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Ignore:
Timestamp:
May 1, 2016, 12:20:15 PM (10 years ago)
Author:
eugene
Message:

fix description labels for various info flags (errors noted by Nigel M.); do NOT delete detections outside of cpt file boundaries; do NOT shift SECF_OBJ_EXT bit (0x0100000 to 0x2000)

File:
1 edited

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Unmodified
Added
Removed

  • trunk/ippToPsps/config/tables.IN.vot

    r39392 r39565  
    659659          <TR><TD>DIFF_WITH_SINGLE</TD>     <TD>0x00000001</TD><TD>1         </TD><TD>Difference source matched to a single positive detection.</TD></TR>
    660660          <TR><TD>DIFF_WITH_DOUBLE</TD>     <TD>0x00000002</TD><TD>2         </TD><TD>Difference source matched to positive detections in both images.</TD></TR>
    661           <TR><TD>MATCHED</TD>              <TD>0x00000004</TD><TD>4         </TD><TD>Difference source matched to positive detections in both images.</TD></TR>
     661          <TR><TD>MATCHED</TD>              <TD>0x00000004</TD><TD>4         </TD><TD>source generated based on another image (forced photometry at source location).</TD></TR>
    662662          <TR><TD>ON_SPIKE</TD>             <TD>0x00000008</TD><TD>8         </TD><TD>More than 25% of (PSF-weighted) pixels land on diffraction spike.</TD></TR>
    663663          <TR><TD>ON_STARCORE</TD>          <TD>0x00000010</TD><TD>16        </TD><TD>More than 25% of (PSF-weighted) pixels land on starcore.</TD></TR>
    … …  
    753753          <TR><TD>POOR</TD>             <TD>0x00000002</TD><TD>2              </TD><TD>Used within relphot; skip star.</TD></TR>
    754754          <TR><TD>ICRF_QSO</TD>         <TD>0x00000004</TD><TD>4              </TD><TD>object IDed with known ICRF quasar (may have ICRF position measurement)</TD></TR>
    755           <TR><TD>OTHEF_QSO</TD>        <TD>0x00000008</TD><TD>8              </TD><TD>identified as likely QSO (Hernitschek et al 2015), without ICRF reference data</TD></TR>
    756           <TR><TD>TRANSIENT</TD>        <TD>0x00000010</TD><TD>16             </TD><TD>identified as a non-periodic (stationary) transient</TD></TR>
    757           <TR><TD>VARIABLE</TD>         <TD>0x00000020</TD><TD>32             </TD><TD>identified as a periodic variable</TD></TR>
    758           <TR><TD>RRLYRA</TD>           <TD>0x00000040</TD><TD>64             </TD><TD>identified as likely RR Lyra (Hernitschek et al 2015)</TD></TR>
    759           <TR><TD>HAS_SOLSYS_DET</TD>   <TD>0x00000080</TD><TD>128            </TD><TD>identified with a known solar-system object (asteroid or other)</TD></TR>
    760           <TR><TD>ALL_SOLSYS_DET</TD>   <TD>0x00000100</TD><TD>256            </TD><TD>identified with a known solar-system object (asteroid or other)</TD></TR>
    761           <TR><TD>UNDEF_1</TD>          <TD>0x00000200</TD><TD>512            </TD><TD>Unused bit value.</TD></TR>
    762           <TR><TD>UNDEF_2</TD>          <TD>0x00000400</TD><TD>1024           </TD><TD>Unused bit value.</TD></TR>
     755          <TR><TD>HERN_QSO_P60</TD>     <TD>0x00000008</TD><TD>8              </TD><TD>identified as likely QSO (Hernitschek et al 2015), P_QSO >= 0.60</TD></TR>
     756          <TR><TD>HERN_QSO_P05</TD>     <TD>0x00000010</TD><TD>16             </TD><TD>identified as possible QSO (Hernitschek et al 2015), P_QSO >= 0.05</TD></TR>
     757          <TR><TD>HERN_RRL_P60</TD>     <TD>0x00000020</TD><TD>32             </TD><TD>identified as likely RR Lyra (Hernitschek et al 2015), P_RRLyra >= 0.60</TD></TR>
     758          <TR><TD>HERN_RRL_P05</TD>     <TD>0x00000040</TD><TD>64             </TD><TD>identified as possible RR Lyra (Hernitschek et al 2015), P_RRLyra >= 0.05</TD></TR>
     759          <TR><TD>HERN_VARIABLE</TD>    <TD>0x00000080</TD><TD>128            </TD><TD>identified as a variable based on ChiSq (Hernitschek et al 2015)</TD></TR>
     760          <TR><TD>TRANSIENT</TD>        <TD>0x00000100</TD><TD>256            </TD><TD>identified as a non-periodic (stationary) transient</TD></TR>
     761          <TR><TD>HAS_SOLSYS_DET</TD>   <TD>0x00000200</TD><TD>512            </TD><TD>at least one detection identified with a known solar-system object (asteroid or other).</TD></TR>
     762          <TR><TD>MOST_SOLSYS_DET</TD>  <TD>0x00000400</TD><TD>1024           </TD><TD>most detections identified with a known solar-system object (asteroid or other).</TD></TR>
    763763          <TR><TD>LARGE_PM</TD>         <TD>0x00000800</TD><TD>2048           </TD><TD>star with large proper motion</TD></TR>
    764764          <TR><TD>RAW_AVE</TD>          <TD>0x00001000</TD><TD>4096           </TD><TD>simple weighted average position was used (no IRLS fitting)</TD></TR>
    … …  
    777777          <TR><TD>GOOD</TD>             <TD>0x02000000</TD><TD>33554432       </TD><TD>good-quality measurement in our data (eg,PS)</TD></TR>
    778778          <TR><TD>GOOD_ALT</TD>         <TD>0x04000000</TD><TD>67108864       </TD><TD>good-quality measurement in  external data (eg, 2MASS)</TD></TR>
    779           <TR><TD>GOOD_STACK</TD>       <TD>0x08000000</TD><TD>134217728      </TD><TD>good-quality object in the stack (> 1 good stack)</TD></TR>
    780           <TR><TD>BEST_STACK</TD>       <TD>0x10000000</TD><TD>268435456      </TD><TD>the primary stack measurement are the best measurements</TD></TR>
    781           <TR><TD>SUSPECT_STACK</TD>    <TD>0x20000000</TD><TD>536870912      </TD><TD>suspect object in the stack (> 1 good or suspect stack, less than 2 good)</TD></TR>
    782           <TR><TD>BAD_STACK</TD>        <TD>0x40000000</TD><TD>1073741824     </TD><TD>good-quality object in the stack (> 1 good stack)</TD></TR>
     779          <TR><TD>GOOD_STACK</TD>       <TD>0x08000000</TD><TD>134217728      </TD><TD>good-quality object in the stack (> 1 good stack measurement)</TD></TR>
     780          <TR><TD>BEST_STACK</TD>       <TD>0x10000000</TD><TD>268435456      </TD><TD>the primary stack measurements are the best measurements</TD></TR>
     781          <TR><TD>SUSPECT_STACK</TD>    <TD>0x20000000</TD><TD>536870912      </TD><TD>suspect object in the stack (no more than 1 good measurement, 2 or more suspect or good stack measurement)</TD></TR>
     782          <TR><TD>BAD_STACK</TD>        <TD>0x40000000</TD><TD>1073741824     </TD><TD>poor-quality stack object (no more than 1 good or suspect measurement)</TD></TR>
    783783        </TABLEDATA>
    784784      </DATA>
    … …  
    809809          <TR><TD>SECF_USE_UBERCAL</TD>  <TD>0x00000008</TD><TD>8              </TD><TD>Ubercal photometry used in average measurement.</TD></TR>
    810810          <TR><TD>SECF_HAS_PS1</TD>      <TD>0x00000010</TD><TD>16             </TD><TD>PS1 photometry used in average measurement.</TD></TR>
    811           <TR><TD>SECF_HAS_STACK</TD>    <TD>0x00000020</TD><TD>32             </TD><TD>PS1 stack photometry exists.</TD></TR>
     811          <TR><TD>SECF_HAS_PS1_STACK</TD><TD>0x00000020</TD><TD>32             </TD><TD>PS1 stack photometry exists.</TD></TR>
    812812
    813813          <TR><TD>SECF_HAS_TYCHO</TD>    <TD>0x00000040</TD><TD>64             </TD><TD>Tycho photometry used for synthetic magnitudes.</TD></TR>
    814814          <TR><TD>SECF_FIX_SYNTH</TD>    <TD>0x00000080</TD><TD>128            </TD><TD>Synthetic magnitudes repaired with zeropoint map.</TD></TR>
    815815
    816           <TR><TD>PHOTOM_PASS_0</TD>     <TD>0x00000100</TD><TD>256            </TD><TD>Average magnitude calculated in 0th pass.</TD></TR>
    817           <TR><TD>PHOTOM_PASS_1</TD>     <TD>0x00000200</TD><TD>512            </TD><TD>Average magnitude calculated in 1th pass.</TD></TR>
    818           <TR><TD>PHOTOM_PASS_2</TD>     <TD>0x00000400</TD><TD>1024           </TD><TD>Average magnitude calculated in 2th pass.</TD></TR>
    819           <TR><TD>PHOTOM_PASS_3</TD>     <TD>0x00000800</TD><TD>2048           </TD><TD>Average magnitude calculated in 3th pass.</TD></TR>
    820           <TR><TD>PHOTOM_PASS_4</TD>     <TD>0x00001000</TD><TD>4096           </TD><TD>Average magnitude calculated in 4th pass.</TD></TR>
    821           <TR><TD>PSPS_OBJ_EXT</TD>      <TD>0x00002000</TD><TD>8192           </TD><TD>Extended in this band (PSPS only).</TD></TR>
     816          <TR><TD>SECF_RANK_0</TD>       <TD>0x00000100</TD><TD>256            </TD><TD>Average magnitude uses only rank 0 detections.</TD></TR>
     817          <TR><TD>SECF_RANK_1</TD>       <TD>0x00000200</TD><TD>512            </TD><TD>Average magnitude uses only rank 1 detections.</TD></TR>
     818          <TR><TD>SECF_RANK_2</TD>       <TD>0x00000400</TD><TD>1024           </TD><TD>Average magnitude uses only rank 2 detections.</TD></TR>
     819          <TR><TD>SECF_RANK_3</TD>       <TD>0x00000800</TD><TD>2048           </TD><TD>Average magnitude uses only rank 3 detections.</TD></TR>
     820          <TR><TD>SECF_RANK_4</TD>       <TD>0x00001000</TD><TD>4096           </TD><TD>Average magnitude uses only rank 4 detections.</TD></TR>
    822821          <TR><TD>SECF_STACK_PRIMARY</TD><TD>0x00004000</TD><TD>16384          </TD><TD>PS1 stack photometry comes from primary skycell.</TD></TR>
     822          <TR><TD>SECF_OBJ_EXT</TD>      <TD>0x01000000</TD><TD>16777216       </TD><TD>Extended in this band.</TD></TR>
    823823        </TABLEDATA>
    824824      </DATA>
    … …  
    847847          <TR><TD>QF_OBJ_GOOD</TD>         <TD>0x00000004</TD><TD>4       </TD><TD>Good-quality measurement in our data (eg,PS).</TD></TR>
    848848          <TR><TD>QF_OBJ_GOOD_ALT</TD>     <TD>0x00000008</TD><TD>8       </TD><TD>Good-quality measurement in  external data (eg, 2MASS).</TD></TR>
    849           <TR><TD>QF_OBJ_GOOD_STACK</TD>   <TD>0x00000010</TD><TD>16      </TD><TD>Good-quality object in the stack (> 1 good stack).</TD></TR>
    850           <TR><TD>QF_OBJ_SUSPECT_STACK</TD><TD>0x00000020</TD><TD>32      </TD><TD>Suspect object in the stack (> 1 good or suspect stack, less tham 2 good).</TD></TR>
    851           <TR><TD>QF_OBJ_BAD_STACK</TD>    <TD>0x00000040</TD><TD>64      </TD><TD>Good-quality object in the stack (> 1 good stack).</TD></TR>
     849          <TR><TD>QF_OBJ_GOOD_STACK</TD>   <TD>0x00000010</TD><TD>16      </TD><TD>good-quality object in the stack (> 1 good stack measurement)</TD></TR>
     850          <TR><TD>QF_OBJ_BEST_STACK</TD>   <TD>0x00000020</TD><TD>32      </TD><TD>the primary stack measurements are the best measurements.</TD></TR>
     851          <TR><TD>QF_OBJ_SUSPECT_STACK</TD><TD>0x00000040</TD><TD>64      </TD><TD>suspect object in the stack (no more than 1 good measurement, 2 or more suspect or good stack measurement).</TD></TR>
     852          <TR><TD>QF_OBJ_BAD_STACK</TD>    <TD>0x00000080</TD><TD>64      </TD><TD>poor-quality stack object (no more than 1 good or suspect measurement).</TD></TR>
    852853        </TABLEDATA>
    853854      </DATA>
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