C100/WFCCD Exposure Times

Date of last modification: July 10 2010, 10:55 pm Chilean time.


                  Landolt's Standard Stars

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Field        RA   (2000)   DEC            U    B    V    R    I      center            RA         DEC
                                         sec  sec  sec  sec  sec                           2000.0
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TPHE       00 30 17  -46 32 34          ---    4    2  ---    2         C            00 30 17    -46 32 34
PG0231     02 33 41  +05 18 40          ---    3    2  ---    2     no label	     02 33 41    +05 18 43
SA98       06 52 12  -00 19 17          ---  ---  ---  ---  ---        670           06 52 12    -00 18 55
RU149      07 24 15  -00 32 55          ---    4    2  ---    2        149	     07 24 13    -00 31 58
RU152      07 29 55  -02 06 18          ---  ---  ---  ---  ---        152	     07 27 29    -01 59 56
PG0918     09 21 28  +02 46 03          ---  ---  ---  ---  ---     no label	     09 21 28    +02 46 06
PG0942     09 45 12  -03 09 24          ---  ---  ---  ---  ---     no label	     09 45 12    -03 09 21
PG1047     10 50 03  -00 00 32          ---    4    2  ---    2     no label	     10 50 03    -00 00 30
PG1323     13 25 39  -08 49 16          ---  ---  ---  ---  ---     no label	     13 25 39    -08 49 18
PG1528     15 30 50  +06 00 56          ---  ---  ---  ---  ---     no label	     15 30 50    +06 00 51
PG1633     16 35 24  +09 47 50          ---  ---  ---  ---  ---     no label	     16 35 24    +09 47 45
PG1657     16 59 32  +07 43 31          ---  ---  ---  ---  ---     no label	     16 59 32    +07 43 25
MARK A     20 43 59  -10 47 42          ---    7    4  ---    4     no label	     20 43 59    -10 47 42
PG2213     22 16 28  -00 21 15          ---  ---  ---  ---  ---     no label	     22 16 28    -00 21 17
PG2331     23 33 44  +05 46 36          ---  ---  ---  ---  ---     no label	     23 33 44    +05 46 35
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  • You may refer to the Landolt Standard Stars charts here Spectrophotometric Standard Stars ---------------------------------------------------- Star RA (2000) DEC V Time (sec) ---------------------------------------------------- LTT 377 00:41:46.6 -33:39:10 11.229 40 LTT 1020 01:54:49.7 -27:28:29 11.522 40 EG 21 03:10:30.4 -68:36:05 11.379 40 LTT 1788 03:48:22.2 -39:08:35 13.155 80 LTT 2415 05:56:24.2 -27:51:26 12.214 60 Hilt 600 06:45:13.5 +02:08:15 10.441 20 L745-46A 07:40:20.9 -17:24:42 13.0 80 LTT 3218 08:41:33.6 -32:56:55 11.858 40 LTT 3864 10:32:13.8 -35:37:42 12.171 60 LTT 4364 11:45:36.6 -64:50:24 11.504 40 Feige 56 12:06:39.7 +11:40:39 11.057 40 LTT 4816 12:38:50.7 -49:47:58 13.794 80 CD 32 14:11:46.3 -33:03:15 10.452 20 LTT 6248 15:38:59.8 -28:35:34 11.797 30 EG 274 16:23:33.7 -39:13:48 11.029 30 LTT 7379 18:36:26.2 -44:18:37 10.225 20 LTT 7987 20:10:57.1 -30:13:03 12.230 40 LTT 9239 22:52:40.9 -20:35:27 12.068 40 Feige 110 23:19:58.3 -05:09:56 11.826 40 LTT 9491 23:19:35.2 -17:05:28 14.112 120 ----------------------------------------------------
  • A list of Spectrophotometric Standard Stars may be found here Standards for telluric features correction -------------------------------------------------------------- Star RA (2000) DEC V Time (sec) -------------------------------------------------------------- L745-46A 07:40:20.9 -17:24:42 13.0 200 DF,Bessell99 LTT 4364 11:45:36.6 -64:50:24 11.504 120 EG131 19:20:35.0 -07:40:00 12.28 120 Bessell99 NGC 7293 22:29:38.6 -20:50:14 13.5 240 PN central star LTT 9491 23:19:35.4 -17:05:28 14.1 300 DC,Bessell99 -------------------------------------------------------------- One telluric standard with narrow slit (followed by a comparison lamp). Click on the star name to get a finding chart. Supernovae for spectroscopy and photometry (sorted by local time of observation) ---------------------------------------------------------------------------------------------------------------- Name B V I spectr. mag Priority RA DEC Comments (suggested exposure times, sec) (1 is highest) (2000.0) --------------------------------------------------------------------------------------------------------------- SN2010fz 3x300 1 09:42:04.77 +00:19:51.0 Ia before max SN2010ev 30 3x600 0.5 10:25:28.99 -39:49:51.2 young Ia SN2010cn 3x900 1 11:04:06.57 +04:49:58.7 Ib SN2009Z 200 4x1800 3 14:01:53.61 -01:20:30.20 redshift SN2010as 3x1200 1 15:49:49.23 -29:23:09.7 Ib/c 07Y like SN2010ds 3x900 3 19:15:51.46 -56:12:30.9 spec. class SN2010eh 3x900 2 20:48:13.54 -05:48:13.0 type Ic? SN2010ex 3x600 1.5 23:00:10.90 +26:05:57.2 young Ia SN2007if 3x1200 1 01:10:51.37 +15:27:39.90 redshift SN2007il 3x1200 1 01:27:09.75 +14:46:46.50 redshift SN2010el 3x900 0.5 04:19:58.83 -54:56:38.5 Ia-pec __________________________________________________________________________________________________________ 2 - 3 Spectrophotometric standards with wide slit One telluric standard with narrow (high s/n) slit. 30s B/V exposures are ok for direct images of all the targets. Note: For ACTIVE SNe we should orient the slit along the paralactic angle. However, if the SN is located close to the host it might be necessary to pick a different and more convenient angle to avoid contamination of the host. If so, it would be convenient to observe the SN at a low airmass. The finding charts can be found HERE and/or HERE.
    WFCCD Obs Log QSOs (Paulina Lira's project): CT803 3-4x800 1 00 04 48.16 -41 57 28.2 CR 214.4 star very bright CT406 3x1200 1 00 34 26.84 -37 12 52.4 CR 140.4 HB89 3x1200 3 03 31 06.3 -38 24 05 CR 164.3 CT320 3x1200 1 13 17 44.16 -31 47 13.3 CR 174.4 J2143 3-4x900 1 21 43 55.1 -29 51 59 CR 198.9 star very bright CT564 3x1200 3 21 50 15.97 -44 11 23.9 CR 213.4 needs observation CT953 3x1200 1 21 59 54.72 -40 05 50.4 CR 143.0 J2215 3x1200 2 22 15 16.02 -29 44 23.3 CR 192.0 CT975 3x1200 2 22 38 13.28 -32 48 24.2 CR 183.6 J2247 3x1200 2 22 47 43.6 -31 03 07 CR 229.8 needs observation ----------------------------------------------------------------------------------------------------------------