Eric Schulman
Alexandria, Virginia
Barack Obama.
1. Introduction
In this fourth paper on measuring fame
quantitatively
we introduce a new unit of fame and discover a new category of
celebrity with only one known member.
Our research over the past ten
years (Schulman
1999, Schulman
and
Boissier 2001, and Schulman
2006) has shown that many people are famous to some
extent and that Internet search engines can measure the exact fame of
such people by comparing the number of search engine hits for the
person to the number of
search
engine hits for a universal standard of
fame comparison. Previous authors (Schulman
1999, Schulman
and
Boissier 2001, and Schulman
2006) identified Monica
Lewinsky as the universal standard of fame, but we show in this
paper that her fame has been decreasing since 2001 and she is therefore
not
a good candidate for the position. We find that George
Harrison's fame has been roughly constant over the past ten years,
making him a more appropriate universal standard of fame.
Schulman
(2006) presented a quantitative method for classifying people as
'A' List
Celebrities, 'B' List Celebrities, and so on, but did not anticipate
that there could be a category of people more famous than 'A' List
Celebrities. Such people would have to be more than 30 times as famous
as the archetypal 'B' List Celebrity. However, we have now identified
one such person and have therefore created a new cateogry of 'A+' List
Celebrities. In order to motivate readers to continue past the
introduction, no revelation will yet be made concerning the identity of
this 'A+' List Celebrity.
2. Methods
One of the foremost experts on measuring fame
quantitatively (Schulman
2006) has asserted that people we perceive as 'A' List Celebrities
are on average ten times more famous than
people we perceive as 'B'
List Celebrities, who are on average ten times more famous than people
we perceive as 'C' List Celebrities, and so on. We extend his
groundbreaking work of classifiying people in seven different fields
(business, film, music, politics, religion, science, and sports) as a
function of their fame by going back to 2001 and forward to 2009 while
using the new logarithmic international
standard unit of
fame, the dBHa (Schulman
2009):
3. Results
Table 1 shows our classification of 49 people in
seven different fields.
The Hits columns list the number of Google hits that each person had in
January 2001, October 2005, October 2008, and February 2009; the Fame
columns list their fame in dBHa; and the
List column shows their celebrity category in February 2009. The
Hits, Fame, and List entries are color-coded so that 'A' List
Celebrity entries are red, 'B' List
Celebrity entries are orange, 'C' List
Celebrity entries are yellow, 'D' List
Celebrity entries are green, 'E' List
Celebrity entries are blue, 'F' List
Celebrity entries are indigo (well, light purple really), 'G' List
Celebrity entries are violet (i.e., dark purple), and 'H' List
Celebrity entries are ultraviolet (the eyes of some readers might
perceive them as white). The names and fields of typical celebrities in
each category are similarly colored. Extraneous bold horizontal lines
were added in the process of converting Microsoft Office Excel 2007
data into an image. No one knows quite why.
Table 1: Classified Celebrities

5. Conclusions
George
Harrison is the archetypal 'B' List Celebrity and Barack Obama is the
most famous person in the world.
References
Schulman,
E. 1999, "Can Fame Be Measured Quantitatively?" AIR,
5, 3, 16.
Schulman,
E. 2006, "Measuring Fame Quantitatively. III. What Does it Take to Make
the 'A' List?" AIR, 12, 1, 11.
Schulman,
E. 2009, "Measuring Fame Quantitatively. IV. Who's the Most Famous of
Them All?" AIR Online,
February 28.
Schulman,
E. and Boissier, S. 2001, "How Should Fame Be Measured
Quantitatively?" AIR Online, November 5.