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Ignore:
Timestamp:
Oct 27, 2017, 3:38:36 PM (9 years ago)
Author:
heather
Message:

tables.IN.vot and the database paper tables are now completely in sync. Includes scripts and instructions to make comparisons in the future.

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1 edited

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

    r40101 r40186  
    576576        <TABLEDATA>
    577577          <TR><TD>NEW</TD>           <TD>0x00000000</TD><TD>0</TD><TD>No relphot / relastro attempted.</TD></TR>
    578           <TR><TD>PHOTOM_NOCAL</TD>  <TD>0x00000001</TD><TD>1</TD><TD>Used within relphot to mean 'don't apply fit'. | user-set value used withing relphot: ignore (EAM!)</TD></TR>
    579           <TR><TD>PHOTOM_POOR</TD>   <TD>0x00000002</TD><TD>2</TD><TD>Relphot says image is bad (dMcal > limit). (EAM!)</TD></TR>
    580           <TR><TD>PHOTOM_SKIP</TD>   <TD>0x00000004</TD><TD>4</TD><TD>External information image has bad photometry (EAM).</TD></TR>
     578          <TR><TD>PHOTOM_NOCAL</TD>  <TD>0x00000001</TD><TD>1</TD><TD>Used within relphot to mean 'don't apply fit'.</TD></TR>
     579          <TR><TD>PHOTOM_POOR</TD>   <TD>0x00000002</TD><TD>2</TD><TD>Relphot says image is bad (dMcal > limit).</TD></TR>
     580          <TR><TD>PHOTOM_SKIP</TD>   <TD>0x00000004</TD><TD>4</TD><TD>External information image has bad photometry.</TD></TR>
    581581          <TR><TD>PHOTOM_FEW</TD>    <TD>0x00000008</TD><TD>8</TD><TD>Currently too few measurements for good value for photometry.</TD></TR>
    582           <TR><TD>ASTROM_NOCAL</TD>  <TD>0x00000010</TD><TD>16</TD><TD>User-set value used within relastro: ignore (EAM!).</TD></TR>
     582          <TR><TD>ASTROM_NOCAL</TD>  <TD>0x00000010</TD><TD>16</TD><TD>User-set value used within relastro: ignore.</TD></TR>
    583583          <TR><TD>ASTROM_POOR</TD>   <TD>0x00000020</TD><TD>32</TD><TD>Relastro says image is bad (dR,dD > limit).</TD></TR>
    584584          <TR><TD>ASTROM_FAIL</TD>   <TD>0x00000040</TD><TD>64</TD><TD>Relastro fit diverged, fit not applied.</TD></TR>
    585           <TR><TD>ASTROM_SKIP</TD>   <TD>0x00000080</TD><TD>128</TD><TD>External information image has bad astrometry. (EAM)</TD></TR>
     585          <TR><TD>ASTROM_SKIP</TD>   <TD>0x00000080</TD><TD>128</TD><TD>External information image has bad astrometry.</TD></TR>
    586586          <TR><TD>ASTROM_FEW</TD>    <TD>0x00000100</TD><TD>256</TD><TD>Currently too few measurements for good value for astrometry.</TD></TR>
    587587          <TR><TD>PHOTOM_UBERCAL</TD><TD>0x00000200</TD><TD>512</TD><TD>Externally-supplied photometry zero point from ubercal analysis.</TD></TR>
    … …  
    614614          <TR><TD>EXTMODEL</TD>        <TD>0x00000002</TD><TD>2         </TD><TD>Source fitted with an extended-source model.</TD></TR>
    615615          <TR><TD>FITTED</TD>          <TD>0x00000004</TD><TD>4         </TD><TD>Source fitted with non-linear model (PSF or EXT; good or bad).</TD></TR>
    616           <TR><TD>FAIL</TD>            <TD>0x00000008</TD><TD>8         </TD><TD>Fit (non-linear) failed (non-converge, off-edge, run to zero).</TD></TR>
     616          <TR><TD>FAIL</TD>            <TD>0x00000008</TD><TD>8         </TD><TD>Fit (non-linear) failed (non-converge; off-edge; run to zero).</TD></TR>
    617617          <TR><TD>POOR</TD>            <TD>0x00000010</TD><TD>16        </TD><TD>Fit succeeds, but low-S/N, high-Chisq, or large (for PSF -- drop?).</TD></TR>
    618618          <TR><TD>PAIR</TD>            <TD>0x00000020</TD><TD>32        </TD><TD>Source fitted with a double PSF.</TD></TR>
    … …  
    669669          <TR><TD>DIFF_WITH_SINGLE</TD>     <TD>0x00000001</TD><TD>1         </TD><TD>Difference source matched to a single positive detection.</TD></TR>
    670670          <TR><TD>DIFF_WITH_DOUBLE</TD>     <TD>0x00000002</TD><TD>2         </TD><TD>Difference source matched to positive detections in both images.</TD></TR>
    671           <TR><TD>MATCHED</TD>              <TD>0x00000004</TD><TD>4         </TD><TD>source generated based on another image (forced photometry at source location).</TD></TR>
     671          <TR><TD>MATCHED</TD>              <TD>0x00000004</TD><TD>4         </TD><TD>Source generated based on another image (forced photometry at source location).</TD></TR>
    672672          <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>
    673673          <TR><TD>ON_STARCORE</TD>          <TD>0x00000010</TD><TD>16        </TD><TD>More than 25% of (PSF-weighted) pixels land on starcore.</TD></TR>
    … …  
    715715        <TABLEDATA>
    716716          <TR><TD>DEFAULT</TD>               <TD>0x00000000</TD><TD>0          </TD><TD>Initial value; resets all bits.</TD></TR>
    717           <TR><TD>NOCAL</TD>                 <TD>0x00000001</TD><TD>1          </TD><TD>Detection ignored for this analysis (photcode, time range) -- internal only.</TD></TR>
     717          <TR><TD>NOCAL</TD>                 <TD>0x00000001</TD><TD>1          </TD><TD>Detection ignored for this analysis (photcode; time range) -- internal only.</TD></TR>
    718718          <TR><TD>POOR_PHOTOM</TD>           <TD>0x00000002</TD><TD>2          </TD><TD>Detection is photometry outlier.</TD></TR>                             
    719719          <TR><TD>SKIP_PHOTOM</TD>           <TD>0x00000004</TD><TD>4          </TD><TD>Detection was ignored for photometry measurement.</TD></TR>                     
    … …  
    770770          <TR><TD>FEW</TD>              <TD>0x00000001</TD><TD>1              </TD><TD>Used within relphot; skip star.</TD></TR>
    771771          <TR><TD>POOR</TD>             <TD>0x00000002</TD><TD>2              </TD><TD>Used within relphot; skip star.</TD></TR>
    772           <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>
    773           <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>
    774           <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>
    775           <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>
    776           <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>
    777           <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>
    778           <TR><TD>TRANSIENT</TD>        <TD>0x00000100</TD><TD>256            </TD><TD>identified as a non-periodic (stationary) transient</TD></TR>
    779           <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>
    780           <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>
    781           <TR><TD>LARGE_PM</TD>         <TD>0x00000800</TD><TD>2048           </TD><TD>star with large proper motion</TD></TR>
    782           <TR><TD>RAW_AVE</TD>          <TD>0x00001000</TD><TD>4096           </TD><TD>simple weighted average position was used (no IRLS fitting)</TD></TR>
    783           <TR><TD>FIT_AVE</TD>          <TD>0x00002000</TD><TD>8192           </TD><TD>average position was fitted</TD></TR>
    784           <TR><TD>FIT_PM</TD>           <TD>0x00004000</TD><TD>16384          </TD><TD>proper motion model was fitted</TD></TR>
    785           <TR><TD>FIT_PAR</TD>          <TD>0x00008000</TD><TD>32768          </TD><TD>parallax model was fitted</TD></TR>
    786           <TR><TD>USE_AVE</TD>          <TD>0x00010000</TD><TD>65536          </TD><TD>average position used (not PM or PAR)</TD></TR>
    787           <TR><TD>USE_PM</TD>           <TD>0x00020000</TD><TD>131072         </TD><TD>proper motion used (not AVE or PAR)</TD></TR>
    788           <TR><TD>USE_PAR</TD>          <TD>0x00040000</TD><TD>262144         </TD><TD>parallax used (not AVE or PM)</TD></TR>
    789           <TR><TD>NO_MEAN_ASTROM</TD>   <TD>0x00080000</TD><TD>524288         </TD><TD>mean astrometry could not be measured</TD></TR>
    790           <TR><TD>STACK_FOR_MEAN</TD>   <TD>0x00100000</TD><TD>1048576        </TD><TD>stack position used for mean astrometry</TD></TR>
    791           <TR><TD>MEAN_FOR_STACK</TD>   <TD>0x00200000</TD><TD>2097152        </TD><TD>mean astrometry used for stack position</TD></TR>
    792           <TR><TD>BAD_PM</TD>           <TD>0x00400000</TD><TD>4194304        </TD><TD>failure to measure proper-motion model</TD></TR>
    793           <TR><TD>EXT</TD>              <TD>0x00800000</TD><TD>8388608        </TD><TD>extended in our data (eg, PS)</TD></TR>
    794           <TR><TD>EXT_ALT</TD>          <TD>0x01000000</TD><TD>16777216       </TD><TD>extended in external data (eg, 2MASS)</TD></TR>
    795           <TR><TD>GOOD</TD>             <TD>0x02000000</TD><TD>33554432       </TD><TD>good-quality measurement in our data (eg,PS)</TD></TR>
    796           <TR><TD>GOOD_ALT</TD>         <TD>0x04000000</TD><TD>67108864       </TD><TD>good-quality measurement in  external data (eg, 2MASS)</TD></TR>
    797           <TR><TD>GOOD_STACK</TD>       <TD>0x08000000</TD><TD>134217728      </TD><TD>good-quality object in the stack (> 1 good stack measurement)</TD></TR>
    798           <TR><TD>BEST_STACK</TD>       <TD>0x10000000</TD><TD>268435456      </TD><TD>the primary stack measurements are the best measurements</TD></TR>
    799           <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>
    800           <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>
     772          <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>
     773          <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>
     774          <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>
     775          <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>
     776          <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>
     777          <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>
     778          <TR><TD>TRANSIENT</TD>        <TD>0x00000100</TD><TD>256            </TD><TD>Identified as a non-periodic (stationary) transient</TD></TR>
     779          <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>
     780          <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>
     781          <TR><TD>LARGE_PM</TD>         <TD>0x00000800</TD><TD>2048           </TD><TD>Star with large proper motion</TD></TR>
     782          <TR><TD>RAW_AVE</TD>          <TD>0x00001000</TD><TD>4096           </TD><TD>Simple weighted average position was used (no IRLS fitting)</TD></TR>
     783          <TR><TD>FIT_AVE</TD>          <TD>0x00002000</TD><TD>8192           </TD><TD>Average position was fitted</TD></TR>
     784          <TR><TD>FIT_PM</TD>           <TD>0x00004000</TD><TD>16384          </TD><TD>Proper motion model was fitted</TD></TR>
     785          <TR><TD>FIT_PAR</TD>          <TD>0x00008000</TD><TD>32768          </TD><TD>Parallax model was fitted</TD></TR>
     786          <TR><TD>USE_AVE</TD>          <TD>0x00010000</TD><TD>65536          </TD><TD>Average position used (not PM or PAR)</TD></TR>
     787          <TR><TD>USE_PM</TD>           <TD>0x00020000</TD><TD>131072         </TD><TD>Proper motion used (not AVE or PAR)</TD></TR>
     788          <TR><TD>USE_PAR</TD>          <TD>0x00040000</TD><TD>262144         </TD><TD>Parallax used (not AVE or PM)</TD></TR>
     789          <TR><TD>NO_MEAN_ASTROM</TD>   <TD>0x00080000</TD><TD>524288         </TD><TD>Mean astrometry could not be measured</TD></TR>
     790          <TR><TD>STACK_FOR_MEAN</TD>   <TD>0x00100000</TD><TD>1048576        </TD><TD>Stack position used for mean astrometry</TD></TR>
     791          <TR><TD>MEAN_FOR_STACK</TD>   <TD>0x00200000</TD><TD>2097152        </TD><TD>Mean astrometry used for stack position</TD></TR>
     792          <TR><TD>BAD_PM</TD>           <TD>0x00400000</TD><TD>4194304        </TD><TD>Failure to measure proper-motion model</TD></TR>
     793          <TR><TD>EXT</TD>              <TD>0x00800000</TD><TD>8388608        </TD><TD>Extended in our data (eg; PS)</TD></TR>
     794          <TR><TD>EXT_ALT</TD>          <TD>0x01000000</TD><TD>16777216       </TD><TD>Extended in external data (eg; 2MASS)</TD></TR>
     795          <TR><TD>GOOD</TD>             <TD>0x02000000</TD><TD>33554432       </TD><TD>Good-quality measurement in our data (eg; PS)</TD></TR>
     796          <TR><TD>GOOD_ALT</TD>         <TD>0x04000000</TD><TD>67108864       </TD><TD>Good-quality measurement in  external data (eg; 2MASS)</TD></TR>
     797          <TR><TD>GOOD_STACK</TD>       <TD>0x08000000</TD><TD>134217728      </TD><TD>Good-quality object in the stack (> 1 good stack measurement)</TD></TR>
     798          <TR><TD>BEST_STACK</TD>       <TD>0x10000000</TD><TD>268435456      </TD><TD>The primary stack measurements are the best measurements</TD></TR>
     799          <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>
     800          <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>
    801801        </TABLEDATA>
    802802      </DATA>
    … …  
    833833          <TR><TD>SECF_FIX_SYNTH</TD>    <TD>0x00000080</TD><TD>128            </TD><TD>Synthetic magnitudes repaired with zeropoint map.</TD></TR>
    834834
    835           <TR><TD>SECF_RANK_0</TD>       <TD>0x00000100</TD><TD>256            </TD><TD>Average magnitude uses only rank 0 detections.</TD></TR>
    836           <TR><TD>SECF_RANK_1</TD>       <TD>0x00000200</TD><TD>512            </TD><TD>Average magnitude uses only rank 1 detections.</TD></TR>
    837           <TR><TD>SECF_RANK_2</TD>       <TD>0x00000400</TD><TD>1024           </TD><TD>Average magnitude uses only rank 2 detections.</TD></TR>
    838           <TR><TD>SECF_RANK_3</TD>       <TD>0x00000800</TD><TD>2048           </TD><TD>Average magnitude uses only rank 3 detections.</TD></TR>
    839           <TR><TD>SECF_RANK_4</TD>       <TD>0x00001000</TD><TD>4096           </TD><TD>Average magnitude uses only rank 4 detections.</TD></TR>
     835          <TR><TD>SECF_RANK_0</TD>       <TD>0x00000100</TD><TD>256            </TD><TD>Average magnitude calculated in 0th pass.</TD></TR>
     836          <TR><TD>SECF_RANK_1</TD>       <TD>0x00000200</TD><TD>512            </TD><TD>Average magnitude calculated in 1st pass.</TD></TR>
     837          <TR><TD>SECF_RANK_2</TD>       <TD>0x00000400</TD><TD>1024           </TD><TD>Average magnitude calculated in 2nd pass.</TD></TR>
     838          <TR><TD>SECF_RANK_3</TD>       <TD>0x00000800</TD><TD>2048           </TD><TD>Average magnitude calculated in 3rd pass.</TD></TR>
     839          <TR><TD>SECF_RANK_4</TD>       <TD>0x00001000</TD><TD>4096           </TD><TD>Average magnitude calculated in 4th pass.</TD></TR>
    840840          <TR><TD>SECF_STACK_PRIMARY</TD><TD>0x00004000</TD><TD>16384          </TD><TD>PS1 stack photometry comes from primary skycell.</TD></TR>
    841841          <TR><TD>SECF_STACK_BESTDET</TD><TD>0x00008000</TD><TD>32768          </TD><TD>PS1 stack best measurement is a detection (not forced).</TD></TR>
    842842          <TR><TD>SECF_STACK_PRIMDET</TD><TD>0x00010000</TD><TD>65536          </TD><TD>PS1 stack primary measurement is a detection (not forced).</TD></TR>
    843           <TR><TD>SECF_HAS_SDSS</TD>     <TD>0x00100000</TD><TD>1048576        </TD><TD>This photcode has SDSS photometry (EAM??).</TD></TR>
    844           <TR><TD>SECF_HAS_HSC</TD>      <TD>0x00200000</TD><TD>2097152        </TD><TD>This photcode has HSC  photometry (EAM??).</TD></TR>
    845           <TR><TD>SECF_HAS_CFH</TD>      <TD>0x00400000</TD><TD>4194304        </TD><TD>This photcode has CFH  photometry (mostly Megacam) (EAM??).</TD></TR>
    846           <TR><TD>SECF_HAS_DES</TD>      <TD>0x00800000</TD><TD>8388608        </TD><TD>This photcode has DES  photometry (EAM??).</TD></TR>
     843          <TR><TD>SECF_HAS_SDSS</TD>     <TD>0x00100000</TD><TD>1048576        </TD><TD>This photcode has SDSS photometry.</TD></TR>
     844          <TR><TD>SECF_HAS_HSC</TD>      <TD>0x00200000</TD><TD>2097152        </TD><TD>This photcode has HSC photometry.</TD></TR>
     845          <TR><TD>SECF_HAS_CFH</TD>      <TD>0x00400000</TD><TD>4194304        </TD><TD>This photcode has CFH photometry (mostly Megacam).</TD></TR>
     846          <TR><TD>SECF_HAS_DES</TD>      <TD>0x00800000</TD><TD>8388608        </TD><TD>This photcode has DES photometry.</TD></TR>
    847847          <TR><TD>SECF_OBJ_EXT</TD>      <TD>0x01000000</TD><TD>16777216       </TD><TD>Extended in this band.</TD></TR>
    848848        </TABLEDATA>
    … …  
    869869        <TABLEDATA>
    870870          <TR><TD>DEFAULT</TD>             <TD>0x00000000</TD><TD>0       </TD><TD>Initial value; resets all bits.</TD></TR>
    871           <TR><TD>QF_OBJ_EXT</TD>          <TD>0x00000001</TD><TD>1       </TD><TD>Extended in our data (eg, PS).</TD></TR>
    872           <TR><TD>QF_OBJ_EXT_ALT</TD>      <TD>0x00000002</TD><TD>2       </TD><TD>Extended in external data (eg, 2MASS).</TD></TR>
    873           <TR><TD>QF_OBJ_GOOD</TD>         <TD>0x00000004</TD><TD>4       </TD><TD>Good-quality measurement in our data (eg,PS).</TD></TR>
    874           <TR><TD>QF_OBJ_GOOD_ALT</TD>     <TD>0x00000008</TD><TD>8       </TD><TD>Good-quality measurement in  external data (eg, 2MASS).</TD></TR>
    875           <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>
    876           <TR><TD>QF_OBJ_BEST_STACK</TD>   <TD>0x00000020</TD><TD>32      </TD><TD>the primary stack measurements are the best measurements.</TD></TR>
    877           <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>
    878           <TR><TD>QF_OBJ_BAD_STACK</TD>    <TD>0x00000080</TD><TD>128      </TD><TD>poor-quality stack object (no more than 1 good or suspect measurement).</TD></TR>
     871          <TR><TD>QF_OBJ_EXT</TD>          <TD>0x00000001</TD><TD>1       </TD><TD>Extended in our data (eg; PS).</TD></TR>
     872          <TR><TD>QF_OBJ_EXT_ALT</TD>      <TD>0x00000002</TD><TD>2       </TD><TD>Extended in external data (eg; 2MASS).</TD></TR>
     873          <TR><TD>QF_OBJ_GOOD</TD>         <TD>0x00000004</TD><TD>4       </TD><TD>Good-quality measurement in our data (eg; PS).</TD></TR>
     874          <TR><TD>QF_OBJ_GOOD_ALT</TD>     <TD>0x00000008</TD><TD>8       </TD><TD>Good-quality measurement in  external data (eg; 2MASS).</TD></TR>
     875          <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>
     876          <TR><TD>QF_OBJ_BEST_STACK</TD>   <TD>0x00000020</TD><TD>32      </TD><TD>The primary stack measurements are the best measurements.</TD></TR>
     877          <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>
     878          <TR><TD>QF_OBJ_BAD_STACK</TD>    <TD>0x00000080</TD><TD>128      </TD><TD>Poor-quality stack object (no more than 1 good or suspect measurement).</TD></TR>
    879879        </TABLEDATA>
    880880      </DATA>
    … …  
    900900        <TABLEDATA>
    901901          <TR><TD>NO_ERROR</TD>     <TD>0x00000000</TD><TD>0 </TD><TD>No error condition raised.</TD></TR>
    902           <TR><TD>FAIL_FIT</TD>     <TD>0x00000001</TD><TD>1 </TD><TD>fit failed to converge or was degenerate</TD></TR>
    903           <TR><TD>TOO_FEW</TD>      <TD>0x00000002</TD><TD>2 </TD><TD>not enough points to fit the model</TD></TR>
    904           <TR><TD>OUT_OF_RANGE</TD> <TD>0x00000004</TD><TD>4 </TD><TD>fit minimum too far outside data range</TD></TR>
    905           <TR><TD>BAD_ERROR</TD>    <TD>0x00000008</TD><TD>8 </TD><TD>invalid size error (nan or inf)</TD></TR>
     902          <TR><TD>FAIL_FIT</TD>     <TD>0x00000001</TD><TD>1 </TD><TD>Fit failed to converge or was degenerate</TD></TR>
     903          <TR><TD>TOO_FEW</TD>      <TD>0x00000002</TD><TD>2 </TD><TD>Not enough points to fit the model</TD></TR>
     904          <TR><TD>OUT_OF_RANGE</TD> <TD>0x00000004</TD><TD>4 </TD><TD>Fit minimum too far outside data range</TD></TR>
     905          <TR><TD>BAD_ERROR</TD>    <TD>0x00000008</TD><TD>8 </TD><TD>Invalid size error (nan or inf)</TD></TR>
    906906        </TABLEDATA>
    907907      </DATA>
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