Zobrazeno 1 - 10
of 835
pro vyhledávání: '"Pohlen M"'
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:
Negrello, M., Hopwood, R., Dye, S., da Cunha, E., Serjeant, S., Fleuren, S., Bussmann, R. S., Cooray, A., Dannerbauer, H., Gonzalez-Nuevo, J., Lapi, A., Omont, A., Amber, S., Auld, R., Baes, M., Buttiglione, S., Cava, A., Danese, L., Dariush, A., De Zotti, G., Dunne, L., Eales, S., Fritz, J., Ibar, E., Ivison, R., Kim, S., Maddox, S., Michalowski, M. J., Pascale, E., Pohlen, M., Rigby, E., Rowlands, K., Smith, D. J. B., Sutherland, W., Temi, P., Wardlow, J.
We report on deep near-infrared observations obtained with the Wide Field Camera 3 (WFC3) onboard the Hubble Space Telescope (HST) of the first five confirmed gravitational lensing events discovered by the Herschel Astrophysical Terahertz Large Area
Externí odkaz:
http://arxiv.org/abs/1311.5898
Autor:
Dowell, C. Darren, Conley, A., Glenn, J., Arumugam, V., Asboth, V., Aussel, H., Bertoldi, F., Bethermin, M., Bock, J., Boselli, A., Bridge, C., Buat, V., Burgarella, D., Cabrera-Lavers, A., Casey, C. M., Chapman, S. C., Clements, D. L., Conversi, L., Cooray, A., Dannerbauer, H., De Bernardis, F., Ellsworth-Bowers, T. P., Farrah, D., Franceschini, A., Griffin, M., Gurwell, M. A., Halpern, M., Hatziminaoglou, E., Heinis, S., Ibar, E., Ivison, R. J., Laporte, N., Marchetti, L., Martinez-Navajas, P., Marsden, G., Morrison, G. E., Nguyen, H. T., O'Halloran, B., Oliver, S. J., Omont, A., Page, M. J., Papageorgiou, A., Pearson, C. P., Petitpas, G., Perez-Fournon, I., Pohlen, M., Riechers, D., Rigopoulou, D., Roseboom, I. G., Rowan-Robinson, M., Sayers, J., Schulz, B., Scott, Douglas, Seymour, N., Shupe, D. L., Smith, A. J., Streblyanska, A., Symeonidis, M., Vaccari, M., Valtchanov, I., Vieira, J. D., Viero, M., Wang, L., Wardlow, J., Xu, C. K., Zemcov, M.
We present a method for selecting $z>4$ dusty, star forming galaxies (DSFGs) using Herschel/SPIRE 250/350/500 $\mu m$ flux densities to search for red sources. We apply this method to 21 deg$^2$ of data from the HerMES survey to produce a catalog of
Externí odkaz:
http://arxiv.org/abs/1310.7583
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:
Rémy-Ruyer, A., Madden, S. C., Galliano, F., Hony, S., Sauvage, M., Bendo, G. J., Roussel, H., Pohlen, M., Smith, M. W. L., Galametz, M., Cormier, D., Lebouteiller, V., Wu, R., Baes, M., Barlow, M. J., Boquien, M., Boselli, A., Ciesla, L., De Looze, I., Karczewski, O. Ł., Panuzzo, P., Spinoglio, L., Vaccari, M., Wilson, C. D., consortium, the Herschel-SAG2
Publikováno v:
A&A 557, A95 (2013)
We present new photometric data from our Herschel Key Programme, the Dwarf Galaxy Survey (DGS), dedicated to the observation of the gas and dust in 48 low-metallicity environments. They were observed with PACS and SPIRE onboard Herschel at 70,100,160
Externí odkaz:
http://arxiv.org/abs/1309.1371
Autor:
Griffin, M. J., North, C. E., Schulz, B., Amaral-Rogers, A., Bendo, G., Bock, J., Conversi, L., Conley, A., Dowell, C. D., Ferlet, M., Glenn, J., Lim, T., Pearson, C., Pohlen, M., Sibthorpe, B., Spencer, L., Swinyard, B., Valtchanov, I.
Publikováno v:
MNRAS 434 (2013) 992-1004
Photometric instruments operating at far infrared to millimetre wavelengths often have broad spectral passbands (central wavelength/bandwidth ~ 3 or less), especially those operating in space. A broad passband can result in significant variation of t
Externí odkaz:
http://arxiv.org/abs/1306.1778
Autor:
Bendo, G. J., Griffin, M. J., Bock, J. J., Conversi, L., Dowell, C. D., Lim, T., Lu, N., North, C. E., Papageorgiou, A., Pearson, C. P., Pohlen, M., Polehampton, E. T., Schulz, B., Shupe, D. L., Sibthorpe, B., Spencer, L. D., Swinyard, B. M., Valtchanov, I., Xu, C. K.
We describe the procedure used to flux calibrate the three-band submillimetre photometer in the Spectral and Photometric Imaging REceiver (SPIRE) instrument on the Herschel Space Observatory. This includes the equations describing the calibration sch
Externí odkaz:
http://arxiv.org/abs/1306.1217
Autor:
Madden, S. C., Ruyer, A. Remy, Galametz, M., Cormier, D., Lebouteiller, V., Galliano, F., Hony, S., Bendo, G. J., Smith, M. W. L., Pohlen, M., Roussel, H., Sauvage, M., Wu, R., Sturm, E., Poglitsch, A., Contursi, A., Doublier, V., Baes, M., Barlow, M. J., Boselli, A., Boquien, M., Carlson, L. R., Ciesla, L., Cooray, A., Cortese, L., De Looze, I., Irwin, J. A., Isaak, K., Kamenetzky, J., Karczewski, O. L., Lu, N., MacHattie, J. A., Halloran, B. O, Parkin, T. J., Rangwala, N., Schirm, M. R. P., Schulz, B., Spinoglio, L., Vaccari, M., Wilson, C. D., Wozniak, H.
The Dwarf Galaxy Survey (DGS) program is studying low-metallicity galaxies using 230h of far-infrared (FIR) and submillimetre (submm) photometric and spectroscopic observations of the Herschel Space Observatory and draws to this a rich database of a
Externí odkaz:
http://arxiv.org/abs/1305.2628
Autor:
Gruppioni, C., Pozzi, F., Rodighiero, G., Delvecchio, I., Berta, S., Pozzetti, L., Zamorani, G., Andreani, P., Cimatti, A., Ilbert, O., Floch, E. Le, Lutz, D., Magnelli, B., Marchetti, L., Monaco, P., Nordon, R., Oliver, S., Popesso, P., Riguccini, L., Roseboom, I., Rosario, D. J., Sargent, M., Vaccari, M., Altieri, B., Aussel, H., Bongiovanni, A., Cepa, J., Daddi, E., Dominguez-Sanchez, H., Elbaz, D., Forster-Schreiber, N., Genzel, R., Iribarrem, A., Magliocchetti, M., Maiolino, R., Poglitsch, A., Garcia, A. Perez, Sanchez-Portal, M., Sturm, E., Tacconi, L., Valtchanov, I., Amblard, A., Arumugam, V., Bethermin, M., Bock, J., Boselli, A., Buat, V., Burgarella, D., Castro-Rodriguez, N., Cava, A., Chanial, P., Clements, D. L., Conley, A., Cooray, A., Dowell, C. D., Dwek, E., Eales, S., Franceschini, A., Glenn, J., Griffin, M., Hatziminaoglou, E., Ibar, E., Isaak, K., Ivison, R. J., Lagache, G., Levenson, L., Lu, N., Madden, S., Maffei, B., Mainetti, G., Nguyen, H. T., Halloran, B. O, Page, M. J., Panuzzo, P., Papageorgiou, A., Pearson, C. P., Perez-Fournon, I., Pohlen, M., Rigopoulou, D., Rowan-Robinson, M., Schulz, B., Scott, D., Seymour, N., Shupe, D. L., Smith, A. J., Stevens, J. A., Symeonidis, M., Trichas, M., Tugwell, K. E., Vigroux, L., Wang, L., Wright, G., Xu, C. K., Zemcov, M., Bardelli, S., Carollo, M., Contini, T., Fevre, O. Le, Lilly, S., Mainieri, V., Renzini, A., Scodeggio, M., Zucca, E.
We exploit the deep and extended far infrared data sets (at 70, 100 and 160 um) of the Herschel GTO PACS Evolutionary Probe (PEP) Survey, in combination with the HERschel Multi tiered Extragalactic Survey (HerMES) data at 250, 350 and 500 um, to deri
Externí odkaz:
http://arxiv.org/abs/1302.5209
Autor:
Karczewski, O. Ł., Barlow, M. J., Page, M. J., Kuin, N. P. M., Ferreras, I., Baes, M., Bendo, G. J., Boselli, A., Cooray, A., Cormier, D., De Looze, I., Galametz, M., Galliano, F., Lebouteiller, V., Madden, S. C., Pohlen, M., Rémy-Ruyer, A., Smith, M. W. L., Spinoglio, L.
Publikováno v:
MNRAS (May 21, 2013) 431(3): 2493-2512
[Abridged] We present an integrated photometric spectral energy distribution (SED) of the Magellanic-type galaxy NGC 4449 from the far-ultraviolet (UV) to the submillimetre, including new observations acquired by the Herschel Space Observatory. We in
Externí odkaz:
http://arxiv.org/abs/1302.5430