Zobrazeno 1 - 10
of 101
pro vyhledávání: '"Rawlings, J. I."'
Autor:
Page, M. J., Dwelly, T., McHardy, I., Seymour, N., Mason, K. O., Sharma, M., Kennea, J. A., Sasseen, T. P., Rawlings, J. I., Breeveld, A. A., Ferreras, I., Loaring, N. S., Walton, D. J., Symeonidis, M.
We use ultraviolet imaging taken with the XMM-Newton Optical Monitor telescope (XMM-OM), covering 280 square arcminutes in the UVW1 band (effective wavelength 2910 Angstroms) to measure rest-frame ultraviolet (1500 Angstrom) luminosity functions of g
Externí odkaz:
http://arxiv.org/abs/2106.08200
Autor:
Rawlings, J. I.
This thesis presents a study of the extragalactic radio source population at infrared (IR) and radio wavelengths of the electromagnetic spectrum. The IR/radio emission from these sources can be the result of star−forming processes and/or the result
Externí odkaz:
http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.626542
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:
Page, M., Yershov, V., Breeveld, A., Kuin, N. P. M., Mignani, R. P., Smith, P. J., Rawlings, J. I., Oates, S. R., Siegel, M., Roming, P. W. A.
We present the first Swift Ultraviolet/Optical Telescope Serendipitous Source Catalogue (UVOTSSC). The catalogue was compiled from 23,059 Swift datasets taken within the first five years of observations with the Swift UVOT. A purpose-built processing
Externí odkaz:
http://arxiv.org/abs/1503.06597
Autor:
Page, M. J., Symeonidis, M., Vieira, J. D., Altieri, B., Amblard, A., Arumugam, V., Aussel, H., Babbedge, T., Blain, A., Bock, J., Boselli, A., Buat, V., Castro-Rodr'iguez, N., Cava, A., Chanial, P., Clements, D. L., Conley, A., Conversi, L., Cooray, A., Dowell, C. D., Dubois, E. N., Dunlop, J. S., Dwek, E., Dye, S., Eales, S., Elbaz, D., Farrah, D., Fox, M., Franceschini, A., Gear, W., Glenn, J., Griffin, M., Halpern, M., Hatziminaoglou, E., Ibar, E., Isaak, K., Ivison, R. J., Lagache, G., Levenson, L., Lu, N., Madden, S., Maffei, B., Mainetti, G., Marchetti, L., Nguyen, H. T., O'Halloran, B., Oliver, S. J., Omont, A., Panuzzo, P., Papageorgiou, A., Pearson, C. P., Perez-Fournon, I., Pohlen, M., Rawlings, J. I., Rigopoulou, D., Riguccini, L., Rizzo, D., Rodighiero, G., Roseboom, I. G., Rowan-Robinson, M., Portal, M. Sanchez, Schulz, B., Scott, Douglas, Seymour, N., Shupe, D. L., Smith, A. J., Stevens, J. A., Trichas, M., Tugwell, K. E., Vaccari, M., Valtchanov, I., Viero, M., Vigroux, L., Wang, L., Ward, R., Wright, G., Xu, C. K., Zemcov, M.
The old, red stars which constitute the bulges of galaxies, and the massive black holes at their centres, are the relics of a period in cosmic history when galaxies formed stars at remarkable rates and active galactic nuclei (AGN) shone brightly from
Externí odkaz:
http://arxiv.org/abs/1310.4147
Autor:
Seymour, N., Altieri, B., De Breuck, C., Barthel, P., Coia, D., Conversi, L., Dannerbauer, H., Dey, A., Dickinson, M., Drouart, G., Galametz, A., Greve, T. R., Haas, M., Hatch, N., Ibar, E., Ivison, R., Jarvis, M., Kovacs, A., Kurk, J., Lehnert, M., Miley, G., Nesvadba, N., Rawlings, J. I., Rettura, A., Rottgering, H., Rocca-Volmerange, B., Sanchez-Portal, M., Santos, J. S., Stern, D., Stevens, J., Valtchanov, I., Vernet, J., Wylezalek, D.
We present a detailed study of the infrared spectral energy distribution of the high-redshift radio galaxy MRC 1138-26 at z = 2.156, also known as the Spiderweb Galaxy. By combining photometry from Spitzer, Herschel and LABOCA we fit the rest-frame 5
Externí odkaz:
http://arxiv.org/abs/1206.5821
Autor:
HerMES Collaboration, Oliver, S. J., Bock, J., Altieri, B., Amblard, A., Arumugam, V., Aussel, H., Babbedge, T., Beelen, A., Béthermin, M., Blain, A., Boselli, A., Bridge, C., Brisbin, D., Buat, V., Burgarella, D., Castro-Rodríguez, N., Cava, A., Chanial, P., Cirasuolo, M., Clements, D. L., Conley, A., Conversi, L., Cooray, A., Dowell, C. D., Dubois, E. N., Dwek, E., Dye, S., Eales, S., Elbaz, D., Farrah, D., Feltre, A., Ferrero, P., Fiolet, N., Fox, M., Franceschini, A., Gear, W., Giovannoli, E., Glenn, J., Gong, Y., Solares, E. A. González, Griffin, M., Halpern, M., Harwit, M., Hatziminaoglou, E., Heinis, S., Hurley, P., Hwang, H. S., Hyde, A., Ibar, E., Ilbert, O., Isaak, K., Ivison, R. J., Lagache, G., Floc'h, E. Le, Levenson, L., Faro, B. Lo, Lu, N., Madden, S., Maffei, B., Magdis, G., Mainetti, G., Marchetti, L., Marsden, G., Marshall, J., Mortier, A. M. J., Nguyen, H. T., O'Halloran, B., Omont, A., Page, M. J., Panuzzo, P., Papageorgiou, A., Patel, H., Pearson, C. P., Pérez-Fournon, I., Pohlen, M., Rawlings, J. I., Raymond, G., Rigopoulou, D., Riguccini, L., Rizzo, D., Rodighiero, G., Roseboom, I. G., Rowan-Robinson, M., Portal, M. Sánchez, Schulz, B., Scott, Douglas, Seymour, N., Shupe, D. L., Smith, A. J., Stevens, J. A., Symeonidis, M., Trichas, M., Tugwell, K. E., Vaccari, M., Valtchanov, I., Vieira, J. D., Viero, M., Vigroux, L., Wang, L., Ward, R., Wardlow, J., Wright, G., Xu, C. K., Zemcov, M.
The Herschel Multi-tiered Extragalactic Survey, HerMES, is a legacy program designed to map a set of nested fields totalling ~380 deg^2. Fields range in size from 0.01 to ~20 deg^2, using Herschel-SPIRE (at 250, 350 and 500 \mu m), and Herschel-PACS
Externí odkaz:
http://arxiv.org/abs/1203.2562
Autor:
Smith, A. J., Wang, L., Oliver, S. J., Auld, R., Bock, J., Brisbin, D., Burgarella, D., Chanial, P., Chapin, E., Clements, D. L., Conversi, L., Cooray, A., Dowell, C. D., Eales, S., Farrah, D., Franceschini, A., Glenn, J., Griffin, M., Ivison, R. J., Mortier, A. M. J., Page, M. J., Papageorgiou, A., Pearson, C. P., Pérez-Fournon, I., Pohlen, M., Rawlings, J. I., Raymond, G., Rodighiero, G., Roseboom, I. G., Rowan-Robinson, M., Savage, R., Scott, Douglas, Seymour, N., Symeonidis, M., Tugwell, K. E., Vaccari, M., Valtchanov, I., Vigroux, L., Ward, R., Wright, G., Zemcov, M.
We describe the generation of single-band point source catalogues from submillimetre Herschel-SPIRE observations taken as part of the Science Demonstration Phase of the Herschel Multi-tiered Extragalactic Survey (HerMES). Flux densities are found by
Externí odkaz:
http://arxiv.org/abs/1109.5186
Autor:
Roseboom, I. G., Ivison, R. J., Greve, T. R., Amblard, A., Arumugam, V., Auld, R., Aussel, H., Bethermin, M., Blain, A., Bock, J., Boselli, A., Brisbin, D., Buat, V., Burgarella, D., Castro-Rodriguez, N., Cava, A., Chanial, P., Chapin, E., Chapman, S., Clements, D. L., Conley, A., Conversi, L., Cooray, A., Dowell, C. D., Dunlop, J. S., Dwek, E., Eales, S., Elbaz, D., Farrah, D., Franceschini, A., Glenn, J., Griffin, M., Halpern, M., Hatziminaoglou, E., Ibar, E., Isaak, K., Lagache, G., Levenson, L., Lu, N., Madden, S., Maffei, B., Mainetti, G., Marchetti, L., Marsden, G., Morrison, G., Mortier, A. M. J., Nguyen, H. T., O'Halloran, B., Oliver, S. J., Omont, A., Page, M. J., Panuzzo, P., Papageorgiou, A., Pearson, C. P., Perez-Fournon, I., Pohlen, M., Rawlings, J. I., Raymond, G., Rigopoulou, D., Rizzo, D., Rodighiero, G., Rowan-Robinson, M., Schulz, B., Scott, Douglas, Seymour, N., Shupe, D. L., Smith, A. J., Stevens, J. A., Symeonidis, M., Trichas, M., Tugwell, K. E., Vaccari, M., Valtchanov, I., Vieira, J. D., Viero, M. P., Vigroux, L., Wardlow, J., Wang, L., Wright, G., Xu, C. K., Zemcov, M.
We investigate the potential of submm-mm and submm-mm-radio photometric redshifts using a sample of mm-selected sources as seen at 250, 350 and 500 {\mu}m by the SPIRE instrument on Herschel. From a sample of 63 previously identified mm-sources with
Externí odkaz:
http://arxiv.org/abs/1109.2887
Autor:
Symeonidis, M., Georgakakis, A., Seymour, N., Auld, R., Bock, J., Brisbin, D., Buat, V., Burgarella, D., Chanial, P., Clements, D. L., Cooray, A., Eales, S., Farrah, D., Franceschini, A., Glenn, J., Griffin, M., Hatziminaoglou, E., Ibar, E., Ivison, R. J., Mortier, A. M. J., Oliver, S. J., Page, M. J., Papageorgiou, A., Pearson, C. P., Pérez-Fournon, I., Pohlen, M., Rawlings, J. I., Raymond, G., Rodighiero, G., Roseboom, I. G., Rowan-Robinson, M., Scott, Douglas, Smith, A. J., Tugwell, K. E., Vaccari, M., Vieira, J. D., Vigroux, L., Wang, L., Wright, G.
For the first time, we investigate the X-ray/infrared (IR) correlation for star-forming galaxies at z~1, using SPIRE submm data from the recently-launched Herschel Space Observatory and deep X-ray data from the 2Ms Chandra deep field north (CDFN) sur
Externí odkaz:
http://arxiv.org/abs/1107.1373