Peter will normally update the OVRO and CARMA machines, as well as the 32 bit version ('astroload miriad') and 64 bit version ('astroload -v 64 miriad') on the UMD machines. For anybody else, check the procedure below if that is what you do:
A summary of the software components modified for PACS:
- gpbuddy: writes out (unwrapped) phaseatm from a gain solution (that came from selfcal) [V1.7 and up]
- gplist: handle 23 ants (SZA files now use 23, CARMA still uses nants=15). Can also list subsets of ants now.
- uvcal: has new options=atmcal to apply the atmphase to a dataset. Make sure you have a good freqatm value in your dataset (for now)
- uvwide: SZA data do not have narrow flags, this program was updated for this. [25-nov or later]
- bldelay: baseline based
- panda: baseline based
- maxdim: new program that just displays your miriad version and the MAX parameters. MAXBUF increased.
- selfcal/mselfcal/mfcal: to handle the large number (around 10,000) integrations. maxdim.h also updated, see below.
- listobs: handle SZA data [V1.25 and up]
MIRIAD/SZA data issues
The procedure to convert SZA data into miriad format is still changing, here are some known issues. Most of these are to be resolved in the new filler that writes data from Dec 11 onwards:
Version 1.1 issues
- systemp is erroneously written with the wrong dimension. listobs has been patched to look at wsystemp in this case.
- There are no linelength data (phasem1), but this is a known issue and won't be added for a while.
Older issues from before Dec 11
- Time sorting (solved in 1.1). If the data is not time sorted, mfcal won't work. Rest should be ok. See comments on uvsort/uvwide below.
- The antpos uv variable is not correct. (fixed in 1.1)
- The freq variable is missing, listobs now works around that
- There is no version keyword in the data. (fixed in 1.1)
- Only wide band data are flagged (fixed in 1.1), you must run
uvwide vis=SZA narrow=t
- 3QSO track (zrct015.3QSO_3C273.3mm.1.mir)
- no wide band data (this may be a result of running uvsort, probably uvwide narrow=t should have been run first
- first few integrations after a source change are bad. this may actually be a result of uvsort, To Be Resolved. It is possible that the SMA routine qvack can fix this, but keep in mind that the number of bad integrations may be not constant (4,5 and 6 of 2" each have been observed)
- missing NOISE source data.(zrcx252.Arp220_12CO.1.mir.tar)
- (now resolved) prior to about Dec 3, data had the wrong sign in the U-V coordinates. You can solve that by using scale < 1 in gpbuddy. To check if your data has the wrong sign of the phases, check a similarly oriented antenna pair using UV list and see in which quadrant the UV coordinates are, viz.
uvlist vis=SZA select='ant(21)(23),time(15:00,15:01),-source(noise)' uvlist vis=CAR select='ant(2)(4),time(15:00,15:01),-source(noise)'
- systemp's are constant, but this is a feature. Need to double check if the array is properly written as systemp(nants,nwide), and not the other way around.
- There are two versions of the 3QSO dataset (zrct015.3QSO_3c273.3mm.1.mir.tar.gz and zrct015.3QSO_3C273.3mm.1.mir.tar.gz) that have a 30MB difference in size. The latter (upper case C) one is smaller and sorted in time, but has lost the wide band data. After the following procedure
uvwide vis=zrct015.3QSO_3c273.3mm.1.mir narrow=t uvsort vis=zrct015.3QSO_3c273.3mm.1.mir out=sza1 uvwide vis=sza1 out=sza2 nwide=16
all flags are correct, including the bad data after a source change.
Reminder on updating MIRIAD (old style)
It is assumed you have a CVS enabled release of MIRIAD (i.e. you have files such as $MIR/CVS)
- MAXDIM: two header files describing maximum sizes were updated: $MIRINC/maxdim.h and $MIRINC/maxdimc.h. Edit this files and modify the MAXBUF parameter in both files to at least 10000000 (4 times the amount is the memory used by programs that use MAXBUF).
cd $MIRINC $EDITOR maxdim.h maxdimc.h
and if to properly update the CVS status of these files (they changed on Dec 4, 2008) a one time is needed to old MIRIAD installs:
mkdir tmp mv maxdim.h maxdimc.h tmp cvs update mv tmp/max*h .
- CVS: always query your source tree first and look for C (conflicts) and M (locally modified) files. The U (to be updated) files will be new ones you will get:
cvs -nq update
and if happy with this, issue the real update
- Old style updates: (you can give these commands from any directory and it assumed you have write permission in $MIR)
mirboss mir.install subs prog
for a blanket re-install of the library and programs. You need this if e.g. maxdim.h was changed, and/or your miriad does not use shared libraries. This is also the safest way to update. On most computers this will only take 2-3 minutes. If however you know exactly what the impact of a new file is, you can pick any of the following examples, which will take 2-3 seconds:
mir.subs fitsio.for uvio
mir.prog itemize gpbuddy
Notice a file extension is optional, and multiple arguments can be given. Watch the output carefully for fatal compile or link errors.
Either way, a quick way to check if you had no disastrous compile issues, count the number of binaries in $MIRBIN, there should be about 400:
ls $MIRBIN | wc
The output of a single mir.prog cgdisp command should be clean, and not give any compile or linking problems. If so, you may have either corrupt miriad library, or a misconfigured system to begin with.
- New style updates: (these can take 10 minutes)
cd $MIR make make install
uvwide vis=$VIS narrow=t
fixes the narrow band flags by copying them from the wide band flags. This issue will probably disappear when the SZA data filler is updated to write the narrow flags directly.
- puthd: manually need to put freqatm in the dataset that came out of gpbuddy (phaseatm needs it in uvcal). Ideally selfcal would write the freq0 variable. E.g.
puthd vis=$VIS/freqatm value=30.1 type=double
- gpbuddy time ranges: if carma data (vis=) and sza data (vis2=) do not share the same time range, erroneous phases can be applied. Sampling can be slighly different, but there are caveats to using a long interval for phaseatm: UV variables only remember the past, selfcal gains are interpolated.