Planck intermediate results: XXXIX. The Planck list of high-redshift source candidates
The <i>Planck<i/> 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 n...
Gespeichert in:
| Hauptverfasser: | , |
|---|---|
| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
12 December 2016
|
| In: |
Astronomy and astrophysics
Year: 2016, Jahrgang: 596, Pages: 1-28 |
| ISSN: | 1432-0746 |
| DOI: | 10.1051/0004-6361/201527206 |
| Online-Zugang: | Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1051/0004-6361/201527206 Verlag, lizenzpflichtig, Volltext: https://www.aanda.org/articles/aa/abs/2016/12/aa27206-15/aa27206-15.html 
|
| Verfasserangaben: | Planck Collaboration: P.A.R. Ade, N. Aghanim, M. Arnaud, J. Aumont, C. Baccigalupi, A.J. Banday, R. B. Barreiro, N. Bartolo, E. Battaner, K. Benabed, A. Benoit-Lévy, J.-P. Bernard, M. Bersanelli, P. Bielewicz, A. Bonaldi, L. Bonavera, J.R. Bond, J. Borrill, F.R. Bouchet, F. Boulanger, C. Burigana, R.C. Butler, E. Calabrese, A. Catalano, H.C. Chiang, P.R. Christensen, D.L. Clements, L.P.L. Colombo, F. Couchot, A. Coulais, B.P. Crill, A. Curto, F. Cuttaia, L. Danese, R.D. Davies, R.J. Davis, P. de Bernardis, A. de Rosa, G. de Zotti, J. Delabrouille, C. Dickinson, J.M. Diego, H. Dole, O. Doré, M. Douspis, A. Ducout, X. Dupac, F. Elsner, T.A. Enßlin, H.K. Eriksen, E. Falgarone, F. Finelli, I. Flores-Cacho, M. Frailis, A.A. Fraisse, E. Franceschi, S. Galeotta, S. Galli, K. Ganga, M. Giard, Y. Giraud-Héraud, E. Gjerløw, J. González-Nuevo, K.M. Górski, A. Gregorio, A. Gruppuso, J.E. Gudmundsson, F.K. Hansen, D.L. Harrison, G. Helou, C. Hernández-Monteagudo, D. Herranz, S.R. Hildebrandt, E. Hivon, M. Hobson, A. Hornstrup, W. Hovest, K.M. Huffenberger, G. Hurier, A.H. Jaffe, T.R. Jaffe, E. Keihänen, R. Keskitalo, T.S. Kisner, R. Kneissl, J. Knoche, M. Kunz, H. Kurki-Suonio, G. Lagache, J.-M. Lamarre, A. Lasenby, M. Lattanzi, C.R. Lawrence, R. Leonardi, F. Levrier, M. Liguori, P.B. Lilje, M. Linden-Vørnle, M. López-Caniego, P.M. Lubin, J.F. Macías-Pérez, B. Maffei, G. Maggio, D. Maino, N. Mandolesi, A. Mangilli, M. Maris, P. G. Martin, E. Martínez-González, S. Masi, S. Matarrese, A. Melchiorri, A. Mennella, M. Migliaccio, S. Mitra, M.-A. Miville-Deschênes, A. Moneti, L. Montier, G. Morgante, D. Mortlock, D. Munshi, J.A. Murphy, F. Nati, P. Natoli, N.P.H. Nesvadba, F. Noviello, D. Novikov, I. Novikov, C.A. Oxborrow, L. Pagano, F. Pajot, D. Paoletti, B. Partridge, F. Pasian, T.J. Pearson, O. Perdereau, L. Perotto, V. Pettorino, F. Piacentini, M. Piat, S. Plaszczynski, E. Pointecouteau, G. Polenta, G.W. Pratt, S. Prunet, J.-L. Puget, J.P. Rachen, M. Reinecke, M. Remazeilles, C. Renault, A. Renzi, I. Ristorcelli, G. Rocha, C. Rosset, M. Rossetti, G. Roudier, J.A. Rubiño-Martín, B. Rusholme, M. Sandri, D. Santos, M. Savelainen, G. Savini, D. Scott, L. D. Spencer, V. Stolyarov, R. Stompor, R. Sudiwala, R. Sunyaev, A.-S. Suur-Uski, J.-F. Sygnet, J.A. Tauber, L. Terenzi, L. Toffolatti, M. Tomasi, M. Tristram, M. Tucci, M. Türler, G. Umana, L. Valenziano, J. Valiviita, F. Van Tent, P. Vielva, F. Villa, L.A. Wade, B.D. Wandelt, I.K. Wehus, N. Welikala, D. Yvon, A. Zacchei, and A. Zonca |
MARC
| LEADER | 00000caa a2200000 c 4500 | ||
|---|---|---|---|
| 001 | 1726592537 | ||
| 003 | DE-627 | ||
| 005 | 20220818171220.0 | ||
| 007 | cr uuu---uuuuu | ||
| 008 | 200806s2016 xx |||||o 00| ||eng c | ||
| 024 | 7 | |a 10.1051/0004-6361/201527206 |2 doi | |
| 035 | |a (DE-627)1726592537 | ||
| 035 | |a (DE-599)KXP1726592537 | ||
| 035 | |a (OCoLC)1341352202 | ||
| 040 | |a DE-627 |b ger |c DE-627 |e rda | ||
| 041 | |a eng | ||
| 084 | |a 29 |2 sdnb | ||
| 100 | 1 | |a Ade, Peter A. |e VerfasserIn |0 (DE-588)1139847449 |0 (DE-627)897714911 |0 (DE-576)427743273 |4 aut | |
| 245 | 1 | 0 | |a Planck intermediate results |b XXXIX. The Planck list of high-redshift source candidates |c Planck Collaboration: P.A.R. Ade, N. Aghanim, M. Arnaud, J. Aumont, C. Baccigalupi, A.J. Banday, R. B. Barreiro, N. Bartolo, E. Battaner, K. Benabed, A. Benoit-Lévy, J.-P. Bernard, M. Bersanelli, P. Bielewicz, A. Bonaldi, L. Bonavera, J.R. Bond, J. Borrill, F.R. Bouchet, F. Boulanger, C. Burigana, R.C. Butler, E. Calabrese, A. Catalano, H.C. Chiang, P.R. Christensen, D.L. Clements, L.P.L. Colombo, F. Couchot, A. Coulais, B.P. Crill, A. Curto, F. Cuttaia, L. Danese, R.D. Davies, R.J. Davis, P. de Bernardis, A. de Rosa, G. de Zotti, J. Delabrouille, C. Dickinson, J.M. Diego, H. Dole, O. Doré, M. Douspis, A. Ducout, X. Dupac, F. Elsner, T.A. Enßlin, H.K. Eriksen, E. Falgarone, F. Finelli, I. Flores-Cacho, M. Frailis, A.A. Fraisse, E. Franceschi, S. Galeotta, S. Galli, K. Ganga, M. Giard, Y. Giraud-Héraud, E. Gjerløw, J. González-Nuevo, K.M. Górski, A. Gregorio, A. Gruppuso, J.E. Gudmundsson, F.K. Hansen, D.L. Harrison, G. Helou, C. Hernández-Monteagudo, D. Herranz, S.R. Hildebrandt, E. Hivon, M. Hobson, A. Hornstrup, W. Hovest, K.M. Huffenberger, G. Hurier, A.H. Jaffe, T.R. Jaffe, E. Keihänen, R. Keskitalo, T.S. Kisner, R. Kneissl, J. Knoche, M. Kunz, H. Kurki-Suonio, G. Lagache, J.-M. Lamarre, A. Lasenby, M. Lattanzi, C.R. Lawrence, R. Leonardi, F. Levrier, M. Liguori, P.B. Lilje, M. Linden-Vørnle, M. López-Caniego, P.M. Lubin, J.F. Macías-Pérez, B. Maffei, G. Maggio, D. Maino, N. Mandolesi, A. Mangilli, M. Maris, P. G. Martin, E. Martínez-González, S. Masi, S. Matarrese, A. Melchiorri, A. Mennella, M. Migliaccio, S. Mitra, M.-A. Miville-Deschênes, A. Moneti, L. Montier, G. Morgante, D. Mortlock, D. Munshi, J.A. Murphy, F. Nati, P. Natoli, N.P.H. Nesvadba, F. Noviello, D. Novikov, I. Novikov, C.A. Oxborrow, L. Pagano, F. Pajot, D. Paoletti, B. Partridge, F. Pasian, T.J. Pearson, O. Perdereau, L. Perotto, V. Pettorino, F. Piacentini, M. Piat, S. Plaszczynski, E. Pointecouteau, G. Polenta, G.W. Pratt, S. Prunet, J.-L. Puget, J.P. Rachen, M. Reinecke, M. Remazeilles, C. Renault, A. Renzi, I. Ristorcelli, G. Rocha, C. Rosset, M. Rossetti, G. Roudier, J.A. Rubiño-Martín, B. Rusholme, M. Sandri, D. Santos, M. Savelainen, G. Savini, D. Scott, L. D. Spencer, V. Stolyarov, R. Stompor, R. Sudiwala, R. Sunyaev, A.-S. Suur-Uski, J.-F. Sygnet, J.A. Tauber, L. Terenzi, L. Toffolatti, M. Tomasi, M. Tristram, M. Tucci, M. Türler, G. Umana, L. Valenziano, J. Valiviita, F. Van Tent, P. Vielva, F. Villa, L.A. Wade, B.D. Wandelt, I.K. Wehus, N. Welikala, D. Yvon, A. Zacchei, and A. Zonca |
| 264 | 1 | |c 12 December 2016 | |
| 300 | |a 28 | ||
| 336 | |a Text |b txt |2 rdacontent | ||
| 337 | |a Computermedien |b c |2 rdamedia | ||
| 338 | |a Online-Ressource |b cr |2 rdacarrier | ||
| 500 | |a Gesehen am 06.08.2020 | ||
| 520 | |a The <i>Planck<i/> 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 <i>Planck<i/> 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 857 GHz at 5′ resolution. A total of 2151 <i>Planck<i/> high-<i>z<i/> source candidates (the PHZ) have been detected in the cleanest 26% of the sky, with flux density at 545 GHz above 500 mJy. Embedded in the cosmic infrared background close to the confusion limit, these high-<i>z<i/> candidates exhibit colder colours than their surroundings, consistent with redshifts <i>z<i/> > 2, assuming a dust temperature of <i>T<i/><sub>xgal<sub/> = 35 K and a spectral index of <i>β<i/><sub>xgal<sub/> = 1.5. Exhibiting extremely high luminosities, larger than 10<sup>14<sup/><i>L<i/><sub>⊙<sub/>, 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 <i>z<i/> > 2, and may be considered as proto-cluster candidates. The PHZ provides an original sample, which is complementary to the <i>Planck<i/> Sunyaev-Zeldovich Catalogue (PSZ2); by extending the population of virialized massive galaxy clusters detected below <i>z<i/> < 1.5 through their SZ signal to a population of sources at <i>z<i/> > 1.5, the PHZ may contain the progenitors of today’s clusters. Hence the <i>Planck<i/> 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-<i>z<i/>. | ||
| 700 | 1 | |a Pettorino, Valeria |d 1979- |e VerfasserIn |0 (DE-588)1047310236 |0 (DE-627)778096912 |0 (DE-576)400358832 |4 aut | |
| 773 | 0 | 8 | |i Enthalten in |t Astronomy and astrophysics |d Les Ulis : EDP Sciences, 1969 |g 596(2016) Artikel-Nummer A100, 28 Seiten |h Online-Ressource |w (DE-627)253390222 |w (DE-600)1458466-9 |w (DE-576)072283351 |x 1432-0746 |7 nnas |a Planck intermediate results XXXIX. The Planck list of high-redshift source candidates |
| 773 | 1 | 8 | |g volume:596 |g year:2016 |g pages:1-28 |g extent:28 |a Planck intermediate results XXXIX. The Planck list of high-redshift source candidates |
| 856 | 4 | 0 | |u https://doi.org/10.1051/0004-6361/201527206 |x Verlag |x Resolving-System |z lizenzpflichtig |3 Volltext |
| 856 | 4 | 0 | |u https://www.aanda.org/articles/aa/abs/2016/12/aa27206-15/aa27206-15.html |x Verlag |z lizenzpflichtig |3 Volltext |
| 951 | |a AR | ||
| 992 | |a 20200806 | ||
| 993 | |a Article | ||
| 994 | |a 2016 | ||
| 998 | |g 1047310236 |a Pettorino, Valeria |m 1047310236:Pettorino, Valeria |p 138 | ||
| 999 | |a KXP-PPN1726592537 |e 3736100795 | ||
| BIB | |a Y | ||
| SER | |a journal | ||
| JSO | |a {"physDesc":[{"extent":"28 S."}],"relHost":[{"origin":[{"dateIssuedDisp":"1969-","dateIssuedKey":"1969","publisher":"EDP Sciences ; Springer","publisherPlace":"Les Ulis ; Berlin ; Heidelberg"}],"id":{"zdb":["1458466-9"],"eki":["253390222"],"issn":["1432-0746"]},"name":{"displayForm":["European Southern Observatory (ESO)"]},"physDesc":[{"extent":"Online-Ressource"}],"title":[{"title":"Astronomy and astrophysics","subtitle":"an international weekly journal","title_sort":"Astronomy and astrophysics"}],"pubHistory":["1.1969 -"],"part":{"pages":"1-28","year":"2016","extent":"28","text":"596(2016) Artikel-Nummer A100, 28 Seiten","volume":"596"},"titleAlt":[{"title":"Astronomy & astrophysics"},{"title":"a European journal"}],"disp":"Planck intermediate results XXXIX. The Planck list of high-redshift source candidatesAstronomy and astrophysics","note":["Gesehen am 21.06.2024","Erscheint 36mal jährlich in 12 Bänden zu je 3 Ausgaben","Fortsetzung der Druck-Ausgabe"],"type":{"media":"Online-Ressource","bibl":"periodical"},"corporate":[{"display":"European Southern Observatory","roleDisplay":"Herausgebendes Organ","role":"isb"}],"language":["eng"],"recId":"253390222"}],"origin":[{"dateIssuedDisp":"12 December 2016","dateIssuedKey":"2016"}],"id":{"doi":["10.1051/0004-6361/201527206"],"eki":["1726592537"]},"name":{"displayForm":["Planck Collaboration: P.A.R. Ade, N. Aghanim, M. Arnaud, J. Aumont, C. Baccigalupi, A.J. Banday, R. B. Barreiro, N. Bartolo, E. Battaner, K. Benabed, A. Benoit-Lévy, J.-P. Bernard, M. Bersanelli, P. Bielewicz, A. Bonaldi, L. Bonavera, J.R. Bond, J. Borrill, F.R. Bouchet, F. Boulanger, C. Burigana, R.C. Butler, E. Calabrese, A. Catalano, H.C. Chiang, P.R. Christensen, D.L. Clements, L.P.L. Colombo, F. Couchot, A. Coulais, B.P. Crill, A. Curto, F. Cuttaia, L. Danese, R.D. Davies, R.J. Davis, P. de Bernardis, A. de Rosa, G. de Zotti, J. Delabrouille, C. Dickinson, J.M. Diego, H. Dole, O. Doré, M. Douspis, A. Ducout, X. Dupac, F. Elsner, T.A. Enßlin, H.K. Eriksen, E. Falgarone, F. Finelli, I. Flores-Cacho, M. Frailis, A.A. Fraisse, E. Franceschi, S. Galeotta, S. Galli, K. Ganga, M. Giard, Y. Giraud-Héraud, E. Gjerløw, J. González-Nuevo, K.M. Górski, A. Gregorio, A. Gruppuso, J.E. Gudmundsson, F.K. Hansen, D.L. Harrison, G. Helou, C. Hernández-Monteagudo, D. Herranz, S.R. Hildebrandt, E. Hivon, M. Hobson, A. Hornstrup, W. Hovest, K.M. Huffenberger, G. Hurier, A.H. Jaffe, T.R. Jaffe, E. Keihänen, R. Keskitalo, T.S. Kisner, R. Kneissl, J. Knoche, M. Kunz, H. Kurki-Suonio, G. Lagache, J.-M. Lamarre, A. Lasenby, M. Lattanzi, C.R. Lawrence, R. Leonardi, F. Levrier, M. Liguori, P.B. Lilje, M. Linden-Vørnle, M. López-Caniego, P.M. Lubin, J.F. Macías-Pérez, B. Maffei, G. Maggio, D. Maino, N. Mandolesi, A. Mangilli, M. Maris, P. G. Martin, E. Martínez-González, S. Masi, S. Matarrese, A. Melchiorri, A. Mennella, M. Migliaccio, S. Mitra, M.-A. Miville-Deschênes, A. Moneti, L. Montier, G. Morgante, D. Mortlock, D. Munshi, J.A. Murphy, F. Nati, P. Natoli, N.P.H. Nesvadba, F. Noviello, D. Novikov, I. Novikov, C.A. Oxborrow, L. Pagano, F. Pajot, D. Paoletti, B. Partridge, F. Pasian, T.J. Pearson, O. Perdereau, L. Perotto, V. Pettorino, F. Piacentini, M. Piat, S. Plaszczynski, E. Pointecouteau, G. Polenta, G.W. Pratt, S. Prunet, J.-L. Puget, J.P. Rachen, M. Reinecke, M. Remazeilles, C. Renault, A. Renzi, I. Ristorcelli, G. Rocha, C. Rosset, M. Rossetti, G. Roudier, J.A. Rubiño-Martín, B. Rusholme, M. Sandri, D. Santos, M. Savelainen, G. Savini, D. Scott, L. D. Spencer, V. Stolyarov, R. Stompor, R. Sudiwala, R. Sunyaev, A.-S. Suur-Uski, J.-F. Sygnet, J.A. Tauber, L. Terenzi, L. Toffolatti, M. Tomasi, M. Tristram, M. Tucci, M. Türler, G. Umana, L. Valenziano, J. Valiviita, F. Van Tent, P. Vielva, F. Villa, L.A. Wade, B.D. Wandelt, I.K. Wehus, N. Welikala, D. Yvon, A. Zacchei, and A. Zonca"]},"type":{"bibl":"article-journal","media":"Online-Ressource"},"note":["Gesehen am 06.08.2020"],"recId":"1726592537","language":["eng"],"title":[{"title_sort":"Planck intermediate results","subtitle":"XXXIX. The Planck list of high-redshift source candidates","title":"Planck intermediate results"}],"person":[{"given":"Peter A.","family":"Ade","role":"aut","roleDisplay":"VerfasserIn","display":"Ade, Peter A."},{"role":"aut","roleDisplay":"VerfasserIn","display":"Pettorino, Valeria","given":"Valeria","family":"Pettorino"}]} | ||
| SRT | |a ADEPETERAPPLANCKINTE1220 | ||