MBOSS-Colors
Minor Bodies in the Outer Solar System:
Magnitudes and Colors
1. Introduction
These pages collect the magnitudes and colors published for Minor
Bodies in the Outer Solar System. These objects include TNOs (classic
Cubewanos, Plutinos and Scattered), Centaurs, Trojans, and cometary
nuclei. Currently, the distribution of the objects among the various
classes is that of the MPC pages (
centaurs/Scattered and TNOs).
The database itself and how it is built are descrived in Hainaut
and Delsanti (2002) A&A (available below for reference). The
tables and plots on these web-pages are generated using the up-to-date
version of the database, which contains much more data than the one
used for the original paper. Also, the A&A paper contains only a
subset of the figures; the links below points to a complete collection
of all the figures.
Currently, the database contains all publications (well, it is not
complete - working on it), without any filtering. A new, separate
version of the database will be included, filtering out the data
points that are considered as "bad", either because in strong
disagreement with other measurements, or because they were reported in
"old" papers or with a too bad S/N. More soon.
Original reference paper:
O.R. Hainaut & A.C. Delsanti (2002)
Colors of Minor Bodies in the Outer Solar System -
a Statistical Analysis
Astronomy & Astrophysics 389, 641
|
mboss_AA.ps.gz (~0.5Mb)
(database frozen as for the A&A paper - use as reference for
methods and techniques used)
|
2. The Data Base
2.1 Database Status
The current content of the database is listed below, together with the
last update date.
| Item | Count
|
| Centaurs | 30 |
| Plutinos | 39 |
| Cubewanos | 105 |
| ScattDO | 34 |
| SPComets | 22 |
| Trojans | 62 |
| Objects | 292 |
| Epochs | 1324 |
| Update | Wed Jun 20 18:36:09 CLT 2007
|
2.2 Database input
Colors and magnitudes were originally compiled from the papers listed
in the "Distant EKO" publication page (Parker, 2001), and then
from many additional papers. The full list of papers included in the
current database can be found in the reference list linked below (in
bibTex format). For most of the paper, a link to the corresponding ADS
page is included.
| Referenced paper database |
BibTeX
(using A&A mnemonics) |
We encourage observers to send us their measurements
electronically, ideally using the following format:
- One line per object per epoch
- First word = name of the object (e.g. 1994TG2, NOT 1994 TG2).
- second word = date of the observations, in yyyymmdd (eg 19920825)
- following words: a space separated list of color=value or
magnitude=value with their errors after a slash (eg R=22.54/0.04
or V-R=0.55/0.09 ). The analysis program understand about U, B, V, R, I,
J, H, K, L, M, N. No distinction is foreseen between the different photometric
systems (R_Bessel, R_ck, K, Ks, K', ...).
- a field ref=key can be used to identify the publication. The
codes used are the same as those used in EKO
To add data into these files, pls email them to me. Upon request,
we will return you all the plots (color-color, color vs orbit and
histograms and CPFs) for your sample.
Examples:
Ideal: only magnitudes
1998XY95S 20000104 B=24.3339/0.2058 V=23.3951/0.1204 R=22.7502/0.0708 I=21.9781/0.1359 ref=CA2000
Also OK: Magnitudes and colors:
1996TP99 19980123 B=22.60/0.05 B-V=0.80/0.05 V-R=0.55/0.04 ref=XX01
2.3 MBOSS color database
The input database is read in, and for each object, is filled in with
additional information (such as orbital element, helio- and
geo-centric distances, etc). The dynamical class, as defined as on the
MPC pages, is included. The average magnitudes and colors are computed
(taking care not to mix magnitudes of different epochs in the
computation of colors). The spectral gradient (Grt, in %/100nm)
and absolute magnitudes M(1,1,alpha) are computed. The output file has
one line per object. The format is fixed, and each collumn has a
header indicating its content. Upon request, other colors can be
generated.
| MBOSS color database: |
ASCII |
| References per object |
ASCII
HTML with links to the papers
|
The average colors of each of the dynamical classes are also computed, with the corresponding dispersion.
| Average colors per class |
ASCII |
3. Plots
3.0 Legend
These symbols and colors are used in all the figures.
3.1 Color-Color plots
This page links all the color-color
plots.
3.2 Color vs Orbital Parameters
This page links the plots of the color
indexes as a function of various orbital parameters and absolute magnitude.
3.3 Color histograms and cummulative probability functions
This page links the plots of the
color histograms and cummulative distributions for the various MBOSS
classes, together with the M11 (absolute mag) and spectral slope
distributions.
3.4 Reflectivity Spectra
This page links to the
reflectivity spectra of the objects, sorted by increasing
gradient. The one below is the first one, for bluest objects.
3.5 All plots and tables in one PostScript
Updated on Wed Jun 20 18:36:08 CLT 2007
Copyright
You may use the content of these pages, but not re-distribute it.
If you use of these data or these plots in a publication, pls make reference to the original paper
Color of Minor Bodies in the Outer Solar System,
Hainaut & Delsanti (2002)
Astronomy & Astrophysics, 389, 641
and/or to this page:
http://www.sc.eso.org/~ohainaut/MBOSS
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