**PLEASE READE THIS WIKI FOR A DESCRIPTION OF THIS PROJECT'S CONTENT**
Raw files needed to reproduce the results in Alvarez-Candal (2024, A&A accepted).
arXiv version: https://arxiv.org/abs/2402.11113
The folder **data** contains the following unformatted files:
- 29039_dmag-02.dat size: 15.3 kB
Probability distribution of rotational periods associated to objects 29039. The file contains 302 lines and 2 columns.
1st line is an internal header
2nd line is a first estimate of Hv and its uncertainty
from the 3rd line
1st column is the \Delta m
2nd column the probability
- angles-09_hg12.dat size: 6.0 MB
Angular informartion.
Each line corresponds to a different object (in the same order as names-09_hg12.dat)
1st column is the minimum alpha of the corresponding phase curve.
2nd colums is the maximum span in phase angle.
- color_gi.dat size: 93.2 MB
g-i color vs. alpha
Each line corresponds to a different object (in the same order as names-09_hg12.dat).
Each column corresponds to a 0.5 deg increase in phase angle from 0 deg up to 35 deg.
- color_iz.dat size: 96.7 MB
i-z color vs. alpha
Each line corresponds to a different object (in the same order as names-09_hg12.dat).
Each column corresponds to a 0.5 deg increase in phase angle from 0 deg up to 35 deg.
- Colors_m.dat size: 23.9 MB
Phase angle where the weighted average is closer to an individual color measurement (alpha_w) and corresponding individual color.
Each line corresponds to a different object (in the same order as names-09_hg12.dat).
**Colums 1,3,5,7** correspond to the indivudual color: u-g, g-r, r-i, i-z
**Columns 2,4,6,8** correspond to alpha_w for each color.
- Colors-w.dat size: 23.9 MB
Weighted average colors.
Each line corresponds to a different object (in the same order as names-09_hg12.dat).
**Columns 1,3,5,7**: u-g, g-r, r-i, i-z
**Columns 2,4,6,8**: corresponding errors
- ecolor_gi.dat size: 93.2 MB
Errors in the colors g-i vs. alpha.
Each line corresponds to a different object (in the same order as names-09_hg12.dat).
Each column corresponds to a 0.5 deg increase in phase angle from 0 deg up to 35 deg.
The error was computed as the convolution of the P(g) and P(i).
- ecolor_iz.dat size: 93.2 MB
Errors in the colors i-z vs. alpha.
Each line corresponds to a different object (in the same order as names-09_hg12.dat).
Each column corresponds to a 0.5 deg increase in phase angle from 0 deg up to 35 deg.
The error was computed as the convolution of the P(z) and P(i).
- elems.dat size: 8.9 MB
Osculating orbital elements from astorb.dat
Each line corresponds to a different object (in the same order as names-09_hg12.dat).
**Column 1** = semi-major axis [au]
**Column 2** = eccentricity
**Column 3** = Inclination [deg]
- eslopes.dat size: 103.5 MB
Errors in the 'realistic' spectral slopes vs. alpha.
Each line corresponds to a different object (in the same order as names-09_hg12.dat).
Each column corresponds to a 0.5 deg increase in phase angle from 0 deg up to 35 deg.
The error was computed as the standard deviation of the distribution of slopes.
- Hcoefs-09_hg12.dat size: 148.1 MB
Absolute magnitudes, phase coefficients and number of data used in the fit.
Each line corresponds to a different object (in the same order as names-09_hg12.dat).
**Colums 1-4**: Hu, Hu-, Hu+, Nu
Hu = median of P(Hu).
Hu- = 16th percentile of P(Hu)
Hu+ = 84th percentile of P(Hu)
Nu = Number of points used in phase curve
**Columns 5-8**: Same as above for Hg
**Columns 9-12**: Same as above for Hr
**Columns 13-16**: Same as above for Hi
**Columns 17-20**: Same as above for Hz
**Columns 21-24**: Same as above for HV
**Columns 25-28**: Same as above for HR
**Columns 29-31**: Gu, Gu-,Gu+
Gu = median of P(Gu).
Gu- = 16th percentile of P(Gu)
Gu+ = 84th percentile of P(Gu)
**Colums 32-34**: Same as above for Gg
**Colums 35-37**: Same as above for Gr
**Colums 38-40**: Same as above for Gi
**Colums 41-43**: Same as above for Gz
**Colums 44-46**: Same as above for GV
**Colums 47-49**: Same as above for GR
- names-09_hg12.dat size: 5.0 MB
Each line corresponds to a different objects.
**Column 1** = ID as given in the original catalog.
**Column 2** = MPC ASCII code.
- sim_slopes.dat size: 217.2 MB
Simulated slopes as computed from reflectances from Eq. 5 in the paper and a linear fit. The magnitudes are computed using the nominal values of H and G fed directly into Eq. 2.
Each line corresponds to a different object (in the same order as names-09_hg12.dat).
Each column corresponds to a 0.5 deg increase in phase angle from 0 deg up to 35 deg.
- slopes.dat size: 104.0 MB
Simulated slopes as computed from reflectances from Eq. 5 in the paper and a linear fit. The magnitudes are computed using the full P(H) and P(G) fed directly into Eq. 2.
Each line corresponds to a different object (in the same order as names-09_hg12.dat).
Each column corresponds to a 0.5 deg increase in phase angle from 0 deg up to 35 deg.
The folder **pdfs** contains the following unformatted files:
- pdfs_XX.tar
Each tarbal file contains an ensemble of Probability Distributions(*):
**0X -->** files beginning with number X.
**_@ -->** files beginning with letter @. *C* indicates capital letter and *l* indicates lowercase.
Each file has the following naming:
MPCid_filterid-09.dat (or .dat.Z)
In some cases no MPCid could be assigned, then the name is x-CatalogName. filterid = Su, Sg, Sr, Si, Sz (SDSS filters) or JV, JR (Johnson's V and R).
Each file has N lines (<= 10001). The first line is a first guess of HV and its corresponding uncertainty.
If N == 1, then only the first guess of HV is provided. Else, N > 100. After line 1, the first column indicates the value of H after the processing described in the paper, and the second column the corresponding G.
To actually describe a Probability distribution, the H and G distributions should be normalized to unity area, i.e., multiplied by a factor $1/N$ such that $N=\int_{-\infty}^{+\infty}{P(x)dx}$, and $x$ runs in H or G.
