| | 115 | |
| | 116 | }}} |
| | 117 | |
| | 118 | The survey table is a copy of the PSPS table Survey. |
| | 119 | |
| | 120 | {{{ |
| | 121 | |
| | 122 | +----------+------+------------------------------------+ |
| | 123 | | surveyID | surveyName | description | |
| | 124 | +----------+------------+--------------------------------------------------------------+ |
| | 125 | | 0 | 3PI | PS1 3PI Survey | |
| | 126 | | 1 | MD01 | PS1 MD01 XMM-LSS-DXS 022224-043000 | |
| | 127 | | 2 | MD02 | PS1 MD02 CDFS/GOODS/GEMS 033224-274800 | |
| | 128 | | 3 | MD03 | PS1 MD03 IFA/Lynx 084300+444000 | |
| | 129 | | 4 | MD04 | PS1 MD04 COSMOS 100000+021200 | |
| | 130 | | 5 | MD05 | PS1 MD05 Lockman-DXS 110000+570000 | |
| | 131 | | 6 | MD06 | PS1 MD06 NGC 4258 121857+471814 | |
| | 132 | | 7 | MD07 | PS1 MD07 VISTA-Video1 140000+050000 | |
| | 133 | | 8 | MD08 | PS1 MD08 EliasN1-DXS 160000+570000 | |
| | 134 | | 9 | MD09 | PS1 MD09 Vimos4-DXS-SSA 220000+003000 | |
| | 135 | | 10 | MD10 | PS1 MD10 Deep2 233000+000000 | |
| | 136 | | 11 | M31 | PS1 M31 Andromeda 004242+411600 | |
| | 137 | | 12 | STS1 | PS1 STS1 Outskirts of Bulge 195048+170339 | |
| | 138 | | 13 | CAL01 | PS1 Cal North Pole 000000+900000 | |
| | 139 | | 14 | CAL02 | PS1 Cal SA92 Dense Landolt Std Field 005808+004232 | |
| | 140 | | 15 | CAL03 | PS1 Cal Perseus Cluster / Abell 426 031900+413300 | |
| | 141 | | 16 | CAL04 | PS1 Cal SA95 Dense Landolt Std Field 065207+001710 | |
| | 142 | | 17 | CAL05 | PS1 Cal Taurus dark cloud (diverse extinction) 043000+250000 | |
| | 143 | | 18 | CAL06 | PS1 Cal SA98 Densle Landolt Std Field 065207+001710 | |
| | 144 | | 19 | CAL07 | PS1 Cal M81-M82-HolmIX (Local Group) 095640+692200 | |
| | 145 | | 20 | CAL08 | PS1 Cal Virgo Cluster (Center) 123000+130000 | |
| | 146 | | 21 | CAL09 | PS1 Cal Hercules Cluster (Center) 160508+1745+28 | |
| | 147 | | 22 | CAL10 | PS1 Cal M17-M24 Region 181400+000544 | |
| | 148 | | 23 | CAL11 | PS1 Cal SA110 Dense Landolt Std Field 184207+000544 | |
| | 149 | | 24 | CAL12 | PS1 Cal Kepler Mission Astrometric field 192240+443000 | |
| | 150 | | 25 | CAL13 | PS1 Cal 3C454.1 (Northern field) 225033+712919 | |
| | 151 | | 26 | STS2 | PS1 STS2 Hyades 004000+150000 | |
| | 152 | | 27 | STS3 | PS1 STS3 Praesepe 083000+200000 | |
| | 153 | | 28 | SSS | PS1 Solar System Sweet Spot Survey | |
| | 154 | +----------+------------+--------------------------------------------------------------+ |
| | 155 | }}} |
| | 156 | |
| | 157 | === ippRelease === |
| | 158 | {{{ |
| 115 | | +-------------+-------------+------+-----+---------+----------------+ |
| 116 | | | Field | Type | Null | Key | Default | Extra | |
| 117 | | +-------------+-------------+------+-----+---------+----------------+ |
| 118 | | | rel_id | smallint(6) | NO | PRI | NULL | auto_increment | |
| 119 | | | surveyID | tinyint(8) | YES | MUL | NULL | | |
| 120 | | | releaseName | varchar(16) | YES | MUL | NULL | | |
| 121 | | | state | varchar(16) | YES | MUL | NULL | | |
| 122 | | | dataRelease | tinyint(8) | YES | | NULL | | |
| 123 | | +-------------+-------------+------+-----+---------+----------------+ |
| 124 | | 5 rows in set (0.00 sec) |
| 125 | | }}} |
| 126 | | |
| 127 | | The survey table is a copy of the PSPS table Survey. Example entries are |
| 128 | | |
| 129 | | {{{ |
| 130 | | +----------+------+------------------------------------+ |
| 131 | | | surveyID | name | description | |
| 132 | | +----------+------+------------------------------------+ |
| 133 | | | 0 | 3PI | PS1 3PI Survey | |
| 134 | | | 1 | MD01 | PS1 MD01 XMM-LSS-DXS 022224-043000 | |
| 135 | | +----------+------+------------------------------------+ |
| | 160 | +---------------+-------------+------+-----+---------+----------------+ |
| | 161 | | Field | Type | Null | Key | Default | Extra | |
| | 162 | +---------------+-------------+------+-----+---------+----------------+ |
| | 163 | | rel_id | int(8) | NO | PRI | NULL | auto_increment | |
| | 164 | | surveyID | int(8) | YES | MUL | NULL | | |
| | 165 | | releaseName | varchar(64) | YES | MUL | NULL | | |
| | 166 | | release_state | varchar(16) | YES | MUL | NULL | | |
| | 167 | | dataRelease | int(8) | YES | | NULL | | |
| | 168 | | priority | int(11) | YES | | NULL | | |
| | 169 | +---------------+-------------+------+-----+---------+----------------+ |
| | 170 | 6 rows in set (0.00 sec) |
| 147 | | * dataRelease - If not null, the dataRelease value in the corresponding PSPS tables. |
| 148 | | |
| 149 | | Some examples |
| 150 | | {{{ |
| 151 | | +--------+----------+-------------+---------+-------------+ |
| 152 | | | rel_id | surveyID | releaseName | state | dataRelease | |
| 153 | | +--------+----------+-------------+---------+-------------+ |
| 154 | | | 1 | 0 | 3PI.nightly | active | NULL | |
| 155 | | | 2 | 0 | 3PI.GR0 | active | 0 | |
| 156 | | | 3 | 0 | 3PI.GR1 | pending | 1 | |
| 157 | | | 4 | 0 | SAS.V8 | archive | 8 | |
| 158 | | | 5 | 0 | SAS.V9 | active | 9 | |
| 159 | | +--------+----------+-------------+---------+-------------+ |
| 160 | | }}} |
| 161 | | |
| 162 | | The 3PI.nightly release is active. Data is being currently added to it and is available to users who request |
| 163 | | data from that processing. Since these data are no longer being ingested into PSPS the dataRelease field is |
| 164 | | null. |
| 165 | | |
| 166 | | 3PI.GR0 refers to the version of LAP processing that is currently in the PSPS database PS1_3PI. Data |
| 167 | | corresponding to that release is identified by dataRelease 0, while 3PI.GR1 refers to the future |
| 168 | | LAP release which will begin construction soon. Once that release gets under way it's state will be set |
| 169 | | to active while 3PI.GR0 will be set to "archive". XXX: insure that PSPS uses a different dataRelease ... |
| 170 | | |
| 171 | | The two SAS entries refer to PS1_SAS_08 and PS1_SAS_09. |
| | 182 | * dataRelease - If not negative, the dataRelease value in the PSPS tables corresponding to this ippRelease. |
| | 183 | * priority - An integer value giving the priority of the various releases for the survey. |
| | 184 | |
| | 185 | Here is an example of how this system might work for the 3pi survey. Assume that we have finished the |
| | 186 | current grand reprocessing and are ready to start the next one. |
| | 187 | |
| | 188 | {{{ |
| | 189 | mysql> select * from ippRelease where releaseName like '3%' order by priority desc; |
| | 190 | +--------+----------+-------------+---------------+-------------+----------+ |
| | 191 | | rel_id | surveyID | releaseName | release_state | dataRelease | priority | |
| | 192 | +--------+----------+-------------+---------------+-------------+----------+ |
| | 193 | | 5 | 0 | 3PI.GR1 | active | 1 | 2 | |
| | 194 | | 1 | 0 | 3PI.nightly | active | -1 | 0 | |
| | 195 | | 2 | 0 | 3PI.GR0 | archive | 0 | -1 | |
| | 196 | | 6 | 0 | 3PI.GR2 | pending | 2 | NULL | |
| | 197 | +--------+----------+-------------+---------------+-------------+----------+ |
| | 198 | 4 rows in set (0.00 sec) |
| | 199 | }}} |
| | 200 | |
| | 201 | There are 4 releases shown here. |
| | 202 | |
| | 203 | The 3PI.nightly release is active. Data is being currently added to it by the IPP nightly science |
| | 204 | processing. Since these data are not being ingested into PSPS the dataRelease column is -1. |
| | 205 | |
| | 206 | 3PI.GR1 refers to the current 3PI "grand reprocessing". This release is active. dataRelease == 1 |
| | 207 | |
| | 208 | The 2011 grand reprocessing is named here 3PI.GR0 (LAP.ThreePi.20110809). The state for this |
| | 209 | release is archive. Data corresponding to that release is identified by dataRelease == 0. |
| | 210 | |
| | 211 | 3PI.GR2 is the next grand reprocessing dataRelease == 2. The state of this release is pending. |
| | 212 | |
| | 213 | The priority column is used to select the release of the data that should returned by the IPP |
| | 214 | when users request a given exposure or skycell. The query above demonstrates the idea. It orders the |
| | 215 | releases by descending priority. The postage stamp server and other release mechanisms |
| | 216 | will use queries ordered this way. |
| | 217 | |
| | 218 | Data will be returned from the highest priority release. In our example this is 3PI.GR1. If the |
| | 219 | given exposure or skycell has not been (successfully) processed in the highest priority release |
| | 220 | data will be returned from a lower priority release. |
| | 221 | |
| | 222 | Note: This scheme will be used for request where the user has not explicitly listed the release of interest. |
| | 223 | All IPP data will be still be available if the user can identify it. |
| | 224 | |
| | 225 | == Released Exposure == |
| 188 | | | relexp_id | bigint(20) | NO | PRI | NULL | auto_increment | Primary key for the table |
| 189 | | | rel_id | smallint(6) | YES | MUL | NULL | | The corresponding release |
| 190 | | | exp_id | bigint(20) | YES | | NULL | | The IPP exposure identifier |
| 191 | | | chip_id | bigint(20) | YES | | NULL | | id for chipRun |
| 192 | | | cam_id | bigint(20) | YES | | NULL | | id for camRun |
| 193 | | | warp_id | bigint(20) | YES | | NULL | | id for warpRun |
| 194 | | | add_id | bigint(20) | YES | | NULL | | id for addRun (addstar injest into DVO) |
| 195 | | | state | varchar(16) | YES | MUL | NULL | | state for this row see below |
| 196 | | | data_state | varchar(16) | YES | MUL | NULL | | see below |
| | 242 | | relexp_id | bigint(20) | NO | PRI | NULL | auto_increment | |
| | 243 | | rel_id | int(8) | YES | MUL | NULL | | |
| | 244 | | exp_id | bigint(20) | YES | MUL | NULL | | |
| | 245 | | chip_id | bigint(20) | YES | MUL | NULL | | |
| | 246 | | cam_id | bigint(20) | YES | MUL | NULL | | |
| | 247 | | state | varchar(16) | YES | MUL | NULL | | |
| 210 | | Each time an exposure is released a new row will be added to the table. |
| 211 | | |
| 212 | | Here are a couple of examples showing the releases for one of the SAS exposures: |
| 213 | | {{{ |
| 214 | | mysql> mysql> select ippRelease.releaseName, relExp.* from ippRelease join relExp using(rel_id) where exp_id = 356773; |
| 215 | | +-------------+-----------+--------+--------+---------+--------+---------+--------+----------+------------+-------+---------+-----------+-----------+---------------------+---------------------+ |
| 216 | | | releaseName | relexp_id | rel_id | exp_id | chip_id | cam_id | warp_id | add_id | state | data_state | flags | zpt_obs | zpt_stdev | path_base | registered | time_stamp | |
| 217 | | +-------------+-----------+--------+--------+---------+--------+---------+--------+----------+------------+-------+---------+-----------+-----------+---------------------+---------------------+ |
| 218 | | | SAS.V8 | 1 | 4 | 356773 | 496671 | 473031 | 453844 | 883989 | archive | inpsps | 0 | 24.4298 | 0.042454 | NULL | 2012-09-19 15:16:36 | 2012-09-19 15:16:36 | |
| 219 | | | SAS.V9 | 621 | 5 | 356773 | 496671 | 473031 | 453844 | 888750 | released | inpsps | 0 | 24.4298 | 0.042454 | NULL | 2012-09-19 15:18:51 | 2012-09-19 15:18:51 | |
| 220 | | +-------------+-----------+--------+--------+---------+--------+---------+--------+----------+------------+-------+---------+-----------+-----------+---------------------+---------------------+ |
| 221 | | 2 rows in set (0.00 sec) |
| 222 | | |
| 223 | | }}} |
| 224 | | |
| 225 | | |
| 226 | | Note that the list of ids are the same except for the add_id. This is because SAS_v9 was constructed |
| 227 | | using the SAS_v8 pixels. For single frame exposures only the DVO injest and calibration was redone. This is |
| 228 | | indicated by the change in add_id. |
| 229 | | |
| 230 | | ==== state / data_state / flags ==== |
| 231 | | There are three columns related to the state of the released exposure. We haven't yet settled on which of |
| 232 | | these data are required to manage the releases. Information that we might want to record include |
| 233 | | * state - active, drop, archive (note that the release state |
| 234 | | * has the released exposure been imported into PSPS |
| 235 | | * did the calibration apply ubercal. Perhaps: if so which version? |
| 236 | | * was the data the result of a recalibration, relphot, relastro, something else ... |
| | 261 | Each time an exposure is added to a release a new row will be added to this table. |
| | 262 | |
| | 263 | ==== state ==== |
| | 264 | A released exposure may go through a sequence of states |
| | 265 | |
| | 266 | * processed - The initial results of the camera stage for the exposure. |
| | 267 | * poor_quality - The camRun failed to find a solution for the exposure. |
| | 268 | * calibrated - The calibration information (zero point and astrometry) has been updated by a DVO calibration operation |
| | 269 | * psps - The information from the exposure has been added to the PSPS database corresponding to the release. |
| | 270 | * drop - This relExp is to be dropped for some reason. |
| | 271 | |
| | 272 | The full results and history of any calibration operations will be stored in files referenced by the relExp's path_base. |
| 239 | | ==== Nightly science ==== |
| 240 | | We envision the following potential events in the history of a released exposure for the nightly science |
| 241 | | releases |
| 242 | | * created during nightly science processing once the warp has been completed before the addRun is processed. State active. |
| 243 | | * updated to include the add_id of the addRun |
| 244 | | |
| 245 | | ==== Grand Reprocessing ==== |
| 246 | | For the grand reprocessing, the relExp goes through two states |
| 247 | | |
| 248 | | * row is created when addstar is performed. State set to pending. |
| 249 | | * row is updated when ipptoPSPS is run. At that time the calibration data is updated with the resulting values and the state columns are changed to reflect the PSPS export. state => active |
| 250 | | |
| 251 | | Separating the state into two steps allows the results of the re-processing to be made available prior to |
| 252 | | PSPS injest if the user requests data from the corresponding release. The data will not be the "default" for |
| 253 | | the given exposure until the calibration is complete at the time of PSPS ingest. |
| 254 | | |
| 255 | | ==== DVO Release ==== |
| 256 | | This schema allows (but does not require) the contents of DVO releases to be recorded. This would allow users |
| 257 | | of the DVO catalog to refer explicitly to a given set of pixels and calibration. |
| 258 | | |
| 259 | | == Released Skycell == |
| | 275 | |
| | 276 | |
| | 277 | |
| | 278 | == Released Stack == |
| 261 | | release and (tess_id, skycell_id). |
| 262 | | |
| 263 | | Here is the proposed table definition |
| 264 | | |
| 265 | | {{{ |
| 266 | | REATE TABLE relSkycell ( |
| 267 | | relstack_id BIGINT AUTO_INCREMENT, |
| 268 | | rel_id BIGINT, |
| 269 | | skycell_id varchar(64) |
| 270 | | tess_id varchar(64) |
| 271 | | state VARCHAR(16), -- current, pending, archive, drop |
| 272 | | data_state VARCHAR(16), -- nightly, relphot, relastro, psps |
| 273 | | stack_id BIGINT, -- id of the stack (pixels) |
| 274 | | skycal_id BIGINT, -- id of the sky calibration run that supplied the calibration |
| 275 | | -- for this release. |
| 276 | | -- NOTE: it is the skycal_id that we save, |
| 277 | | -- not the stack_id |
| 278 | | add_id BIGINT, |
| 279 | | zpt_obs FLOAT, -- calibrated zero point for this release of |
| 280 | | -- this skycell |
| 281 | | zpt_stdev FLOAT, |
| 282 | | path_base VARCHAR(255), -- path_base of any supporting files, |
| 283 | | -- updated WCS for example, |
| 284 | | -- we may just build a new cmf |
| 285 | | flags UNSIGNED INT, |
| 286 | | registered DATETIME, |
| 287 | | time_stamp DATETIME, |
| 288 | | PRIMARY KEY (rel_id), |
| 289 | | KEY (rel_id, tess_id, skycell_id), -- NOTE: no foreign key constraint |
| 290 | | -- becase we don't reference the |
| 291 | | -- stack directly. Insert query should |
| 292 | | -- enforce match. |
| 293 | | FOREIGN KEY(rel_id) REFERENCES ippRelease(rel_id), |
| 294 | | FOREIGN KEY(skycal_id) REFERENCES skycalRun(skycal_id), |
| 295 | | FOREIGN KEY(add_id) REFERENCES addRun(add_id) |
| 296 | | ) ENGINE=innodb DEFAULT CHARASET=latin1; |
| 297 | | }}} |
| 298 | | |
| 299 | | Stacks will also be released in two steps: |
| 300 | | * When the stack is constructed the relSkycell will be created in state pending. The calibration will not be set |
| 301 | | * Once the stack photometry and sky calibration are run the skycal_id will be included. |
| 302 | | |
| | 280 | release, tess_id, and skycell_id. |
| | 281 | |
| | 282 | {{ |
| | 283 | mysql> describe relStack; |
| | 284 | +-------------+------------------+------+-----+---------+----------------+ |
| | 285 | | Field | Type | Null | Key | Default | Extra | |
| | 286 | +-------------+------------------+------+-----+---------+----------------+ |
| | 287 | | relstack_id | bigint(20) | NO | PRI | NULL | auto_increment | |
| | 288 | | rel_id | int(8) | YES | MUL | NULL | | |
| | 289 | | skycal_id | bigint(20) | YES | MUL | NULL | | |
| | 290 | | skycell_id | varchar(64) | YES | | NULL | | |
| | 291 | | tess_id | varchar(64) | YES | MUL | NULL | | |
| | 292 | | state | varchar(16) | YES | | NULL | | |
| | 293 | | flags | int(10) unsigned | YES | | NULL | | |
| | 294 | | stack_type | varchar(16) | YES | | NULL | | |
| | 295 | | zpt_obs | float | YES | | NULL | | |
| | 296 | | zpt_stdev | float | YES | | NULL | | |
| | 297 | | fwhm_major | float | YES | | NULL | | |
| | 298 | | path_base | varchar(255) | YES | | NULL | | |
| | 299 | | registered | datetime | YES | | NULL | | |
| | 300 | | time_stamp | datetime | YES | | NULL | | |
| | 301 | +-------------+------------------+------+-----+---------+----------------+ |
| | 302 | 14 rows in set (0.00 sec) |
| | 303 | |
| | 304 | }}} |
| | 305 | |
| | 306 | There are differences between relStack and the single frame table. |
| | 307 | |
| | 308 | * stack_type will have one of three values "deep", "reference", or "nightly" |
| | 309 | * fwhm_major will contain the measurement of the seeing as measured by psphotStack. This is currently not stored anywhere in the ipp database so it will be extracted from the cmf header by the process that creates the relStack entry. |