Weekly Information about Bright Comets (2019 Mar. 30: North)

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 Updated on April 1, 2019
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Best time and the azimuth, altitude (A,h) are at lat. 35 deg in the Northern Hemisphere.
Azimuth indicates 0 for south, 90 for west, 180 for north, 270 for east.

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* C/2018 Y1 ( Iwamoto )

It approached to Earth down to 0.3 a.u. in mid February, and brightened up to 5.5 mag (Feb. 13, Juan Jose Gonzalez). Now it is fading. But it is still bright as 9.8 mag (Mar. 25, Carlos Labordena). In the Southern Hemisphere, it will be unobservable soon. In the Northern Hemisphere, it will be getting lower gradually after this. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30   4 26.52   33 23.3   1.672   1.494    62   10.7  19:44 (105, 44)  
Apr.  6   4 24.59   33 19.5   1.886   1.548    55   11.2  19:51 (108, 37)

* C/2016 M1 ( PanSTARRS )

It brightened up to 7.7 mag in June (June 19, Juan Jose Gonzalez). Now it is fading. But it is still bright as 11.2 mag (Mar. 4, Chris Wyatt). In the Southern Hemisphere, it stays observable in good condition for a long time until the comet will fade out. In the Northern Hemisphere, it is not observable for a long time until autumn when the comet fades out down to 16 mag. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30   4 26.95  -49 44.4   3.535   3.384    73   12.2  19:44 ( 33, -8)  
Apr.  6   4 36.67  -47  8.4   3.616   3.439    71   12.4  19:51 ( 38, -9)

* 78P/Gehrels 2

Now it is not observable. It will appear in the morning sky again at 13-14 mag in August. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30   1 56.11   10 59.3   2.904   2.014    22   12.4  19:44 (101,  3)  
Apr.  6   2 12.41   12 13.0   2.930   2.014    19   12.4  19:51 (105,  0)

* C/2018 N2 ( ASASSN )

Now it is not observable. It will appear in the morning sky in mid May in the Southern Hemisphere, or in late June in the Northern Hemisphere. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30   1 33.10  -11 34.0   4.711   3.799    21   13.2  19:44 ( 86,-15)  
Apr.  6   1 37.82   -9 57.9   4.694   3.762    18   13.1  19:51 ( 92,-20)

* C/2018 A6 ( Gibbs )

Now it is bright as 13.5 mag (Mar. 3, Taras Prystavski). It stays 13 mag for a long time in 2019. In the Southern Hemisphere, it is observable in excellent condition. In the Northern Hemisphere, it is not observasble until summer in 2020. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30   8 14.06  -59 18.1   2.740   3.161   105   13.2  19:44 (  0, -4)  
Apr.  6   7 59.09  -58 25.1   2.759   3.143   103   13.2  19:51 (  7, -4)

* 46P/Wirtanen

It approached to Earth down to 0.08 a.u. in mid December, and it brightened up to 3.4 mag (Dec. 14, Seiichi Yoshida). it looked so large as 3 times of Moon. Now it is fading. It has already faded down to 11.4 mag (Mar. 25, Carlos Labordena). In the Northern Hemisphere, it stays observable in excellent condition. It locates low in the Southern Hemisphere. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30   9 57.74   36 14.3   0.909   1.703   126   13.3  21:28 (180, 89)  
Apr.  6  10  4.12   34  6.1   1.010   1.763   122   14.0  21:07 (  0, 89)

* C/2017 M4 ( ATLAS )

Now it is 13.9 mag (Mar. 13, Ken Harikae). It stays 13-14 mag until summer. It is observable in excellent condition in the Southern Hemisphere. In the Northern Hemisphere, it will be getting lower gradually, and it will be unobservable in July. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30  17 21.42  -27 50.2   2.885   3.321   107   13.5   4:25 (353, 27)  
Apr.  6  17 14.49  -29 45.9   2.781   3.335   115   13.5   4:14 (359, 25)

* 123P/West-Hartley

Now it is 12.3 mag (Mar. 5, Marco Goiato). It is observable in excellent condition in the Northern Hemisphere. It locates somewhat low in the Southern Hemisphere. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30  11  4.75   29 36.3   1.299   2.167   140   13.6  22:34 (  0, 84)  
Apr.  6  11  1.90   28 22.6   1.348   2.178   135   13.7  22:04 (  0, 83)

* 29P/Schwassmann-Wachmann 1

It is not observable now. It will appear in the morning sky in May. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30  23 59.46    6 32.8   6.752   5.767     8   13.9   4:25 (255,-10)  
Apr.  6   0  4.70    7 10.8   6.737   5.767    13   13.8   4:14 (256, -7)

* C/2018 L2 ( ATLAS )

Now it is 12.6 mag (Mar. 8, Ken Harikae). It will be fading gradually after this. In the Northern Hemisphere, it stays observable for a long time until it fades out. But it stays extremely low. It will never be observable again in the Southern Hemisphere. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30  23 46.58   43  5.4   2.932   2.273    40   14.3   4:25 (227, 15)  
Apr.  6   0  7.53   44  0.7   3.014   2.330    39   14.6   4:14 (226, 15)

* C/2016 N6 ( PanSTARRS )

Now it is 14.0 mag (Mar. 8, Toshihiko Ikemura, Hirohisa Sato). It will be fading after this. In the Northern Hemisphere, it will be unobservable soon. In the Southern Hemisphere, it stays observable for a long time until it fades out. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30   5 33.67  -20 16.7   3.806   3.721    77   14.4  19:44 ( 41, 23)  
Apr.  6   5 34.12  -20  2.3   3.941   3.768    72   14.5  19:51 ( 48, 18)

* C/2017 T2 ( PanSTARRS )

Now it is 13.6 mag (Feb. 27, S. Szabo). It is expected to brighten up to 7 mag in 2020. It will be unobservable temporarily in April. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30   3 13.91    5 17.6   5.601   4.883    40   14.8  19:44 ( 86, 15)  
Apr.  6   3 17.86    6  7.9   5.607   4.820    34   14.8  19:51 ( 91, 10)

* 64P/Swift-Gehrels

It brightened up to 9.0 mag from autumn to winter (Nov. 16, Maik Meyer). Now it is fading. But it is bright as 12.4 mag still now (Feb. 23, Seiichi Yoshida). It is observable in excellent condition in the Northern Hemisphere. It stays low in the Southern Hemisphere. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30   6  9.40   23 29.7   2.028   2.155    83   14.8  19:44 ( 75, 61)  
Apr.  6   6 23.01   23  3.0   2.157   2.209    79   15.2  19:51 ( 79, 57)

* 38P/Stephan-Oterma

It brightened up to 9.5 mag from autumn to winter (Dec. 14, Marco Goiato). Now it is fading. But it is bright as 12.6 mag still now (Feb. 23, Seiichi Yoshida). In the Northern Hemisphere, it stays observable in good condition for a long time until it fades out. It locates low in the Southern Hemispehre. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30   8 51.97   41 53.2   1.736   2.312   112   14.8  20:23 (180, 83)  
Apr.  6   8 59.51   40 39.1   1.858   2.370   108   15.2  20:03 (180, 85)

* C/2016 R2 ( PanSTARRS )

Now it is 15.3 mag (Mar. 8, Toshihiko Ikemura, Hirohisa Sato). It will be fading slowly after this. It is observable in good condition in the Northern Hemisphere. In the Southern Hemisphere, it stays extremely low for a while. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30  15 55.00   47 44.2   3.702   4.185   112   14.8   3:28 (180, 77)  
Apr.  6  15 49.61   48  7.1   3.730   4.236   113   14.9   2:55 (180, 77)

* 60P/Tsuchinshan 2

Now it is 13.5 mag (Mar. 4, Chris Wyatt). It will be fading after this, and it will be fainter than 18 mag in May. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30  11 23.07   -3 57.9   0.953   1.930   162   14.9  22:53 (  0, 51)  
Apr.  6  11 20.98   -3 24.2   1.009   1.965   155   15.2  22:23 (  0, 52)

* C/2017 B3 ( LINEAR )

Now it is 14.5 mag (Aug. 16, P. Camilleri, H. Williams). It stays 15 mag from 2018 to 2019, and it will be observable for a long time in the Southern Hemisphere. In the Northern Hemisphere, it will never be observable again. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30  23 12.41  -50 57.9   4.404   3.951    57   14.9   4:25 (314,-29)  
Apr.  6  23 22.75  -49 59.1   4.366   3.959    59   14.9   4:14 (313,-28)

* C/2015 O1 ( PanSTARRS )

Now it is 14.9 mag (Mar. 1, Toshihiko Ikemura, Hirohisa Sato). It will be fading slowly after this. It is observable in excellent condition until spring in the Northern Hemispehre. In the Southern Hemisphere, it will be hardly observable after this. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30   9  9.24   41 59.1   4.597   5.106   115   15.1  20:39 (180, 83)  
Apr.  6   9  2.14   41 10.1   4.740   5.145   108   15.2  20:05 (180, 84)

* C/2018 R3 ( Lemmon )

It will brighten up to 14 mag from May to June. However, it locates very low in the Northern Hemisphere, and it is not observable in the Southern Hemisphere. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30  23  4.64   30 29.6   2.378   1.647    34   15.5   4:25 (243, 15)  
Apr.  6  23 21.91   34 27.1   2.285   1.587    35   15.3   4:14 (239, 17)

* C/2019 D1 ( Flewelling )

Now it is 16.4 mag (Mar. 11, Toshihiko Ikemura, Hirohisa Sato). It will brighten up to 15 mag from May to June, and it will be observable in good condition. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30  20  5.11    0 28.9   1.802   1.680    66   15.5   4:25 (297, 33)  
Apr.  6  20 24.91    3 54.6   1.741   1.650    67   15.4   4:14 (293, 35)

* (944) Hidalgo

Now it is 14.2 mag (Feb. 4, ATLAS-MLO, Mauna Loa). It will be fading gradually after this. It is observable in excellent condition in the Northern Hemisphere. In the Southern Hemisphere, it is not observable until summer. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30   9 25.41   64 54.0   2.020   2.456   103   15.4  20:56 (180, 60)  
Apr.  6   9 28.06   61 56.4   2.103   2.495   100   15.5  20:31 (180, 63)

* C/2018 W2 ( Africano )

It is expected to brighten up to 10 mag in autumn. Now it is 16.5 mag (Feb. 27, Thomas Lehmann). In the Northern Hemisphere, it stays observable for a long time while the comet is brightening. In the Southern Hemisphere, it it not observable until mid September. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30   2 44.74   81 15.8   2.575   2.582    79   15.7  19:44 (169, 36)  
Apr.  6   2 59.85   78 29.6   2.597   2.512    73   15.6  19:51 (166, 35)

* P/2014 C1 ( TOTAS )

First return of a new periodic comet discovered in 2014. The condition of this apparition is excelllent. It was expected to brighten rapidly, and to be observable at 15.5 mag in excellent condition in March. But it has not been recovered yet. Now it is fainter than 19 mag (Mar. 28, Jean-Francois Soulier). 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30  10  6.78   11 55.9   0.831   1.724   140   16.0  21:37 (  0, 67)  
Apr.  6  10  8.82   12  5.8   0.857   1.712   134   16.0  21:12 (  0, 67)

* C/2018 A3 ( ATLAS )

Now it is 16.5 mag (Mar. 7, Toshihiko Ikemura, Hirohisa Sato). It will be fading after this. In the Northern Hemisphere, it stays observable for a long time, but it will be extremely low from May to June. It is not observable at all in the Southern Hemisphere. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30   3 41.64   55 57.9   3.659   3.355    64   16.1  19:44 (137, 40)  
Apr.  6   3 43.26   54 35.5   3.779   3.370    58   16.2  19:51 (136, 36)

* C/2018 F4 ( PanSTARRS )

Now it is 17.4 mag (Jan. 3, Toshihiko Ikemura, Hirohisa Sato). It stays 16 mag for a long time from 2019 to 2020. It is observable in excellent condition in the Southern Hemisphere. It is hardly observable in the Northern Hemisphere. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30  13 26.60  -55 36.1   3.448   4.123   126   16.3   1:01 (  0, -1)  
Apr.  6  13 11.72  -56 43.2   3.381   4.089   129   16.3   0:19 (  0, -2)

* A/2017 U7

Asteroid, but it brightened rapidly. Now it is 17.3 mag (Nov. 14, Kunihiro Shima). It is observable in excellent condition in the Southern Hemisphere. It is hardly observable in the Northern Hemisphere. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30  22 26.51  -36  3.7   7.123   6.514    49   16.7   4:25 (304,-15)  
Apr.  6  22 27.51  -36  3.0   7.029   6.507    54   16.6   4:14 (305,-13)

* C/2010 U3 ( Boattini )

Now it is 16.8 mag (Mar. 8, Toshihiko Ikemura, Hirohisa Sato). It stays 16-17 mag for a long time until 2020. It is observable in good condition in the Northern Hemisphere. It is not observable at all in the Southern Hemisphere. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30  11  1.77   73 23.4   8.186   8.448   101   16.7  22:32 (180, 52)  
Apr.  6  10 56.78   72 54.0   8.240   8.449    98   16.7  21:59 (180, 52)

* 240P/NEAT

Although it was faint as 16-17 mag in November, it brightened up to 14.7 mag in December (Dec. 12, Toshihiko Ikemura, Hirohisa Sato). It is bright as 15.6 mag still now (Mar. 8, Toshihiko Ikemura, Hirohisa Sato). In the Northern Hemisphere, it stays observable in excellent condition after this. It stays extremely low in the Southern Hemisphere. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30  10 34.24   42 24.6   2.415   3.119   126   16.8  22:04 (180, 83)  
Apr.  6  10 31.36   41 43.3   2.508   3.150   121   17.0  21:34 (180, 83)

* 74P/Smirnova-Chernykh

Now it is 17.2 mag (Mar. 7, Toshihiko Ikemura, Hirohisa Sato). It is observable at 17 mag in good condition in 2019. It locates somewhat low in the Northern Hemisphere. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30  15 57.17  -16 29.0   3.121   3.818   128   16.9   3:30 (  0, 38)  
Apr.  6  15 55.76  -16 26.2   3.050   3.826   135   16.9   3:01 (  0, 39)

* 239P/LINEAR

Now it is 17.5 mag (Mar. 8, Toshihiko Ikemura, Hirohisa Sato). It had been brightening even after the perihelion passage, but it is fading now. It will be fainter than 18 mag in May. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30   8 37.64   -0 55.7   1.116   1.845   121   17.1  20:08 (  0, 54)  
Apr.  6   8 47.13   -0 41.5   1.195   1.877   117   17.2  19:51 (  0, 54)

* C/2017 K2 ( PanSTARRS )

Now it is 16.3 mag (Mar. 11, Toshihiko Ikemura, Hirohisa Sato). It is expected to be observable at 5-6 mag for a long time from 2022 to 2023. In the Northern Hemisphere, it is not observable at the highlight from 2022 summer to 2023 summer. In the Southern Hemisphere, it stays unobservable for a while. But it will be observable in good condition at the highlight. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30  18 13.91   55 29.6  11.940  11.977    89   17.2   4:25 (208, 65)  
Apr.  6  18 13.41   55 58.0  11.871  11.931    91   17.1   4:14 (203, 66)

* C/2018 KJ3 ( Lemmon )

Now it is 18.2 mag (Oct. 8, Toshihiko Ikemura, Hirohisa Sato). It will brighten up to 16.5 mag in June. It is observable in excellent condition in the Southern Hemisphere. It locates low in the Northern Hemisphere. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30  18 53.02  -27 18.7   3.837   3.913    86   17.3   4:25 (331, 21)  
Apr.  6  18 49.92  -28 25.2   3.680   3.890    94   17.2   4:14 (336, 22)

* C/2014 B1 ( Schwartz )

Now it is 17.1 mag (Mar. 7, Toshihiko Ikemura, Hirohisa Sato). Fading slowly. It stays observable at 17 mag in good condition until summer. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30  11 32.20    9 37.0   9.113  10.057   160   17.3  23:02 (  0, 65)  
Apr.  6  11 30.87    9 53.6   9.167  10.070   153   17.3  22:33 (  0, 65)

* C/2018 X2 ( Fitzsimmons )

Now it is 17.2 mag (Mar. 7, Toshihiko Ikemura, Hirohisa Sato). It stays 17 mag from spring to summer. But it is hardly observable. In the Northern Hemisphere, it is observable only until May. In the Southern Hemisphere, it stays locating extremely low. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30   5  6.30   41 39.0   2.544   2.424    71   17.4  19:44 (115, 53)  
Apr.  6   5 21.25   40 50.4   2.578   2.387    67   17.3  19:51 (114, 50)

* P/2018 X1 ( LONEOS )

First return of a new periodic comet which brightened up to 16.5 mag in 2005. Now it is 18.7 mag (Mar. 8, Toshihiko Ikemura, Hirohisa Sato). It will brighten up to 17.5 mag in spring. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30  13 12.73   -9 21.7   2.141   3.125   168   17.6   0:46 (  0, 46)  
Apr.  6  13  8.81   -9  0.2   2.106   3.105   176   17.5   0:15 (  0, 46)

* 21P/Giacobini-Zinner

It brightened up to 6.8 mag in September (Sept. 17, Seiichi Yoshida). Now it is fading. Now it is 17.2 mag (Mar. 11, Toshihiko Ikemura, Hirohisa Sato). 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30   6 40.93  -10 27.7   2.315   2.566    92   17.5  19:44 ( 30, 40)  
Apr.  6   6 48.74   -9  5.9   2.446   2.623    88   17.8  19:51 ( 38, 38)

* 68P/Klemola

Now it is 19.3 mag (Mar. 11, Toshihiko Ikemura, Hirohisa Sato). It will brighten rapidly after this. It will be observable at 13.5 mag in good condition in autumn. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30  17 33.85  -11  4.7   2.351   2.781   104   17.9   4:25 (346, 43)  
Apr.  6  17 39.06  -10 29.3   2.222   2.737   110   17.6   4:14 (350, 44)

* 159P/LONEOS

Now it is 17.1 mag (Mar. 7, Toshihiko Ikemura, Hirohisa Sato). It will be fading after this, and it will be fainter than 18 mag in May. It locates very low in the Southern Hemisphere. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30   6  5.39   42  6.2   4.005   4.003    82   17.7  19:44 (116, 64)  
Apr.  6   6 11.85   41 51.8   4.116   4.018    77   17.8  19:51 (115, 59)

* (6478) Gault

Main-belt asteroid. But it shows a straight tail like a comet. Now it is 17.0 mag (Mar. 11, Toshihiko Ikemura, Hirohisa Sato). It stays observable in excellent condition until early summer. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30  10  1.61    0 32.1   1.431   2.302   142   17.8  21:31 (  0, 56)  
Apr.  6   9 59.74    2 18.9   1.469   2.287   134   18.0  21:02 (  0, 57)

* 49P/Arend-Rigaux

Now it is 17.6 mag (Mar. 7, Toshihiko Ikemura, Hirohisa Sato). It is observable at 18 mag in good condition from March to April. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30  14 19.38   15 58.0   1.943   2.833   147   17.9   1:53 (  0, 71)  
Apr.  6  14 13.27   16 47.2   1.966   2.878   150   17.9   1:19 (  0, 72)

* 186P/Garradd

In the Southern Hemisphere, it is observable at 17.5 mag in good condition from spring to summer. In the Northern Hemisphere, it is not observable at all. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30  17 15.49  -53 46.9   4.041   4.391   104   18.0   4:25 (356,  1)  
Apr.  6  17 17.02  -54 27.3   3.955   4.390   109   17.9   4:14 (359,  1)

* C/2017 E3 ( PanSTARRS )

It was observed at 16 mag from 2017 to 2018. Now it is fading. It is observable at 18 mag in good condition in this spring. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 30  16  6.72    9 14.1   6.875   7.493   125   17.9   3:40 (  0, 64)  
Apr.  6  16  5.30   10  6.1   6.833   7.522   130   17.9   3:11 (  0, 65)

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