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@article{Collaboration:2016:0004-6361/201525819,
author = {Collaboration, P and Ade, PAR and Aghanim, N and Arnaud, M and Ashdown, M and Aumont, J and Baccigalupi, C and Banday, AJ and Barreiro, RB and Bartolo, N and Battaner, E and Benabed, K and Benoît, A and Benoit-Lévy, A and Bernard, J-P and Bersanelli, M and Bielewicz, P and Bonaldi, A and Bonavera, L and Bond, JR and Borrill, J and Bouchet, FR and Boulanger, F and Bucher, M and Burigana, C and Butler, RC and Calabrese, E and Catalano, A and Chamballu, A and Chiang, HC and Christensen, PR and Clements, DL and Colombi, S and Colombo, LPL and Combet, C and Couchot, F and Coulais, A and Crill, BP and Curto, A and Cuttaia, F and Danese, L and Davies, RD and Davis, RJ and Bernardis, PD and Rosa, AD and Zotti, GD and Delabrouille, J and Désert, F-X and Dickinson, C and Diego, JM and Dole, H and Donzelli, S and Doré, O and Douspis, M and Ducout, A and Dupac, X and Efstathiou, G and Elsner, F and Enßlin, TA and Eriksen, HK and Falgarone, E and Fergusson, J and Finelli, F and Forni, O and Frailis},
doi = {0004-6361/201525819},
journal = {Astronomy & Astrophysics},
title = {Planck 2015 results. XXVIII. The Planck Catalogue of Galactic Cold  Clumps},
url = {http://dx.doi.org/10.1051/0004-6361/201525819},
volume = {594},
year = {2016}
}

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TY  - JOUR
AB  - We present the Planck Catalogue of Galactic Cold Clumps (PGCC), an all-skycatalogue of Galactic cold clump candidates detected by Planck. This catalogueis the full version of the Early Cold Core (ECC) catalogue, which was madeavailable in 2011 with the Early Release Compact Source Catalogue (ERCSC) andcontained 915 high S/N sources. It is based on the Planck 48 months missiondata that are currently being released to the astronomical community. The PGCCcatalogue is an observational catalogue consisting exclusively of Galactic coldsources. The three highest Planck bands (857, 545, 353 GHz) have been combinedwith IRAS data at 3 THz to perform a multi-frequency detection of sourcescolder than their local environment. After rejection of possible extragalacticcontaminants, the PGCC catalogue contains 13188 Galactic sources spread acrossthe whole sky, i.e., from the Galactic plane to high latitudes, following thespatial distribution of the main molecular cloud complexes. The mediantemperature of PGCC sources lies between 13 and 14.5 K, depending on thequality of the flux density measurements, with a temperature ranging from 5.8to 20 K after removing sources with the 1% largest temperature estimates. Usingseven independent methods, reliable distance estimates have been obtained for5574 sources, which allows us to derive their physical properties such as theirmass, physical size, mean density and luminosity. The PGCC sources are locatedmainly in the solar neighbourhood, up to a distance of 10.5 kpc towards theGalactic centre, and range from low-mass cores to large molecular clouds.Because of this diversity and because the PGCC catalogue contains sources invery different environments, the catalogue is useful to investigate theevolution from molecular clouds to cores. Finally, the catalogue also includes54 additional sources located in the SMC and LMC.
AU  - Collaboration,P
AU  - Ade,PAR
AU  - Aghanim,N
AU  - Arnaud,M
AU  - Ashdown,M
AU  - Aumont,J
AU  - Baccigalupi,C
AU  - Banday,AJ
AU  - Barreiro,RB
AU  - Bartolo,N
AU  - Battaner,E
AU  - Benabed,K
AU  - Benoît,A
AU  - Benoit-Lévy,A
AU  - Bernard,J-P
AU  - Bersanelli,M
AU  - Bielewicz,P
AU  - Bonaldi,A
AU  - Bonavera,L
AU  - Bond,JR
AU  - Borrill,J
AU  - Bouchet,FR
AU  - Boulanger,F
AU  - Bucher,M
AU  - Burigana,C
AU  - Butler,RC
AU  - Calabrese,E
AU  - Catalano,A
AU  - Chamballu,A
AU  - Chiang,HC
AU  - Christensen,PR
AU  - Clements,DL
AU  - Colombi,S
AU  - Colombo,LPL
AU  - Combet,C
AU  - Couchot,F
AU  - Coulais,A
AU  - Crill,BP
AU  - Curto,A
AU  - Cuttaia,F
AU  - Danese,L
AU  - Davies,RD
AU  - Davis,RJ
AU  - Bernardis,PD
AU  - Rosa,AD
AU  - Zotti,GD
AU  - Delabrouille,J
AU  - Désert,F-X
AU  - Dickinson,C
AU  - Diego,JM
AU  - Dole,H
AU  - Donzelli,S
AU  - Doré,O
AU  - Douspis,M
AU  - Ducout,A
AU  - Dupac,X
AU  - Efstathiou,G
AU  - Elsner,F
AU  - Enßlin,TA
AU  - Eriksen,HK
AU  - Falgarone,E
AU  - Fergusson,J
AU  - Finelli,F
AU  - Forni,O
AU  - Frailis,M
AU  - Fraisse,AA
AU  - Franceschi,E
AU  - Frejsel,A
AU  - Galeotta,S
AU  - Galli,S
AU  - Ganga,K
AU  - Giard,M
AU  - Giraud-Héraud,Y
AU  - Gjerløw,E
AU  - González-Nuevo,J
AU  - Górski,KM
AU  - Gratton,S
AU  - Gregorio,A
AU  - Gruppuso,A
AU  - Gudmundsson,JE
AU  - Hansen,FK
AU  - Hanson,D
AU  - Harrison,DL
AU  - Helou,G
AU  - Henrot-Versillé,S
AU  - Hernández-Monteagudo,C
AU  - Herranz,D
AU  - Hildebrandt,SR
AU  - Hivon,E
AU  - Hobson,M
AU  - Holmes,WA
AU  - Hornstrup,A
AU  - Hovest,W
AU  - Huffenberger,KM
AU  - Hurier,G
AU  - Jaffe,AH
AU  - Jaffe,TR
AU  - Jones,WC
AU  - Juvela,M
AU  - Keihänen,E
AU  - Keskitalo,R
AU  - Kisner,TS
AU  - Knoche,J
AU  - Kunz,M
AU  - Kurki-Suonio,H
AU  - Lagache,G
AU  - Lamarre,J-M
AU  - Lasenby,A
AU  - Lattanzi,M
AU  - Lawrence,CR
AU  - Leonardi,R
AU  - Lesgourgues,J
AU  - Levrier,F
AU  - Liguori,M
AU  - Lilje,PB
AU  - Linden-Vørnle,M
AU  - López-Caniego,M
AU  - Lubin,PM
AU  - Macías-Pérez,JF
AU  - Maggio,G
AU  - Maino,D
AU  - Mandolesi,N
AU  - Mangilli,A
AU  - Marshall,DJ
AU  - Martin,PG
AU  - Martínez-González,E
AU  - Masi,S
AU  - Matarrese,S
AU  - Mazzotta,P
AU  - McGehee,P
AU  - Melchiorri,A
AU  - Mendes,L
AU  - Mennella,A
AU  - Migliaccio,M
AU  - Mitra,S
AU  - Miville-Deschênes,M-A
AU  - Moneti,A
AU  - Montier,L
AU  - Morgante,G
AU  - Mortlock,D
AU  - Moss,A
AU  - Munshi,D
AU  - Murphy,JA
AU  - Naselsky,P
AU  - Nati,F
AU  - Natoli,P
AU  - Netterfield,CB
AU  - Nørgaard-Nielsen,HU
AU  - Noviello,F
AU  - Novikov,D
AU  - Novikov,I
AU  - Oxborrow,CA
AU  - Paci,F
AU  - Pagano,L
AU  - Pajot,F
AU  - Paladini,R
AU  - Paoletti,D
AU  - Pasian,F
AU  - Patanchon,G
AU  - Pearson,TJ
AU  - Pelkonen,V-M
AU  - Perdereau,O
AU  - Perotto,L
AU  - Perrotta,F
AU  - Pettorino,V
AU  - Piacentini,F
AU  - Piat,M
AU  - Pierpaoli,E
DO  - 0004-6361/201525819
PY  - 2016///
SN  - 1432-0746
TI  - Planck 2015 results. XXVIII. The Planck Catalogue of Galactic Cold  Clumps
T2  - Astronomy & Astrophysics
UR  - http://dx.doi.org/10.1051/0004-6361/201525819
UR  - http://hdl.handle.net/10044/1/29628
VL  - 594
ER  -

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