FORS Standard Fields and Stars
The lists of available calibration fields and stars are given here for various FORS setups, i.e. for Stetson Fields for standard filters, Landolt Fields for other broadband filters, Spectroscopy, empty Fields for Twilight Flats and Polarimetry. The name of the Observation Blocks already prepared by PSO and available for any visiting observer is given, as well as some information on the field or star.Photometric Standard Stars: Stetson Fields
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Photometric Standard Stars: Landolt Fields
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Spectroscopic Standard Stars - and Imaging Standards for Gunn & interference filters
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Empty Fields for Twilight Flats
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| twil-UBIVR-SR-0048 | SGP | 00:48:30.3, -28:03:01.0 |
| twil-UBIVR-SR-0102 | 0102-265 | 01:02:48.5, -26:34:25.0 |
| twil-UBIVR-SR-0247 | 0248-196 | 02:47:46.6, -19:46:11.1 |
| twil-UBIVR-SR-0427 | 0427-36 | 04:27:26.1, -36:25:16.0 |
| twil-UBIVR-SR-0909 | 9090-7 | 09:09:32.6, -07:38:26.0 |
| twil-UBIVR-SR-1004 | CT1 | 10:04:27.0, -02:19:00.0 |
| twil-UBIVR-SR-1102 | 1101-264 | 11:02:23.5, -26:43:56.7 |
| twil-UBIVR-SR-1226 | CT5 | 12:26:08.7, -06:38:29.0 |
| twil-UBIVR-SR-1254 | CT2 | 12:54:58.7, -02:07:04.0 |
| twil-UBIVR-SR-1513 | SER1 | 15:13:13.9, -00:31:47.5 |
| twil-UBIVR-SR-1539 | SPKS 04 | 15:39:43.0, -33:56:54.0 |
| twil-UBIVR-SR-1649 | SPKS 12 | 16:49:42.0, -15:21:00.0 |
| twil-UBIVR-SR-1731 | SPKS 08 | 17:31:06.0, -25:44:24.0 |
| twil-UBIVR-SR-1802 | SPKS 09 | 18:02:01.0, -04:32:36.0 |
| twil-UBIVR-SR-1900 | SPKS 10 | 19:00:48.0, -37:21:18.0 |
| twil-UBIVR-SR-1919 | SPKS 13 | 19:19:09.0, +12:22:05.0 |
| twil-UBIVR-SR-2126 | SPKS 14 | 21:26:54.4, -08:51:41.0 |
| twil-UBIVR-SR-2334 | 2335-40 | 23:34:34.6, -39:49:04.0 |
| twil-UBIVR-SR-2345 | 2345+007 | 23:45:45.9, +00:40:40.0 |
Highly Polarized Standard Stars for Imaging Polarimetry (IPOL) OT QUEUE: Polar Std IPOL
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none |
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none |
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none |
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none |
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none |
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none |
Please check that the CCD is well exposed (> 10000 counts each exposure) but not saturated! You may need to adjust the exposure time.
Additional information on (some of) these stars are given on the FORS polarimetry page
Finding charts are obtained from 6.8' x 6.8' images from the DSS2 (red) database.
Highly Polarized Standard Stars for Spectropolarimetry (PMOS) OT QUEUE: Polar Std PMOS
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none |
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none |
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none |
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none |
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none |
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none |
Please check that the CCD is well exposed (> 10000 counts each exposure) but not saturated! You may need to adjust the exposure time.
Additional information on (some of) these stars are given on the FORS polarimetry page
Finding charts are obtained from 6.8'x6.8' images from the DSS2 (red)as database.
Unpolarized Standard Stars for Imaging Polarimetry OT QUEUE: Polar Std IPOL
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White dwarf, plx=120 mas. The target is the brightest one. Only one guiding star in the field, with some vignetting. Non magnetic according to Koester et al. (1998) |
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White dwarf (EG 21), plx=120 mas |
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White Dwarf, plx =?, high proper motion |
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White Dwarf, plx =48, high proper motion, SE star of the binary |
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White Dwarf, plx=60 mas, high proper motion |
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White Dwarf, plx=78 mas, high proper motion star ~30 arcsecs SE of our coordinates? |
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White Dwarf, plx=47 mas, high proper motion |
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White Dwarf, plx=40 mas, high proper motion star ~1arcmin East or our coordinates? |
Please check that the CCD is well exposed (> 10000 counts each exposure) but not saturated! You may need to adjust the exposure time.
Finding charts are obtained from 6.8'x6.8' images from the DSS2 (red) database.
Unpolarized Standard Stars for Spectropolarimetry OT QUEUE: Polar Std PMOS
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Bright Am, plx=6.4 mas, no need for finding charts; slit width=1.0 arcsec |
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Bright Am, plx=6.4 mas, no need for finding charts; slit width=1.0 arcsec |
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Bright Am, plx=10.13, no need for finding charts; slit width=1.0 arcsec |
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Bright Am, plx=12.13, no need for finding charts; slit width=1.0 arcsec |
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White Dwarf, plx =?, high proper motion; see finding chart; slit width=2.5 arcsec |
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White Dwarf, plx=78 mas, high proper motion; see finding chart; slit width=2.5 arcsec |
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White Dwarf, plx=47 mas, high proper motion; see finding chart; slit width=2.5 arcsec |
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White Dwarf, plx=40 mas, high proper motion; see finding chart; slit width=2.5 arcsec |
Please check that the CCD is well exposed (> 10000 counts each exposure) but not saturated! You may need to adjust the exposure time.
Finding charts are obtained from 6.8'x6.8' images from the DSS2 (red) database.
