Galaxy formation and evolution

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The Herschel-SPIRE instrument and its in-flight performance

(2010)

Authors:

MJ Griffin, A Abergel, A Abreu, PAR Ade, P André, J-L Augueres, T Babbedge, Y Bae, T Baillie, J-P Baluteau, MJ Barlow, G Bendo, D Benielli, JJ Bock, P Bonhomme, D Brisbin, C Brockley-Blatt, M Caldwell, C Cara, N Castro-Rodriguez, R Cerulli, P Chanial, S Chen, E Clark, DL Clements, L Clerc, J Coker, D Communal, L Conversi, P Cox, D Crumb, C Cunningham, F Daly, GR Davis, P De Antoni, J Delderfield, N Devin, A Di Giorgio, I Didschuns, K Dohlen, M Donati, A Dowell, CD Dowell, L Duband, L Dumaye, RJ Emery, M Ferlet, D Ferrand, J Fontignie, M Fox, A Franceschini, M Frerking, T Fulton, J Garcia, R Gastaud, WK Gear, J Glenn, A Goizel, DK Griffin, T Grundy, S Guest, L Guillemet, PC Hargrave, M Harwit, P Hastings, E Hatziminaoglou, M Herman, B Hinde, V Hristov, M Huang, P Imhof, KJ Isaak, U Israelsson, RJ Ivison, D Jennings, B Kiernan, KJ King, AE Lange, W Latter, G Laurent, P Laurent, SJ Leeks, E Lellouch, L Levenson, B Li, J Li, J Lilienthal, T Lim, J Liu, N Lu, S Madden, G Mainetti, P Marliani, D McKay, K Mercier, S Molinari, H Morris, H Moseley, J Mulder, M Mur, DA Naylor, H Nguyen, B O'Halloran, S Oliver, G Olofsson, H-G Olofsson, R Orfei, MJ Page, I Pain, P Panuzzo, A Papageorgiou, G Parks, P Parr-Burman, A Pearce, C Pearson, I Pérez-Fournon, F Pinsard, G Pisano, J Podosek, M Pohlen, ET Polehampton, D Pouliquen, D Rigopoulou, D Rizzo, IG Roseboom, H Roussel, M Rowan-Robinson, B Rownd, P Saraceno, M Sauvage, R Savage, G Savini, E Sawyer, C Scharmberg, D Schmitt, N Schneider, B Schulz, A Schwartz, R Shafer, DL Shupe, B Sibthorpe, S Sidher, A Smith, AJ Smith, D Smith, L Spencer, B Stobie, R Sudiwala, K Sukhatme, C Surace, JA Stevens, BM Swinyard, M Trichas, T Tourette, H Triou, S Tseng, C Tucker, A Turner, M Vaccari, I Valtchanov, L Vigroux, E Virique, G Voellmer, H Walker, R Ward, T Waskett, M Weilert, R Wesson, GJ White, N Whitehouse, CD Wilson, B Winter, AL Woodcraft, GS Wright, CK Xu, A Zavagno, M Zemcov, L Zhang, E Zonca
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On the filamentary environment of galaxies

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) (2010)

Authors:

C Gay, C Pichon, D Le Borgne, R Teyssier, T Sousbie, J Devriendt

Abstract:

The correlation between the large-scale distribution of galaxies and their spectroscopic properties at z=1.5 is investigated using the Horizon MareNostrum cosmological run. We have extracted a large sample of 10^5 galaxies from this large hydrodynamical simulation featuring standard galaxy formation physics. Spectral synthesis is applied to these single stellar populations to generate spectra and colours for all galaxies. We use the skeleton as a tracer of the cosmic web and study how our galaxy catalogue depends on the distance to the skeleton. We show that galaxies closer to the skeleton tend to be redder, but that the effect is mostly due to the proximity of large haloes at the nodes of the skeleton, rather than the filaments themselves. This effects translate into a bimodality in the colour distribution of our sample. The origin of this bimodality is investigated and seems to follow from the ram pressure stripping of satellite galaxies within the more massive clusters of the simulation. The virtual catalogues (spectroscopical properties of the MareNostrum galaxies at various redshifts) are available online at http://www.iap.fr/users/pichon/MareNostrum/catalogues

The WFC3 Infrared Spectroscopic Parallel (WISP) Survey

(2010)

Authors:

H Atek, M Malkan, P McCarthy, H Teplitz, C Scarlata, B Siana, A Henry, J Colbert, NR Ross, C Bridge, AJ Bunker, A Dressler, RAE Fosbury, C martin, H Shim
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HerMES: Halo Occupation Number and Bias Properties of Dusty Galaxies from Angular Clustering Measurements

(2010)

Authors:

Asantha Cooray, A Amblard, L Wang, B Altieri, V Arumugam, R Auld, H Aussel, T Babbedge, A Blain, J Bock, A Boselli, V Buat, D Burgarella, N Castro-Rodriguez, A Cava, P Chanial, DL Clements, A Conley, L Conversi, CD Dowell, E Dwek, S Eales, D Elbaz, D Farrah, M Fox, A Franceschini, W Gear, J Glenn, M Griffin, M Halpern, E Hatziminaoglou, E Ibar, K Isaak, RJ Ivison, AA Khostovan, G Lagache, L Levenson, N Lu, S Madden, B Maffei, G Mainetti, L Marchetti, G Marsden, K Mitchell-Wynne, AMJ Mortier, HT Nguyen, B O'Halloran, SJ Oliver, A Omont, MJ Page, P Panuzzo, A Papageorgiou, CP Pearson, I Pérez-Fournon, M Pohlen, JI Rawlings, G Raymond, D Rigopoulou, D Rizzo, IG Roseboom, M Rowan-Robinson, M Sanchez Portal, B Schulz, Douglas Scott, P Serra, N Seymour, DL Shupe, AJ Smith, JA Stevens, M Symeonidis, M Trichas, KE Tugwell, M Vaccari, I Valtchanov, JD Vieira, L Vigroux, R Ward, G Wright, CK Xu, M Zemcov
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Herschel unveils a puzzling uniformity of distant dusty galaxies

(2010)

Authors:

D Elbaz, HS Hwang, B Magnelli, E Daddi, H Aussel, B Altieri, A Amblard, P Andreani, V Arumugam, R Auld, T Babbedge, S Berta, A Blain, J Bock, A Bongiovanni, A Boselli, V Buat, D Burgarella, N Castro-Rodriguez, A Cava, J Cepa, P Chanial, R-R Chary, A Cimatti, DL Clements, A Conley, L Conversi, A Cooray, M Dickinson, H Dominguez, CD Dowell, JS Dunlop, E Dwek, S Eales, D Farrah, N Forster Schreiber, M Fox, A Franceschini, W Gear, R Genzel, J Glenn, M Griffin, C Gruppioni, M Halpern, E Hatziminaoglou, E Ibar, K Isaak, RJ Ivison, G Lagache, D Le Borgne, E Le Floc'h, L Levenson, N Lu, D Lutz, S Madden, B Maffei, G Magdis, G Mainetti, R Maiolino, L Marchetti, AMJ Mortier, HT Nguyen, R Nordon, B O'Halloran, K Okumura, SJ Oliver, A Omont, MJ Page, P Panuzzo, A Papageorgiou, CP Pearson, I Perez Fournon, AM Perez Garcıa, A Poglitsch, M Pohlen, P Popesso, F Pozzi, JI Rawlings, D Rigopoulou, L Riguccini, D Rizzo, G Rodighiero, IG Roseboom, M Rowan-Robinson, A Saintonge, M Sanchez-Portal, P Santini, M Sauvage, B Schulz, Douglas Scott, N Seymour, L Shao, DL Shupe, AJ Smith, JA Stevens, E Sturm, M Symeonidis, L Tacconi, M Trichas, KE Tugwell, M Vaccari, I Valtchanov, J Vieira, L Vigroux, L Wang, R Ward, G Wright, CK Xu, M Zemcov
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