[daip] UVSUB and memory allocation
Andy Biggs
abiggs at eso.org
Fri Mar 30 11:26:40 EDT 2012
Hi there. UVSUB is failing for me with the following message:
localh> UVSUB1: Task UVSUB (release of 31DEC12) begins
localh> UVSUB1: You are using a non-standard program
localh> UVSUB1: SETGDS: imaging done with reprojected tangent point(s)
localh> UVSUB1: Using Clean Component source model
localh> UVSUB1: FACSET: 0.897173 Jy found from 7919 components
localh> UVSUB1: Create GROTHN4 .UVSUB . 3 (UV) on disk 1 cno 203
localh> UVSUB1: ZMEMRY: MEMORY ALLOCATION FAILS AT UVSUB
localh> UVSUB1: QINIT: ERROR 3 FROM ZMEMRY DOING GET KWORDS 283791
localh> UVSUB1: GRDSUB: FAILED TO GET THE NEEDED AP MEMORY
localh> UVSUB1: Destroyed UV image file: catno= 203 disk= 1
localh> UVSUB1: Purports to die of UNNATURAL causes
localh> UVSUB1: pc016987 31DEC12 TST: Cpu= 3.1 Real= 18 IO= 5
I ran a midnight job immediately beforehand. It seems that CMETHOD='DFT' will work, but will probably take a very long time. If AP size is an issue, I currently have:
>setmaxap
AIPS 1: SETMAXAP: current max dynamic AP is 1500.000 Mbytes
AIPS 1: SETMAXAP: allowed range is 20 to 1536 Mbytes
My UVSUB inputs are:
AIPS 1: UVSUB Task to subtract CLEAN components from a uv data base.
AIPS 1: Adverbs Values Comments
AIPS 1: ----------------------------------------------------------------
AIPS 1: (or, to divide observed visi-
AIPS 1: bility by model visibility)
AIPS 1: INNAME 'GROTHN4' Input UV file name (name)
AIPS 1: INCLASS 'SPLIT' Input UV file name (class)
AIPS 1: INSEQ 3 Input UV file name (seq. #)
AIPS 1: INDISK 1 Input UV file disk unit #
AIPS 1: NMAPS 93 No. maps to use for model.
AIPS 1: CHANNEL 0 Spectral channel (0=>all)
AIPS 1: Use 0 for continuum
AIPS 1: BIF 0 First IF (0=>1)
AIPS 1: EIF 0 Highest IF (0=>BIF to last)
AIPS 1: IN2NAME 'GROTHN4' Cleaned map name (name)
AIPS 1: IN2CLASS 'ICL001' Cleaned map name (class)
AIPS 1: IN2SEQ 6 Cleaned map name (seq. #)
AIPS 1: IN2DISK 1 Cleaned map disk unit #
AIPS 1: INVERS 0 CC file version #.
AIPS 1: OUTNAME ' ' Output UV file name (name)
AIPS 1: OUTCLASS ' ' Output UV file name (class)
AIPS 1: OUTSEQ 0 Output UV file name (seq. #)
AIPS 1: OUTDISK 1 Output UV file disk unit #.
AIPS 1: BCOMP *all 0 First CLEAN comp to sub.
AIPS 1: 1 per field.
AIPS 1: NCOMP *all 0 Last CLEAN comp to sub.
AIPS 1: to use (0 => all)
AIPS 1: FLUX 0 Lowest CC component used.
AIPS 1: CMETHOD ' ' Modeling method:
AIPS 1: 'DFT','GRID',' '
AIPS 1: CMODEL ' ' Model type: 'COMP','IMAG'
AIPS 1: 'SUBI' (see HELP re images)
AIPS 1: FACTOR 0 Factor times CLEAN fluxes.
AIPS 1: 0->1.0 Subtract
AIPS 1: -1.0 Add
AIPS 1: OPCODE ' ' 'DIV ' => divide visibility
AIPS 1: observation by model vis.
AIPS 1: 'MODL' => replace visibility
AIPS 1: with model visibility
AIPS 1: anything else => subtract
AIPS 1: SMODEL *all 0 Source model, 1=flux,2=x,3=y
AIPS 1: See HELP SMODEL for models.
AIPS 1: BADDISK *all 0 Disks to avoid for scratch
Cheers,
Andy
More information about the Daip
mailing list