Search Results - Cosmos Redshift 7

CANDELS multi-wavelength catalogs: source identification and photometry in the CANDELS COSMOS survey field by Nayyeri, H., Hemmati, S., Mobasher, B., Ferguson, H.C., Cooray, A., Barro, G., Faber, S.M., Dickinson, M., Koekemoer, A.M., Peth, M., Ashby, M.L.N., Salvato, M., Darvish, B., Donley, J., Durbin, M., Finkelstein, S., Fontana, A., Grogin, N.A., Gruetzbauch, R., Huang, K., Khostovan, A.A., Kocevski, D., Kodra, D., Lee, B., Newman, J., Pacifici, C., Pforr, J., Stefanon, M., Wiklind, T., Willner, S.P., Wuyts, S., Castellano, M., Conselice, Christopher J., Dolch, T., Dunlop, J.S., Galametz, A., Hathi, N.P., Lucas, R.A., Yan, H.

Get full text

MIGHTEE: Multi-wavelength counterparts in the COSMOS field by Whittam, I.H., Prescott, M., Hale, C.L., Jarvis, M.J., Heywood, I., An, F., Glowacki, Marcin, Maddox, N., Marchetti, L., Morabito, L.K., Adams, N.J., Bowler, R.A.A., Hatfield, P.W., Varadaraj, R.G., Collier, J., Frank, B., Taylor, A.R., Santos, M.G., Vaccari, M., Afonso, J., Ao, Y., Delhaize, J., Knowles, K., Kolwa, S., Randriamampandry, S.M., Randriamanakoto, Z., Smirnov, O., Smith, D.J.B., White, S.V.

“…The radio data used in this work covers 0.86 deg2 of the COSMOS field, reaches a thermal noise of 1.7 μJy beam-1 and contains 6102 radio components. …”
Get full text
Get full text

Physical properties of z > 4 submillimeter galaxies in the COSMOS field by Smolcic, V., Karim, A., Miettinen, O., Novak, M., Magnelli, B., Riechers, D., Schinnerer, E., Capak, P., Bondi, M., Ciliegi, P., Aravena, M., Bertoldi, F., Bourke, S., Banfield, J., Carilli, C., Civano, F., Ilbert, O., Intema, Hubertus, Le Fèvre, O., Finoguenov, A., Hallinan, G., Klöckner, H., Koekemoer, A., Laigle, C., Masters, D., McCracken, H., Mooley, K., Murphy, E., Navarette, F., Salvato, M., Sargent, M., Sheth, K., Toft, S., Zamorani, G.

“…We investigate the physical properties of a sample of six submillimeter galaxies (SMGs) in the COSMOS field, spectroscopically confirmed to lie at redshifts z > 4. …”
Get full text

An ALMA survey of submillimetre galaxies in the COSMOS field: Physical properties derived from energy balance spectral energy distribution modelling by Miettinen, O., Delvecchio, I., Smolcic, V., Aravena, M., Brisbin, D., Karim, A., Magnelli, B., Novak, M., Schinnerer, E., Albrecht, M., Aussel, H., Bertoldi, F., Capak, P., Casey, C., Hayward, C., Ilbert, O., Intema, Hubertus, Jiang, C., Le Fèvre, O., McCracken, H., Munõz Arancibia, A., Navarrete, F., Padilla, N., Riechers, D., Salvato, M., Scott, K., Sheth, K., Tasca, L.

“…The Mdust/M⋆ ratio was found to decrease as a function of redshift, while the Mgas/Mdust ratio shows the opposite, positive correlation with redshift. …”
Get full text

(Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxies: IV. Physical properties derived from spectral energy distributions by Miettinen, O., Delvecchio, I., Smolcic, V., Novak, M., Aravena, M., Karim, A., Murphy, E., Schinnerer, E., Capak, P., Ilbert, O., Intema, Hubertus, Laigle, C., McCracken, H.

“…We attempt to characterise the physical nature of a 1.1 mm selected, flux-limited, and interferometrically followed up sample of SMGs in the COSMOS field. Methods. We used the latest release of the MAGPHYS code to fit the multiwavelength (UV to radio) spectral energy distributions (SEDs) of 16 of the target SMGs, which lie at redshifts z ~ 1.6-5.3. …”
Get full text

HerMES: Deep number counts at 250 µm, 350 µm and 500 µm in the COSMOS and GOODS-N fields and the build-up of the cosmic infrared background by Béthermin, M., Le Floc'H, E., Ilbert, O., Conley, A., Lagache, G., Amblard, A., Arumugam, V., Aussel, H., Berta, S., Bock, J., Boselli, A., Buat, V., Casey, C., Castro-Rodríguez, N., Cava, A., Clements, D., Cooray, A., Dowell, C., Eales, S., Farrah, D., Franceschini, A., Glenn, J., Griffin, M., Hatziminaoglou, E., Heinis, S., Ibar, E., Ivison, R., Kartaltepe, J., Levenson, L., Magdis, G., Marchetti, L., Marsden, G., Nguyen, H., O'Halloran, B., Oliver, S., Omont, A., Page, M., Panuzzo, P., Papageorgiou, A., Pearson, C., Pérez-Fournon, I., Pohlen, M., Rigopoulou, D., Roseboom, I., Rowan-Robinson, M., Salvato, M., Schulz, B., Scott, D., Seymour, Nick, Shupe, D., Smith, A., Symeonidis, M., Trichas, M., Tugwell, K., Vaccari, M., Valtchanov, I., Vieira, J., Viero, M., Wang, L., Xu, C., Zemcov, M.

“…We individually extracted the bright SPIRE sources (>20 mJy) in the COSMOS field with a method using the positions, the flux densities, and the redshifts of the 24 μm sources as a prior, and derived the number counts and redshift distributions of the bright SPIRE sources. …”
Get full text

SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES): faint-end counts at 450 μm by Wang, Wei-Hao, Lin, Wei-Ching, Lim, Chen-Fatt, Smail, Ian, Chapman, Scott C., Zheng, Xian Zhong, Shim, Hyunjin, Kodama, Tadayuki, Almaini, Omar, Ao, Yiping, Blain, Andrew W., Bourne, Nathan, Bunker, Andrew J., Chang, Yu-Yen, Chao, Dani C.-Y., Chen, Chian-Chou, Clements, David L., Conselice, Christopher J., Cowley, William I., Dannerbauer, Helmut, Dunlop, James S., Geach, James E., Goto, Tomotsugu, Jiang, Linhua, Ivison, Rob J., Jeong, Woong-Seob, Kohno, Kotaro, Kong, Xu, Lee, Chien-Hsu, Lee, Hyung Mok, Lee, Minju, Michałowski, Michał J., Oteo, Iván, Sawicki, Marcin, Scott, Douglas, Shu, Xin Wen, Simpson, James M., Tee, Wei-Leong, Toba, Yoshiki, Valiante, Elisabetta, Wang, Jun-Xian, Wang, Ran, Wardlow, Julie L.

“…The SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES) is a three-year JCMT Large Program aiming to reach the 450 μm confusion limit in the COSMOS-CANDELS region to study a representative sample of the high-redshift far-infrared galaxy population that gives rise to the bulk of the far-infrared background. …”
Get full text

Tracking the activity of supermassive black holes and the habitats of their hosts by Krishnan, Charutha

“…Our galaxy catalogues comprise deep, multi-wavelength data provided by the UKIDSS Ultra Deep Survey (UDS) and Cosmic Evolution Survey (COSMOS). The UDS field contains a dense structure at z ∼ 1.6 with additional narrow-band imaging tailored to its redshift, allowing for the selection of protocluster members using precise photometric redshifts (Hatch et al. 2016). …”
Get full text

Formation and evolution of discs and bulges through cosmic time in CANDELS by Margalef Bentabol, Berta

“…We show that spiral galaxies, and in particular clumpy spirals, dominate the star formation at all redshifts, with average SFRs of SFR = 40 ± 3 Moyr−1 and SFR = 50 ± 7 Moyr−1 respectively, and that there is no benefit of having a large mass to produce spiral structures.…”
Get full text

Herschel reveals the obscured star formation in HiZELS Ha emitters at z = 1.47 by Ibar, E., Sobral, D., Best, P., Ivison, R., Smail, I., Arumugam, V., Berta, S., Béthermin, M., Bock, J., Cava, A., Conley, A., Farrah, D., Geach, J., Ikarashi, S., Kohno, K., Le Floc'h, E., Lutz, D., Magdis, G., Magnelli, B., Marsden, G., Oliver, S., Page, M., Pozzi, F., Riguccini, L., Schulz, B., Seymour, Nick, Smith, A., Symeonidis, M., Wang, L., Wardlow, J., Zemcov, M.

“…We describe the far-infrared (far-IR; rest-frame 8–1000-μm) properties of a sample of 443 Hα-selected star-forming galaxies in the Cosmic Evolution Survey (COSMOS) and Ultra Deep Survey (UDS) fields detected by the High-redshift Emission Line Survey (HiZELS) imaging survey. …”
Get full text