 2013gd SN* 03 49 05.64 -03 03 28.3           SNIIP 10 1
23 SN 1999em SN* 04 41 27.04 -02 51 45.2   13.79 13.7     SNIIP 727 1
24 UGC 3232 AG? 05 03 18.3655216608 +18 27 09.103846896   17       ~ 26 0
25 SN 2017iit SN* 05 03 20.160 +18 27 03.14           SNII 5 0
26 SN 2009kr SN* 05 12 03.30 -15 41 52.2           SNII 93 1
27 NGC 1832 Sy2 05 12 03.3433348776 -15 41 16.021694220   12.2   11.07 11.8 ~ 245 1
28 NGC 1843 Sy2 05 14 06.1155775464 -10 37 36.949807884   12.8   11.95 12.8 ~ 40 0
29 SN 2015be SN* 05 14 06.24 -10 37 30.0           SNIIP 6 1
30 SN 2013fp SN* 05 32 07.25 -07 54 23.8           SNIIP 2 1
31 IC 421 AG? 05 32 08.5516302264 -07 55 05.264062428   12.6   16.18 12.7 ~ 26 0
32 SN 2016adg SN* 05 54 40.63 +15 10 27.4           SNII 3 0
33 UGC 3376 AG? 05 54 40.728 +15 10 13.45   15.5       ~ 27 0
34 NGC 2273B AG? 06 46 31.6119515088 +60 20 25.427246748   14.1       ~ 50 0
35 SN 2011fd SN* 06 46 39.85 +60 21 02.8           SNIIP 9 1
36 SN 2015W SN* 06 57 43.03 +13 34 45.7           SNII 16 1
37 UGC 3617 AG? 06 57 45.1866955296 +13 34 31.189510992   16.0       ~ 15 0
38 SN 2015X SN* 07 16 42.58 +29 51 22.7           SNIIP 7 1
39 Z 146-44 G 07 16 42.874 +29 51 17.72   14.5       ~ 39 0
40 MCG-01-24-010 EmG 09 20 21.9574885200 -07 52 50.686562208   13.93   13.05 13.2 ~ 48 0
41 SN 2008if SN* 09 20 23.47 -07 52 33.1           SNII 28 1
42 NGC 2939 GiG 09 38 07.9018488384 +09 31 26.138516952   13.5       ~ 89 0
43 SN 2009ao SN* 09 38 08.54 +09 31 00.7           ~ 25 1
44 SN 1999gi SN* 10 18 16.66 +41 26 28.2   14.8       SNIIP 248 1
45 NGC 3239 AG? 10 25 04.867 +17 09 49.21   13.5       ~ 202 0
46 SN 2012A SN* 10 25 07.39 +17 09 14.6           SNIIP 135 0
47 SN 2012aw SN* 10 43 53.735 +11 40 17.63       15   SNIIP 252 1
48 M 95 GiP 10 43 57.7313485800 +11 42 13.301191332 10.71 10.51 9.73 9.48   ~ 1238 2
49 SN 2014G SN* 10 54 34.13 +54 17 56.9           SNIIL 95 1
50 NGC 3448 AG? 10 54 39.240 +54 18 18.82   12.2       ~ 238 1
51 M 65 GiP 11 18 55.9084654776 +13 05 32.300703672   9.6       ~ 458 1
52 SN 2013am SN* 11 18 56.95 +13 03 49.4           SNII 52 1
53 M 66 AGN 11 20 15.0 +12 59 29 9.85 9.65 8.92     ~ 1509 4
54 SN 2016cok SN* 11 20 19.09 +12 58 57.2           SNII 35 0
55 NGC 4134 LIN 12 09 10.0033415256 +29 10 36.781347720   13.8 13.10     ~ 79 0
56 SN 2014cn SN* 12 09 11.54 +29 10 20.9           SNIIP 7 1
57 M 61 Sy2 12 21 54.9282582888 +04 28 25.597367184 10.07 10.18 9.65     ~ 1084 1
58 SN 2008in SN* 12 22 01.77 +04 28 47.5           SNIIP 117 1
59 NGC 4487 EmG 12 31 04.4731449720 -08 03 14.548820040   11.7   11.9 11.6 ~ 189 0
60 SN 2009N SN* 12 31 09.46 -08 02 56.3           SNIIP 111 1
61 Z 15-37 EmG 12 55 12.6507011952 +00 07 00.036186204   14.694   16.214 12.7 ~ 155 0
62 SN 2016X SN* 12 55 15.50 +00 05 59.7           SNIIb 61 0
63 SN 2008aw SN* 13 04 14.11 -10 19 12.9     15.9     SNII 34 1
64 NGC 4939 Sy2 13 04 14.3280524928 -10 20 22.300454724   14.81 13.80 10.92   ~ 332 1
65 IC 4221 Sy1 13 18 30.3595530480 -14 36 32.170225356   13.93   12.94   ~ 62 0
66 SN 2015C SN* 13 18 30.47 -14 36 44.6           SNIIP 6 1
67 SN 2005cs SN* 13 29 53.37 +47 10 28.2   14.5       SNIIP 450 1
68 NGC 5301 GiG 13 46 24.60933 +46 06 26.6650   13.0       ~ 135 1
69 SN 2009at SN* 13 46 26.68 +46 06 08.7           ~ 18 1
70 NGC 5669 H2G 14 32 43.476 +09 53 25.47   13.2       ~ 213 0
71 SN 2013ab SN* 14 32 44.49 +09 53 12.3           SNIIP 71 1
72 Z 75-65 AG? 14 32 53.525 +11 35 41.47   14.3       ~ 80 0
73 SN 2011cj SN* 14 32 53.81 +11 35 49.3           SNIIP 14 1
74 SN 2008bx SN* 14 54 39.00 +42 01 22.5           SNII 14 1
75 SN 2013by SN* 16 59 02.43 -60 11 41.8           SNII 83 1
76 NGC 6479 AG? 17 48 21.5885228184 +54 08 56.485217508   14.5       ~ 32 0
77 SN 2009ay SN* 17 48 22.97 +54 08 54.7           SNII 17 1
78 Z 199-23 AG? 17 49 26.660 +36 08 42.80   14.0       ~ 47 0
79 SN 2015V SN* 17 49 27.05 +36 08 36.0           SNIIP 15 1
80 2MASX J18134886+1314222 G 18 13 48.8694609312 +13 14 22.048090584           ~ 3 0
81 SN 2015O SN* 18 13 49.23 +13 14 15.9           SNII 4 1
82 Z 172-29 G 18 23 04.1781016368 +29 54 04.960842840   14.9       ~ 28 0
83 SN 2007ck SN* 18 23 05.59 +29 54 01.0     18.5     SNIIP 10 1
84 SN 2012ck SN* 19 19 27.93 +44 14 50.9           SNII 7 1
85 MCG+05-45-006 AG? 19 20 28.5247446264 +30 49 31.856567160   14.5       ~ 31 0
86 SN 2008ex SN* 19 20 28.68 +30 49 42.0           SNII 11 1
87 Z 230-8 GiC 19 21 19.4899912896 +43 59 53.864602404   15.7       ~ 4 0
88 Z 257-21 G 19 56 48.6644337960 +49 53 09.055954500   15.7       ~ 8 0
89 AT 2018iml CV* 19 56 50.61 +49 53 15.7           SNII: 6 1
90 SN 2004et SN* 20 35 25.33 +60 07 17.7   12.88       SNIIP 547 1
91 Z 473-3 AG? 22 05 08.9398613904 +26 36 25.859976012   15.00       ~ 45 0
92 SN 2006ek SN* 22 05 09.23 +26 36 31.4     19.2     SNII 11 1
93 SN 2014dq SN* 22 23 16.120 -28 58 30.78           SNIc 22 1
94 MCG-05-52-070 GiP 22 23.3 -28 59   14.53   13.83   ~ 55 0
95 SN 2013bu SN* 22 37 02.17 +34 24 05.2           SNIIP 22 1
96 NGC 7331 LIN 22 37 04.0506038088 +34 24 56.800076508 10.65 10.35 9.48     ~ 1284 2
97 NGC 7483 GiG 23 05 48.2715121248 +03 32 42.256625424   14.3       ~ 57 0
98 SN 2010id SN* 23 05 48.88 +03 31 25.5           SNII 44 1
99 SN 2008ea SN* 23 20 22.58 +27 19 10.2           SNIIP 13 1
100 NGC 7624 GiG 23 20 22.632 +27 18 56.67   13.7       ~ 105 0
101 SN 2014ce SN* 23 27 40.86 +23 35 21.4           SNIIP 7 1
102 NGC 7673 EmG 23 27 41.060 +23 35 20.18 12.84 13.17 12.76     ~ 282 2
103 Z 431-78 AG? 23 30 56.799 +15 29 25.96   15.6       ~ 34 0
104 SN 2011ef SN* 23 30 57.02 +15 29 24.3           SNIIb 14 1
105 SN 2013ft SN* 23 41 35.20 +03 43 30.5           SNIIP 11 1
106 NGC 7742 GiP 23 44 15.7534099368 +10 46 01.533226872   12.5       ~ 226 0
107 SN 2014cy SN* 23 44 16.03 +10 46 12.5           SNIb/c 22 1
108 MCG+03-01-002 AG? 23 55 46.025 +18 25 33.60   17       ~ 65 0
109 SN 2007od SN* 23 55 48.68 +18 24 54.8       14.4   SNIIP 147 1

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