Zobrazeno 1 - 10
of 211
pro vyhledávání: '"Cluver, M E"'
Autor:
Van Kempen, W., Cluver, M. E., Jarrett, T. H., Croton, D. J., Lambert, T. S., Kilborn, V. A., Taylor, E. N., Magoulas, C., Yao, H. F. M.
Environment has long been known to impact the evolution of galaxies, but disentangling its effects from mass evolution requires careful analysis of statistically significant samples. By implementing advanced visualisation methods to test group-findin
Externí odkaz:
http://arxiv.org/abs/2410.15548
Autor:
Cluver, M. E., Jarrett, T. H., Dale, D. A., Smith, J. -D. T., Brown, M. J. I., van Kempen, W., Lengerer, E., Incoll, R., Davey, C., Holloway, R., Cameron, J., Sheth, K.
In this work we present source-tailored WISE mid-infrared photometry (at 3.4$\mu$m, 4.6$\mu$m, 12$\mu$m, and 23$\mu$m) of 2812 galaxies in the extended Spitzer Survey of Stellar Structure in Galaxies (S$^4$G) sample, and characterise the mid-infrared
Externí odkaz:
http://arxiv.org/abs/2410.13483
It has been suggested that the bulge-to-total stellar mass ratio or feedback from black holes (BHs), traced by the BH-to-(total stellar) mass ratio, might establish a galaxy's specific star formation rate (sSFR). We reveal that a galaxy's morphology
Externí odkaz:
http://arxiv.org/abs/2312.03999
Autor:
Jarrett, T. H., Cluver, M. E., Taylor, Edward N., Bellstedt, Sabine, Robotham, A. S. G, Yao, H. F. M.
We derive new empirical scaling relations between WISE mid-infrared galaxy photometry and well-determined stellar masses from SED modeling of a suite of optical-infrared photometry provided by the DR4 Catalogue of the GAMA-KiDS-VIKING survey of the s
Externí odkaz:
http://arxiv.org/abs/2301.05952
Autor:
Yao, H. F. M., Cluver, M. E., Jarrett, T. H., Jozsa, Gyula I. G., Santos, M. G., Marchetti, L., Brown, M. J. I., Gordon, Y. A., Brough, S., Hopkins, A. M., Holwerda, B. W., Driver, S. P., Sadler, E. M.
The identification of AGN in large surveys has been hampered by seemingly discordant classifications arising from differing diagnostic methods, usually tracing distinct processes specific to a particular wavelength regime. However, as shown in Yao et
Externí odkaz:
http://arxiv.org/abs/2208.01679
Autor:
Sureshkumar, U., Durkalec, A., Pollo, A., Bilicki, M., Cluver, M. E., Bellstedt, S., Farrow, D. J., Loveday, J., Taylor, E. N., Bland-Hawthorn, J.
Publikováno v:
A&A 669, A27 (2023)
We investigate how different mid-infrared (mid-IR) properties of galaxies trace the environment in which the galaxies are located. For this purpose, we first study the dependence of galaxy clustering on the absolute magnitude at 3.4 $\mu$m and redshi
Externí odkaz:
http://arxiv.org/abs/2201.10480
Autor:
Murugeshan, C., Kilborn, V. A., For, B. -Q., Wong, O. I., Wang, J., Westmeier, T., Stevens, A. R. H., Spekkens, K., Kamphuis, P., Staveley-Smith, L., Lee-Waddell, K., Kleiner, D., Koribalski, B. S., Cluver, M. E., Oh, S. -H., Rhee, J., Catinella, B., Reynolds, T. N., Denes, H., Elagali, A.
We use high-resolution ASKAP observations of galaxies in the Eridanus supergroup to study their HI, angular momentum and star formation properties, as part of the WALLABY pre-pilot survey efforts. The Eridanus supergroup is composed of three sub-grou
Externí odkaz:
http://arxiv.org/abs/2108.04414
Autor:
Chen, Qingxiang, Meyer, Martin, Popping, Attila, Staveley-Smith, Lister, Bryant, Julia, Delhaize, Jacinta, Holwerda, B. W., Cluver, M. E., Loveday, J., Lopez-Sanchez, Angel R., Zwaan, Martin, Taylor, E. N., Hopkins, A. M., Wright, Angus, Driver, Simon, Brough, S.
We use the 21 cm emission line data from the DINGO-VLA project to study the atomic hydrogen gas H\,{\textsc i} of the Universe at redshifts $z<0.1$. Results are obtained using a stacking analysis, combining the H\,{\textsc i} signals from 3622 galaxi
Externí odkaz:
http://arxiv.org/abs/2104.07973
Autor:
Guillard, P., Appleton, P. N, Boulanger, F., Shull, J. M., Lehnert, M. D., Forets, G. Pineau des, Falgarone, E., Cluver, M. E., Xu, C. K., Gallagher, S. C., Duc, P. A.
We present Hubble Space Telescope Cosmic Origin Spectrograph (COS) UV line spectroscopy and integral-field unit (IFU) observations of the intra-group medium in Stephan's Quintet (SQ). SQ hosts a 30 kpc long shocked ridge triggered by a galaxy collisi
Externí odkaz:
http://arxiv.org/abs/2102.06843
Autor:
Vázquez-Mata, J. A., Loveday, J., Riggs, S. D., Baldry, I. K., Davies, L. J. M., Robotham, A. S. G., Holwerda, B. W., Brown, M. J. I., Cluver, M. E., Wang, L., Alpaslan, M., Bland-Hawthorn, J., Brough, S., Driver, S. P., Hopkins, A. M., Taylor, E. N., Wright, A. H.
How do galaxy properties (such as stellar mass, luminosity, star formation rate, and morphology) and their evolution depend on the mass of their host dark matter halo? Using the Galaxy and Mass Assembly (GAMA) group catalogue, we address this questio
Externí odkaz:
http://arxiv.org/abs/2009.08212