Tom Boles’ 125 supernova discoveries

 

Bob Marriott

 

 

 

The following shows a few statistics relating to Tom Boles’ discoveries of supernovae – from his first, on 1997 October 29, to his 125th, on 2009 August 21. Some discoveries were made on the same date but on different nights, and others were made on the same night but on different dates. Discovery times have therefore been converted to Greenwich Mean Astronomical Time, so that each plot on the graph shows the number of discoveries on one night before and after 00.00 UT.

 

125 discoveries on 105 nights over a period of 11 years 9 months 23 days

 

 

 

 

 

Nights of more than one discovery

 

Discoveries at each magnitude

 

 

 

1999

November 6/7

2

 

14.0

1

 

17.3

4

 

 

2002

November 4/5

2

 

14.4

1

 

17.4

4

 

 

2003

February 5/6

2

 

15.2

1

 

17.5

5

 

 

 

April 6/7

2

 

15.5

2

 

17.6

7

 

 

 

August 19/20

4

 

15.6

1

 

17.7

9

 

 

2004

June 27/28

2

 

15.7

1

 

17.8

2

 

 

 

September 7/8

2

 

15.9

1

 

17.9

3

 

 

 

November 20/21

2

 

16.0

3

 

18.0

6

 

 

2005

April 10/11

2

 

16.2

4

 

18.1

8

 

 

2006

March 5/6

2

 

16.3

2

 

18.2

5

 

 

 

April 3/4

2

 

16.5

2

 

18.3

2

 

 

2008

February 12/13

3

 

16.6

4

 

18.4

5

 

 

 

August 2/3

3

 

16.8

3

 

18.5

10

 

 

2009

January 2/3

2

 

16.9

4

 

18.6

3

 

 

 

August 20/21

3

 

17.0

7

 

18.7

1

 

 

 

 

 

 

17.1

6

 

18.9

1

 

 

 

 

 

 

17.2

6

 

19.6

1

 

 

Totals per year

 

 

1997 :   1

1998 :   1

1999 :   4

2000 :   1

 

 

2001 : 12

2002 : 11

2003 : 30

2004 : 22

 

 

2005 : 12

2006 : 11

2007 :   3

2008 :   9

 

 

 

2009 : 8

 

 

 

Discoveries

 

 

SN1997dn

SN1998eg

SN1999bt

SN1999ev

SN1999gg

SN1999gl

SN2000D

SN2001bg

SN2001dk

SN2001dn

SN2001ds

SN2001dw

SN2001dz

SN2001eb

SN2001ew

SN2001ex

SN2001if

SN2001ih

SN2001it

SN2002bx

SN2002cb

SN2002cc

SN2002eh

SN2002gc

SN2002hg

SN2002hl

SN2002hm

SN2002ho

SN2002hu

SN2002jn

SN2003L

SN2003P

SN2003U

SN2003X

SN2003ab

SN2003aq

SN2003ar

SN2003as

SN2003bm

SN2003bq

SN2003bv

SN2003cr

SN2003da

SN2003db

SN2003gx

SN2003hc

SN2003hi

SN2003hj

SN2003hk

SN2003hm

SN2003hr

SN2003hy

SN2003ii

SN2003ij

SN2003ik

SN2003iw

SN2003jf

SN2003ki

SN2003kz

SN2003la

SN2004Z

SN2004aw

SN2004ay

SN2004bt

SN2004bu

SN2004ct

SN2004da

SN2004df

SN2004dq

SN2004dx

SN2004ec

SN2004ed

SN2004ef

SN2004eh

SN2004ei

SN2004ek

SN2004en

SN2004eu

SN2004fd

SN2004fz

SN2004gf

SN2004gl

SN2005C

SN2005B

SN2005R

SN2005L

SN2005bd

SN2005bi

SN2005bj

SN2005dj

SN2005ej

SN2005io

SN2005ip

SN2005lx

SN2006A

SN2006ao

SN2006ap

SN2006aq

SN2006ar

SN2006bk

SN2006bl

SN2006bo

SN2006cr

SN2006ow

SN2006ss

SN2007ck

SN2007iq

SN2007iv

SN2008X

SN2008af

SN2008ai

SN2008aj

SN2008ak

SN2008en

SN2008eo

SN2008ep

SN2008er

SN2009B

SN2009E

SN2009es

SN2009fi

SN2009ih

SN2009ii

SN2009ij

SN2009io

 

 

 

In addition, on 2003 September 17 Tom Boles discovered a nova (magnitude 18.1) in M31

This list of discoveries, with links to the images and accompanying information, is also included in Articles/Images

See also Tom Boles’ observatory, including a link to his website

 

 

On 3 September 2009 the following BAA E-Bulletin 00437 was issued:

 

It is with great pleasure that we announce that Tom Boles is now the leading discoverer of supernovae worldwide, with a total of 125 discoveries. This includes all individuals, whether professional or amateur, who have personally searched for these objects, but excludes all supernovae discovered via automated surveys. Tom reached this milestone on August 20/21 this year with the discovery of SN2009ij. This brought Tom’s total to 124, thus surpassing Fritz Zwicky, who discovered 123 (including one with P. Wild). Zwicky’s first was on 1921 April 6 with SN1921B, and his final discovery was on 1973 April 26 with SN1973K. Zwicky used a 16-inch Schmidt in his early days and the 48-inch Oschin Schmidt later. Tom made his first discovery, SN1997dn, on 1997 October 29, and so overtook Zwicky in less than 12 years; but there again, Tom now uses three 14-inch telescopes! But this was not enough for Tom, and another discovery followed with SN2009io in UGC 11666, although this was actually discovered earlier, on August 13. We are grateful to Professor Ian Howarth (a former Director of the Variable Star Section) for initially bringing Tom’s record to our attention.                                              Roger Pickard, President : Stewart Moore, Director, Deep Sky Section