Coverage for python / lsst / pipe / tasks / ssp / schema.py: 100%
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« prev ^ index » next coverage.py v7.13.5, created at 2026-04-15 00:08 +0000
1# ***** GENERATED FILE, DO NOT EDIT BY HAND *****
2# flake8: noqa
3# ruff: noqa: W505
4# generated with /Users/mjuric/miniforge3/envs/ddpp-dev/bin/ssp-generate-dtypes /Users/mjuric/projects/github.com/lsst/sdm_schemas/yml/lsstcam.yaml # noqa: E501
6import numpy as np
8# SSObject: LSST-computed per-object quantities.
9SSObjectDtype = np.dtype([
10 ('ssObjectId', '<i8'), # Unique identifier.
11 ('designation', '<U16'), # The unpacked primary provisional designation for this object.
12 ('nObs', '<i4'), # Total number of LSST observations of this object.
13 ('arc', '<f4'), # [d] Timespan ("arc") of all LSST observations, t_{last} - t_{first}
14 ('firstObservationMjdTai', '<f8'), # [d] The time of the first LSST observation of this object (could be
15 # precovered), TAI.
16 ('MOIDEarth', '<f4'), # [AU] Minimum orbit intersection distance to Earth.
17 ('MOIDEarthDeltaV', '<f4'), # [km/s] DeltaV at the MOID point.
18 ('MOIDEarthEclipticLongitude', '<f4'), # [deg] Ecliptic longitude of the MOID point (Earth's orbit).
19 ('MOIDEarthTrueAnomaly', '<f4'), # [deg] True anomaly of the MOID point on Earth's orbit.
20 ('MOIDEarthTrueAnomalyObject', '<f4'), # [deg] True anomaly of the MOID point on the object's orbit.
21 ('tisserand_J', '<f4'), # Tisserand parameter with respect to Jupiter (T_J).
22 ('extendednessMax', '<f4'), # Maximum `extendedness` value from the DiaSource.
23 ('extendednessMedian', '<f4'), # Median `extendedness` value from the DiaSource.
24 ('extendednessMin', '<f4'), # Minimum `extendedness` value from the DiaSource.
25 ('u_nObs', '<i4'), # Total number of data points (u band).
26 ('u_H', '<f4'), # [mag] Best fit absolute magnitude (u band).
27 ('u_HErr', '<f4'), # [mag] Error in the estimate of H (u band).
28 ('u_G12', '<f4'), # Best fit G12 slope parameter (u band).
29 ('u_G12Err', '<f4'), # Error in the estimate of G12 (u band).
30 ('u_H_u_G12_Cov', '<f4'), # [mag**2] H–G12 covariance (u band).
31 ('u_nObsUsed', '<i4'), # The number of data points used to fit the phase curve (u band).
32 ('u_Chi2', '<f4'), # Chi^2 statistic of the phase curve fit (u band).
33 ('u_phaseAngleMin', '<f4'), # [deg] Minimum phase angle observed (u band).
34 ('u_phaseAngleMax', '<f4'), # [deg] Maximum phase angle observed (u band).
35 ('u_slope_fit_failed', '|b1'), # G12 fit failed in u band. G12 contains a fiducial value used to fit H.
36 ('g_nObs', '<i4'), # Total number of data points (g band).
37 ('g_H', '<f4'), # [mag] Best fit absolute magnitude (g band).
38 ('g_HErr', '<f4'), # [mag] Error in the estimate of H (g band).
39 ('g_G12', '<f4'), # Best fit G12 slope parameter (g band).
40 ('g_G12Err', '<f4'), # Error in the estimate of G12 (g band).
41 ('g_H_g_G12_Cov', '<f4'), # [mag**2] H–G12 covariance (g band).
42 ('g_nObsUsed', '<i4'), # The number of data points used to fit the phase curve (g band).
43 ('g_Chi2', '<f4'), # Chi^2 statistic of the phase curve fit (g band).
44 ('g_phaseAngleMin', '<f4'), # [deg] Minimum phase angle observed (g band).
45 ('g_phaseAngleMax', '<f4'), # [deg] Maximum phase angle observed (g band).
46 ('g_slope_fit_failed', '|b1'), # G12 fit failed in g band. G12 contains a fiducial value used to fit H.
47 ('r_nObs', '<i4'), # Total number of data points (r band).
48 ('r_H', '<f4'), # [mag] Best fit absolute magnitude (r band).
49 ('r_HErr', '<f4'), # [mag] Error in the estimate of H (r band).
50 ('r_G12', '<f4'), # Best fit G12 slope parameter (r band).
51 ('r_G12Err', '<f4'), # Error in the estimate of G12 (r band).
52 ('r_H_r_G12_Cov', '<f4'), # [mag**2] H–G12 covariance (r band).
53 ('r_nObsUsed', '<i4'), # The number of data points used to fit the phase curve (r band).
54 ('r_Chi2', '<f4'), # Chi^2 statistic of the phase curve fit (r band).
55 ('r_phaseAngleMin', '<f4'), # [deg] Minimum phase angle observed (r band).
56 ('r_phaseAngleMax', '<f4'), # [deg] Maximum phase angle observed (r band).
57 ('r_slope_fit_failed', '|b1'), # G12 fit failed in r band. G12 contains a fiducial value used to fit H.
58 ('i_nObs', '<i4'), # Total number of data points (i band).
59 ('i_H', '<f4'), # [mag] Best fit absolute magnitude (i band).
60 ('i_HErr', '<f4'), # [mag] Error in the estimate of H (i band).
61 ('i_G12', '<f4'), # Best fit G12 slope parameter (i band).
62 ('i_G12Err', '<f4'), # Error in the estimate of G12 (i band).
63 ('i_H_i_G12_Cov', '<f4'), # [mag**2] H–G12 covariance (i band).
64 ('i_nObsUsed', '<i4'), # The number of data points used to fit the phase curve (i band).
65 ('i_Chi2', '<f4'), # Chi^2 statistic of the phase curve fit (i band).
66 ('i_phaseAngleMin', '<f4'), # [deg] Minimum phase angle observed (i band).
67 ('i_phaseAngleMax', '<f4'), # [deg] Maximum phase angle observed (i band).
68 ('i_slope_fit_failed', '|b1'), # G12 fit failed in i band. G12 contains a fiducial value used to fit H.
69 ('z_nObs', '<i4'), # Total number of data points (z band).
70 ('z_H', '<f4'), # [mag] Best fit absolute magnitude (z band).
71 ('z_HErr', '<f4'), # [mag] Error in the estimate of H (z band).
72 ('z_G12', '<f4'), # Best fit G12 slope parameter (z band).
73 ('z_G12Err', '<f4'), # Error in the estimate of G12 (z band).
74 ('z_H_z_G12_Cov', '<f4'), # [mag**2] H–G12 covariance (z band).
75 ('z_nObsUsed', '<i4'), # The number of data points used to fit the phase curve (z band).
76 ('z_Chi2', '<f4'), # Chi^2 statistic of the phase curve fit (z band).
77 ('z_phaseAngleMin', '<f4'), # [deg] Minimum phase angle observed (z band).
78 ('z_phaseAngleMax', '<f4'), # [deg] Maximum phase angle observed (z band).
79 ('z_slope_fit_failed', '|b1'), # G12 fit failed in z band. G12 contains a fiducial value used to fit H.
80 ('y_nObs', '<i4'), # Total number of data points (y band).
81 ('y_H', '<f4'), # [mag] Best fit absolute magnitude (y band).
82 ('y_HErr', '<f4'), # [mag] Error in the estimate of H (y band).
83 ('y_G12', '<f4'), # Best fit G12 slope parameter (y band).
84 ('y_G12Err', '<f4'), # Error in the estimate of G12 (y band).
85 ('y_H_y_G12_Cov', '<f4'), # [mag**2] H–G12 covariance (y band).
86 ('y_nObsUsed', '<i4'), # The number of data points used to fit the phase curve (y band).
87 ('y_Chi2', '<f4'), # Chi^2 statistic of the phase curve fit (y band).
88 ('y_phaseAngleMin', '<f4'), # [deg] Minimum phase angle observed (y band).
89 ('y_phaseAngleMax', '<f4'), # [deg] Maximum phase angle observed (y band).
90 ('y_slope_fit_failed', '|b1'), # G12 fit failed in y band. G12 contains a fiducial value used to fit H.
91])
93# SSSource: LSST-computed per-source quantities. 1::1 relationship with DiaSource.
94SSSourceDtype = np.dtype([
95 ('diaSourceId', '<i8'), # Unique identifier of the observation (matching DiaSource.diaSourceId).
96 ('ssObjectId', '<i8'), # Unique LSST identifier of the Solar System object.
97 ('designation', '<U16'), # The unpacked primary provisional designation for this object.
98 ('eclLambda', '<f8'), # [deg] Ecliptic longitude, converted from the observed coordinates.
99 ('eclBeta', '<f8'), # [deg] Ecliptic latitude, converted from the observed coordinates.
100 ('galLon', '<f8'), # [deg] Galactic longitude, converted from the observed coordinates.
101 ('galLat', '<f8'), # [deg] Galactic latitude, converted from the observed coordinates.
102 ('elongation', '<f4'), # [deg] Solar elongation of the object at the time of observation.
103 ('phaseAngle', '<f4'), # [deg] Phase angle between the Sun, object, and observer.
104 ('topoRange', '<f4'), # [AU] Topocentric distance (delta) at light-emission time.
105 ('topoRangeRate', '<f4'), # [km/s] Topocentric radial (line-of-sight) velocity (deldot); positive
106 # values indicate motion away from the observer.
107 ('helioRange', '<f4'), # [AU] Heliocentric distance (r) at light-emission time.
108 ('helioRangeRate', '<f4'), # [km/s] Heliocentric radial velocity (rdot); positive values indicate
109 # motion away from the Sun.
110 ('ephRa', '<f8'), # [deg] Predicted ICRS right ascension from the orbit in mpc_orbits.
111 ('ephDec', '<f8'), # [deg] Predicted ICRS declination from the orbit in mpc_orbits.
112 ('ephVmag', '<f4'), # [mag] Predicted magnitude in V band, computed from mpc_orbits data
113 # including the mpc_orbits-provided (H, G) estimates
114 ('ephRate', '<f4'), # [deg/d] Total predicted on-sky angular rate of motion.
115 ('ephRateRa', '<f4'), # [deg/d] Predicted on-sky angular rate in the R.A. direction (includes
116 # the cos(dec) factor).
117 ('ephRateDec', '<f4'), # [deg/d] Predicted on-sky angular rate in the declination direction.
118 ('ephOffset', '<f4'), # [arcsec] Total observed versus predicted angular separation on the sky.
119 ('ephOffsetRa', '<f8'), # [arcsec] Offset between observed and predicted position in the R.A.
120 # direction (includes cos(dec) term).
121 ('ephOffsetDec', '<f8'), # [arcsec] Offset between observed and predicted position in declination.
122 ('ephOffsetAlongTrack', '<f4'), # [arcsec] Offset between observed and predicted position in the
123 # along-track direction on the sky.
124 ('ephOffsetCrossTrack', '<f4'), # [arcsec] Offset between observed and predicted position in the
125 # cross-track direction on the sky.
126 ('helio_x', '<f4'), # [AU] Cartesian heliocentric X coordinate at light-emission time (ICRS).
127 ('helio_y', '<f4'), # [AU] Cartesian heliocentric Y coordinate at light-emission time (ICRS).
128 ('helio_z', '<f4'), # [AU] Cartesian heliocentric Z coordinate at light-emission time (ICRS).
129 ('helio_vx', '<f4'), # [km/s] Cartesian heliocentric X velocity at light-emission time (ICRS).
130 ('helio_vy', '<f4'), # [km/s] Cartesian heliocentric Y velocity at light-emission time (ICRS).
131 ('helio_vz', '<f4'), # [km/s] Cartesian heliocentric Z velocity at light-emission time (ICRS).
132 ('helio_vtot', '<f4'), # [km/s] The magnitude of the heliocentric velocity vector, sqrt(vx*vx +
133 # vy*vy + vz*vz).
134 ('topo_x', '<f4'), # [AU] Cartesian topocentric X coordinate at light-emission time (ICRS).
135 ('topo_y', '<f4'), # [AU] Cartesian topocentric Y coordinate at light-emission time (ICRS).
136 ('topo_z', '<f4'), # [AU] Cartesian topocentric Z coordinate at light-emission time (ICRS).
137 ('topo_vx', '<f4'), # [km/s] Cartesian topocentric X velocity at light-emission time (ICRS).
138 ('topo_vy', '<f4'), # [km/s] Cartesian topocentric Y velocity at light-emission time (ICRS).
139 ('topo_vz', '<f4'), # [km/s] Cartesian topocentric Z velocity at light-emission time (ICRS).
140 ('topo_vtot', '<f4'), # [km/s] The magnitude of the topocentric velocity vector, sqrt(vx*vx +
141 # vy*vy + vz*vz).
142 ('diaDistanceRank', '<i2'), # The rank of the diaSourceId-identified source in terms of its closeness
143 # to the predicted SSO position. If diaSourceId is the nearest DiaSour...
144])
146# mpc_orbits: Table of orbital elements and related information of known (sun-orbiting and unbound) Solar
147# System objects. Replicated from the Minor Planet Center (Postgres) database. This schema will generally
148# closely follow the schema of the upstream table, to allow end-users to rerun queries developed elsewhere on
149# the RSP.
150mpc_orbitsDtype = np.dtype([
151 ('id', '<i4'), # Internal ID (generally not seen/used by the user)
152 ('designation', '<U16'), # The primary provisional designation in unpacked form (e.g. 2008 AB).
153 ('packed_primary_provisional_designation', '<U16'), # The primary provisional designation in packed form
154 # (e.g. K08A00B)
155 ('unpacked_primary_provisional_designation', '<U16'), # The primary provisional designation in unpacked
156 # form (e.g. 2008 AB)
157 ('mpc_orb_jsonb', '|O'), # Details of the orbit solution in JSON form
158 ('created_at', '<M8[ns]'), # When this row was created
159 ('updated_at', '<M8[ns]'), # When this row was updated
160 ('orbit_type_int', '<i4'), # Orbit Type (Integer)
161 ('u_param', '<i4'), # U parameter
162 ('nopp', '<i4'), # number of oppositions
163 ('arc_length_total', '<f8'), # [d] Arc length over total observations [days]
164 ('arc_length_sel', '<f8'), # [d] Arc length over total observations *selected* [days]
165 ('nobs_total', '<i4'), # Total number of all observations (optical + radar) available
166 ('nobs_total_sel', '<i4'), # Total number of all observations (optical + radar) selected for use in
167 # orbit fitting
168 ('a', '<f8'), # [AU] Semi Major Axis [au]
169 ('q', '<f8'), # [AU] Pericenter Distance [au]
170 ('e', '<f8'), # Eccentricity
171 ('i', '<f8'), # [deg] Inclination [degrees]
172 ('node', '<f8'), # [deg] Longitude of Ascending Node [degrees]
173 ('argperi', '<f8'), # [deg] Argument of Pericenter [degrees]
174 ('peri_time', '<f8'), # [d] Time from Pericenter Passage [days]
175 ('yarkovsky', '<f8'), # [1e-10.au.d-2] Yarkovsky Component [10^(-10)*au/day^2]
176 ('srp', '<f8'), # [m2.t-1] Solar-Radiation Pressure Component [m^2/ton]
177 ('a1', '<f8'), # [m2.t-1] A1 non-grav components [m^2/ton]
178 ('a2', '<f8'), # [m2.t-1] A2 non-grav components [m^2/ton]
179 ('a3', '<f8'), # [m2.t-1] A3 non-grav components [m^2/ton]
180 ('dt', '<f8'), # DT non-grav component
181 ('mean_anomaly', '<f8'), # [deg] Mean Anomaly [degrees]
182 ('period', '<f8'), # [d] Orbital Period [days]
183 ('mean_motion', '<f8'), # [deg.d-1] Orbital Mean Motion [degrees per day]
184 ('a_unc', '<f8'), # [AU] Uncertainty on Semi Major Axis [au]
185 ('q_unc', '<f8'), # [AU] Uncertainty on Pericenter Distance [au]
186 ('e_unc', '<f8'), # Uncertainty on Eccentricity
187 ('i_unc', '<f8'), # [deg] Uncertainty on Inclination [degrees]
188 ('node_unc', '<f8'), # [deg] Uncertainty on Longitude of Ascending Node [degrees]
189 ('argperi_unc', '<f8'), # [deg] Uncertainty on Argument of Pericenter [degrees]
190 ('peri_time_unc', '<f8'), # [d] Uncertainty on Time from Pericenter Passage [days]
191 ('yarkovsky_unc', '<f8'), # [1e-10.au.d-2] Uncertainty on Yarkovsky Component [10^(-10)*au/day^2]
192 ('srp_unc', '<f8'), # [m2.t-1] Uncertainty on Solar-Radiation Pressure Component [m^2/ton]
193 ('a1_unc', '<f8'), # [m2.t-1] Uncertainty on A1 non-grav components [m^2/ton]
194 ('a2_unc', '<f8'), # [m2.t-1] Uncertainty on A2 non-grav components [m^2/ton]
195 ('a3_unc', '<f8'), # [m2.t-1] Uncertainty on A3 non-grav components [m^2/ton]
196 ('dt_unc', '<f8'), # Uncertainty on DT non-grav component
197 ('mean_anomaly_unc', '<f8'), # [deg] Uncertainty on Mean Anomaly [degrees]
198 ('period_unc', '<f8'), # [d] Uncertainty on Orbital Period [days]
199 ('mean_motion_unc', '<f8'), # [deg.d-1] Uncertainty on Orbital Mean Motion [degrees per day]
200 ('epoch_mjd', '<f8'), # [d] Epoch of the Orbfit-Solution in MJD
201 ('h', '<f8'), # [mag] H-Magnitude
202 ('g', '<f8'), # G-Slope Parameter
203 ('not_normalized_rms', '<f8'), # [arcsec] unnormalized rms of the fit [arcsec]
204 ('normalized_rms', '<f8'), # rms of the fit [unitless]
205 ('earth_moid', '<f8'), # [AU] Minimum Orbit Intersection Distance [au] with respect to the
206 # Earths Orbit
207 ('fitting_datetime', '<M8[ns]'), # Date of the last orbit fit
208])
210# current_identifications: All single-designations, and all identifications between designations. Always uses
211# primary provisional designation (even for numbered objects). Includes all comets and satellites. Replicated
212# from the Minor Planet Center (Postgres) database. This schema will generally closely follow the schema of
213# the upstream table, to allow end-users to rerun queries developed elsewhere on the RSP.
214current_identificationsDtype = np.dtype([
215 ('id', '<i4'), # Internal ID (generally not seen/used by the user)
216 ('packed_primary_provisional_designation', '<U16'), # The primary provisional designation in packed form
217 # (e.g. K08A00B)
218 ('packed_secondary_provisional_designation', '<U16'), # The secondary provisional designation in packed
219 # form (e.g. K08A00B). May be the same-as (A=A)...
220 ('unpacked_primary_provisional_designation', '<U16'), # The primary provisional designation in unpacked
221 # form (e.g. 2008 AB)
222 ('unpacked_secondary_provisional_designation', '<U16'), # The secondary provisional designation in
223 # unpacked form (e.g. 2008 AB). May be the...
224 ('published', '|b1'), # Has this been published yet? i.e. has it been released to the public?
225 ('identifier_ids', '|O'), # This is a set of unique identifier_ids in an array that points to the
226 # identification_metadata table.
227 ('object_type', '<i4'), # Integer to indicate the object type. To be linked (foreign key) to
228 # object_type lookup table
229 ('numbered', '|b1'), # Has the object been numbered and hence does it appear in the
230 # numbered_objects table?
231 ('created_at', '<M8[ns]'), # When this row was created
232 ('updated_at', '<M8[ns]'), # When this row was updated
233])
235# numbered_identifications: The numbered identification table contains all the numbered objects (minor
236# planets, comets and natural satellites) with their primary provisional designations. The table is
237# continously updated everytime a new object is numbered. Replicated from the Minor Planet Center (Postgres)
238# database. This schema will generally closely follow the schema of the upstream table, to allow end-users to
239# rerun queries developed elsewhere on the RSP.
240numbered_identificationsDtype = np.dtype([
241 ('id', '<i4'), # Internal ID (generally not seen/used by the user)
242 ('packed_primary_provisional_designation', '<U16'), # The primary provisional designation in packed form
243 # (e.g. K08A00B)
244 ('unpacked_primary_provisional_designation', '<U16'), # The primary provisional designation in unpacked
245 # form (e.g. 2008 AB)
246 ('permid', '<U16'), # Permanent designation (number)
247 ('iau_designation', '|O'), # IAU-approved designation (not filled at the moment)
248 ('iau_name', '<U32'), # IAU-approved name (not filled at the moment)
249 ('numbered_publication_references', '|O'), # MPEC where this object was numbered
250 ('named_publication_references', '|O'), # MPEC where this object was named
251 ('naming_credit', '|O'), # Credit for suggesting the name
252 ('created_at', '<M8[ns]'), # When this row was created
253 ('updated_at', '<M8[ns]'), # When this row was updated
254])