Zobrazeno 1 - 10
of 207
pro vyhledávání: '"Tuffs, R J"'
Autor:
van der Giessen, S. A., Leslie, S. K., Groves, B., Hodge, J. A., Popescu, C. C., Sargent, M. T., Schinnerer, E., Tuffs, R. J.
Publikováno v:
A&A 662, A26 (2022)
(Abridged) In this paper, we use the Tuffs et al. attenuation - inclination models in ultraviolet (UV), optical, and near-infrared (NIR) bands to investigate the average global dust properties in galaxies as a function of stellar mass $M_{*}$, stella
Externí odkaz:
http://arxiv.org/abs/2201.10568
Autor:
Grootes, M. W., Dvornik, A., Laureijs, R. J., Tuffs, R. J., Popescu, C. C., Robotham, A. S. G., Liske, J., Brown, M. J. I., Holwerda, B. W., Wang, L.
We present a detailed analysis of the specific star formation rate -- stellar mass ($\mathrm{sSFR}-M_*$) of $z\le 0.13$ disk central galaxies using a morphologically selected mass-complete sample ($M_* \ge 10^{9.5} M_{\odot}$). Considering samples of
Externí odkaz:
http://arxiv.org/abs/1803.04962
We present a solution for the ultraviolet (UV) - submillimeter (submm) interstellar radiation fields (ISRFs) of the Milky Way, derived from modelling COBE, IRAS and Planck maps of the all-sky emission in the near-, mid-, far-infrared and submm.The an
Externí odkaz:
http://arxiv.org/abs/1705.06652
Autor:
Grootes, M. W., Tuffs, R. J., Popescu, C. C., Norberg, P., Robotham, A. S. G., Liske, J., Andrae, E., Baldry, I. K., Gunawardhana, M., Kelvin, L. S., Madore, B. F., Seibert, M., Taylor, E. N., Alpaslan, M., Brown, M. J. I., Cluver, M. E., Driver, S. P., Bland-Hawthorn, J., Holwerda, B. W., Hopkins, A. M., Lopez-Sanchez, A. R., Loveday, J., Rushton, M.
Abridged - We quantify the effect of the galaxy group environment (for 12.5 < log(M_group/Msun) < 14.0) on the star formation rates of the (morphologically-selected) population of disk-dominated local Universe spiral galaxies (z < 0.13) with stellar
Externí odkaz:
http://arxiv.org/abs/1612.07322
Autor:
Lavoie, S., Willis, J. P., Democles, J., Eckert, D., Gastaldello, F., Smith, G. P., Lidman, C., Adami, C., Pacaud, F., Pierre, M., Clerc, N., Giles, P., Lieu, M., Chiappetti, L., Altieri, B., Ardila, F., Baldry, I., Bongiorno, A., Desai, S., Elyiv, A., Faccioli, L., Gardner, B., Garilli, B., Groote, M. W., Guennou, L., Guzzo, L., Hopkins, A. M., Liske, J., McGee, S., Melnyk, O., Owers, M. S., Poggianti, B., Ponman, T. J., Scodeggio, M., Spitler, L., Tuffs, R. J.
The growth of brightest cluster galaxies is closely related to the properties of their host cluster. We present evidence for dry mergers as the dominant source of BCG mass growth at $z\lesssim1$ in the XXL 100 brightest cluster sample. We use the glo
Externí odkaz:
http://arxiv.org/abs/1608.01223
Autor:
Wang, L., Norberg, P., Gunawardhana, M. L. P., Heinis, S., Baldry, I. K., Bland-Hawthorn, J., Bourne, N., Brough, S., Brown, M. J. I., Cluver, M. E., Cooray, A., da Cunha, E., Driver, S. P., Dunne, L., Dye, S., Eales, S., Grootes, M. W., Holwerda, B. W., Hopkins, A. M., Ibar, E., Ivison, R., Lacey, C., Lara-Lopez, M. A., Loveday, J., Maddox, S. J., lowski, M. J. Micha, Oteo, I., Owers, M. S., Popescu, C. C., Smith, D. J. B., Taylor, E. N., Tuffs, R. J., van der Werf, P.
We compare common star-formation rate (SFR) indicators in the local Universe in the GAMA equatorial fields (around 160 sq. deg.), using ultraviolet (UV) photometry from GALEX, far-infrared (FIR) and sub-millimetre (sub-mm) photometry from H-ATLAS, an
Externí odkaz:
http://arxiv.org/abs/1607.02971
Autor:
Jarrett, T. H., Cluver, M. E., Magoulas, C., Bilicki, M., Alpaslan, M., Bland-Hawthorn, J., Brough, S., Brown, M. J. I., Croom, S., Driver, S., Holwerda, B. W., Hopkins, A. M., Loveday, J., Norberg, P., Peacock, J. A., Popescu, C. C., Sadler, E. M., Taylor, E. N., Tuffs, R. J., Wang, L.
We present an analysis of the mid-infrared WISE sources seen within the equatorial GAMA G12 field, located in the North Galactic Cap. Our motivation is to study and characterize the behavior of WISE source populations in anticipation of the deep mult
Externí odkaz:
http://arxiv.org/abs/1607.01190
Autor:
Bourne, N., Dunne, L., Maddox, S. J., Dye, S., Furlanetto, C., Hoyos, C., Smith, D. J. B., Eales, S., Smith, M. W. L., Valiante, E., Alpaslan, M., Andrae, E., Baldry, I. K., Cluver, M. E., Cooray, A., Driver, S. P., Dunlop, J. S., Grootes, M. W., Ivison, R. J., Jarrett, T. H., Liske, J., Madore, B. F., Popescu, C. C., Robotham, A. G., Rowlands, K., Seibert, M., Thompson, M. A., Tuffs, R. J., Viaene, S., Wright, A. H.
This paper is the second in a pair of articles presenting data release 1 (DR1) of the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS), the largest single open-time key project carried out with the Herschel Space Observatory. The H-ATLAS
Externí odkaz:
http://arxiv.org/abs/1606.09254
Autor:
Davies, L. J. M., Driver, S. P., Robotham, A. S. G., Grootes, M. W., Popescu, C. C., Tuffs, R. J., Hopkins, A., Alpaslan, M., Andrews, S. K., Bland-Hawthorn, J., Bremer, M. N., Brough, S., Brown, M. J. I., Cluver, M. E., Croom, S., da Cunha, E., Dunne, L., Lara-Lopez, M. A., Liske, J., Loveday, J., Moffett, A. J., Owers, M., Phillipps, S., Sansom, A. E., Taylor, E. N., Michalowski, M. J., Ibar, E., Smith, M., Bourne, N.
We present a meta-analysis of star-formation rate (SFR) indicators in the GAMA survey, producing 12 different SFR metrics and determining the SFR-M* relation for each. We compare and contrast published methods to extract the SFR from each indicator,
Externí odkaz:
http://arxiv.org/abs/1606.06299
Autor:
Wright, A. H., Robotham, A. S. G., Bourne, N., Driver, S. P., Dunne, L., Maddox, S. J., Alpaslan, M., Andrews, S. K., Bauer, A. E., Bland-Hawthorn, J., Brough, S., Brown, M. J. I., Cluver, M., Davies, L. J. M., Holwerda, B. W., Hopkins, A. M., Jarrett, T. H., Kafle, P. R., Lange, R., Liske, J., Loveday, J., Moffett, A. J., Norberg, P., Popescu, C. C., Smith, M., Taylor, E. N., Tuffs, R. J., Wang, L., Wilkins, S. M.
We present the Lambda Adaptive Multi-Band Deblending Algorithm in R (LAMBDAR), a novel code for calculating matched aperture photometry across images that are neither pixel- nor PSF-matched, using prior aperture definitions derived from high resoluti
Externí odkaz:
http://arxiv.org/abs/1604.01923