Photometry (UV  to far-IR) and  IRAC/MIPS images are provided  for the
red 2MASS selected  QSO sample described in Georgakakis  et al. (2009,
MNRAS, in press, http://arxiv.org/abs/0812.2034).

The  multiwavelength  photometry  (UV  to  far-IR) of  PG  QSOs  (both
individual sources and  their median SED) used in  the above paper can
also be  downloaded. The  mid and  far-IR data for  PG QSOs  have been
compiled from the paper of Haas et al. (2003, A&A, 402, 87)

For any questions please email Antonis Georgakakis (age@astro.noa.gr).

TAR files:

2MASSQSO_PHOTOMETRY.TAR: photometry for the  2MASS QSOs. The ID number
of each  source in Georgakakis  et al. is  given in the  filename (see
list below).   Each file has 3  columns, (1) wavelength  (A), (2) flux
density (micro-Jy) and (3) error in flux density (micro-Jy).

ero10.photo_final 
ero11.photo_final 
ero12.photo_final 
ero2.photo_final
ero3.photo_final  
ero4.photo_final  
ero5.photo_final  
ero6.photo_final
ero7.photo_final 
ero8.photo_final


PGQSO_PHOTOMETRY.TAR:  includes photometry  for PG  QSOs  that overlap
with the SDSS  DR-6. The id of  each PG QSO is coded  in the filename.
Each  file  has  3  columns,  (1) wavelength  (A),  (2)  flux  density
(micro-Jy) and (3) error in flux density in (micro-Jy). The median SED
of the PG QSO is in the file PG_QSO_MEDIAN.SED

PG0157+001.DAT
PG1001+054.DAT
PG1008+133.DAT
PG1114+445.DAT
PG1211+143.DAT
PG1216+069.DAT
PG1226+023.DAT
PG1229+204.DAT
PG1244+026.DAT
PG1248+401.DAT
PG1309+355.DAT
PG1322+659.DAT
PG1338+416.DAT
PG1351+640.DAT
PG1352+183.DAT
PG1354+213.DAT
PG1402+261.DAT
PG1404+226.DAT
PG1407+265.DAT
PG1425+267.DAT
PG1426+015.DAT
PG1440+356.DAT
PG1444+407.DAT
PG1501+106.DAT
PG1512+370.DAT
PG1519+226.DAT
PG1543+489.DAT
PG1545+210.DAT
PG1626+554.DAT
PG1630+377.DAT
PG1704+608.DAT
PG2130+099.DAT
PG_QSO_MEDIAN.SED


2MASSQSO_IRAC_IMAGES.TAR: IRAC fits images of the 2MASS QSOs. The
science image of each IRAC channel is at 

IRAC_ERO2MASS2/ch1/pbcd/maic.fits (e.g. IRAC ch1 image of 2MASS QSO #2)


2MASSQSO_MIPS_IMAGES.TAR: MIPS fits images of the 2MASS QSOs

MIPS/EROS2MASS8_160_image.fits
MIPS/EROS2MASS7_160_image_v5-3.fits
MIPS/EROS2MASS6_24_image.fits
MIPS/EROS2MASS4_160_image_v5-3.fits
MIPS/EROS2MASS5_160_image_v7-1.fits
MIPS/EROS2MASS10_24_image_v5-3.fits
MIPS/EROS2MASS12_160_image.fits
MIPS/EROS2MASS4_70_image_v5-3.fits
MIPS/EROS2MASS2_24_image.fits
MIPS/EROS2MASS5_24_image_v7-1.fits
MIPS/EROS2MASS3_24_image.fits
MIPS/EROS2MASS10_160_image_v5-3.fits
MIPS/EROS2MASS3_160_image.fits
MIPS/EROS2MASS12_24_image.fits
MIPS/EROS2MASS11_70_image.fits
MIPS/EROS2MASS2_160_image.fits
MIPS/EROS2MASS2_70_image.fits
MIPS/EROS2MASS11_24_image.fits
MIPS/EROS2MASS12_70_image.fits
MIPS/EROS2MASS6_70_image.fits
MIPS/EROS2MASS5_70_image_v7-1.fits
MIPS/EROS2MASS3_70_image.fits
MIPS/EROS2MASS7_24_image_v5-3.fits
MIPS/EROS2MASS8_70_image.fits
MIPS/EROS2MASS8_24_image.fits
MIPS/EROS2MASS11_160_image.fits
MIPS/EROS2MASS6_160_image.fits
MIPS/EROS2MASS10_70_image_v5-3.fits
MIPS/EROS2MASS7_70_image_v5-3.fits
MIPS/EROS2MASS4_24_image_v5-3.fits