. | a . | q . | e . | I . | Hi . |
---|---|---|---|---|---|
r s | 0.738 | 0.571 | −0.095 | 0.429 | −0.238 |
Pt | 0.037 | 0.139 | 0.823 | 0.289 | 0.570 |
. | a . | q . | e . | I . | Hi . |
---|---|---|---|---|---|
r s | 0.738 | 0.571 | −0.095 | 0.429 | −0.238 |
Pt | 0.037 | 0.139 | 0.823 | 0.289 | 0.570 |
*Significance of correlation between g − i color and other quantities: semi-major axis (a), perihelion distance (q), eccentricity (e), inclination (I), and absolute magnitude in the i band (Hi). rs is the Spearman rank-order correlation coefficient, and Pt is the probability that such a correlation value would be seen when the null hypothesis of no correlation is true. Note that the retrograde object 2014 AT28 was excluded from the analysis of correlations.
. | a . | q . | e . | I . | Hi . |
---|---|---|---|---|---|
r s | 0.738 | 0.571 | −0.095 | 0.429 | −0.238 |
Pt | 0.037 | 0.139 | 0.823 | 0.289 | 0.570 |
. | a . | q . | e . | I . | Hi . |
---|---|---|---|---|---|
r s | 0.738 | 0.571 | −0.095 | 0.429 | −0.238 |
Pt | 0.037 | 0.139 | 0.823 | 0.289 | 0.570 |
*Significance of correlation between g − i color and other quantities: semi-major axis (a), perihelion distance (q), eccentricity (e), inclination (I), and absolute magnitude in the i band (Hi). rs is the Spearman rank-order correlation coefficient, and Pt is the probability that such a correlation value would be seen when the null hypothesis of no correlation is true. Note that the retrograde object 2014 AT28 was excluded from the analysis of correlations.
This PDF is available to Subscribers Only
View Article Abstract & Purchase OptionsFor full access to this pdf, sign in to an existing account, or purchase an annual subscription.