A catalog of near-IR absolute magnitudes of Solar System small bodies

Open Access

Table 2

Sample of the catalog.

(1) ID-MPC designation	H_J	$H_{J}^{-}$ $\$\[H_{J}^{-}\]$$	$H_{J}^{+}$ $\$\[H_{J}^{+}\]$$	N	G_J	$G_{J}^{-}$ $\$\[G_{J}^{-}\]$$	$G_{J}^{+}$ $\$\[G_{J}^{+}\]$$	α_min (deg)	Δα (deg)
Ceres − 00001	−8.0	−8.0	−8.0	1	−8.0	−8.0	−8.0	8.94	7.76
Iris − 00007	4.089	4.193	3.985	9	0.836	0.290	1.306	16.32	7.77
Psyche − 00016	4.291	4.433	4.138	3	0.639	0.190	1.198	2.35	9.76
(2) ID-MPC designation	H_Jl	$H_{J l}^{-}$ $\$\[H_{J l}^{-}\]$$	$H_{J l}^{+}$ $\$\[H_{J l}^{+}\]$$	N	β_J (mag per deg)	$β_{J}^{-}$ $\$\[\beta_{J}^{-}\]$$	$β_{J}^{+}$ $\$\[\beta_{J}^{+}\]$$	α_min (deg)	Δα (deg)
Ceres − 00001	−8.0	−8.0	−8.0	1	−8.0	−8.0	−8.0	8.94	7.76
Iris − 00007	4.424	4.966	3.887	9	0.034	0.010	0.059	16.32	7.77
Psyche − 00016	4.467	4.680	4.256	3	0.041	0.012	0.071	2.35	9.76
(3) ID-MPC designation	H_Je	$H_{J e}^{-}$ $\$\[H_{J e}^{-}\]$$	$H_{J e}^{+}$ $\$\[H_{J e}^{+}\]$$	N	β_Je (mag per deg)	$β_{J e}^{-}$ $\$\[\beta_{J e}^{-}\]$$	$β_{J e}^{+}$ $\$\[\beta_{J e}^{+}\]$$	α_min (deg)	Δα (deg)
Ceres − 00001	−8.0	−8.0	−8.0	1	−8.0	−8.0	−8.0	8.94	7.76
Iris − 00007	4.419	4.971	3.887	9	0.034	0.010	0.058	16.32	7.77
Psyche − 00016	−8.0	−8.0	−8.0	3	−8.0	−8.0	−8.0	2.35	9.76

Notes. The first column shows the ID of the object and its Minor Planets Center ASCII designation. H_J is the median of the probability distribution, while ⁻ and ⁺ designate the absolute magnitude at the 16th and 84th percentiles. The number of observations considered is shown in the fifth column. $G_{J}, G_{J}^{-}$ $\$\[G_{J}, G_{J}^{-}\]$$ , and $G_{J}^{+}$ $\$\[G_{J}^{+}\]$$ (or β) from column six to eight. The last two columns show the minimum α and its total span. Flag −8 indicates objects with fewer than three observations in a given filter or Δα < 5 deg, while flag −9 indicates that not enough valid solutions were obtained (that is, less than 100). The complete catalog is available at the CDS, the Open Science Framework⁷, or upon request. (1) Indicates results obtained using the ${H G}_{12}^{*}$ $\[\mathrm{HG}_{12}^{*}\]$ model, (2) obtained with the linear model, and (3) with the linear model restricted to α_min > 9.5 deg. We simplified the notation of the $G_{12 λ}^{*}$ $\$\[G_{12 \lambda}^{*}\]$$ for clarity.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.