FORS1 Standard Fields and Stars
|
The lists of available calibration fields and stars are given here for
various FORS1 setups, i.e. for Bessell filters,
Gunn 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. These OBs can be retrieved in the /home/visitor/impex/FORS1/ directory.
For service mode, PSO staff will use the same observing blocks.
Photometric
Standard Stars: 1. Bessell filters
Template name
|
Star field
|
Center coordinates Ra, Dec
|
Photom-std-SA92-high
|
SA92-249
|
00:54:35.5, +00:40:19.5
|
Photom-std-PG0231+051-high
|
PG0231+051
|
02:33:39.8, +05:18:37.7
|
Photom-std-SA95-high
|
SA95-105
|
03:53:20.0, +00:00:57.8
|
Photom-std-SA98-high
|
SA98-670
|
06:52:14.4, -00:19:49.9
|
Photom-std-Rubin149-high
|
Rubin149
|
07:24:15.3, -00:32:20.9
|
Photom-std-Rubin152-high
|
Rubin152
|
07:29:58.1, -02:05:45.5
|
Photom-std-SA100-high
|
SA100-269
|
08:53:16.1, -00:42:19.3
|
Photom-std-PG0942-029-high
|
PG0942-029
|
09:45:12.1, -03:08:03.2
|
Photom-std-SA101-high
|
SA101-429
|
09:57:35.9, -00:18:50.3
|
Photom-std-PG1047+003-high
|
PG1047+003
|
10:50:08.5, -00:01:04.3
|
Photom-std-PG1323-high
|
PG1323-086
|
13:25:52.5, -08:49:56.6
|
Photom-std-PG1528+062-high
|
PG1528+062
|
15:30:44.7, +06:01:04.8
|
Photom-std-PG1633+099-high
|
PG1633+099
|
16:35:36.0, +09:46:33.4
|
Photom-std-PG1657+078-high
|
PG1657+078
|
16:59:32.4, +07:42:52.0
|
Photom-std-SA109-high
|
SA109-949
|
17:44:15.0, -00:02:17.0
|
Photom-std-SA110-high
|
SA110-362
|
18:42:52.4, +00:06:28.1
|
Photom-std-SA111-high
|
SA111-2088
|
19:38:22.0, +00:31:01.0
|
Photom-std-MarkA-high
|
MarkA
|
20:43:59.5, -10:46:32.8
|
Photom-std-SA113-high
|
SA113-239
|
21:41:09.5, +00:23:00.0
|
Photom-std-PG2213-006-high
|
PG2213-006
|
22:16:23.2, -00:21:40.8
|
Photom-std-PG2331+055-high
|
PG2331+055
|
23:33:47.9, +05:46:16.8
|
Notes: (1)
The OB are prepared both with high CCD gain, four-port readout, (2) The
coordinates of the field center have been chosen so that a good coverage
of the Landolt star fields is obtained with both SR and HR collimators,
(3) Reference: Bessel
et al. 1979, UBVRI Photometry (1979PASP...91..589B) and Landolt 1992,
(4) The links provide Postscript charts of the areas with SR and HR fields
indicated, (5) Coordinates are J2000.
Photometric
Standard Stars: 2. Gunn filters (no OBs prepared! not in Calibration Plan!)
Template name
|
Star field
|
Center coordinates Ra, Dec
|
Photom-std-Gunn-SA92
|
SA92-249
|
00:54:35.5, +00:40:19.5
|
Photom-std-Gunn-F762-9
|
F762-9
|
03:33:16.4, -06:05:22.1
|
Photom-std-Gunn-E4
|
E4
|
09:23:41.7, -45:25:22.1
|
Photom-std-Gunn-E5
|
E5
|
12:05:11.3, -45:34:03.0
|
Photom-std-Gunn-PG1633+099
|
PG1633+099
|
16:35:36.0, +09:46:33.4
|
Photom-std-Gunn-E7
|
E7
|
17:27:22.7, -45:01:38.0
|
Photom-std-Gunn-SA110
|
SA110-503
|
18:43:10.3, +00:28:58.0
|
Photom-std-Gunn-MarkA
|
MarkA
|
20:43:59.5, -10:46:32.8
|
Photom-std-Gunn-F1038-6
|
F1038-6
|
23:33:40.1, +10:07:05.4
|
Notes: (1)
The OB are prepared with high CCD gain, four-port readout, (2) The coordinates
of the field center have been chosen so that a good coverage of the Landolt
star fields is obtained with both SR and HR collimators, (3) References:
Thuan-Gunn
system (1976PASP...88..543T) and secondary
standards (1994PASP..106..967J), (4) The links provide Postscript charts
of the areas with SR and HR fields indicated, (5) Coordinates are J2000.
Spectroscopic
Standard Stars - and Imaging Standards for Gunn & interference filters
Template name
|
Star name
|
Coordinates Ra, Dec
|
specphot-std-G158-100
|
G158-100
|
00:33:54.32, -12:07:57.1
|
specphot-std-LTT377
|
LTT377
|
00:41:46.82, -33:39:08.2
|
specphot-std-BPM16274
|
BPM16274(*)
|
00:50:03.18, -52:08:17.4
|
specphot-std-LTT1020
|
LTT1020
|
01:54:49.68, -27:28:29.7
|
specphot-std-EG21
|
EG21
|
03:10:30.98, -68:36:02.2
|
specphot-std-LTT1788
|
LTT1788
|
03:48:22.17, -39:08:33.6
|
specphot-std-GD50
|
GD50
|
03:48:50.06, -00:58:30.4
|
specphot-std-SA95-42
|
SA95-42
|
03:53:43.68, -00:04:33.0
|
specphot-std-HZ4
|
HZ4
|
03:55:21.70, +09:47:18.7
|
specphot-std-LB227
|
LB227
|
04:09:28.76, +17:07:54.4
|
specphot-std-HZ2
|
HZ2
|
04:12:43.51, +11:51:50.4
|
specphot-std-GD71
|
GD71
|
05:52:27.51, +15:53:16.6
|
specphot-std-LTT2415
|
LTT2415
|
05:56:24.30, -27:51:28.8
|
specphot-std-HD49798
|
HD49798(*)
|
06:48:04.64, -44:18:59.3
|
specphot-std-LTT3218
|
LTT3218
|
08:41:34.10, -32:57:00.1
|
specphot-std-GD108
|
GD108
|
10:00:47.33, -07:33:31.2
|
specphot-std-LTT3864
|
LTT3864
|
10:32:13.90, -35:37:42.4
|
specphot-std-LTT4364
|
LTT4364
|
11:45:37.70, -64:50:25.1
|
specphot-std-Feige56
|
Feige56
|
12:06:39.7, +11:40:39.0
|
specphot-std-HZ21
|
HZ21
|
12:13:56.42, +32:56:30.8
|
specphot-std-Feige66
|
Feige66
|
12:37:23.55, +25:04:00.3
|
specphot-std-LTT4816
|
LTT4816
|
12:38:50.94, -49:47:58.8
|
specphot-std-Feige67
|
Feige67
|
12:41:51.83, +17:31:20.5
|
specphot-std-GD153
|
GD153
|
12:57:02.37, +22:01:56.0
|
specphot-std-G60-54
|
G60-54
|
13:00:09.53, +03:28:55.7
|
specphot-std-HZ43
|
HZ43
|
13:16:22.0, +29:05:57.0
|
specphot-std-HZ44
|
HZ44
|
13:23:35.37, +36:07:60.0
|
specphot-std-CD-32d9927
|
CD-32d9927
|
14:11:46.37, -33:03:14.3
|
specphot-std-LTT6248
|
LTT6248
|
15:39:00.0, -28:35:33.0
|
specphot-std-BD33d2642
|
BD33d2642
|
15:51:59.8, +32:56:54.8
|
specphot-std-EG274
|
EG274
|
16:23:33.75, -39:13:47.5
|
specphot-std-G138-31
|
G138-31
|
16:27:53.59, +09:12:24.5
|
specphot-std-LTT7379
|
LTT7379
|
18:36:26.29, -44:18:33.0
|
specphot-std-LTT7987
|
LTT7987
|
20:10:57.38, -30:13:01.2
|
specphot-std-G24-9
|
G24-9
|
20:13:56.05, +06:42:55.2
|
specphot-std-LDS749B
|
LDS749B
|
21:32:15.75, +00:15:13.6
|
specphot-std-BD28d4211
|
BD28d4211
|
21:51:11.07, +28:51:51.8
|
specphot-std-G93-48
|
G93-48
|
21:52:25.33, +02:23:24.3
|
specphot-std-BD25d4655
|
BD25d4655
|
21:59:42.02, +26:25:58.1
|
specphot-std-NGC7293
|
NGC7293
|
22:29:38.46, -20:50:13.3
|
specphot-std-LTT9239
|
LTT9239
|
22:52:40.88, -20:35:26.3
|
specphot-std-LTT9491
|
LTT9491
|
23:19:34.98, -17:05:29.8
|
specphot-std-Feige110
|
Feige110
|
23:19:58.39, -05:09:55.8
|
specphot-std-GD248
|
GD248
|
23:26:06.69, +16:00:21.4
|
Notes: (*)
These stars only have model data above 3200Å, (1) The OB are prepared
with high CCD gain, one-port readout, (2) The OB exist in MOS setup (three
5" slitlets) and in LSS, using the largest 2.5" slit -then the OB name
contains "lss-" at the beginning, (3) The links provide detailed information
on individual stars, (4) There is also a
general
description as well as an RA
ordered list and an RA-Dec
skymap for standards including the above listed, (5) Coordinates are
J2000.
Empty
Fields for Twilight Flats
Template name
|
Field name
|
Center coordinates Ra, Dec
|
twil-ABCD-high-UBIVR-SR-0048 |
SGP |
00:48:30.3, -28:03:01.0 |
twil-ABCD-high-UBIVR-SR-0102 |
0102-265 |
01:02:48.5, -26:34:25.0 |
twil-ABCD-high-UBIVR-SR-0247 |
0248-196 |
02:47:46.6, -19:46:11.1 |
twil-ABCD-high-UBIVR-SR-0427 |
0427-36 |
04:27:26.1, -36:25:16.0 |
twil-ABCD-high-UBIVR-SR-0909 |
9090-7 |
09:09:32.6, -07:38:26.0 |
twil-ABCD-high-UBIVR-SR-1004 |
CT1 |
10:04:27.0, -02:19:00.0 |
twil-ABCD-high-UBIVR-SR-1102 |
1101-264 |
11:02:23.5, -26:43:56.7 |
twil-ABCD-high-UBIVR-SR-1226 |
CT5 |
12:26:08.7, -06:38:29.0 |
twil-ABCD-high-UBIVR-SR-1254 |
CT2 |
12:54:58.7, -02:07:04.0 |
twil-ABCD-high-UBIVR-SR-1513 |
SER1 |
15:13:13.9, -00:31:47.5 |
twil-ABCD-high-UBIVR-SR-1539 |
SPKS
04 |
15:39:43.0, -33:56:54.0 |
twil-ABCD-high-UBIVR-SR-1649 |
SPKS
12 |
16:49:42.0, -15:21:00.0 |
twil-ABCD-high-UBIVR-SR-1731 |
SPKS
08 |
17:31:06.0, -25:44:24.0 |
twil-ABCD-high-UBIVR-SR-1802 |
SPKS
09 |
18:02:01.0, -04:32:36.0 |
twil-ABCD-high-UBIVR-SR-1900 |
SPKS
10 |
19:00:48.0, -37:21:18.0 |
twil-ABCD-high-UBIVR-SR-1919 |
SPKS
13 |
19:19:09.0, +12:22:05.0 |
twil-ABCD-high-UBIVR-SR-2126 |
SPKS
14 |
21:26:54.4, -08:51:41.0 |
twil-ABCD-high-UBIVR-SR-2334 |
2335-40 |
23:34:34.6, -39:49:04.0 |
twil-ABCD-high-UBIVR-SR-2345 |
2345+007 |
23:45:45.9, +00:40:40.0 |
Notes: (1)
The OB are prepared with high CCD gain, four-port readout, Standard Resolution
Collimator, (2) Filters defined in the OB are UBIVR for the evening dusk.
For the morning the OB are named ..-RVIBU-.. instead, (4) The links call
6.8'x6.8' images from the DSS1
database, (5) Coordinates are B1950.
Imaging
and Spectropolarimetric Polarized Standard Stars
Template name
|
OB Total Execution Time (in min.)
|
Ra & Dec 2000
|
Comments
|
PMOS_NGC2024_5arcs
IPOL_NGC2024
|
??
|
05:41:38 -01:54:37
|
none |
PMOS_Vela1_95_5arc_high
|
??
|
09:06:00 -47:19:00
|
none |
PMOS_Hiltner652_5arcs
|
??
|
17:43:20 -28:40:33
|
none |
PMOS_HDE316232_5arcs
IPOL_HDE316232
|
??
|
17:45:44 -29:13:18
|
none |
PMOS_BD_14_51333_5arcs
IPOL_BD_14_51333
|
??
|
18:11:58 -14:56:09
|
none |
PMOS_BD12_5133_5arcs
IPOL_BD12_5133
|
??
|
18:40:02 -12:24:07
|
none |
The OB are prepared with high CCD gain. PMOS have
1-port readout (window with 400 pixels in y), IPOL 4-ports readout. There
are 4 exposures with the retarder waveplate at 0, 22.5, 45, and 67.5 deg.
The data for these stars are given on the
FORS
polarimetry page
Unpolarized Spectropolarimetric
Standard Stars
Template name
|
OB Total Execution Time (in min.)
|
Ra & Dec 2000
|
Comments
|
Zero_PMOS_HD10038
|
10
|
01:37:18.59 -40:10:38.46
|
Bright Am, plx=6.4 mas, no need for finding charts; slit width=1.0" |
Zero_PMOS_HD13588
|
10
|
02:11:16.69 -46:35:06.16
|
Bright Am, plx=6.4 mas, no need for finding charts; slit width=1.0" |
Zero_PMOS_HD42078
|
10
|
06:06:41.04 -42:17:55.69
|
Bright Am, plx=10.13, no need for finding charts; slit width=1.0" |
Zero_PMOS_HD97689
|
10
|
11:13:50.74 -52:51:21.22
|
Bright Am, plx=12.13, no need for finding charts; slit width=1.0" |
Zero_PMOS_WD1615-154
|
18
|
16:17:55.2 -15:35:51.2
|
White Dwarf, plx =?, high proper motion; see finding chart; slit width=2.5" |
Zero_PMOS_WD1620-391
|
11
|
16:23:35.7 -39:13:21.8
|
White Dwarf, plx=78 mas, high proper motion; see finding chart; slit
width=2.5" |
Zero_PMOS_WD2039-202
|
18
|
20:42:34.7 -20:04:35.7
|
White Dwarf, plx=47 mas, high proper motion; see finding chart; slit
width=2.5" |
Zero_PMOS_WD2149+021
|
22
|
21:52:21.5 +02:23:07.2
|
White Dwarf, plx=40 mas, high proper motion; see finding chart; slit
width=2.5" |
The OB are prepared with high gain, 1-port readout
(window with 500 pixels in y). We have 4 exposures with the retarder waveplate
at 0, 22.5, 45, and 67.5 deg. Exposure times are set such as with 0.4 arcsec
seeing we get a S/N=400 for each exposure.
The coordinates are very doubtfull due to the high PM and we suggest
to compare DSS1 and DSS2 to select the fastest star in the field.
We'll fix this page later,... sorry!
Unpolarized Imaging
Polarimetric Standard Stars
Template name
|
OB Total Execution Time (in min.)
|
Ra & Dec 2000
|
Comments
|
Zero_IPOL_WD2359-434
|
??
|
00:02:10.7 -43:09:55.2
|
White dwarf, plx=120 mas |
Zero_IPOL_WD0310-688
|
??
|
03:10:30.98 -68:36:02.2
|
White dwarf (EG 21), plx=120 mas |
Zero_IPOL_WD0752-676
|
??
|
07:53:08.5 -67:47:33.2
|
White Dwarf, plx =?, high proper motion |
Zero_IPOL_WD1344+106
|
??
|
13:47:24.3 +10:21:38.1
|
White Dwarf, plx =48, high proper motion, SE star of the binary |
Zero_IPOL_WD1615-154
|
??
|
16:17:55.2 -15:35:51.2
|
White Dwarf, plx=60 mas, high proper motion |
Zero_IPOL_WD1620-391
|
??
|
16:23:35.7 -39:13:21.8
|
White Dwarf, plx=78 mas, high proper motion star ~30 arcsecs SE of
our coordinates? |
Zero_IPOL_WD2039-202
|
??
|
20:42:34.7 -20:04:35.7
|
White Dwarf, plx=47 mas, high proper motion |
Zero_IPOL_WD2149+021
|
??
|
21:52:21.5 +02:23:07.2
|
White Dwarf, plx=40 mas, high proper motion star ~1arcmin East or our
coordinates? |
The OB are prepared with high CCD gain, 4-ports
readout. We have 4 exposures with the retarder waveplate at 0, 22.5, 45,
and 67.5 deg. The links call 6.8'x6.8' images from the
DSS2 database (red).
The coordinates are very doubtfull due to the high PM and we suggest
to compare DSS1 and DSS2 to select the fastest star in the field.
We'll fix this page later,... sorry!