Zobrazeno 1 - 10
of 169
pro vyhledávání: '"Samui, S."'
We present results of our time variability studies of Mg II and Al III absorption lines in a sample of 22 Low Ionization Broad Absorption Line QSOs (LoBAL QSOs) at 0.2 <= zem <= 2.1 using the 2m telescope at IUCAA Girawali Observatory over a time-sca
Externí odkaz:
http://arxiv.org/abs/1402.2980
Autor:
Thompson, M. A., Smith, D. J. B., Stevens, J. A., Jarvis, M. J., Perez, E. Vidal, Marshall, J., Dunne, L., Eales, S., White, G. J., Leeuw, L., Sibthorpe, B., Baes, M., Gonzalez-Solares, E., Scott, D., Vieiria, J., Amblard, A., Auld, R., Bonfield, D. G., Burgarella, D., Buttiglione, S., Cava, A., Clements, D. L., Cooray, A., Dariush, A., de Zotti, G., Dye, S., Frayer, D., Fritz, J., Gonzalez-Nuevo, J., Herranz, D., Ibar, E., Ivison, R. J., Lagache, G., Lopez-Caniego, M., Maddox, S., Negrello, M., Pascale, E., Pohlen, M., Rigby, E., Rodighiero, G., Samui, S., Serjeant, S., Temi, P., Valtchanov, I., Verma, A.
Aims: We aim to demonstrate that the Herschel ATLAS (H-ATLAS) is suitable for a blind and unbiased survey for debris disks by identifying candidate debris disks associated with main sequence stars in the initial science demonstration field of the sur
Externí odkaz:
http://arxiv.org/abs/1005.3018
Autor:
Dye, S., Dunne, L., Eales, S., Smith, D. J. B., Amblard, A., Auld, R., Baes, M., Baldry, I. K., Bamford, S., Blain, A. W., Bonfield, D. G., Bremer, M., Burgarella, D., Buttiglione, S., Cameron, E., Cava, A., Clements, D. L., Cooray, A., Croom, S., Dariush, A., de Zotti, G., Driver, S., Dunlop, J. S., Frayer, D., Fritz, J., Gardner, Jonathan P., Gomez, H. L., Gonzalez-Nuevo, J., Herranz, D., Hill, D., Hopkins, A., Ibar, E., Ivison, R. J., Jarvis, M. J., Jones, D. H., Kelvin, L., Lagache, G., Leeuw, L., Liske, J., Lopez-Caniego, M., Loveday, J., Maddox, S., Michałowski, M. J., Negrello, M., Norberg, P., Page, M. J., Parkinson, H., Pascale, E., Peacock, J. A., Pohlen, M., Popescu, C., Prescott, M., Rigopoulou, D., Robotham, A., Rigby, E., Rodighiero, G., Samui, S., Scott, D., Serjeant, S., Sharp, R., Sibthorpe, B., Temi, P., Thompson, M. A., Tuffs, R., Valtchanov, I., van der Werf, P. P., van Kampen, E., Verma, A.
Publikováno v:
Astron.Astrophys. 518 (2010) L10
We have determined the luminosity function of 250um-selected galaxies detected in the ~14 sq.deg science demonstration region of the Herschel-ATLAS project out to a redshift of z=0.5. Our findings very clearly show that the luminosity function evolve
Externí odkaz:
http://arxiv.org/abs/1005.2411
Autor:
Maddox, S. J., Dunne, L., Rigby, E., Eales, S., Cooray, A., Scott, D., Peacock, J. A., Negrello, M., Smith, D. J. B., Benford, D., Amblard, A., Auld, R., Baes, M., Bonfield, D., Burgarella, D., Buttiglione, S., Cava, A., Clements, D., Dariush, A., de Zotti, G., Dye, S., Frayer, D., Fritz, J., Gonzalez-Nuevo, J., Herranz, D., Ibar, E., Ivison, R., Jarvis, M. J., Lagache, G., Leeuw, L., Lopez-Caniego, M., Pascale, E., Pohlen, M., Rodighiero, G., Samui, S., Serjeant, S., Temi, P., Thompson, M., Verma, A.
We present measurements of the angular correlation function of galaxies selected from the first field of the H-ATLAS survey. Careful removal of the background from galactic cirrus is essential, and currently dominates the uncertainty in our measureme
Externí odkaz:
http://arxiv.org/abs/1005.2406
Autor:
Serjeant, S., Bertoldi, F., Blain, A. W., Clements, D. L., Cooray, A., Danese, L., Dunlop, J., Dunne, L., Eales, S., Falder, J., Hatziminaoglou, E., Hughes, D. H., Ibar, E., Jarvis, M. J., Lawrence, A., Lee, M. G., Michałowski, M., Negrello, M., Omont, A., Page, M., Pearson, C., van der Werf, P. P., White, G., Amblard, A., Auld, R., Baes, M., Bonfield, D. G., Burgarella, D., Buttiglione, S., Cava, A., Dariush, A., de Zotti, G., Dye, S., Frayer, D., Fritz, J., Gonzalez-Nuevo, J., Herranz, D., Ivison, R. J., Lagache, G., Leeuw, L., Lopez-Caniego, M., Maddox, S., Pascale, E., Pohlen, M., Rigby, E., Rodighiero, G., Samui, S., Sibthorpe, B., Smith, D. J. B., Temi, P., Thompson, M., Valtchanov, I., Verma, A.
We present a derivation of the star formation rate per comoving volume of quasar host galaxies, derived from stacking analyses of far-infrared to mm-wave photometry of quasars with redshifts 0I_AB>-32. We use t
Externí odkaz:
http://arxiv.org/abs/1005.2410
Autor:
Clements, D. L., Rigby, E., Maddox, S., Dunne, L., Mortier, A., Pearson, C., Amblard, A., Auld, R., Baes, M., Bonfield, D., Burgarella, D., Buttiglione, S., Cava, A., Cooray, A., Dariush, A., de Zotti, G., Dye, S., Eales, S., Frayer, D., Fritz, J., Gardner, Jonathan P., Gonzalez-Nuevo, J., Herranz, D., Ibar, E., Ivison, R., Jarvis, M. J., Lagache, G., Leeuw, L., Lopez-Caniego, M., Negrello, M., Pascale, E., Pohlen, M., Rodighiero, G., Samui, S., Serjeant, S., Sibthorpe, B., Scott, Douglas, Smith, D. J. B., Temi, P., Thompson, M., Valtchanov, I., van der Werf, P., Verma, A.
Aims. The Herschel-ATLAS survey (H-ATLAS) will be the largest area survey to be undertaken by the Herschel Space Observatory. It will cover 550 sq. deg. of extragalactic sky at wavelengths of 100, 160, 250, 350 and 500 microns when completed, reachin
Externí odkaz:
http://arxiv.org/abs/1005.2409
Autor:
González-Nuevo, J., De Zotti, G., Andreani, P., Barton, E. J., Bertoldi, F., Birkinshaw, M., Bonavera, L., Buttiglione, S., Cooke, J., Cooray, A., Danese, G., Dunne, L., Eales, S., Fan, L., Jarvis, M. J., Klöckner, H-R., Hatziminaoglou, E., Herranz, D., Hughes, D. H., Lapi, A., Lawrence, A., Leeuw, L., López-Caniego, M., Massardi, M., Mauch, T., Michalowski, M. J., Negrello, M., Rawlings, S., Rodighiero, G., Samui, S., Serjeant, S., Vieira, J. D., White, G., Amblard, A., Auld, R., Baes, M., Bonfield, D. G., Burgarella, D., Cava, A., Clements, D. L., Dariush, A., Dye, S., Frayer, D., Fritz, J., Ibar, E., Ivison, R. J., Lagache, G., Maddox, S., Pascale, E., Pohlen, M., Rigby, E., Sibthorpe, B., Smith, D. J. B., Temi, P., Thompson, M., Valtchanov, I., Verma, A.
To investigate the poorly constrained sub-mm counts and spectral properties of blazars we searched for these in the Herschel-ATLAS (H-ATLAS) science demostration phase (SDP) survey catalog. We cross-matched 500$\mu$m sources brighter than 50 mJy with
Externí odkaz:
http://arxiv.org/abs/1005.2407
Autor:
Amblard, A., Cooray, A., Serra, P., Temi, P., Barton, E., Negrello, M., Auld, R., Baes, M., Baldry, I. K., Bamford, S., Blain, A., Bock, J., Bonfield, D., Burgarella, D., Buttiglione, S., Cameron, E., Cava, A., Clements, D., Croom, S., Dariush, A., de Zotti, G., Driver, S., Dunlop, J., Dunne, L., Dye, S., Eales, S., Frayer, D., Fritz, J., Gardner, Jonathan P., Gonzalez-Nuevo, J., Herranz, D., Hill, D., Hopkins, A., Hughes, D. H., Ibar, E., Ivison, R. J., Jarvis, M., Jones, D. H., Kelvin, L., Lagache, G., Leeuw, L., Liske, J., Lopez-Caniego, M., Loveday, J., Maddox, S., Michalowski, M., Norberg, P., Parkinson, H., Peacock, J. A., Pearson, C., Pascale, E., Pohlen, M., Popescu, C., Prescott, M., Robotham, A., Rigby, E., Rodighiero, G., Samui, S., Sansom, A., Scott, D., Serjeant, S., Sharp, R., Sibthorpe, B., Smith, D. J. B., Thompson, M. A., Tuffs, R., Valtchanov, I., Van Kampen, E., Van der Werf, P., Verma, A., Vieira, J., Vlahakis, C.
We present colour-colour diagrams of detected sources in the Herschel-ATLAS Science Demonstration Field from 100 to 500 microns using both PACS and SPIRE. We fit isothermal modified black bodies to the spectral energy distribution (SED) to extract th
Externí odkaz:
http://arxiv.org/abs/1005.2412
Autor:
Baes, M., Fritz, J., Gadotti, D. A., Smith, D. J. B., Dunne, L., da Cunha, E., Amblard, A., Auld, R., Bendo, G. J., Bonfield, D., Burgarella, D., Buttiglione, S., Cava, A., Clements, D., Cooray, A., Dariush, A., de Zotti, G., Dye, S., Eales, S., Frayer, D., Gonzalez-Nuevo, J., Herranz, D., Ibar, E., Ivison, R., Lagache, G., Leeuw, L., Lopez-Caniego, M., Jarvis, M., Maddox, S., Negrello, M., Michalowski, M., Pascale, E., Pohlen, M., Rigby, E., Rodighiero, G., Samui, S., Serjeant, S., Temi, P., Thompson, M., van der Werf, P., Verma, A., Vlahakis, C.
We use Herschel PACS and SPIRE observations of the edge-on spiral galaxy UGC 4754, taken as part of the H-ATLAS SDP observations, to investigate the dust energy balance in this galaxy. We build detailed SKIRT radiative models based on SDSS and UKIDSS
Externí odkaz:
http://arxiv.org/abs/1005.1773
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.