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Ninety-Four DEIMOS Masks
MaskNo. SlitsDate-Obs
1100151 2003-05-03
1101148 2003-05-06
1102144 2003-06-30
1103142 2003-05-03
1104159 2003-05-30
1105137 2003-07-01
1106142 2003-05-05
1107140 2004-05-22
1108141 2004-05-21
1109143 2003-05-06
1110152 2003-05-04
1111148 2003-05-28
1112151 2003-05-04
1113151 2003-05-30
1114153 2003-06-01
1115146 2003-05-05
1140141 2003-05-05
1141132 2003-05-06
1142131 2004-04-21
1143126 2003-05-05
1144135 2003-05-30
1145149 2003-05-30
1146143 2003-05-06
1150139 2003-05-04
1151136 2003-05-28
1152132 2003-05-04
1153133 2003-06-01
1154143 2004-05-22
1155146 2003-06-30
1156146 2004-04-19
1200146 2004-04-21
1201142 2005-03-09
1202135 2004-05-23
1203154 2004-05-23
1204146 2004-06-19
1205146 2004-06-19
1206141 2004-04-17
1207139 2004-05-22
1208142 2004-06-20
1209138 2004-06-20
1210149 2004-07-15
1211155 2004-07-15
1212152 2004-07-16
1213143 2004-07-16
1214154 2005-04-03
1215144 2005-04-03
1240136 2004-04-18
1241149 2004-04-21
1242133 2004-05-21
1243143 2004-05-21
1244146 2004-05-22
1245128 2003-06-01
1246142 2004-05-23
1250153 2004-05-23
1251146 2004-06-19
1252136 2004-06-20
1253144 2004-04-17
1254141 2005-02-10
1255135 2005-02-10
1256146 2005-02-10
1300145 2005-04-03
1301142 2005-04-04
1302150 2005-05-08
1303143 2005-05-09
1304150 2005-05-10
1305144 2005-06-05
1306153 2005-06-05
1307149 2005-06-05
1308156 2005-06-06
1309159 2005-06-06
1310148 2005-06-06
1311156 2005-06-07
1312157 2005-06-07
1313150 2005-07-07
1314148 2005-07-07
1315151 2005-07-08
1340149 2005-02-11
1341159 2005-02-11
1342142 2005-02-11
1343143 2005-03-09
1344140 2005-03-09
1345140 2005-04-03
1346145 2005-06-05
1350145 2005-04-04
1351136 2005-04-04
1352141 2005-05-09
1353145 2005-05-08
1354148 2005-05-08
1355148 2005-05-10
1356153 2005-05-09
1400140 2005-07-08
1440137 2005-06-06
1441129 2005-06-07
1442145 2005-05-10

This plot shows the right ascension and declination for each DEEP2 target (black) and those with positive ACS identifications (yellow).


The redshifts were measured using emission lines (Balmer Series, [NII], [SII], [OIII], [OII]) and the Calcium (H, K and other ) absorption features. Each redshift measurement was assigned a “quality” identifier according to at least two independent measurements . In the center the quality distribution is shown.


Quality codes were assigned on the basis of a set of criteria: a value of 4 is assigned to a “rock-solid” z measurement obtained from a spectrum with at least two clear features. A value of 3 indicates a good z value, with a 90% probability to be correct. At least two features are still required but ID is more doubtful than Q=4. A value of 2 indicates a non-usable measurement for the present catalog but the spectrum will be later revisited because a useful z value might be extracted from it. Q=1 means that the redshift is not usable and the data will never yield one. Q=-1 is reserved for stars.


This plot shows the z-magnitude diagram: magnitudes were obtained from Sextractor



Last modified: Wed Nov 29, 2006