diff options
| author | Joseph Hunkeler <jhunkeler@gmail.com> | 2015-03-05 18:32:20 -0500 |
|---|---|---|
| committer | Joseph Hunkeler <jhunkeler@gmail.com> | 2015-03-05 18:32:20 -0500 |
| commit | 428f915e6b31e1801c318b388e2eb28bb2448148 (patch) | |
| tree | f75abbe16ff158af66a6e8879b19e54f92b825bb | |
| parent | 968754311d038c1b02634a504b4b2eed43dfc4e8 (diff) | |
| download | calfuse-428f915e6b31e1801c318b388e2eb28bb2448148.tar.gz | |
Remove calibration files
| -rw-r--r-- | parmfiles/bchr1a003.fit | bin | 14400 -> 0 bytes | |||
| -rw-r--r-- | parmfiles/bchr1b003.fit | bin | 14400 -> 0 bytes | |||
| -rw-r--r-- | parmfiles/bchr2a003.fit | bin | 14400 -> 0 bytes | |||
| -rw-r--r-- | parmfiles/bchr2b003.fit | bin | 14400 -> 0 bytes | |||
| -rw-r--r-- | parmfiles/master_calib_file.dat | 453 | ||||
| -rw-r--r-- | parmfiles/parm1a015.fit | 1 | ||||
| -rw-r--r-- | parmfiles/parm1b015.fit | 1 | ||||
| -rw-r--r-- | parmfiles/parm2a015.fit | 1 | ||||
| -rw-r--r-- | parmfiles/parm2b015.fit | 1 | ||||
| -rw-r--r-- | parmfiles/scrn1a015.fit | 1 | ||||
| -rw-r--r-- | parmfiles/scrn1b015.fit | 1 | ||||
| -rw-r--r-- | parmfiles/scrn2a015.fit | 1 | ||||
| -rw-r--r-- | parmfiles/scrn2b015.fit | 1 |
13 files changed, 0 insertions, 461 deletions
diff --git a/parmfiles/bchr1a003.fit b/parmfiles/bchr1a003.fit Binary files differdeleted file mode 100644 index 7f21089..0000000 --- a/parmfiles/bchr1a003.fit +++ /dev/null diff --git a/parmfiles/bchr1b003.fit b/parmfiles/bchr1b003.fit Binary files differdeleted file mode 100644 index a9427a7..0000000 --- a/parmfiles/bchr1b003.fit +++ /dev/null diff --git a/parmfiles/bchr2a003.fit b/parmfiles/bchr2a003.fit Binary files differdeleted file mode 100644 index 7ded2f4..0000000 --- a/parmfiles/bchr2a003.fit +++ /dev/null diff --git a/parmfiles/bchr2b003.fit b/parmfiles/bchr2b003.fit Binary files differdeleted file mode 100644 index 0f003b8..0000000 --- a/parmfiles/bchr2b003.fit +++ /dev/null diff --git a/parmfiles/master_calib_file.dat b/parmfiles/master_calib_file.dat deleted file mode 100644 index 6f67b95..0000000 --- a/parmfiles/master_calib_file.dat +++ /dev/null @@ -1,453 +0,0 @@ -# This is an example of the master calibration database file that -# lists the valid dates of each calibration file. -# This file is read by cf_fuv_init. -# Though it is not strictly required by cf_fuv_init, this file -# should be kept in time order. -# There should be no blank lines in this file. -# Reminder: -# interp flag of 0 => stepwise -# interp flag of 1 => interpolate -# -# The items must appear in the following columns: -# Columns Item -# 1- 4 Keyword name -# 5- 6 Blank -# 7 Detector number (or blank) -# 8 Detector segment (or blank) -# 9-10 Blank -# 11-23 Filename -# 24-25 Blank -# 26-34 Modified Julian Date -# 35-36 Blank -# 37 Interpolation method -# -# 03/15/2001 wvd Change ASTG files to version 5 -# 03/19/2001 wvd Change SCRN files to version 4 -# 03/27/2001 wvd Change BKGD files to version 2 -# Change SCRN files to version 5 -# Add AIRG files -# 03/28/2001 wvd Change WGTS files to version 7 -# 03/29/2001 wvd Change PARM files to version 5 -# 04/02/2001 wvd Add WALK files -# 04/09/2001 wvd Change WAVE files to version 10 -# Change QUAL files to version 2 -# 04/10/2001 wvd Add PHAM files -# Change WGTS files to version 8 -# 04/11/2001 wvd Add multiple PHAM files -# 04/17/2001 wvd Change WGTS files to version 9 -# 04/24/2001 wvd Change WALK files to version 2 -# 05/23/2001 wvd Delete DRFT files; not used -# 06/12/2001 wvd Change ASTG files to version 6 -# 07/03/2001 wvd Delete AIRG files; not used -# Change BKGD files to versions 3&4 -# Change SCRN files to version 7 -# 07/25/2001 wvd Change PHAM files to versions 72-84 -# Change SCRN files to version 8 -# 07/26/2001 wvd Change WAVE files to version 11 -# Change FLUX files to version 7 -# 08/15/2001 wvd Added GAIN files versions 17-22 -# Added TCNT files version 10 -# 08/23/2001 wvd Change PARM files to version 6 -# 08/30/2001 wvd Change WAVE files to version 12 -# 09/12/2001 wvd Change WALK files to version 3 -# 09/13/2001 wvd Change WAVE files to version 13 -# 09/14/2001 wvd Change SCRN files to version 9 -# 09/21/2001 wvd Change SCRN files to version 10 -# 10/02/2001 wvd Change WAVE files to version 14 -# 10/10/2001 wvd Change FLUX files to version 8 -# 11/20/2001 wvd Added QUAL files versions 3-10 -# 11/27/2001 wvd Change SCRN files to version 11 -# 11/29/2001 wvd Change PARM files to version 7 -# 12/07/2001 wvd Add YSTR files -# 02/11/2002 wvd Add VOLT files -# 02/19/2002 wvd Change VOLT files to version 2 -# 03/29/2002 wvd Added BKGD files versions 5-8 -# Change SCRN files to version 12 -# 04/02/2002 wvd Added BCHR files -# 04/10/2002 wvd Change SCRN files to version 13 -# 04/15/2002 wvd Change PARM files to version 8 -# Remove SPEX files version 1 -# 05/02/2002 wvd Change VOLT files to version 3 -# 05/17/2002 wvd Change WAVE files to version 15 -# 05/29/2002 wvd Change GEOM files to version 8 -# Change QUAL files to versions 11-19 -# Change YSTR files to version 2 -# 06/12/2002 wvd Added BKGD files version 9 -# 18/12/2002 rdr added AIRG files -# change BCHR files -# 01/14/2003 wvd Change VOLT files to version 5 -# 01/17/2003 wvd Change WAVE files to version 14 -# Added DIGI file version 1 -# Added SPEC file version 1 -# 02/07/2003 wvd Added FLUX files versions 9-13 -# 02/11/2003 wvd Change VOLT files to version 6 -# 02/13/2003 wvd Replace FLUX files with AEFF files -# 02/14/2003 wvd Change effective date of aeff*008.fit files -# to 51403, which was HV first turned on. -# 02/25/2003 wvd Change PARM files to version 10 -# 02/28/2003 wvd Added AEFF files versions 8-13 -# 03/07/2003 peb Change GEOM files to version 12 -# 03/25/2003 wvd Change CHID files to version 10 -# for SIDE 2 ONLY!!! -# 04/07/2003 wvd Change ASTG files to version 7 -# for SIDE 2 ONLY!!! -# 04/09/2003 rdr Added QUAL files to CalFUSE v3.0 -# 06/17/2003 wvd Change AIRG files to version 2 -# 06/25/2003 djs Change GEOM files to version 13 for 1B only -# 07/09/2003 rdr Change all GEOM files to version 13 -# 07/23/2003 rdr Change all CHID files to version 11 -# 07/31/2003 wvd Change ELEC file to version 2 -# 08/19/2003 wvd Added AEFF files versions 14-15 -# 08/20/2003 wvd Change ELEC file to version 3 -# 08/20/2003 wvd Change VOLT files to version 7 -# 08/21/2003 wvd Change SPEC file to version 2 -# 08/27/2003 wvd Change SAAC file to version 4 -# 09/05/2003 wvd Change BCHR file to version 3 -# Change BKGD files to versions 11-16 -# 09/10/2003 djs Change ASTG files to version 8 -# 09/17/2003 wvd Change ASTG files to version 9 -# 09/22/2003 wvd Change WAVE files to version 15 -# 10/02/2003 wvd Change WGTS files to version 10 -# 10/10/2003 rdr Change QUAL files to version 20 -# 10/14/2003 wvd Change PHAX files to version 4 -# 02/09/2004 wvd Change ELEC file to version 4 -# 02/20/2004 rdr Change CHID files to version 12 -# 03/03/2004 rdr Change WGTS files to version 11 -# 03/26/2004 rdr Change GEOM files to version 14 -# 03/30/2004 wvd Change WAVE files to version 16 -# 04/21/2003 rdr Added BKGD files version 17 -# 04/27/2004 wvd Change PARM files to version 11 -# 06/08/2004 wvd Change PHAX files to version 5 -# Change ASTG files to version 10 -# 07/02/2004 wvd Added AEFF files versions 16-21 -# 07/07/2004 rdr Change MIRR file to version 2 -# 07/28/2004 wvd Change VOLT files to version 8 -# 08/11/2004 wvd Change GEOM files to version 15 -# 08/11/2004 wvd Change WAVE files to version 17 -# 08/20/2004 wvd Change SCRN files to version 14 -# 08/24/2004 wvd Change GEOM files to version 16 -# 10/21/2004 wvd Change PARM files to version 12 -# 01/21/2005 wvd Change ASTG files to version 11 -# 02/22/2005 wvd Change WAVE files to version 18 -# 03/02/2005 wvd Added PHAH files -# Added STIM files -# 03/10/2005 wvd Change AIRG files to version 03 -# Change MJD of initial AEFF_CAL -# file to 50000. -# 03/14/2005 wvd Change CHID files to version 13 -# 03/16/2005 wvd Added BKGD files version 18 -# 03/24/2005 wvd Change VOLT files to version 9 -# 04/07/2005 wvd Change SCRN files to version 15 -# 06/01/2005 wvd Change WAVE files to version 19 -# 06/13/2005 wvd Change AEFF files to versions 100-119 -# 06/22/2005 wvd Change WAVE files to version 20 -# 07/06/2005 wvd Change PARM files to version 13 -# 07/19/2005 wvd Change GRAT file to version 02 -# 09/07/2005 wvd Change WAVE files to version 21 -# 02/22/2006 wvd Change WAVE files to version 22 -# 05/11/2006 wvd Add AEFF files version 120 -# 05/23/2006 wvd Change AIRG files to version 04 -# 06/14/2006 wvd Change PARM files to version 14 -# 07/06/2006 wvd Change GRAT file to version 03 -# 10/24/2006 wvd Change PARM files to version 15 -# 11/02/2006 wvd Add TMXY files -# 11/22/2006 wvd Change TMXY files to version 001 -# 11/28/2006 wvd Change GRAT file to version 04 -# 12/29/2006 wvd Change ELEC file to version 05 -# 01/19/2007 wvd Change TMXY files to version 002 -# 01/24/2007 wvd Change GRAT file to version 05 -# 02/16/2007 wvd Add AEFF files version 121 -# 03/02/2007 wvd Change WAVE files to version 23 -# 04/06/2007 wvd Change CHID files to version 14 -# 08/15/2007 wvd Add AEFF files version 122 -# 09/12/2007 wvd Add BKGD files version 019 -# 09/17/2007 wvd Change use-after date for bkgd 019 -# 02/08/2008 wvd Change PHAH files to version 02 -# Change STIM files to version 02 -# 03/07/2008 wvd Change PHAX files to version 06 -# -# 1 2 3 4 -#234567890123456789012345678901234567890 -# -# Use after Interp -#Key Seg Filename MJD method -# -AIRG 1A airg1a004.fit 50000.000 0 -# -AIRG 1B airg1b004.fit 50000.000 0 -# -AIRG 2A airg2a004.fit 50000.000 0 -# -AIRG 2B airg2b004.fit 50000.000 0 -# -BKGD 1A bkgd1a011.fit 50000.000 0 -BKGD 1A bkgd1a012.fit 51911.000 0 -BKGD 1A bkgd1a013.fit 52120.000 0 -BKGD 1A bkgd1a014.fit 52202.000 0 -BKGD 1A bkgd1a015.fit 52324.000 0 -BKGD 1A bkgd1a016.fit 52426.000 0 -BKGD 1A bkgd1a017.fit 52845.000 0 -BKGD 1A bkgd1a018.fit 53118.000 0 -BKGD 1A bkgd1a019.fit 53371.500 0 -# -BKGD 1B bkgd1b011.fit 50000.000 0 -BKGD 1B bkgd1b012.fit 51911.000 0 -BKGD 1B bkgd1b013.fit 52120.000 0 -BKGD 1B bkgd1b014.fit 52202.000 0 -BKGD 1B bkgd1b015.fit 52324.000 0 -BKGD 1B bkgd1b016.fit 52426.000 0 -BKGD 1B bkgd1b017.fit 52845.000 0 -BKGD 1B bkgd1b018.fit 53118.000 0 -BKGD 1B bkgd1b019.fit 53371.500 0 -# -BKGD 2A bkgd2a011.fit 50000.000 0 -BKGD 2A bkgd2a012.fit 51911.000 0 -BKGD 2A bkgd2a013.fit 52120.000 0 -BKGD 2A bkgd2a014.fit 52202.000 0 -BKGD 2A bkgd2a015.fit 52324.000 0 -BKGD 2A bkgd2a016.fit 52426.000 0 -BKGD 2A bkgd2a017.fit 52845.000 0 -BKGD 2A bkgd2a018.fit 53118.000 0 -BKGD 2A bkgd2a019.fit 53371.500 0 -# -BKGD 2B bkgd2b011.fit 50000.000 0 -BKGD 2B bkgd2b012.fit 51911.000 0 -BKGD 2B bkgd2b013.fit 52120.000 0 -BKGD 2B bkgd2b014.fit 52202.000 0 -BKGD 2B bkgd2b015.fit 52324.000 0 -BKGD 2B bkgd2b016.fit 52426.000 0 -BKGD 2B bkgd2b017.fit 52845.000 0 -BKGD 2B bkgd2b018.fit 53118.000 0 -BKGD 2B bkgd2b019.fit 53371.500 0 -# -DIGI digi001.fit 50000.000 0 -# -ELEC elec005.fit 50000.000 0 -# -RATE 1A rate1a002.fit 50000.000 0 -# -RATE 1B rate1b002.fit 50000.000 0 -# -RATE 2A rate2a002.fit 50000.000 0 -# -RATE 2B rate2b002.fit 50000.000 0 -# -TMXY 1A tmxy1a002.fit 50000.000 0 -# -TMXY 1B tmxy1b002.fit 50000.000 0 -# -TMXY 2A tmxy2a002.fit 50000.000 0 -# -TMXY 2B tmxy2b002.fit 50000.000 0 -# -GEOM 1A geom1a016.fit 50000.000 0 -# -GEOM 1B geom1b016.fit 50000.000 0 -# -GEOM 2A geom2a016.fit 50000.000 0 -# -GEOM 2B geom2b016.fit 50000.000 0 -# -PHAX 1A phax1a006.fit 50000.000 0 -# -PHAX 1B phax1b006.fit 50000.000 0 -# -PHAX 2A phax2a006.fit 50000.000 0 -# -PHAX 2B phax2b006.fit 50000.000 0 -# -CHID 1A chid1a014.fit 50000.000 0 -# -CHID 1B chid1b014.fit 50000.000 0 -# -CHID 2A chid2a014.fit 50000.000 0 -# -CHID 2B chid2b014.fit 50000.000 0 -# -GRAT grat005.fit 50000.000 0 -# -WAVE 1A wave1a023.fit 50000.000 0 -# -WAVE 1B wave1b023.fit 50000.000 0 -# -WAVE 2A wave2a023.fit 50000.000 0 -# -WAVE 2B wave2b023.fit 50000.000 0 -# -MIRR mirr002.fit 50000.000 0 -# -ASTG 1A astg1a011.fit 50000.000 0 -# -ASTG 1B astg1b011.fit 50000.000 0 -# -ASTG 2A astg2a011.fit 50000.000 0 -# -ASTG 2B astg2b011.fit 50000.000 0 -# -VOLT 1A volt1a009.fit 50000.000 0 -# -VOLT 1B volt1b009.fit 50000.000 0 -# -VOLT 2A volt2a009.fit 50000.000 0 -# -VOLT 2B volt2b009.fit 50000.000 0 -# -BCHR 1A bchr1a003.fit 50000.000 0 -# -BCHR 1B bchr1b003.fit 50000.000 0 -# -BCHR 2A bchr2a003.fit 50000.000 0 -# -BCHR 2B bchr2b003.fit 50000.000 0 -# -PARM 1A parm1a015.fit 50000.000 0 -# -PARM 1B parm1b015.fit 50000.000 0 -# -PARM 2A parm2a015.fit 50000.000 0 -# -PARM 2B parm2b015.fit 50000.000 0 -# -PHAH 1A phah1a002.fit 50000.000 0 -# -PHAH 1B phah1b002.fit 50000.000 0 -# -PHAH 2A phah2a002.fit 50000.000 0 -# -PHAH 2B phah2b002.fit 50000.000 0 -# -SAAC saac004.fit 50000.000 0 -# -SCRN 1A scrn1a015.fit 50000.000 0 -# -SCRN 1B scrn1b015.fit 50000.000 0 -# -SCRN 2A scrn2a015.fit 50000.000 0 -# -SCRN 2B scrn2b015.fit 50000.000 0 -# -SPEC spec002.fit 50000.000 0 -# -STIM 1A stim1a002.fit 50000.000 0 -# -STIM 1B stim1b002.fit 50000.000 0 -# -STIM 2A stim2a002.fit 50000.000 0 -# -STIM 2B stim2b002.fit 50000.000 0 -# -QUAL 1A qual1a020.fit 50000.000 0 -# -QUAL 1B qual1b020.fit 50000.000 0 -# -QUAL 2A qual2a020.fit 50000.000 0 -# -QUAL 2B qual2b020.fit 50000.000 0 -# -WGTS 1A wgts1a011.fit 50000.000 0 -# -WGTS 1B wgts1b011.fit 50000.000 0 -# -WGTS 2A wgts2a011.fit 50000.000 0 -# -WGTS 2B wgts2b011.fit 50000.000 0 -# -AEFF 1A aeff1a100.fit 50000.000 1 -AEFF 1A aeff1a100.fit 51543.000 1 -AEFF 1A aeff1a101.fit 51634.000 1 -AEFF 1A aeff1a102.fit 51725.000 1 -AEFF 1A aeff1a103.fit 51817.000 1 -AEFF 1A aeff1a104.fit 51909.000 1 -AEFF 1A aeff1a105.fit 51999.000 1 -AEFF 1A aeff1a106.fit 52090.000 1 -AEFF 1A aeff1a107.fit 52182.000 1 -AEFF 1A aeff1a108.fit 52274.000 1 -AEFF 1A aeff1a109.fit 52364.000 1 -AEFF 1A aeff1a110.fit 52455.000 1 -AEFF 1A aeff1a111.fit 52547.000 1 -AEFF 1A aeff1a112.fit 52639.000 1 -AEFF 1A aeff1a113.fit 52729.000 1 -AEFF 1A aeff1a114.fit 52820.000 1 -AEFF 1A aeff1a115.fit 52912.000 1 -AEFF 1A aeff1a116.fit 53004.000 1 -AEFF 1A aeff1a117.fit 53095.000 1 -AEFF 1A aeff1a118.fit 53186.000 1 -AEFF 1A aeff1a119.fit 53278.000 1 -AEFF 1A aeff1a120.fit 53818.000 1 -AEFF 1A aeff1a121.fit 54046.800 1 -AEFF 1A aeff1a122.fit 54179.800 1 -# -AEFF 1B aeff1b100.fit 50000.000 1 -AEFF 1B aeff1b100.fit 51543.000 1 -AEFF 1B aeff1b101.fit 51634.000 1 -AEFF 1B aeff1b102.fit 51725.000 1 -AEFF 1B aeff1b103.fit 51817.000 1 -AEFF 1B aeff1b104.fit 51909.000 1 -AEFF 1B aeff1b105.fit 51999.000 1 -AEFF 1B aeff1b106.fit 52090.000 1 -AEFF 1B aeff1b107.fit 52182.000 1 -AEFF 1B aeff1b108.fit 52274.000 1 -AEFF 1B aeff1b109.fit 52364.000 1 -AEFF 1B aeff1b110.fit 52455.000 1 -AEFF 1B aeff1b111.fit 52547.000 1 -AEFF 1B aeff1b112.fit 52639.000 1 -AEFF 1B aeff1b113.fit 52729.000 1 -AEFF 1B aeff1b114.fit 52820.000 1 -AEFF 1B aeff1b115.fit 52912.000 1 -AEFF 1B aeff1b116.fit 53004.000 1 -AEFF 1B aeff1b117.fit 53095.000 1 -AEFF 1B aeff1b118.fit 53186.000 1 -AEFF 1B aeff1b119.fit 53278.000 1 -AEFF 1B aeff1b120.fit 53818.000 1 -AEFF 1B aeff1b121.fit 54046.800 1 -AEFF 1B aeff1b122.fit 54179.800 1 -# -AEFF 2A aeff2a100.fit 50000.000 1 -AEFF 2A aeff2a100.fit 51543.000 1 -AEFF 2A aeff2a101.fit 51634.000 1 -AEFF 2A aeff2a102.fit 51725.000 1 -AEFF 2A aeff2a103.fit 51817.000 1 -AEFF 2A aeff2a104.fit 51909.000 1 -AEFF 2A aeff2a105.fit 51999.000 1 -AEFF 2A aeff2a106.fit 52090.000 1 -AEFF 2A aeff2a107.fit 52182.000 1 -AEFF 2A aeff2a108.fit 52274.000 1 -AEFF 2A aeff2a109.fit 52364.000 1 -AEFF 2A aeff2a110.fit 52455.000 1 -AEFF 2A aeff2a111.fit 52547.000 1 -AEFF 2A aeff2a112.fit 52639.000 1 -AEFF 2A aeff2a113.fit 52729.000 1 -AEFF 2A aeff2a114.fit 52820.000 1 -AEFF 2A aeff2a115.fit 52912.000 1 -AEFF 2A aeff2a116.fit 53004.000 1 -AEFF 2A aeff2a117.fit 53095.000 1 -AEFF 2A aeff2a118.fit 53186.000 1 -AEFF 2A aeff2a119.fit 53278.000 1 -AEFF 2A aeff2a120.fit 53818.000 1 -AEFF 2A aeff2a121.fit 54046.800 1 -AEFF 2A aeff2a122.fit 54179.800 1 -# -AEFF 2B aeff2b100.fit 50000.000 1 -AEFF 2B aeff2b100.fit 51543.000 1 -AEFF 2B aeff2b101.fit 51634.000 1 -AEFF 2B aeff2b102.fit 51725.000 1 -AEFF 2B aeff2b103.fit 51817.000 1 -AEFF 2B aeff2b104.fit 51909.000 1 -AEFF 2B aeff2b105.fit 51999.000 1 -AEFF 2B aeff2b106.fit 52090.000 1 -AEFF 2B aeff2b107.fit 52182.000 1 -AEFF 2B aeff2b108.fit 52274.000 1 -AEFF 2B aeff2b109.fit 52364.000 1 -AEFF 2B aeff2b110.fit 52455.000 1 -AEFF 2B aeff2b111.fit 52547.000 1 -AEFF 2B aeff2b112.fit 52639.000 1 -AEFF 2B aeff2b113.fit 52729.000 1 -AEFF 2B aeff2b114.fit 52820.000 1 -AEFF 2B aeff2b115.fit 52912.000 1 -AEFF 2B aeff2b116.fit 53004.000 1 -AEFF 2B aeff2b117.fit 53095.000 1 -AEFF 2B aeff2b118.fit 53186.000 1 -AEFF 2B aeff2b119.fit 53278.000 1 -AEFF 2B aeff2b120.fit 53818.000 1 -AEFF 2B aeff2b121.fit 54046.800 1 -AEFF 2B aeff2b122.fit 54179.800 1 diff --git a/parmfiles/parm1a015.fit b/parmfiles/parm1a015.fit deleted file mode 100644 index 5f63130..0000000 --- a/parmfiles/parm1a015.fit +++ /dev/null @@ -1 +0,0 @@ -SIMPLE = T / Fits standard BITPIX = 16 / Bits per pixel NAXIS = 0 / Number of axes EXTEND = T / File may contain extensions COMMENT FITS (Flexible Image Transport System) format defined in Astronomy andCOMMENT Astrophysics Supplement Series v44/p363, v44/p371, v73/p359, v73/p365.COMMENT Contact the NASA Science Office of Standards and Technology for the COMMENT FITS Definition document #100 and other FITS information. CALFTYPE= 'PARM ' / Calibration file type CALFVERS= 15 / Calibration file version DETECTOR= '1A ' / detector (1A, 1B, 2A, 2B) EFFMJD = 50000. / Date on which file should be applied (MJD) DATE = '2006-11-30T17:33:00' COMMENT COMMENT The SPEX_SIC and SPEX_LIF keywords allow the user to center the extracCOMMENT tion windows along a given row rather than having the pipeline try to COMMENT centroid the spectrum. A number less than 0 or greater than 1023 willCOMMENT default to pipeline centroiding. A value between 0 and 1023 will defCOMMENT ine the center of the extraction window. Since the pipeline expands hCOMMENT istogram images out to 1023 pixels in Y, the number must be given for COMMENT a full 1023 image height. That is, if the center is determined from bCOMMENT inned images, the center must be multiplied by the binning factor befoCOMMENT re entering it in this file. COMMENT SPEX_SIC= -1 / SiC extraction window Y center (0-1023) SPEX_LIF= -1 / LiF extraction window Y center (0-1023) COMMENT COMMENT The EMAX_SIC and EMAX_LIF keywords allow the user to limit the amount COMMENT that the pipeline can shift the extraction windows based on the centroCOMMENT id of the spectrum. In cases where the source is very faint, the centCOMMENT roid routine may find bright detector artifacts or other apertures insCOMMENT tead of the desired aperture. If the calculated centroid differs fromCOMMENT the predicted centroid by more than EMAX_SIC or EMAX_LIF, the pipelinCOMMENT e uses the default extraction window location. COMMENT EMAX_SIC= 40 / SiC extraction window maximum Y movement EMAX_LIF= 40 / LiF extraction window maximum Y movement COMMENT COMMENT The following keywords allow the user to skip various COMMENT steps of the pipeline. Change value from 'YES' to 'NO' COMMENT to skip the corresponding step. COMMENT RUN_PHAX= 'YES' / PHA X correction RUN_BRST= 'YES' / Burst rejection RUN_JITR= 'YES' / Jitter correction RUN_ASTG= 'YES' / Astigmatism correction RUN_BKGD= 'YES' / Background subtraction RUN_OPTI= 'YES' / Optimal extraction COMMENT COMMENT These keywords control the jitter-screening routine. Only tabulated COMMENT pointing errors with quality flags greater than TRKFLG are considered.COMMENT Times when the pointing errors exceed the allowed limits are flagged COMMENT as bad. Limits are applied to both the LiF and SiC channels. COMMENT TRKFLG = 1 / Minimum trustworthy value of TRKFLG DX_MAX = 30 / [arcsec] Allowed pointing error DY_MAX = 30 / [arcsec] Allowed pointing error COMMENT COMMENT These keywords allow the user to specify the range and bin size of COMMENT the output wavelength array. If not set, default values are used. COMMENT LIF_W0 = / [A] Requested initial wavelength LIF_WMAX= / [A] Requested final wavelength LIF_WPC = / [A] Requested wavelength per channel SIC_W0 = / [A] Requested initial wavelength SIC_WMAX= / [A] Requested final wavelength SIC_WPC = / [A] Requested wavelength per channel END
\ No newline at end of file diff --git a/parmfiles/parm1b015.fit b/parmfiles/parm1b015.fit deleted file mode 100644 index 8f8b8fb..0000000 --- a/parmfiles/parm1b015.fit +++ /dev/null @@ -1 +0,0 @@ -SIMPLE = T / Fits standard BITPIX = 16 / Bits per pixel NAXIS = 0 / Number of axes EXTEND = T / File may contain extensions COMMENT FITS (Flexible Image Transport System) format defined in Astronomy andCOMMENT Astrophysics Supplement Series v44/p363, v44/p371, v73/p359, v73/p365.COMMENT Contact the NASA Science Office of Standards and Technology for the COMMENT FITS Definition document #100 and other FITS information. CALFTYPE= 'PARM ' / Calibration file type CALFVERS= 15 / Calibration file version DETECTOR= '1B ' / detector (1A, 1B, 2A, 2B) EFFMJD = 50000. / Date on which file should be applied (MJD) DATE = '2006-11-30T17:33:00' COMMENT COMMENT The SPEX_SIC and SPEX_LIF keywords allow the user to center the extracCOMMENT tion windows along a given row rather than having the pipeline try to COMMENT centroid the spectrum. A number less than 0 or greater than 1023 willCOMMENT default to pipeline centroiding. A value between 0 and 1023 will defCOMMENT ine the center of the extraction window. Since the pipeline expands hCOMMENT istogram images out to 1023 pixels in Y, the number must be given for COMMENT a full 1023 image height. That is, if the center is determined from bCOMMENT inned images, the center must be multiplied by the binning factor befoCOMMENT re entering it in this file. COMMENT SPEX_SIC= -1 / SiC extraction window Y center (0-1023) SPEX_LIF= -1 / LiF extraction window Y center (0-1023) COMMENT COMMENT The EMAX_SIC and EMAX_LIF keywords allow the user to limit the amount COMMENT that the pipeline can shift the extraction windows based on the centroCOMMENT id of the spectrum. In cases where the source is very faint, the centCOMMENT roid routine may find bright detector artifacts or other apertures insCOMMENT tead of the desired aperture. If the calculated centroid differs fromCOMMENT the predicted centroid by more than EMAX_SIC or EMAX_LIF, the pipelinCOMMENT e uses the default extraction window location. COMMENT EMAX_SIC= 40 / SiC extraction window maximum Y movement EMAX_LIF= 40 / LiF extraction window maximum Y movement COMMENT COMMENT The following keywords allow the user to skip various COMMENT steps of the pipeline. Change value from 'YES' to 'NO' COMMENT to skip the corresponding st COMMENT RUN_PHAX= 'YES' / PHA X correction RUN_BRST= 'YES' / Burst rejection RUN_JITR= 'YES' / Jitter correction RUN_ASTG= 'YES' / Astigmatism correction RUN_BKGD= 'YES' / Background subtraction RUN_OPTI= 'YES' / Optimal extraction COMMENT COMMENT These keywords control the jitter-screening routine. Only tabulated COMMENT pointing errors with quality flags greater than TRKFLG are considered.COMMENT Times when the pointing errors exceed the allowed limits are flagged COMMENT as bad. Limits are applied to both the LiF and SiC channels. COMMENT TRKFLG = 1 / Minimum trustworthy value of TRKFLG DX_MAX = 30 / [arcsec] Allowed pointing error DY_MAX = 30 / [arcsec] Allowed pointing error COMMENT COMMENT These keywords allow the user to specify the range and bin size of COMMENT the output wavelength array. If not set, default values are used. COMMENT LIF_W0 = / [A] Requested initial wavelength LIF_WMAX= / [A] Requested final wavelength LIF_WPC = / [A] Requested wavelength per channel SIC_W0 = / [A] Requested initial wavelength SIC_WMAX= / [A] Requested final wavelength SIC_WPC = / [A] Requested wavelength per channel END
\ No newline at end of file diff --git a/parmfiles/parm2a015.fit b/parmfiles/parm2a015.fit deleted file mode 100644 index 95e96d6..0000000 --- a/parmfiles/parm2a015.fit +++ /dev/null @@ -1 +0,0 @@ -SIMPLE = T / Fits standard BITPIX = 16 / Bits per pixel NAXIS = 0 / Number of axes EXTEND = T / File may contain extensions COMMENT FITS (Flexible Image Transport System) format defined in Astronomy andCOMMENT Astrophysics Supplement Series v44/p363, v44/p371, v73/p359, v73/p365.COMMENT Contact the NASA Science Office of Standards and Technology for the COMMENT FITS Definition document #100 and other FITS information. CALFTYPE= 'PARM ' / Calibration file type CALFVERS= 15 / Calibration file version DETECTOR= '2A ' / detector (1A, 1B, 2A, 2B) EFFMJD = 50000. / Date on which file should be applied (MJD) DATE = '2006-11-30T17:33:00' COMMENT COMMENT The SPEX_SIC and SPEX_LIF keywords allow the user to center the extracCOMMENT tion windows along a given row rather than having the pipeline try to COMMENT centroid the spectrum. A number less than 0 or greater than 1023 willCOMMENT default to pipeline centroiding. A value between 0 and 1023 will defCOMMENT ine the center of the extraction window. Since the pipeline expands hCOMMENT istogram images out to 1023 pixels in Y, the number must be given for COMMENT a full 1023 image height. That is, if the center is determined from bCOMMENT inned images, the center must be multiplied by the binning factor befoCOMMENT re entering it in this file. COMMENT SPEX_SIC= -1 / SiC extraction window Y center (0-1023) SPEX_LIF= -1 / LiF extraction window Y center (0-1023) COMMENT COMMENT The EMAX_SIC and EMAX_LIF keywords allow the user to limit the amount COMMENT that the pipeline can shift the extraction windows based on the centroCOMMENT id of the spectrum. In cases where the source is very faint, the centCOMMENT roid routine may find bright detector artifacts or other apertures insCOMMENT tead of the desired aperture. If the calculated centroid differs fromCOMMENT the predicted centroid by more than EMAX_SIC or EMAX_LIF, the pipelinCOMMENT e uses the default extraction window location. COMMENT EMAX_SIC= 40 / SiC extraction window maximum Y movement EMAX_LIF= 40 / LiF extraction window maximum Y movement COMMENT COMMENT The following keywords allow the user to skip various COMMENT steps of the pipeline. Change value from 'YES' to 'NO' COMMENT to skip the corresponding step. COMMENT RUN_PHAX= 'YES' / PHA X correction RUN_BRST= 'YES' / Burst rejection RUN_JITR= 'YES' / Jitter correction RUN_ASTG= 'YES' / Astigmatism correction RUN_BKGD= 'YES' / Background subtraction RUN_OPTI= 'YES' / Optimal extraction COMMENT COMMENT These keywords control the jitter-screening routine. Only tabulated COMMENT pointing errors with quality flags greater than TRKFLG are considered.COMMENT Times when the pointing errors exceed the allowed limits are flagged COMMENT as bad. Limits are applied to both the LiF and SiC channels. COMMENT TRKFLG = 1 / Minimum trustworthy value of TRKFLG DX_MAX = 30 / [arcsec] Allowed pointing error DY_MAX = 30 / [arcsec] Allowed pointing error COMMENT COMMENT These keywords allow the user to specify the range and bin size of COMMENT the output wavelength array. If not set, default values are used. COMMENT LIF_W0 = / [A] Requested initial wavelength LIF_WMAX= / [A] Requested final wavelength LIF_WPC = / [A] Requested wavelength per channel SIC_W0 = / [A] Requested initial wavelength SIC_WMAX= / [A] Requested final wavelength SIC_WPC = / [A] Requested wavelength per channel END
\ No newline at end of file diff --git a/parmfiles/parm2b015.fit b/parmfiles/parm2b015.fit deleted file mode 100644 index e5289f4..0000000 --- a/parmfiles/parm2b015.fit +++ /dev/null @@ -1 +0,0 @@ -SIMPLE = T / Fits standard BITPIX = 16 / Bits per pixel NAXIS = 0 / Number of axes EXTEND = T / File may contain extensions COMMENT FITS (Flexible Image Transport System) format defined in Astronomy andCOMMENT Astrophysics Supplement Series v44/p363, v44/p371, v73/p359, v73/p365.COMMENT Contact the NASA Science Office of Standards and Technology for the COMMENT FITS Definition document #100 and other FITS information. CALFTYPE= 'PARM ' / Calibration file type CALFVERS= 15 / Calibration file version DETECTOR= '2B ' / detector (1A, 1B, 2A, 2B) EFFMJD = 50000. / Date on which file should be applied (MJD) DATE = '2006-11-30T17:33:00' COMMENT COMMENT The SPEX_SIC and SPEX_LIF keywords allow the user to center the extracCOMMENT tion windows along a given row rather than having the pipeline try to COMMENT centroid the spectrum. A number less than 0 or greater than 1023 willCOMMENT default to pipeline centroiding. A value between 0 and 1023 will defCOMMENT ine the center of the extraction window. Since the pipeline expands hCOMMENT istogram images out to 1023 pixels in Y, the number must be given for COMMENT a full 1023 image height. That is, if the center is determined from bCOMMENT inned images, the center must be multiplied by the binning factor befoCOMMENT re entering it in this file. COMMENT SPEX_SIC= -1 / SiC extraction window Y center (0-1023) SPEX_LIF= -1 / LiF extraction window Y center (0-1023) COMMENT COMMENT The EMAX_SIC and EMAX_LIF keywords allow the user to limit the amount COMMENT that the pipeline can shift the extraction windows based on the centroCOMMENT id of the spectrum. In cases where the source is very faint, the centCOMMENT roid routine may find bright detector artifacts or other apertures insCOMMENT tead of the desired aperture. If the calculated centroid differs fromCOMMENT the predicted centroid by more than EMAX_SIC or EMAX_LIF, the pipelinCOMMENT e uses the default extraction window location. COMMENT EMAX_SIC= 40 / SiC extraction window maximum Y movement EMAX_LIF= 40 / LiF extraction window maximum Y movement COMMENT COMMENT The following keywords allow the user to skip various COMMENT steps of the pipeline. Change value from 'YES' to 'NO' COMMENT to skip the corresponding step. COMMENT RUN_PHAX= 'YES' / PHA X correction RUN_BRST= 'YES' / Burst rejection RUN_JITR= 'YES' / Jitter correction RUN_ASTG= 'YES' / Astigmatism correction RUN_BKGD= 'YES' / Background subtraction RUN_OPTI= 'YES' / Optimal extraction COMMENT COMMENT These keywords control the jitter-screening routine. Only tabulated COMMENT pointing errors with quality flags greater than TRKFLG are considered.COMMENT Times when the pointing errors exceed the allowed limits are flagged COMMENT as bad. Limits are applied to both the LiF and SiC channels. COMMENT TRKFLG = 1 / Minimum trustworthy value of TRKFLG DX_MAX = 30 / [arcsec] Allowed pointing error DY_MAX = 30 / [arcsec] Allowed pointing error COMMENT COMMENT These keywords allow the user to specify the range and bin size of COMMENT the output wavelength array. If not set, default values are used. COMMENT LIF_W0 = / [A] Requested initial wavelength LIF_WMAX= / [A] Requested final wavelength LIF_WPC = / [A] Requested wavelength per channel SIC_W0 = / [A] Requested initial wavelength SIC_WMAX= / [A] Requested final wavelength SIC_WPC = / [A] Requested wavelength per channel END
\ No newline at end of file diff --git a/parmfiles/scrn1a015.fit b/parmfiles/scrn1a015.fit deleted file mode 100644 index 14fbae7..0000000 --- a/parmfiles/scrn1a015.fit +++ /dev/null @@ -1 +0,0 @@ -SIMPLE = T / Fits standard BITPIX = 16 / Bits per pixel NAXIS = 0 / Number of axes EXTEND = T / File may contain extensions ORIGIN = 'NOAO-IRAF FITS Image Kernel December 2001' / FITS file originator IRAF-TLM= '17:33:33 (13/04/2005)' COMMENT FITS (Flexible Image Transport System) format defined in Astronomy andCOMMENT Astrophysics Supplement Series v44/p363, v44/p371, v73/p359, v73/p365.COMMENT Contact the NASA Science Office of Standards and Technology for the COMMENT FITS Definition document #100 and other FITS information. CALFTYPE= 'SCRN ' / Calibration file type CALFVERS= 15 / Calibration file version DETECTOR= '1A ' / detector (1A, 1B, 2A, 2B) EFFMJD = 50000. / Date on which file should be applied (MJD) DATE = 'Tue Apr 2 14:20:04 2002' / Date file was created AUTHOR = 'R.D. Robinson' / Author SAA_SCR = 'ON ' / SAA screening ON/OFF LIMB_SCR= 'ON ' / Limb angle screening ON/OFF DAYNIGHT= 'BOTH ' / Use only DAY, NIGHT or BOTH PHALOW = 2 / Minimum acceptable PHA value PHAHIGH = 25 / Maximum acceptable PHA value BRITLIMB= 15. / [deg] Bright limb avoidance angle DARKLIMB= 10. / [deg] Dark limb avoidance angle NUSERGTI= 0 / Number of user defined good time intervals GTIBEG01= 0. / [sec] Beginning good time interval GTIEND01= 0. / [sec] Ending good time interval GTIBEG02= 0. / [sec] Beginning good time interval GTIEND02= 0. / [sec] Ending good time interval MNCNT = 5 / minimum cnt rate for burst STDREJ = 5 / std dev from median for burst rej NBIN = 15 / binning factor for time sequence NSMED = 600 / averaging factor (s) in det med flt SRCFRAC = 0.00100000 / fraction of source intensity needed BKGDTYPE= 1 / flag for type of background model END
\ No newline at end of file diff --git a/parmfiles/scrn1b015.fit b/parmfiles/scrn1b015.fit deleted file mode 100644 index eb9a195..0000000 --- a/parmfiles/scrn1b015.fit +++ /dev/null @@ -1 +0,0 @@ -SIMPLE = T / Fits standard BITPIX = 16 / Bits per pixel NAXIS = 0 / Number of axes EXTEND = T / File may contain extensions ORIGIN = 'NOAO-IRAF FITS Image Kernel December 2001' / FITS file originator IRAF-TLM= '17:33:33 (13/04/2005)' COMMENT FITS (Flexible Image Transport System) format defined in Astronomy andCOMMENT Astrophysics Supplement Series v44/p363, v44/p371, v73/p359, v73/p365.COMMENT Contact the NASA Science Office of Standards and Technology for the COMMENT FITS Definition document #100 and other FITS information. CALFTYPE= 'SCRN ' / Calibration file type CALFVERS= 15 / Calibration file version DETECTOR= '1B ' / detector (1A, 1B, 2A, 2B) EFFMJD = 50000. / Date on which file should be applied (MJD) DATE = 'Tue Apr 2 14:20:04 2002' / Date file was created AUTHOR = 'R.D. Robinson' / Author SAA_SCR = 'ON ' / SAA screening ON/OFF LIMB_SCR= 'ON ' / Limb angle screening ON/OFF DAYNIGHT= 'BOTH ' / Use only DAY, NIGHT or BOTH PHALOW = 2 / Minimum acceptable PHA value PHAHIGH = 24 / Maximum acceptable PHA value BRITLIMB= 15. / [deg] Bright limb avoidance angle DARKLIMB= 10. / [deg] Dark limb avoidance angle NUSERGTI= 0 / Number of user defined good time intervals GTIBEG01= 0. / [sec] Beginning good time interval GTIEND01= 0. / [sec] Ending good time interval GTIBEG02= 0. / [sec] Beginning good time interval GTIEND02= 0. / [sec] Ending good time interval MNCNT = 5 / minimum cnt rate for burst STDREJ = 5 / std dev from median for burst rej NBIN = 15 / binning factor for time sequence NSMED = 600 / averaging factor (s) in det med flt SRCFRAC = 0.00100000 / fraction of source intensity needed BKGDTYPE= 1 / flag for type of background model END
\ No newline at end of file diff --git a/parmfiles/scrn2a015.fit b/parmfiles/scrn2a015.fit deleted file mode 100644 index 25a48f3..0000000 --- a/parmfiles/scrn2a015.fit +++ /dev/null @@ -1 +0,0 @@ -SIMPLE = T / Fits standard BITPIX = 16 / Bits per pixel NAXIS = 0 / Number of axes EXTEND = T / File may contain extensions ORIGIN = 'NOAO-IRAF FITS Image Kernel December 2001' / FITS file originator IRAF-TLM= '17:33:33 (13/04/2005)' COMMENT FITS (Flexible Image Transport System) format defined in Astronomy andCOMMENT Astrophysics Supplement Series v44/p363, v44/p371, v73/p359, v73/p365.COMMENT Contact the NASA Science Office of Standards and Technology for the COMMENT FITS Definition document #100 and other FITS information. CALFTYPE= 'SCRN ' / Calibration file type CALFVERS= 15 / Calibration file version DETECTOR= '2A ' / detector (1A, 1B, 2A, 2B) EFFMJD = 50000. / Date on which file should be applied (MJD) DATE = 'Tue Apr 2 14:20:05 2002' / Date file was created AUTHOR = 'R.D. Robinson' / Author SAA_SCR = 'ON ' / SAA screening ON/OFF LIMB_SCR= 'ON ' / Limb angle screening ON/OFF DAYNIGHT= 'BOTH ' / Use only DAY, NIGHT or BOTH PHALOW = 3 / Minimum acceptable PHA value PHAHIGH = 23 / Maximum acceptable PHA value BRITLIMB= 15. / [deg] Bright limb avoidance angle DARKLIMB= 10. / [deg] Dark limb avoidance angle NUSERGTI= 0 / Number of user defined good time intervals GTIBEG01= 0. / [sec] Beginning good time interval GTIEND01= 0. / [sec] Ending good time interval GTIBEG02= 0. / [sec] Beginning good time interval GTIEND02= 0. / [sec] Ending good time interval MNCNT = 5 / minimum cnt rate for burst STDREJ = 5 / std dev from median for burst rej NBIN = 15 / binning factor for time sequence NSMED = 600 / averaging factor (s) in det med flt SRCFRAC = 0.00100000 / fraction of source intensity needed BKGDTYPE= 1 / flag for type of background model END
\ No newline at end of file diff --git a/parmfiles/scrn2b015.fit b/parmfiles/scrn2b015.fit deleted file mode 100644 index 3a85c3c..0000000 --- a/parmfiles/scrn2b015.fit +++ /dev/null @@ -1 +0,0 @@ -SIMPLE = T / Fits standard BITPIX = 16 / Bits per pixel NAXIS = 0 / Number of axes EXTEND = T / File may contain extensions ORIGIN = 'NOAO-IRAF FITS Image Kernel December 2001' / FITS file originator IRAF-TLM= '17:33:33 (13/04/2005)' COMMENT FITS (Flexible Image Transport System) format defined in Astronomy andCOMMENT Astrophysics Supplement Series v44/p363, v44/p371, v73/p359, v73/p365.COMMENT Contact the NASA Science Office of Standards and Technology for the COMMENT FITS Definition document #100 and other FITS information. CALFTYPE= 'SCRN ' / Calibration file type CALFVERS= 15 / Calibration file version DETECTOR= '2B ' / detector (1A, 1B, 2A, 2B) EFFMJD = 50000. / Date on which file should be applied (MJD) DATE = 'Tue Apr 2 14:20:05 2002' / Date file was created AUTHOR = 'R.D. Robinson' / Author SAA_SCR = 'ON ' / SAA screening ON/OFF LIMB_SCR= 'ON ' / Limb angle screening ON/OFF DAYNIGHT= 'BOTH ' / Use only DAY, NIGHT or BOTH PHALOW = 3 / Minimum acceptable PHA value PHAHIGH = 24 / Maximum acceptable PHA value BRITLIMB= 15. / [deg] Bright limb avoidance angle DARKLIMB= 10. / [deg] Dark limb avoidance angle NUSERGTI= 0 / Number of user defined good time intervals GTIBEG01= 0. / [sec] Beginning good time interval GTIEND01= 0. / [sec] Ending good time interval GTIBEG02= 0. / [sec] Beginning good time interval GTIEND02= 0. / [sec] Ending good time interval MNCNT = 5 / minimum cnt rate for burst STDREJ = 5 / std dev from median for burst rej NBIN = 15 / binning factor for time sequence NSMED = 600 / averaging factor (s) in det med flt SRCFRAC = 0.00100000 / fraction of source intensity needed BKGDTYPE= 1 / flag for type of background model END
\ No newline at end of file |