The full HerMES Herschel-SWIRE galaxy sample discussed in Rowan-Robinson et al 2016 (MNRAS 461, 1100) is located at

http://www.mattiavaccari.net/df/mrr/lockxmms1cdfsn1cathsubm.dat

A revision of the infrared template fitting and estimation of infrared luminosities, star-formation rates and dust masses has been carried out (Jan 2017), in which the normalisation is carried out using a least squares fit at 24-500 mu (previously if 8 mu flux was available, the normalisation was at 8 mu, otherwise it was at 24 mu).  This mainly affects the very highest luminosities and star-formation rates in the redshift range 2-4.  This resolves some anomalously high star-formation rate function values at the very highest star-formation rates, but has a small effect on the final star-formation rate density (see Rowan-Robinson et al, 2018, AA).

The catalogue consists of 250-350-500 mu galaxies from Lockman (857), XMM-LSS (700), ES1 (427), CDFS (109), EN1 (108), total 2201.

[The SPIRE surveys in the EN1 and CDFS areas were shallower than the other areas and were not included in the analysis of Rowan-Robinson et al 2016]

The format is 

          write(7,138)nidir,nidopt,ra,dec,s36,s45,s58,s8,s24,err36,
     1  err45,err58,
     1  err8,err24,am1,am2,am3,am4,am5,em1,em2,em3,em4,
     2  em5,am21,am22,am23,am25,am26,em21,em22,em23,em25,em26,
     3  am6,am7,am8,em6,em7,em8,
     1  m1,m2,m3,m4,m5,mst,j1,alz,err0,n91,j2,alz2,av1,err1,alb,
     2  spectz0,nflk1,
     1  nir,alp1,alp2,alp3,alp4,alp5,alp6,errir3,alcirr,alsb,alagn,
     7  ala220,alysb,alosb,alir,nirtem
     8  ,als70,als160,als350,als450,als850,als1250
     1   ,ra1,dec1,
     1  s250,err250,s350,err350,s500,err500,
     2  dist1,dist2
     1   ,al36,alm,sfr,almd
     1  ,zf,zcomb,alir9,ntyp,chi
c
138     format(2i8,2f10.5,10f10.2,26f7.2,6i4,i3,f6.3,f10.3,
     1  2i3,f6.3,f5.2,f10.3,f7.2,
     1  f8.4,i6,
     3  3x,i3,6f6.2,2x,f9.5,2x,6f7.2,
     5  2x,f7.2,i4,3x,6f6.2,
     7  5x,2f12.6,6f9.3,3x,2f8.3,
     1  3x,4f7.2,5x,3f8.3,i6,f8.3)
c
[for explanation of these quantities, see http://www.mattiavaccari.net/df/mrr/readmeSWIRErev
zf is the subm redshift, estimated from 250-500 mu data, zcomb is the redshift estimated from the combined submillimetre and SWIRE-photz chi^2, alir9 is the infrared luminosity from the subm redshift fit, ntyp is the template type for the best subm redshift, chi is the chi^2 for the subm fit (see RR et al 2016 for details of the subm z fit) ]

A catalogue of 275 lensing candidates in the same areas (Lockman 109, XMM 84, ES1 54, CDFS 20, EN1 8) is located at

http://www.mattiavaccari.net/df/mrr/lockxmms1cdfsn1lenscatsubm.dat

with the same format.  The numbers differ slightly from those given in Table 1 of RR et al 2016 partly because of the reprocessing
described above, and because the detailed sed modelling carried out for Lockman in Rowan-Robinson et al 2014 (MN 444, 3848) has
now been extended to the other areas.

A catalogue of 833 Lockman (369), XMM-LSS (205), and ES1 (259) SPIRE sources which were not associated with SWIRE galaxies is located at

http://www.mattiavaccari.net/df/mrr/lockxmms1unidcat.dat

with format

        write(7,100)ra1,dec1,ra2,dec2,ra3,dec3,s250,err250,
     1  s350,err350,s500,err500
     2  ,zf,alir,ntyp,chi
c
100       format(6f12.5,6f8.2,2f8.3,i6,f8.3)

where

zf is the submm redshift estimate (see RR et al 2016)

ntyp=1 means M82 starburst selected, =2 means A220 starburst selected, =3 means young starburst selected

chi is the chi^2 for the submm redshift fit

MRR 31/10/16, revised 1/8/18