Zobrazeno 1 - 10
of 302
pro vyhledávání: '"Roseboom, I"'
Autor:
Geach, J. E., Dunlop, J. S., Halpern, M., Smail, Ian, van der Werf, P., Alexander, D. M., Almaini, O., Aretxaga, I., Arumugam, V., Asboth, V., Banerji, M., Beanlands, J., Best, P. N., Blain, A. W., Birkinshaw, M., Chapin, E. L., Chapman, S. C., Chen, C-C., Chrysostomou, A., Clarke, C., Clements, D. L., Conselice, C., Coppin, K. E. K., Cowley, W. I., Danielson, A. L. R., Eales, S., Edge, A. C., Farrah, D., Gibb, A., Harrison, C. M., Hine, N. K., Hughes, D., Ivison, R. J., Jarvis, M., Jenness, T., Jones, S. F., Karim, A., Koprowski, M., Knudsen, K. K., Lacey, C. G., Mackenzie, T., Marsden, G., McAlpine, K., McMahon, R., Meijerink, R., Michalowski, M. J., Oliver, S. J., Page, M. J., Peacock, J. A., Rigopoulou, D., Robson, E. I., Roseboom, I., Rotermund, K., Scott, Douglas, Serjeant, S., Simpson, C., Simpson, J. M., Smith, D. J. B., Spaans, M., Stanley, F., Stevens, J. A., Swinbank, A. M., Targett, T., Thomson, A. P., Valiante, E., Webb, T. M. A., Willott, C., Zavala, J. A., Zemcov, M.
We present a catalogue of nearly 3,000 submillimetre sources detected at 850um over ~5 square degrees surveyed as part of the James Clerk Maxwell Telescope (JCMT) SCUBA-2 Cosmology Legacy Survey (S2CLS). This is the largest survey of its kind at 850u
Externí odkaz:
http://arxiv.org/abs/1607.03904
Autor:
Marchetti, L., Vaccari, M., Franceschini, A., Arumugam, V., Aussel, H., Bethermin, M., Bock, J., Boselli, A., Buat, V., Burgarella, D., Clements, D. L., Conley, A., Conversi, L., Cooray, A., Dowell, C. D., Farrah, D., Feltre, A., Glenn, J., Griffin, M., Hatziminaoglou, E., Heinis, S., Ibar, E., Ivison, R. J., Nguyen, H. T., O'Halloran, B., Oliver, S. J., Omont, A., Page, M. J., Papageorgiou, A., Pearson, C. P., Perez-Fournon, I., Pohlen, M., Rigopoulou, D., Roseboom, I. G., Rowan-Robinson, M., Schulz, B., Scott, Douglas, Seymour, N., Shupe, D. L., Smith, A. J., Symeonidis, M., Valtchanov, I., Viero, M., Wang, L., Wardlow, J., Xu, C. K., Zemcov, M.
We used wide area surveys over 39 deg$^2$ by the HerMES collaboration, performed with the Herschel Observatory SPIRE multi-wavelength camera, to estimate the low-redshift, $0.02
Externí odkaz:
http://arxiv.org/abs/1511.06167
Autor:
Koprowski, M., Dunlop, J. S., Michalowski, M. J., Roseboom, I., Geach, J. E., Cirasuolo, M., Aretxaga, I., Bowler, R. A. A., Banerji, M., Bourne, N., Coppin, K. E. K., Chapman, S., Hughes, D. H., Jenness, T., McLure, R. J., Symeonidis, M., van der Werf, P.
We investigate the properties of the galaxies selected from the deepest 850-micron survey undertaken to date with SCUBA-2 on the JCMT. This deep 850-micron imaging was taken in parallel with deep 450-micron imaging in the very best observing conditio
Externí odkaz:
http://arxiv.org/abs/1509.07144
Autor:
Rawlings, J. I., Page, M. J., Symeonidis, M., Bock, J., Cooray, A., Farrah, D., Guo, K., Hatziminaoglou, E., Ibar, E., Oliver, S. J., Roseboom, I. G., Scott, Douglas, Seymour, N., Vaccari, M., Wardlow, J. L.
We separate the extragalactic radio source population above ~50 uJy into active galactic nuclei (AGN) and star-forming sources. The primary method of our approach is to fit the infrared spectral energy distributions (SEDs), constructed using Spitzer/
Externí odkaz:
http://arxiv.org/abs/1507.07044
Autor:
Riguccini, L., Floc'h, E. Le, Mullaney, J. R., Menendez-Delmestre, K., Aussel, H., Berta, S., Calanog, J., Capak, P., Cooray, A., Ilbert, O., Kartaltepe, J., Koekemoer, A., Lutz, D., Magnelli, B., McCracken, H., Oliver, S., Roseboom, I., Salvato, M., Sanders, D., Scoville, N., Taniguchi, Y., Treister, E.
Dust-Obscured galaxies (DOGs) are bright 24 um-selected sources with extreme obscuration at optical wavelengths. They are typically characterized by a rising power-law continuum of hot dust (T_D ~ 200-1000K) in the near-IR indicating that their mid-I
Externí odkaz:
http://arxiv.org/abs/1506.05475
Autor:
Bussmann, R. S., Riechers, D., Fialkov, A., Scudder, J., Hayward, C. C., Cowley, W. I., Bock, J., Calanog, J., Chapman, S. C., Cooray, A., De Bernardis, F., Farrah, D., Fu, Hai, Gavazzi, R., Hopwood, R., Ivison, R. J., Jarvis, M., Lacey, C., Loeb, A., Oliver, S. J., Perez-Fournon, I., Rigopoulou, D., Roseboom, I. G., Scott, Douglas, Smith, A. J., Vieira, J. D., Wang, L., Wardlow, J.
The Herschel Multi-tiered Extragalactic Survey (HerMES) has identified large numbers of dusty star-forming galaxies (DSFGs) over a wide range in redshift. A detailed understanding of these DSFGs is hampered by the limited spatial resolution of Hersch
Externí odkaz:
http://arxiv.org/abs/1504.05256
Autor:
Magnelli, B., Ivison, R. J., Lutz, D., Valtchanov, I., Farrah, D., Berta, S., Bertoldi, F., Bock, J., Cooray, A., Ibar, E., Karim, A., Floc'h, E. Le, Nordon, R., Oliver, S. J., Page, M., Popesso, P., Pozzi, F., Rigopoulou, D., Riguccini, L., Rodighiero, G., Rosario, D., Roseboom, I., Wang, L., Wuyts, S.
Publikováno v:
A&A 573, A45 (2015)
[Abridged] We study the evolution of the radio spectral index and far-infrared/radio correlation (FRC) across the star-formation rate-stellar masse (i.e. SFR-M*) plane up to z 2. We start from a M*-selected sample of galaxies with reliable SFR and re
Externí odkaz:
http://arxiv.org/abs/1410.7412
Autor:
Symeonidis, M., Georgakakis, A., Page, M. J., Bock, J., Bonzini, M., Buat, V., Farrah, D., Franceschini, A., Ibar, E., Lutz, D., Magnelli, B., Magdis, G., Oliver, S. J., Pannella, M., Paolillo, M., Rosario, D., Roseboom, I. G., Vaccari, M., Villforth, C.
We present the most complete study to date of the X-ray emission from star-formation in high redshift (median z=0.7; z<1.5), IR-luminous (L_IR=10^10-10^13 L_sun) galaxies detected by Herschel's PACS and SPIRE instruments. For our purpose we take adva
Externí odkaz:
http://arxiv.org/abs/1407.4511
Autor:
Huang, J. -S., Rigopoulou, D., Magdis, G., Rowan-Robinson, M., Dai, Y., Bock, J. J., Burgarella, D., Chapman, S., Clements, D. L., Cooray, A., Farrah, D., Glenn, J., Oliver, S., Smith, A. J., Wang, L., Page, M., Riechers, D., Roseboom, I., Symeonidis, M., Fazio, G. G., Yun, M., Webb, T. M. A., Efstathiou, A.
We present a study of the infrared properties for a sample of seven spectroscopically confirmed submillimeter galaxies at $z>$4.0. By combining ground-based near-infrared, Spitzer IRAC and MIPS, Herschel SPIRE, and ground-based submillimeter/millimet
Externí odkaz:
http://arxiv.org/abs/1401.6079
Autor:
Roseboom, I. G., Best, P . N.
The promise of multi-wavelength astronomy has been tempered by the large disparity in sensitivity and resolution between different wavelength regimes. Here we present a statistical approach which attempts to overcome this by fitting parametric models
Externí odkaz:
http://arxiv.org/abs/1312.5347