J/ApJ/857/64  Multiwavelength catalog in the SEP field. II. (Baronchelli+, 2018)
The Spitzer-IRAC/MIPS Extragalactic Survey (SIMES).
II. Enhanced nuclear accretion rate in galaxy groups at z ∼ 0.2.
    Baronchelli I., Rodighiero G., Teplitz H.I., Scarlata C.M.,
    Franceschini A., Berta S., Barrufet L., Vaccari M., Bonato M., Ciesla L.,
    Zanella A., Carraro R., Mancini C., Puglisi A., Malkan M., Mei S.,
    Marchetti L., Colbert J., Sedgwick C., Serjeant S., Pearson C.,
    Radovich M., Grado A., Limatola L., Covone G.
   <Astrophys. J., 857, 64-64 (2018)>
   =2018ApJ...857...64B    (SIMBAD/NED BibCode)
ADC_Keywords: Surveys ; Galaxies, photometry ;  Photometry, infrared ;
              Photometry, millimetric/submm ; Photometry, ultraviolet ;
              Photometry, SDSS ; Photometry, UBVRI
Keywords: galaxies: evolution - galaxies: groups: general -
          galaxies: star formation - infrared: galaxies -
          quasars: supermassive black holes - submillimeter: galaxies

Abstract:
    For a sample of star-forming galaxies in the redshift interval
    0.15<z<0.3, we study how both the relative strength of the active
    galactic nucleus (AGN) infrared emission, compared to that due to the
    star formation (SF), and the numerical fraction of AGNs change as a
    function of the total stellar mass of the hosting galaxy group
    (Mgroup*) between 1010.25 and 1011.9M☉. Using a
    multicomponent spectral energy distribution SED fitting analysis, we
    separate the contribution of stars, AGN torus, and star formation to
    the total emission at different wavelengths. This technique is applied
    to a new multiwavelength data set in the SIMES field (23 not-redundant
    photometric bands), spanning the wavelength range from the UV (GALEX)
    to the far-IR (Herschel) and including crucial AKARI and WISE mid-IR
    observations (4.5µm<λ<24µm), where the black hole thermal
    emission is stronger. This new photometric catalog, which includes our
    best photo-z estimates, is released through the NASA/IPAC Infrared
    Science Archive (IRSA). Groups are identified through a
    friends-of-friends algorithm (∼62% purity, ∼51% completeness). We
    identified a total of 45 galaxies requiring an AGN emission component,
    35 of which are in groups and 10 in the field. We find the black hole
    accretion rate (BHAR)∝(Mgroup*)1.21±0.27 and
    (BHAR/SFR) ∝ (Mgroup*)^1.04± 0.24^, while, in the same
    range of Mgroup*, we do not observe any sensible change in the
    numerical fraction of AGNs. Our results indicate that the nuclear
    activity (i.e., the BHAR and the BHAR/SFR ratio) is enhanced when
    galaxies are located in more massive and richer groups.

Description:
    The Spitzer-IRAC/MIPS Extragalactic survey (SIMES) in the South
    Ecliptic Pole field (SEP) covers an area of 7.74 sq. deg to a depth of
    ∼5.80 microJy (3sigma) at 3.6 microns and 5.25 microJy at 4.5 microns.
    The 90% and 50% completeness limits are at 14 and 9 microJy,
    respectively. The multiwavelength catalog includes the WFI-Rc, MIPS-24
    micron, SPIRE 250, 350 and 500 micron fluxes of the counterparts that
    were identified by searching for the closest neighbor.

    The indicator P quantifies the reliability of each association
    (example, for P1: SPIRE to MIPS) considering both the distance between
    the SPIRE source and the closest MIPS association and the presence of
    further possible MIPS associations in the MIPS-SPIRE searching radius.

    For bands other than IRAC 3.6 microns, a null flux means no coverage
    in that band, while a flux of zero means that the position is covered
    in that band but the source is not detected.

File Summary:

       FileName      Lrecl  Records   Explanations

ReadMe            80        .   This file
catalog.dat     1875   341066   SEP multiwavelength photometric catalog


See also:
    J/ApJS/223/1 : Multiwavelength catalog in the SEP field (Baronchelli+, 2016)


Byte-by-byte Description of file: catalog.dat

   Bytes Format Units   Label      Explanations

   1-  6  I6    ---     ID         ID number (ID)
   8- 24 F17.14 deg     RAdeg      Right Ascension (J2000) of IRAC 3.6 micron
                                       source (ra)
  26- 44 F19.15 deg     DEdeg      Declination (J2000) of IRAC 3.6 micron
                                       source (dec)
  46- 56  F11.7 ---     zph        ?=-99 Photometric redshift (PHOTO_Z)
  58- 70  F13.9 ---     e_zph      ?=-99 Photometric redshift uncertainty
                                       (PHOTOZERR)
  72- 83  E12.7 mJy     F3.6       ?=-99 IRAC 3.6 micron total flux (FLUX_I1)
  85- 96  E12.7 mJy     e_F3.6     ?=-99 IRAC 3.6 micron total flux
                                       uncertainty (FLUXERR_I1)
  98-110  F13.7 ---     S/N        ?=-99 IRAC 3.6 micron signal to noise
                                       ratio (N_SIGMA)
 112-124  E13.8 mJy     F4.5       ?=-99 IRAC 4.5 micron total flux (FLUX_I2)
 126-138  E13.8 mJy     e_F4.5     ?=-99 IRAC 4.5 micron total flux
                                       uncertainty (FLUXERR_I2)
 140-157 F18.14 deg     RA24degC   ?=-99 Corrected RA of 24 micron sources
                                       (RA_24)
 159-177 F19.15 deg     DE24degC   ?=-99 Corrected Dec of 24 micron sources
                                       (DEC_24)
 179-186  F8.4  deg     RA24deg    ?=-99 Original RA of 24 micron sources
                                       (ORA24)
 188-195  F8.4  deg     DE24deg    ?=-99 Original Dec of 24 micron sources
                                       (ODEC24)
 197-208  F12.8 mJy     F24        ?=-99 MIPS 24 micron flux (FLUX_24)
 210-222  F13.9 mJy     e_F24      ?=-99 MIPS 24 micron flux uncertainty
                                       (FLUXERR_24)
 224-228  F5.1  mJy     F70        ?=-99 MIPS 70 micron flux (FLUX_70)
 230-241  F12.8 mJy     e_F70      ?=-99 MIPS 70 micron flux uncertainty
                                       (FLUXERR_70)
 243-260 F18.14 deg     RASdegC    ?=-99 Corrected RA of SPIRE sources
                                       (RA_SPIRE)
 262-280 F19.15 deg     DESdegC    ?=-99 Corrected Dec of SPIRE sources
                                       (DEC_SPIRE)
 282-291  F10.6 deg     RASdeg     ?=-99 Original RA of SPIRE sources
                                       (ORASPIRE)
 293-302  F10.6 deg     DESdeg     ?=-99 Original Dec of SPIRE sources
                                       (ODECSPIRE)
 304-324 F21.17 mJy     F250       ?=-99 SPIRE 250 micron flux (FLUX_250)
 326-345 F20.16 mJy     e_F250     ?=-99 SPIRE 250 micron flux uncertainty
                                       (FLUXERR_250)
 347-367 F21.17 mJy     F350       ?=-99 SPIRE 350 micron flux (FLUX_350)
 369-388 F20.16 mJy     e_F350     ?=-99 SPIRE 350 micron flux uncertainty
                                       (FLUXERR_350)
 390-411 F22.18 mJy     F500       ?=-99 SPIRE 500 micron flux (FLUX_500)
 413-432 F20.16 mJy     e_F500     ?=-99 SPIRE 500 micron flux uncertainty
                                       (FLUXERR_500)
 434-451 F18.14 deg     RAGdegC    ?=-99 Corrected RA of GALEX sources
                                       (RA_GALEX)
 453-471 F19.15 deg     DEGdegC    ?=-99 Corrected Dec of GALEX sources
                                       (DEC_GALEX)
 473-482  F10.6 deg     RAGdeg     ?=-99 Original RA of GALEX sources
                                       (ORAGALEX)
 484-493  F10.6 deg     DEGdeg     ?=-99 Original Dec of GALEX sources
                                       (ODECGALEX)
 495-508 F14.10 mJy     FFUV       ?=-99 GALEX FUV flux (FLUXFUVGALEX)
 510-521  E12.7 mJy     e_FFUV     ?=-99 GALEX FUV flux uncertainty
                                       (FLUXERRFUVGALEX)
 523-536 F14.10 mJy     FNUV       ?=-99 GALEX NUV flux (FLUXNUVGALEX)
 538-549  E12.7 mJy     e_FNUV     ?=-99 GALEX NUV flux uncertainty
                                       (FLUXERRNUVGALEX)
 551-559  F9.5  deg     RAOdeg     ?=-99 average RA for optical sources
                                       (RA_OPT)
 561-569  F9.5  deg     DEOdeg     ?=-99 average Dec for optical sources
                                       (DEC_OPT)
 571-580  F10.6 mJy     Fuctio     ?=-99 CTIO u-band flux (FLUX_U)
 582-592  E11.6 mJy     e_Fuctio   ?=-99 CTIO u-band flux uncertainty
                                       (FLUXERR_U)
 594-603  F10.6 mJy     FBctio     ?=-99 CTIO B-band flux (FLUX_B)
 605-615  E11.6 mJy     e_FBctio   ?=-99 CTIO B-band flux uncertainty
                                       (FLUXERR_B)
 617-626  F10.6 mJy     FVctio     ?=-99 CTIO V-band flux (FLUX_V)
 628-638  E11.6 mJy     e_FVctio   ?=-99 CTIO V-band flux uncertainty
                                       (FLUXERR_V)
 640-649  F10.6 mJy     FIctio     ?=-99 CTIO I-band flux (FLUX_I)
 651-661  E11.6 mJy     e_FIctio   ?=-99 CTIO I-band flux uncertainty
                                       (FLUXERR_I)
 663-674  E12.7 mJy     FRcwfi     ?=-99 WFI Rc-band flux (FLUXRWFI)
 676-688  E13.8 mJy     e_FRcwfi   ?=-99 WFI Rc-band flux uncertainty
                                       (FLUXERRRWFI)
 690-701  E12.7 mJy     Fgvst      ?=-99 VST g-band flux (FLUXGVST)
 703-715  E13.8 mJy     e_Fgvst    ?=-99 VST g-band flux uncertainty
                                       (FLUXERRGVST)
 717-728  E12.7 mJy     Fivst      ?=-99 VST i-band flux (FLUXIVST)
 730-742  E13.8 mJy     e_Fivst    ?=-99 VST i-band flux uncertainty
                                       (FLUXERRIVST)
 744-755  E12.7 mJy     Fzvst      ?=-99 VST z-band flux (FLUXZVST)
 757-768  E12.7 mJy     e_Fzvst    ?=-99 VST z-band flux uncertainty
                                       (FLUXERRZVST)
 770-787 F18.14 deg     RAVdegC    ?=-99 Corrected RA of VISTA sources
                                       (RA_VISTA)
 789-807 F19.15 deg     DEVdegC    ?=-99 Corrected Dec of VISTA sources
                                       (DEC_VISTA)
 809-826 F18.14 deg     RAVdeg     ?=-99 Original RA of VISTA sources
                                       (ORAVISTA)
 828-846 F19.15 deg     DEVdeg     ?=-99 Original Dec of VISTA sources
                                       (ODECVISTA)
 848-859  E12.7 mJy     FJvista    ?=-99 VISTA J-band flux (FLUXJVISTA)
 861-872  E12.7 mJy     e_FJvista  ?=-99 VISTA J-band flux uncertainty
                                       (FLUXERRJVISTA)
 874-885  E12.7 mJy     FHvista    ?=-99 VISTA H-band flux (FLUXHVISTA)
 887-898  E12.7 mJy     e_FHvista  ?=-99 VISTA H-band flux uncertainty
                                       (FLUXERRHVISTA)
 900-911  E12.7 mJy     FKsvista   ?=-99 VISTA Ks-band flux (FLUXKSVISTA)
 913-924  E12.7 mJy    e_FKsvista  ?=-99 VISTA Ks-band flux uncertainty
                                       (FLUXERRKSVISTA)
 926-943 F18.14 deg     RAWdegC    ?=-99 Corrected RA of WISE sources (RA_W)
 945-963 F19.15 deg     DEWdegC    ?=-99 Corrected Dec of WISE sources
                                       (DEC_W)
 965-975  F11.7 deg     RAWdeg     ?=-99 Original RA of WISE sources (ORAW)
 977-987  F11.7 deg     DEWdeg     ?=-99 Original Dec of WISE sources
                                       (ODECW)
 989-1012 F24.19 mJy     FW1        ?=-99 WISE W1 flux (FLUX_W1)
 1014-1036 F23.19 mJy     e_FW1      ?=-99 WISE W1 flux uncertainty
                                       (FLUXERR_W1)
 1038-1060 F23.19 mJy     FW2        ?=-99 WISE W2 flux (FLUX_W2)
 1062-1084 F23.19 mJy     e_FW2      ?=-99 WISE W2 flux uncertainty
                                       (FLUXERR_W2)
 1086-1106 F21.17 mJy     FW3        ?=-99 WISE W3 flux (FLUX_W3)
 1108-1129 F22.18 mJy     e_FW3      ?=-99 WISE W3 flux uncertainty
                                       (FLUXERR_W3)
 1131-1150 F20.16 mJy     FW4        ?=-99 WISE W4 flux (FLUX_W4)
 1152-1172 F21.17 mJy     e_FW4      ?=-99 WISE W4 flux uncertainty
                                       (FLUXERR_W4)
 1174-1182  F9.5  deg     RAN3degC   ?=-99 Corrected RA of AKARI N3 sources
                                       (RA_N3)
 1184-1191  F8.4  deg     DEN3degC   ?=-99 Corrected Dec of AKARI N3 sources
                                       (DEC_N3)
 1193-1202  F10.6 deg     RAN3deg    ?=-99 Original RA of AKARI N3 sources
                                       (ORAN3)
 1204-1213  F10.6 deg     DEN3deg    ?=-99 Original Dec of AKARI N3 sources
                                       (ODECN3)
 1215-1225  F11.7 mJy     FN3        ?=-99 AKARI N3 flux (FLUX_N3)
 1227-1238  E12.7 mJy     e_FN3      ?=-99 AKARI N3 flux uncertainty
                                       (FLUXERR_N3)
 1240-1248  F9.5  deg     RAN4degC   ?=-99 Corrected RA of AKARI N4 sources
                                       (RA_N4)
 1250-1257  F8.4  deg     DEN4degC   ?=-99 Corrected Dec of AKARI N4 sources
                                       (DEC_N4)
 1259-1268  F10.6 deg     RAN4deg    ?=-99 Original RA of AKARI N4 sources
                                       (ORAN4)
 1270-1279  F10.6 deg     DEN4deg    ?=-99 Original Dec of AKARI N4 sources
                                       (ODECN4)
 1281-1291  F11.7 mJy     FN4        ?=-99 AKARI N4 flux (FLUX_N4)
 1293-1304  E12.7 mJy     e_FN4      ?=-99 AKARI N4 flux uncertainty
                                       (FLUXERR_N4)
 1306-1314  F9.5  deg     RAS7degC   ?=-99 Corrected RA of AKARI S7 sources
                                       (RA_S7)
 1316-1323  F8.4  deg     DES7degC   ?=-99 Corrected Dec of AKARI S7 sources
                                       (DEC_S7)
 1325-1334  F10.6 deg     RAS7deg    ?=-99 Original RA of AKARI S7 sources
                                       (ORAS7)
 1336-1345  F10.6 deg     DES7deg    ?=-99 Original Dec of AKARI S7 sources
                                       (ODECS7)
 1347-1357  F11.7 mJy     FS7        ?=-99 AKARI S7 flux (FLUX_S7)
 1359-1372 F14.10 mJy     e_FS7      ?=-99 AKARI S7 flux uncertainty
                                       (FLUXERR_S7)
 1374-1382  F9.5  deg     RAS11degC  ?=-99 Corrected RA of AKARI S11 sources
                                       (RA_S11)
 1384-1392  F9.5  deg     DES11degC  ?=-99 Corrected Dec of AKARI S11 sources
                                       (DEC_S11)
 1394-1404  F11.7 deg     RAS11deg   ?=-99 Original RA of AKARI S11 sources
                                       (ORAS11)
 1406-1416  F11.7 deg     DES11deg   ?=-99 Original Dec of AKARI S11 sources
                                       (ODECS11)
 1418-1429  F12.8 mJy     FS11       ?=-99 AKARI S11 flux (FLUX_S11)
 1431-1444 F14.10 mJy     e_FS11     ?=-99 AKARI S11 flux uncertainty
                                       (FLUXERR_S11)
 1446-1454  F9.5  deg     RAL15degC  ?=-99 Corrected RA of AKARI L15 sources
                                       (RA_L15)
 1456-1464  F9.5  deg     DEL15degC  ?=-99 Corrected Dec of AKARI L15 sources
                                       (DEC_L15)
 1466-1476  F11.7 deg     RAL15deg   ?=-99 Original RA of AKARI L15 sources
                                       (ORAL15)
 1478-1488  F11.7 deg     DEL15deg   ?=-99 Original Dec of AKARI L15 sources
                                       (ODECL15)
 1490-1501  F12.8 mJy     FL15       ?=-99 AKARI L15 flux (FLUX_L15)
 1503-1516 F14.10 mJy     e_FL15     ?=-99 AKARI L15 flux uncertainty
                                       (FLUXERR_L15)
 1518-1526  F9.5  deg     RAL24degC  ?=-99 Corrected RA of AKARI L24 sources
                                       (RA_L24)
 1528-1536  F9.5  deg     DEL24degC  ?=-99 Corrected Dec of AKARI L24 sources
                                       (DEC_L24)
 1538-1548  F11.7 deg     RAL24deg   ?=-99 Original RA of AKARI L24 sources
                                       (ORAL24)
 1550-1560  F11.7 deg     DEL24deg   ?=-99 Original Dec of AKARI L24 sources
                                       (ODECL24)
 1562-1573  F12.8 mJy     FL24       ?=-99 AKARI L24 flux (FLUX_L24)
 1575-1587  F13.9 mJy     e_FL24     ?=-99 AKARI L24 flux uncertainty
                                       (FLUXERR_L24)
 1589-1600  F12.8 ---     P1         ?=-99 SPIRE-MIPS reliability
                                       indicator (P1)
 1602-1604  I3    ---     NM-S       [0/3]?=-99 Number of MIPS counterparts
                                       for SPIRE source (NMIPSSPIRE)
 1606-1617  F12.8 ---     P2         ?=-99 MIPS-IRAC reliability
                                       indicator (P2)
 1619-1621  I3    ---     NI-M       [1/2]?=-99 Number of IRAC counterparts
                                       for MIPS source (NIRACMIPS)
 1623-1635  F13.9 ---     P3         ?=-99 SPIRE-IRAC reliability
                                       indicator (P3)
 1637-1639  I3    ---     NI-S       [1/5]?=-99 Number of IRAC counterparts
                                       for SPIRE
                                       source (NIRACSPIRE)
 1641-1653  E13.8 ---     S/G        SExtractor CLASS_STAR parameter at
                                       IRAC 3.6 micron (CLASSSTARI1)
 1655-1665  F11.8 arcsec  amaj       ?=0 Semi-major axis (A_I1)
 1667-1677  F11.8 arcsec  bmin       ?=0 Semi-minor axis (B_I1)
 1679-1692 F14.10 mJy     Sigma      IRAC 3.6 micron sky sigma (SIGMA)
 1694-1705  E12.7 ---     Cov        Average coverage (COVERAGE)
 1706-1719 F14.10 mJy     F3.6a1     ?=-99 IRAC 3.6 micron aperture flux - 4.8"
                                       (AP1FLUXI1)
 1721-1732  E12.7 mJy     e_F3.6a1   ?=-99 uncertainty in AP1FLUXI1
                                       (AP1FLUXERRI1)
 1734-1746  E13.8 mJy     F3.6a2     ?=-99 IRAC 3.6 micron aperture flux - 7.2"
                                       (AP2FLUXI1)
 1748-1759  E12.7 mJy     e_F3.6a2   ?=-99 uncertainty in AP2FLUXI1
                                       (AP2FLUXERRI1)
 1761-1774  E14.9 mJy     F3.6a3     ?=-99 IRAC 3.6 micron aperture flux - 12"
                                       (AP3FLUXI1)
 1776-1788 F13.10 mJy     e_F3.6a3   uncertainty in AP3FLUXI1
                                       (AP3FLUXERRI1)
 1790-1803  E14.9 mJy     F4.5a1     ?=-99 IRAC 4.5 micron aperture flux - 4.8"
                                       (AP1FLUXI2)
 1805-1817  E13.8 mJy     e_F4.5a1   ?=-99 uncertainty in AP1FLUXI2
                                       (AP1FLUXERRI2)
 1819-1832  E14.9 mJy     F4.5a2     ?=-99 IRAC 4.5 micron aperture flux - 7.2"
                                       (AP2FLUXI2)
 1834-1846  E13.8 mJy     e_F4.5a2   ?=-99 uncertainty in AP2FLUXI2
                                       (AP2FLUXERRI2)
 1848-1861  E14.9 mJy     F4.5a3     ?=-99 IRAC 4.5 micron aperture flux - 12"
                                       (AP3FLUXI2)
 1863-1875  E13.8 mJy     e_F4.5a3   ?=-99 uncertainty in AP3FLUXI2
                                       (AP3FLUXERRI2)


History:
 Copied at
 https://irsa.ipac.caltech.edu/data/SPITZER/SEP/catalogs/SEP_catalog8.0_mJy.tbl