Standard Star Instructions¶
- Standard star fields are to be observed every evening and morning twilight that appear to be clear,
where "clear" is determined by a quick visual inspection of the RASICAM image, of the TASCA image, or
(!) of the sky itself.
- If possible, for each twilight period, 3 standard star fields should be observed: one at low airmass
(X<1.25), on at medium airmass (X=1.25-1.65), and one at high airmass (X=1.65-2.10). It is generally
better to observe the high-airmass field first, since its airmass will be changing the most rapidly.
- For half-nights, 1 or 2 fields -- preferably a low-airmass field and a high-airmass field -- should be
observed just before switchover. (If only one field, a high-airmass field is preferred.)
- For evening twilight, use the DES/standard/Yzirg scripts (which start with Y-band and end with g-band);
for morning twilight or pre-switchover, use the DES/standard/grizY scripts (which start with g-band and
end with Y-band). (For those rare nights when we also observe in u-band, please use the corresponding
"DES/standard/Yzirgu" and "DES/standard/ugrizY" scripts.)
- There are several useful scripts in the StdStarPicker package in the DECamObserver account on observer2,
including decamStdFieldsTimeDate.py and decamStdFieldsQueryNextSet.py.
- To check which standard star fields are in a good position to observe (airmass < 2.10, moon separation
> 15 deg, within Blanco horizon limits), use decamStdFieldsTimeDate.py:
source ~/dtucker/bin/setup_StdStarFieldPicker.csh (or .bash if you are using bash shell)
decamStdFieldsTimeDate.py --help (for detailed help)
decamStdFieldsTimeDate.py --UT=now (for a list accessible right now)
decamStdFieldsTimeDate.py --UT='2013/09/17 00:43' (for a list accessible at 00:43UT on Sept 17, 2013)
- To get a preferred triad of standard fields -- a low-airmass field, a medium-airmass field, and a
high-airmass field -- for a given time and date, use decamStdFieldsQueryNextSet.py instead:
decamStdFieldsQueryNextSet.py --help (for detailed help)
decamStdFieldsQueryNextSet.py --UT=now (for a triad accessible right now)
decamStdFieldsQueryNextSet.py --UT='2013/09/17 00:43' (for a triad accessible at 00:43UT on Sept 17, 2013)
(Warning: decamStdFieldsQueryNextSet.py will output a default json file, "stdstar.json". Just ignore it.)
- For simplicity, a look-up table of preferred triads for the nights of August 30-Sepember 30, 2013,
listing the preferred triad for each 15-min interval throughout those nights, can be found here:
The Standard Fields¶
SDSS Equatorial Fields: "Golden Standards"
Field Name |
RA |
_.Dec |
SDSSJ0000-0000 |
00:00:00 |
+00:00:00 |
SDSSJ0100-0000 |
01:00:00 |
+00:00:00 |
SDSSJ0200-0000 |
02:00:00 |
+00:00:00 |
SDSSJ0320-0000 |
03:20:00 |
+00:00:00 |
SDSSJ0843-0000 |
08:43:00 |
+00:00:00 |
SDSSJ0933-0005 |
09:33:00 |
-00:05:00 |
SDSSJ0958-0010 |
09:58:00 |
-00:10:00 |
SDSSJ1048-0000 |
10:48:00 |
+00:00:00 |
SDSSJ1227-0000 |
12:27:00 |
+00:00:00 |
SDSSJ1442-0005 |
14:42:00 |
-00:05:00 |
SDSSJ2140-0000 |
21:40:00 |
+00:00:00 |
SDSSJ2300-0000 |
23:00:00 |
+00:00:00 |
HST CalSpec/Other Fields: "Silver Standards"
Field Name |
RA |
Dec |
C26202/HST |
03:32:30 |
-27:46:05 |
MaxVis |
06:30:00 |
-58:45:00 |
Graham E-Region Fields (Southern u'g'r'i'z' fields): "Bronze Standards"
Field Name |
RA |
Dec |
E1-A |
01:24:50 |
-44:33:40 |
E2-A |
04:03:00 |
-44:41:45 |
E3-A |
06:42:54 |
-45:05:06 |
E4-A |
09:23:44 |
-45:21:02 |
E5-A |
12:04:11 |
-45:24:03 |
E6-A |
14:45:33 |
-45:15:34 |
E8-A |
20:07:22 |
-44:37:01 |
E9-A |
22:45:37 |
-44:22:47 |