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CRIRES-POP Observing Information
General strategy
The CRIRES-POP targets were bright objects which
could be observed also under moderate weather conditions. The concept was,
thus, to have a filler programme which uses time with insufficient seeing
conditions for other programmes. The approximately 200 wavelength settings
per target were split into observing blocks of 20 minutes to 1 hour in
length. These blocks were not observed in a continuous way. In fact, some
of the spectra from 1 to 5 mu have been obtained over a time span of
almost 1.5 years.
List of wavelength settings
covered
| 0971.0nm |
1337.0nm |
2180.0nm |
| 0974.0nm |
1340.9nm |
2186.5nm |
| 0983.3nm |
1349.5nm |
2213.3nm |
| 0986.3nm |
1431.9nm |
2219.8nm |
| 0988.0nm |
1436.2nm |
2232.4nm |
| 0991.0nm |
1441.9nm |
2239.1nm |
| 1000.6nm |
1453.3nm |
2267.2nm |
| 1003.6nm |
1457.7nm |
2273.9nm |
| 1005.6nm |
1469.4nm |
2302.0nm |
| 1008.7nm |
1473.9nm |
2308.7nm |
| 1018.6nm |
1474.7nm |
2325.2nm |
| 1021.6nm |
1479.1nm |
2332.2nm |
| 1023.8nm |
1491.5nm |
2361.7nm |
| 1026.9nm |
1496.0nm |
2368.7nm |
| 1037.1nm |
1509.0nm |
2398.1nm |
| 1040.2nm |
1513.6nm |
2405.1nm |
| 1042.7nm |
1518.1nm |
2425.9nm |
| 1045.9nm |
1531.9nm |
2433.2nm |
| 1056.4nm |
1536.4nm |
2464.4nm |
| 1059.6nm |
1550.8nm |
2471.6nm |
| 1062.3nm |
1554.7nm |
2502.8nm |
| 1065.6nm |
1555.5nm |
2510.0nm |
| 1076.4nm |
1559.3nm |
3426.3nm |
| 1079.6nm |
1574.4nm |
3436.6nm |
| 1082.7nm |
1579.1nm |
3441.5nm |
| 1086.0nm |
1595.0nm |
3451.1nm |
| 1097.2nm |
1598.0nm |
3503.8nm |
| 1100.5nm |
1599.9nm |
3514.0nm |
| 1103.9nm |
1602.7nm |
3581.2nm |
| 1107.2nm |
1619.4nm |
3591.4nm |
| 1118.8nm |
1624.2nm |
3658.4nm |
| 1122.1nm |
1641.8nm |
3668.6nm |
| 1125.9nm |
1643.7nm |
3696.7nm |
| 1129.3nm |
1646.8nm |
3707.5nm |
| 1141.2nm |
1648.6nm |
3778.7nm |
| 1144.6nm |
1667.0nm |
3789.5nm |
| 1148.8nm |
1672.0nm |
3860.5nm |
| 1152.3nm |
1691.5nm |
3871.3nm |
| 1164.6nm |
1692.2nm |
3874.4nm |
| 1168.1nm |
1696.6nm |
3885.9nm |
| 1172.7nm |
1697.2nm |
3961.5nm |
| 1176.2nm |
1717.5nm |
3973.0nm |
| 1188.9nm |
1722.7nm |
4048.6nm |
| 1192.5nm |
1743.6nm |
4060.1nm |
| 1197.5nm |
1744.3nm |
4135.5nm |
| 1201.2nm |
1748.7nm |
4147.0nm |
| 1214.3nm |
1749.6nm |
4174.6nm |
| 1217.9nm |
1771.2nm |
4186.9nm |
| 1223.5nm |
1776.5nm |
4267.4nm |
| 1227.2nm |
1798.1nm |
4279.6nm |
| 1240.7nm |
1984.3nm |
4624.6nm |
| 1244.4nm |
1990.1nm |
4637.6nm |
| 1250.6nm |
1993.3nm |
4723.3nm |
| 1254.4nm |
1999.4nm |
4736.3nm |
| 1268.4nm |
2024.3nm |
4821.9nm |
| 1272.2nm |
2030.3nm |
4834.9nm |
| 1279.0nm |
2055.2nm |
4889.5nm |
| 1282.9nm |
2061.2nm |
4903.4nm |
| 1297.3nm |
2067.1nm |
4920.3nm |
| 1299.2nm |
2073.4nm |
4994.8nm |
| 1301.2nm |
2099.3nm |
5008.7nm |
| 1303.2nm |
2105.5nm |
5100.1nm |
| 1318.1nm |
2131.3nm |
5114.0nm |
| 1322.1nm |
2137.6nm |
5205.3nm |
| 1330.0nm |
2146.6nm |
5219.1nm |
| 1334.1nm |
2153.1nm |
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Observing mode
Slit width: 0.2 arcsec
Resolution around 2.2
mu: 96 000
AO system: not used
Integration time: between 10 and 1200 s
For more information see Lebzelter et al. 2011 (submitted).
In case you have any questions on the instrument
setup or the observations please send email to thomas.lebzelter AT univie.ac.at
last modification: Oct 31 2011
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