README  

Possible barlens targets

BL_CANDIDATES    primary barlens candidates
		 pdf's for individual galaxies +
		 all collected to a single file (bl_candidates.pdf)

OTHERS           other barlens galaxies
		 pdf's for individual galaxies +
		 all collected to a single file (bl_others.pdf)
                 
KPC              All 68 barlens galaxies 
                 collected to single file (weave_chart1_bl_kpc.pdf)
                 The frame size is fixed to 20*20 kpc.                  


Each figure shows the clipped S4G 3.6 micron image, with the Weave FoV
indicated by the green hexagon. The insert figure shows 4 times larger
region, with the red squares indicated the sky fibre locations.  The
numbers in the right indicate 
- log(M_stellar) from S4G Pipeline 3 
- Ron Buta's classification from 3.6 micron 
- Ron's numeric bar type (0-no bar, 1 clear SB) 
- galaxy inclination (S4G Pipeline 4, from outer isophotes) 
- galaxy position angle (-"-) 
- b-band magnitude (HyperLeda, as used in S4G sample selection) 
- 25 magnitude/arcec^2 isophotal radius (Hyperleda)

The galaxies are orderer according to increasing stellar mass.  Most
of them are fairly face-on. However, also some more inclined galaxies
are included, if they appear otherwise interesting (same concerns same
cases where the sky fibre locations would be only marginally outside
the disk).