The VIMOS Public Extragalactic Redshift Survey (VIPERS): galaxy segregation inside filaments at z ≃ 0.7

被引：94

作者：

Malavasi, N. ^{[1
,2
]}

Arnouts, S. ^{[2
]}

Vibert, D.

de la Torre, S. ^{[2
]}

Moutard, T. ^{[2
]}

Pichon, C. ^{[3
,4
]}

Davidzon, I. ^{[2
]}

Kraljic, K. ^{[2
]}

Bolzonella, M.

Guzzo, L. ^{[7
]}

Garilli, B. ^{[8
]}

Scodeggio, M. ^{[8
]}

Granett, B. R.

Abbas, U. ^{[9
]}

Adami, C. ^{[2
]}

Bottini, D. ^{[8
]}

Cappi, A. ^{[5
,10
]}

Cucciati, O. ^{[1
,5
,6
]}

Franzetti, P. ^{[8
]}

Fritz, A. ^{[8
]}

Iovino, A.

Krywult, J. ^{[11
]}

Le Brun, V. ^{[2
]}

Le Fevre, O. ^{[2
]}

Maccagni, D. ^{[8
]}

Malek, K. ^{[12
]}

Marulli, F. ^{[1
,5
,13
]}

Polletta, M. ^{[8
,14
,15
]}

Pollo, A. ^{[16
]}

Tasca, L. ^{[2
]}

Tojeiro, R. ^{[17
]}

Vergani, D. ^{[18
]}

Zanichelli, A. ^{[19
]}

Bel, J. ^{[20
]}

Branchini, E. ^{[21
,22
,23
]}

Coupon, J. ^{[24
]}

De Lucia, G. ^{[25
]}

Dubois, Y. ^{[3
]}

Hawken, A.

Ilbert, O.

Laigle, C. ^{[2
,3
]}

Moscardini, L. ^{[1
,5
]}

Sousbie, T. ^{[3
]}

Treyer, M. ^{[2
]}

Zamorani, G.

机构：

[1] Univ Bologna, Dipartimento Fis & Astron DIFA, I-40127 Bologna, Italy

[2] Aix Marseille Univ, CNRS, Lab Astrophys Marseille, UMR 7326, F-13388 Marseille, France

[3] Univ Paris 06, CNRS, Inst Astrophys Paris, UMR 7095, F-75014 Paris, France

[4] KIAS, 85 Hoegiro, Seoul 02455, South Korea

[5] INAF, Osservatorio Astron Bologna, Via Ranzani 1, I-40127 Bologna, Italy

[6] INAF, Osservatorio Astron Merate, Via Brera 28, I-23807 Merate, Italy

[7] Univ Milan, Via G Celoria 16, I-20130 Milan, Italy

[8] INAF, IASF Milano, Via Bassini 15, I-20133 Milan, Italy

[9] Osserv Astron Torino, INAF, I-10025 Pino Torinese, Italy

[10] Univ Nice Sophia Antipolis, CNRS, Observ Cote Azur, Lab Lagrange,UMR7293, F-06300 Nice, France

[11] Jan Kochanowski Univ, Inst Phys, Swietokrzyska 15, PL-25406 Kielce, Poland

[12] Natl Ctr Nucl Res, Hoza 69, PL-00681 Warsaw, Poland

[13] INFN, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy

[14] Aix Marseille Univ, 58 Bd Charles Livon, F-13284 Marseille 7, France

[15] IRAP, 9 Av Colonel Roche,BP 44346, F-31028 Toulouse, France

[16] Jagiellonian Univ, Astron Observ, PL-30001 Krakow, Poland

[17] Univ St Andrews, Sch Phys & Astron, St Andrews KY16 9SS, Fife, Scotland

[18] INAF, IASF Bolgona, Via Gobetti 101, I-40129 Bologna, Italy

[19] INAF, Ist Radioastron, Via Gobetti 101, I-40129 Bologna, Italy

[20] Aix Marseille Univ, CNRS, CPT, UMR 7332, F-13288 Marseille, France

[21] Univ Rome Tre, Dipartimento Matemat & Fis, Via Vasca Navale 84, I-00146 Rome, Italy

[22] INFN, Sez Roma Tre, Via Vasca Navale 84, I-00146 Rome, Italy

[23] Osserv Astron Roma, INAF, Via Frascati 33, I-00040 Monte Porzio Catone, RM, Italy

[24] Univ Geneva, Astron Observ, Ch Ecogia 16, CH-1290 Versoix, Switzerland

[25] INAF, Osservatorio Astron Trieste, Via G B Tiepolo 11, I-34143 Trieste, Italy

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2017年 / 465卷 / 04期

关键词：

galaxies: evolution; galaxies: high-redshift; galaxies: statistics; cosmology: observations; large-scale structure of Universe; LARGE-SCALE STRUCTURE; MASS ASSEMBLY GAMA; PERSISTENT COSMIC WEB; SPIN ALIGNMENT; DARK HALOES; LUMINOSITY; MORPHOLOGY; EVOLUTION; CLUSTERS;

D O I：

10.1093/mnras/stw2864

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present the first quantitative detection of large-scale filamentary structure at z similar or equal to 0.7 in the large cosmological volume probed by the VIMOS Public Extragalactic Redshift Survey (VIPERS). We use simulations to show the capability of VIPERS to recover robust topological features in the galaxy distribution, in particular the filamentary network. We then investigate how galaxies with different stellar masses and stellar activities are distributed around the filaments, and find a significant segregation, with the most massive or quiescent galaxies being closer to the filament axis than less massive or active galaxies. The signal persists even after downweighting the contribution of peak regions. Our results suggest that massive and quiescent galaxies assemble their stellar mass through successive mergers during their migration along filaments towards the nodes of the cosmic web. On the other hand, low-mass star-forming galaxies prefer the outer edge of filaments, a vorticity-rich region dominated by smooth accretion, as predicted by the recent spin alignment theory. This emphasizes the role of large-scale cosmic flows in shaping galaxy properties.

引用

页码：3817 / 3822

页数：6

共 50 条

[1] The VIMOS Public Extragalactic Redshift Survey (VIPERS) The coevolution of galaxy morphology and colour to z ∼ 1
Krywult, J.
Tasca, L. A. M.
Pollo, A.
Vergani, D.
Bolzonella, M.
Davidzon, I.
Iovino, A.
Gargiulo, A.
Haines, C. P.
Scodeggio, M.
Guzzo, L.
Zamorani, G.
Garilli, B.
Granett, B. R.
de la Torre, S.
Abbas, U.
Adami, C.
Bottini, D.
Cappi, A.
Cucciati, O.
Franzetti, P.
Fritz, A.
Le Brun, V.
Le Fevre, O.
Maccagni, D.
Malek, K.
Marulli, F.
Polletta, M.
Tojeiro, R.
Zanichelli, A.
Arnouts, S.
Bel, J.
Branchini, E.
Coupon, J.
De Lucia, G.
Ilbert, O.
McCracken, H. J.
Moscardini, L.
Takeuchi, T. T.
ASTRONOMY & ASTROPHYSICS, 2017, 598
[2] The VIMOS Public Extragalactic Redshift Survey (VIPERS): Measuring non-linear galaxy bias at z ∼ 0.8
1600, EDP Sciences (594):
[3] The VIMOS Public Extragalactic Redshift Survey (VIPERS) Measuring non-linear galaxy bias at z ∼ 0.8
Di Porto, C.
Branchini, E.
Bel, J.
Marulli, F.
Bolzonella, M.
Cucciati, O.
de la Torre, S.
Granett, B. R.
Guzzo, L.
Marinoni, C.
Moscardini, L.
Abbas, U.
Adami, C.
Arnouts, S.
Bottini, D.
Cappi, A.
Coupon, J.
Davidzon, I.
De Lucia, G.
Fritz, A.
Franzetti, P.
Fumana, M.
Garilli, B.
Ilbert, O.
Iovino, A.
Krywult, J.
Le Brun, V.
Le Fevre, O.
Maccagni, D.
Malek, K.
McCracken, H. J.
Paioro, L.
Polletta, M.
Pollo, A.
Scodeggio, M.
Tasca, L. A. M.
Tojeiro, R.
Vergani, D.
Zanichelli, A.
Burden, A.
Marchetti, A.
Martizzi, D.
Mellier, Y.
Nichol, R. C.
Peacock, J. A.
Percival, W. J.
Viel, M.
Wolk, M.
Zamorani, G.
ASTRONOMY & ASTROPHYSICS, 2016, 594
[4] The VIMOS Public Extragalactic Redshift Survey (VIPERS) Luminosity and stellar mass dependence of galaxy clustering at 0.5 < z < 1.1
1600, EDP Sciences (557):
[5] The VIMOS Public Extragalactic Redshift Survey (VIPERS) Galaxy clustering and redshift-space distortions at z ≃ 0.8 in the first data release
de la Torre, S.
Guzzo, L.
Peacock, J. A.
Branchini, E.
Iovino, A.
Granett, B. R.
Abbas, U.
Adami, C.
Arnouts, S.
Bel, J.
Bolzonella, M.
Bottini, D.
Cappi, A.
Coupon, J.
Cucciati, O.
Davidzon, I.
De Lucia, G.
Fritz, A.
Franzetti, P.
Fumana, M.
Garilli, B.
Ilbert, O.
Krywult, J.
Le Brun, V.
Le Fevre, O.
Maccagni, D.
Malek, K.
Marulli, F.
McCracken, H. J.
Moscardini, L.
Paioro, L.
Percival, W. J.
Polletta, M.
Pollo, A.
Schlagenhaufer, H.
Scodeggio, M.
Tasca, L. A. M.
Tojeiro, R.
Vergani, D.
Zanichelli, A.
Burden, A.
Di Porto, C.
Marchetti, A.
Marinoni, C.
Mellier, Y.
Monaco, P.
Nichol, R. C.
Phleps, S.
Wolk, M.
Zamorani, G.
ASTRONOMY & ASTROPHYSICS, 2013, 557
[6] The VIMOS Public Extragalactic Redshift Survey (VIPERS): Hierarchical scaling and biasing
Cappi, A.
Marulli, F.
Bel, J.
Cucciati, O.
Branchini, E.
De La Torre, S.
Moscardini, L.
Bolzonella, M.
Guzzo, L.
Abbas, U.
Adami, C.
Arnouts, S.
Bottini, D.
Coupon, J.
Davidzon, I.
De Lucia, G.
Fritz, A.
Franzetti, P.
Fumana, M.
Garilli, B.
Granett, B.R.
Ilbert, O.
Iovino, A.
Krywult, J.
Le Brun, V.
Le Fèvre, O.
MacCagni, D.
Malek, K.
McCracken, H.J.
Paioro, L.
Polletta, M.
Pollo, A.
Scodeggio, M.
Tasca, L.A.M.
Tojeiro, R.
Vergani, D.
Zanichelli, A.
Burden, A.
Di Porto, C.
Marchetti, A.
Marinoni, C.
Mellier, Y.
Nichol, R.C.
Peacock, J.A.
Percival, W.J.
Phleps, S.
Schimd, C.
Schlagenhaufer, H.
Wolk, M.
Zamorani, G.
Astronomy and Astrophysics, 2015, 579
[7] The VIMOS Public Extragalactic Redshift Survey (VIPERS) Hierarchical scaling and biasing
Cappi, A.
Marulli, F.
Bel, J.
Cucciati, O.
Branchini, E.
de la Torre, S.
Moscardini, L.
Bolzonella, M.
Guzzo, L.
Abbas, U.
Adami, C.
Arnouts, S.
Bottini, D.
Coupon, J.
Davidzon, I.
De Lucia, G.
Fritz, A.
Franzetti, P.
Fumana, M.
Garilli, B.
Granett, B. R.
Ilbert, O.
Iovino, A.
Krywult, J.
Le Brun, V.
Le Fevre, O.
Maccagni, D.
Malek, K.
McCracken, H. J.
Paioro, L.
Polletta, M.
Pollo, A.
Scodeggio, M.
Tasca, L. A. M.
Tojeiro, R.
Vergani, D.
Zanichelli, A.
Burden, A.
Di Porto, C.
Marchetti, A.
Marinoni, C.
Mellier, Y.
Nichol, R. C.
Peacock, J. A.
Percival, W. J.
Phleps, S.
Schimd, C.
Schlagenhaufer, H.
Wolk, M.
Zamorani, G.
ASTRONOMY & ASTROPHYSICS, 2015, 579
[8] The VIMOS Public Extragalactic Redshift Survey (VIPERS) Ωm0 from the galaxy clustering ratio measured at z ∼ 1
Bel, J.
Marinoni, C.
Granett, B. R.
Guzzo, L.
Peacock, J. A.
Branchini, E.
Cucciati, O.
de la Torre, S.
Iovino, A.
Percival, W. J.
Steigerwald, H.
Abbas, U.
Adami, C.
Arnouts, S.
Bolzonella, M.
Bottini, D.
Cappi, A.
Coupon, J.
Davidzon, I.
De Lucia, G.
Fritz, A.
Franzetti, P.
Fumana, M.
Garilli, B.
Ilbert, O.
Krywult, J.
Le Brun, V.
Le Fevre, O.
Maccagni, D.
Malek, K.
Marulli, F.
McCracken, H. J.
Paioro, L.
Polletta, M.
Pollo, A.
Schlagenhaufer, H.
Scodeggio, M.
Tasca, L. A. M.
Tojeiro, R.
Vergani, D.
Zanichelli, A.
Burden, A.
Di Porto, C.
Marchetti, A.
Mellier, Y.
Moscardini, L.
Nichol, R. C.
Phleps, S.
Wolk, M.
Zamorani, G.
ASTRONOMY & ASTROPHYSICS, 2014, 563
[9] The VIMOS Public Extragalactic Redshift Survey (VIPERS): Ωm0 from the galaxy clustering ratio measured at z ~ 1
1600, EDP Sciences (563):
[10] The VIMOS Public Extragalactic Redshift Survey (VIPERS) Environmental effects shaping the galaxy stellar mass function
Davidzon, I.
Cucciati, O.
Bolzonella, M.
De Lucia, G.
Zamorani, G.
Arnouts, S.
Moutard, T.
Ilbert, O.
Garilli, B.
Scodeggio, M.
Guzzo, L.
Abbas, U.
Adami, C.
Bel, J.
Bottini, D.
Branchini, E.
Cappi, A.
Coupon, J.
de la Torre, S.
Di Porto, C.
Fritz, A.
Franzetti, P.
Fumana, M.
Granett, B. R.
Guennou, L.
Iovino, A.
Krywult, J.
Le Brun, V.
Le Fevre, O.
Maccagni, D.
Malek, K.
Marulli, F.
McCracken, H. J.
Mellier, Y.
Moscardini, L.
Polletta, M.
Pollo, A.
Tasca, L. A. M.
Tojeiro, R.
Vergani, D.
Zanichelli, A.
ASTRONOMY & ASTROPHYSICS, 2016, 586

← 1 2 3 4 5 →