Instruct: Identify the main and secondary category of Arxiv papers based on the titles and abstracts
Query: The late-type stellar density profile in the Galactic Center: A
  statistical approach   The late-type stellar population in the Galactic Center was first predicted
to reside in a dynamically relaxed cusp (power law slope ranging from 3/2 to
7/4). However, observations - which rely on models to correct for projection
effects - have suggested a flat distribution instead. The need for this
correction is due to the lack of information regarding the line-of-sight
distances. With a two decade long baseline in astrometric measurements, we are
now able to measure significant projected radial accelerations, six of which
are newly reported here, that directly constrain line-of-sight distances. Here
we present a statistical approach to take advantage of this information and
more accurately constrain the shape of the radial density profile of the
late-type stellar population in the Galactic Center.

7
The categories of this paper are: hep-th
1
The categories of this paper are: cs
8
The categories of this paper are: hep-ex
11
The categories of this paper are: hep-lat
9
The categories of this paper are: nlin
31
The categories of this paper are: ao-sci
15
The categories of this paper are: nucl-ex
30
The categories of this paper are: q-alg
16
The categories of this paper are: stat
20
The categories of this paper are: acc-phys
22
The categories of this paper are: chao-dyn
0
The categories of this paper are: hep-ph
36
The categories of this paper are: cmp-lg
12
The categories of this paper are: nucl-th
33
The categories of this paper are: plasm-ph
25
The categories of this paper are: patt-sol