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2016A&A...596A.100P+
J/A+A/596/A100 Planck high-z source candidates catalog (PHZ) (Planck+, 2016)
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Planck intermediate results. XXXIX.
The Planck list of high-redshift source candidates.
Planck Collaboration:
Ade P.A.R., Aghanim N., Arnaud M., Aumont J., Baccigalupi C., Banday A.J.,
Barreiro R.B., Bartolo N., Battaner E., Benabed K., Benoit-Levy A.,
Bernard J.-P., Bersanelli M., Bielewicz P., Bonaldi A., Bonavera L.,
Bond J.R., Borrill J., Bouchet F.R., Boulanger F., Burigana C.,
Butler R.C., Calabrese E., Catalano A., Chiang H.C., Christensen P.R.,
Clements D.L., Colombo L.P.L., Couchot F., Coulais A., Crill B.P.,
Curto A., Cuttaia F., Danese L., Davies R.D., Davis R.J., de Bernardis P.,
de Rosa A., de Zotti G., Delabrouille J., Dickinson C., Diego J.M.,
Dole H., Dore O., Douspis M., Ducout A., Dupac X., Elsner F., Ensslin T.A.,
Eriksen H.K., Falgarone E., Finelli F., Flores-Cacho I., Frailis M.,
Fraisse A.A., Franceschi E., Galeotta S., Galli S., Ganga K., Giard M.,
Giraud-Heraud Y., Gjerlow E., Gonzalez-Nuevo J., Gorski K.M., Gregorio A.,
Gruppuso A., Gudmundsson J.E., Hansen F.K., Harrison D.L., Helou G.,
Hernandez-Monteagudo C., Herranz D., Hildebrandt S.R., Hivon E., Hobson M.,
Hornstrup A., Hovest W., Huffenberger K.M., Hurier G., Jaffe A.H.,
Jaffe T.R., Keihanen E., Keskitalo R., Kisner T.S., Kneissl R., Knoche J.,
Kunz M., Kurki-Suonio H., Lagache G., Lamarre J.-M., Lasenby A.,
Lattanzi M., Lawrence C.R., Leonardi R., Levrier F., Liguori M.,
Lilje P.B., Linden-Vornle M., Lopez-Caniego M., Lubin P.M.,
Macias-Perez J.F., Maffei B., Maggio G., Maino D., Mandolesi N.,
Mangilli A., Maris M., Martin P.G., Martinez-Gonzalez E., Masi S.,
Matarrese S., Melchiorri A., Mennella A., Migliaccio M., Mitra S.,
Miville-Deschenes M.-A., Moneti A., Montier L., Morgante G., Mortlock D.,
Munshi D., Murphy J.A., Nati F., Natoli P., Nesvadba N.P.H., Noviello F.,
Novikov D., Novikov I., Oxborrow C.A., Pagano L., Pajot F., Paoletti D.,
Partridge B., Pasian F., Pearson T.J., Perdereau O., Perotto L.,
Pettorino V., Piacentini F., Piat M., Plaszczynski S., Pointecouteau E.,
Polenta G., Pratt G.W., Prunet S., Puget J.-L., Rachen J.P., Reinecke M.,
Remazeilles M., Renault C., Renzi A., Ristorcelli I., Rocha G., Rosset C.,
Rossetti M., Roudier G., Rubino-Martin J.A., Rusholme B., Sandri M.,
Santos D., Savelainen M., Savini G., Scott D., Spencer L.D., Stolyarov V.,
Stompor R., Sudiwala R., Sunyaev R., Suur-Uski A.-S., Sygnet J.-F.,
Tauber J.A., Terenzi L., Toffolatti L., Tomasi M., Tristram M., Tucci M.,
Turler M., Umana G., Valenziano L., Valiviita J., Van Tent F., Vielva P.,
Villa F., Wade L.A., Wandelt B.D., Wehus I.K., Welikala N., Yvon D.,
Zacchei A., Zonca A.
=2016A&A...596A.100P (SIMBAD/NED BibCode)
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ADC_Keywords: Surveys ; Galaxy catalogs ; Morphology ;
Millimetric/submm sources ; Infrared sources
Keywords: catalogs - submillimeter: galaxies - galaxies: high-redshift -
galaxies: clusters: general - large-scale structure of Universe
Abstract:
The Planck mission, thanks to its large frequency range and all-sky
coverage, has a unique potential for systematically detecting the
brightest, and rarest, submillimetre sources on the sky, including
distant objects in the high-redshift Universe traced by their dust
emission. A novel method, based on a component-separation procedure
using a combination of Planck and IRAS data, has been validated and
characterized on numerous simulations, and applied to select the most
luminous cold submillimetre sources with spectral energy distributions
peaking between 353 and 857GHz at 5' resolution. A total of 2151
Planck high-z source candidates (the PHZ) have been detected in the
cleanest 26% of the sky, with flux density at 545GHz above 500mJy.
Embedded in the cosmic infrared background close to the confusion
limit, these high-z candidates exhibit colder colours than their
surroundings, consistent with redshifts z>2, assuming a dust
temperature of Txgal=35K and a spectral index of {beta}xgal=1.5.
Exhibiting extremely high luminosities, larger than 10^14^L_{sun}_,
the PHZ objects may be made of multiple galaxies or clumps at high
redshift, as suggested by a first statistical analysis based on a
comparison with number count models. Furthermore, first follow-up
observations obtained from optical to submillimetre wavelengths, which
can be found in companion papers, have confirmed that this list
consists of two distinct populations. A small fraction (around 3%) of
the sources have been identified as strongly gravitationally lensed
star-forming galaxies at redshift 2 to 4, while the vast majority of
the PHZ sources appear as overdensities of dusty star-forming
galaxies, having colours consistent with being at z>2, and may be
considered as proto-cluster candidates. The PHZ provides an original
sample, which is complementary to the Planck Sunyaev-Zeldovich
Catalogue (PSZ2); by extending the population of virialized massive
galaxy clusters detected below z<1.5 through their SZ signal to a
population of sources at z>1.5, the PHZ may contain the progenitors of
today's clusters. Hence the Planck list of high-redshift source
candidates opens a new window on the study of the early stages of
structure formation, particularly understanding the intensively
star-forming phase at high-z.
Description:
We present in this work the Planck List of Highredshift Source
Candidates (the "PHZ"), which includes 2151 sources distributed
over 26% of the sky, with redshifts likely to be greater than 2.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
phz.dat 1065 2151 Planck high-z source candidates catalog (PHZ)
phz.fits 2880 340 PHZ catalog in fits
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See also:
VIII/88 : Planck Early Release Compact Source Catalogue (Planck, 2011)
VIII/91 : Planck Catalog of Compact Sources Release 1 (Planck, 2013)
J/A+A/581/A14 : Updated Planck catalogue PSZ1 (Planck+, 2015)
Byte-by-byte Description of file: phz.dat
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Bytes Format Units Label Explanations
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1- 17 A17 --- Name Source name, PHz GLLL.ll+BB.bb (NAME)
19- 28 F10.6 deg GLON Galactic longitude based on morphology
fitting (GLON)
30- 37 F8.4 deg GLAT Galactic latitude based on morphology
fitting (GLAT)
39- 48 F10.6 deg RAdeg Right ascension (J2000) (RA)
50- 59 F10.6 deg DEdeg Declination (J2000) (DEC)
61- 68 F8.5 --- SNRX545 S/N in the 545-GHz excess map (SNR_X545)
70- 76 F7.5 --- SNRD857 S/N in the 857-GHz cleaned map (SNR_D857)
78- 85 F8.5 --- SNRD545 S/N in the 545-GHz cleaned map (SNR_D545)
87- 94 F8.5 --- SNRD353 S/N in the 353-GHz cleaned map (SNR_D353)
96- 103 F8.5 arcmin maj FWHM along the major axis of the elliptical
Gaussian (GAU_MAJOR_AXIS)
105- 112 F8.6 arcmin e_maj rms uncertainty of the FWHM along the major
axis (GAU_MAJOR_AXIS_SIG)
114- 121 F8.5 arcmin min FWHM along the minor axis of the elliptical
Gaussian (GAU_MINOR_AXIS)
123- 130 F8.6 arcmin e_min rms uncertainty of the FWHM along the minor
axis (GAU_MINOR_AXIS_SIG)
132- 139 F8.6 rad PA Position angle of the elliptical Gaussian
(GAU_POSITION_ANGLE)
141- 148 F8.6 rad e_PA rms uncertainty of the position angle
(GAU_POSITION_ANGLE_SIG)
150- 157 F8.6 Jy F857 Flux density of the source at 857 GHz
(FLUX_CLEAN_857)
159- 166 F8.6 Jy e_F857s rms uncertainty at 857 GHz due to sky
confusion (FLUX_CLEAN_857_SIG_SKY)
168- 175 F8.6 Jy e_F857d rms uncertainty at 857 GHz due to
measurement error
(FLUX_CLEAN_857_SIG_DATA)
177- 184 F8.6 Jy e_F857g rms uncertainty at 857 GHz due to
elliptical Gaussian fit accuracy
(FLUX_CLEAN_857_SIG_GEOM)
186- 193 F8.6 Jy F545 Flux density of the source at 545 GHz
(FLUX_CLEAN_545)
195- 202 F8.6 Jy e_F545s rms uncertainty at 545 GHz due to sky
confusion (FLUX_CLEAN_545_SIG_SKY)
204- 211 F8.6 Jy e_F545d rms uncertainty at 545 GHz due to
measurement error
(FLUX_CLEAN_545_SIG_DATA)
213- 220 F8.6 Jy e_F545g rms uncertainty at 545 GHz due to
elliptical Gaussian fit accuracy
(FLUX_CLEAN_545_SIG_GEOM)
222- 229 F8.6 Jy F353 Flux density of the source at 353 GHz
(FLUX_CLEAN_353)
231- 238 F8.6 Jy e_F353s rms uncertainty at 353 GHz due to sky
confusion (FLUX_CLEAN_353_SIG_SKY)
240- 247 F8.6 Jy e_F353d rms uncertainty at 353 GHz due to
measurement error
(FLUX_CLEAN_353_SIG_DATA)
249- 256 F8.6 Jy e_F353g rms uncertainty at 353 GHz due to
elliptical Gaussian fit accuracy
(FLUX_CLEAN_353_SIG_GEOM)
258- 265 F8.6 Jy F217 Flux density of the source at 217 GHz
(FLUX_CLEAN_217)
267- 274 F8.6 Jy e_F217s rms uncertainty at 217 GHz due to sky
confusion (FLUX_CLEAN_217_SIG_SKY)
276- 283 F8.6 Jy e_F217d rms uncertainty at 217 GHz due to
measurement error
(FLUX_CLEAN_217_SIG_DATA)
285- 292 F8.6 Jy e_F217g rms uncertainty at 217 GHz due to
elliptical Gaussian fit accuracy
(FLUX_CLEAN_217_SIG_GEOM)
294- 300 F7.5 --- Prob Colour-colour selection probability
(PROB_COLCOL)
302- 309 F8.6 mag E(B-V)mn Mean extinction E(B-V)xgal within the
source PSF (EBV_MEAN)
311- 319 F9.6 mag E(B-V)ap Aperture estimate of the extinction
E(B-V)xgal within the source PSF
(EBV_APER)
321- 328 F8.6 mag e_E(B-V)ap rms uncertainty of the aperture extinction
E(B-V)xgal within the source PSF
(EBV_APER_SIG)
330- 333 F4.2 --- zph25K Submm photometric redshift estimate with
Txgal=25K (ZPHOT_25K)
335- 342 F8.6 --- e_zph25K Lower limit of the 68% confidence level on
zph25K (ZPHOT_25K_LOW)
344- 351 F8.6 --- E_zph25K Upper limit of the 68% confidence level on
zph25K (ZPHOT_25K_UP)
353- 361 F9.6 --- zph25Kc2 Reduced chi2 on the best fits on zph25K
(ZPHOT_25K_CHI2)
363- 366 F4.2 --- zph30K Submm photometric redshift estimate with
Txgal=30K (ZPHOT_30K)
368- 375 F8.6 --- e_zph30K Lower limit of the 68% confidence level on
zph30K (ZPHOT_30K_LOW)
377- 384 F8.6 --- E_zph30K Upper limit of the 68% confidence level on
zph30K (ZPHOT_30K_UP)
386- 394 F9.6 --- zph30Kc2 Reduced chi2 on the best fits on zph30K
(ZPHOT_30K_CHI2)
396- 399 F4.2 --- zph35K Submm photometric redshift estimate with
Txgal=35K (ZPHOT_35K)
401- 408 F8.6 --- e_zph35K Lower limit of the 68% confidence level on
zph35K (ZPHOT_35K_LOW)
410- 417 F8.6 --- E_zph35K Upper limit of the 68% confidence level on
zph35K (ZPHOT_35K_UP)
419- 427 F9.6 --- zph35Kc2 Reduced chi2 on the best fits on zph35K
(ZPHOT_35K_CHI2)
429- 432 F4.2 --- zph40K Submm photometric redshift estimate with
Txgal=40K (ZPHOT_40K)
434- 441 F8.6 --- e_zph40K Lower limit of the 68% confidence level on
zph40K (ZPHOT_40K_LOW)
443- 450 F8.6 --- E_zph40K Upper limit of the 68% confidence level on
zph40K (ZPHOT_40K_UP)
452- 460 F9.6 --- zph40Kc2 Reduced chi2 on the best fits on zph40K
(ZPHOT_40K_CHI2)
462- 465 F4.2 --- zph45K Submm photometric redshift estimate with
Txgal=45k (ZPHOT_45K)
467- 474 F8.6 --- e_zph45K Lower limit of the 68% confidence level on
zph45K (ZPHOT_45K_LOW)
476- 483 F8.6 --- E_zph45K Upper limit of the 68% confidence level on
zph45K (ZPHOT_45K_UP)
485- 493 F9.6 --- zph45Kc2 Reduced chi2 on the best fits on zph45K
(ZPHOT_45K_CHI2)
495- 498 F4.2 --- zph50K Submm photometric redshift estimate with
Txgal=50K (ZPHOT_50K)
500- 507 F8.6 --- e_zph50K Lower limit of the 68% confidence level on
zph50K (ZPHOT_50K_LOW)
509- 516 F8.6 --- E_zph50K Upper limit of the 68% confidence level on
zph50K (ZPHOT_50K_UP)
518- 526 F9.6 --- zph50Kc2 Reduced chi2 on the best fits on zph50K
(ZPHOT_50K_CHI2)
528- 539 E12.6 Lsun LFIR25K FIR luminosity estimate with Txgal=25K
(LFIR_25K)
541- 552 E12.6 Lsun e_LFIR25K Lower limit of the 68% confidence level on
LFIR25K (LFIR_25K_LOW)
554- 565 E12.6 Lsun E_LFIR25K Upper limit of the 68% confidence level on
LFIR25K (LFIR_25K_UP)
567- 578 E12.6 Lsun LFIR30K FIR luminosity estimate with Txgal=30K
(LFIR_30K)
580- 591 E12.6 Lsun e_LFIR30K Lower limit of the 68% confidence level on
LFIR30K (LFIR_30K_LOW)
593- 604 E12.6 Lsun E_LFIR30K Upper limit of the 68% confidence level on
LFIR30K (LFIR_30K_UP)
606- 617 E12.6 Lsun LFIR35K FIR luminosity estimate with Txgal=35K
(LFIR_35K)
619- 630 E12.6 Lsun e_LFIR35K Lower limit of the 68% confidence level on
LFIR35K (LFIR_35K_LOW)
632- 643 E12.6 Lsun E_LFIR35K Upper limit of the 68% confidence level on
LFIR35K (LFIR_35K_UP)
645- 656 E12.6 Lsun LFIR40K FIR luminosity estimate with Txgal=40K
(LFIR_40K)
658- 669 E12.6 Lsun e_LFIR40K Lower limit of the 68% confidence level on
LFIR40K (LFIR_40K_LOW)
671- 682 E12.6 Lsun E_LFIR40K Upper limit of the 68% confidence level on
LFIR40K (LFIR_40K_UP)
684- 695 E12.6 Lsun LFIR45K FIR luminosity estimate with Txgal=45K
(LFIR_45K)
697- 708 E12.6 Lsun e_LFIR45K Lower limit of the 68% confidence level on
LFIR45K (LFIR_45K_LOW)
710- 721 E12.6 Lsun E_LFIR45K Upper limit of the 68% confidence level on
LFIR45K (LFIR_45K_UP)
723- 734 E12.6 Lsun LFIR50K FIR luminosity estimate with Txgal=50K
(LFIR_50K)
736- 747 E12.6 Lsun e_LFIR50K Lower limit of the 68% confidence level on
LFIR50K (LFIR_50K_LOW)
749- 760 E12.6 Lsun E_LFIR50K Upper limit of the 68% confidence level on
LFIR50K (LFIR_50K_UP)
762- 774 E13.6 Msun/yr SFR25K Star Formation Rate estimate with Txgal=25K
(SFR_25K)
776- 788 F13.6 Msun/yr e_SFR25K Lower limit of the 68% confidence level on
SFR25K (SFR_25K_LOW)
790- 802 F13.6 Msun/yr E_SFR25K Upper limit of the 68% confidence level on
SFR25K (SFR_25K_UP)
804- 816 F13.6 Msun/yr SFR30K Star Formation Rate estimate with Txgal=30K
(SFR_30K)
818- 830 F13.6 Msun/yr e_SFR30K Lower limit of the 68% confidence level on
SFR30K (SFR_30K_LOW)
832- 844 F13.6 Msun/yr E_SFR30K Upper limit of the 68% confidence level on
SFR30K (SFR_30K_UP)
846- 858 F13.6 Msun/yr SFR35K Star Formation Rate estimate with Txgal=35K
(SFR_35K)
860- 872 F13.6 Msun/yr e_SFR35K Lower limit of the 68% confidence level on
SFR35K (SFR_35K_LOW)
874- 886 F13.6 Msun/yr E_SFR35K Upper limit of the 68% confidence level on
SFR35K (SFR_35K_UP)
888- 900 F13.6 Msun/yr SFR40K Star Formation Rate estimate with Txgal=40K
(SFR_40K)
902- 914 F13.6 Msun/yr e_SFR40K Lower limit of the 68% confidence level on
SFR40K (SFR_40K_LOW)
916- 928 F13.6 Msun/yr E_SFR40K Upper limit of the 68% confidence level on
SFR40K (SFR_40K_UP)
930- 942 F13.6 Msun/yr SFR45K Star Formation Rate estimate with Txgal=45K
(SFR_45K)
944- 956 F13.6 Msun/yr e_SFR45K Lower limit of the 68% confidence level on
SFR45K (SFR_45K_LOW)
958- 970 F13.6 Msun/yr E_SFR45K Upper limit of the 68% confidence level on
SFR45K (SFR_45K_UP)
972- 984 F13.6 Msun/yr SFR50K Star Formation Rate estimate with Txgal=50K
(SFR_50K)
986- 998 F13.6 Msun/yr e_SFR50K Lower limit of the 68% confidence level on
SFR50K (SFR_50K_LOW)
1000-1012 F13.6 Msun/yr E_SFR50K Upper limit of the 68% confidence level on
SFR50K (SFR_50K_UP)
1014-1063 A50 --- Pflag Contains the list of Planck catalogues
matching the source (XFLAG_PLANCK)
1065 I1 --- Hflag [0/1] 1 if present in the Herschel
follow-up programme (XFLAG_HERSCHEL)
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Acknowledgements:
Copied at http://pla.esac.esa.int/pla/#catalogues
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(End) Patricia Vannier [CDS] 08-Dec-2016