Spin-isospin selectivity in three-nucleon forces (2009)
Mardanpour, H., Amir-Ahmadi, H. R., Benard, R., Biegun, A., Eslami-Kalantari, M., Joulaeizadeh, L., ...
Precision data are presented for the break-up reaction, $^2{\rm H}(\vec p,pp)n$, within the framework of nuclear-force studies. The experiment was carried out at KVI using a polarized-proton beam of...
A 3-D study of the photosphere of HD99563: I. Pulsation analysis (2009)
Freyhammer, L. M., Kurtz, D. W., Elkin, V. G., Mathys, G., Savanov, I., Zima, W., ...
We have used high-speed spectroscopy of the rapidly oscillating Ap (roAp) star HD99563 to study the pulsation amplitude and phase behaviour of elements in its stratified atmosphere over one 2.91-d...
Properties of X-ray-selected broad absorption-line quasars (2008)
Blustin, A. J., Dwelly, T., Page, M. J., McHardy, I. M., Seymour, N., Kennea, J. A., ...
Broad absorption-line quasars (commonly termed BALQSOs) contain the most dramatic examples of active galactic nucleus (AGN) driven winds. The high absorbing columns in these winds, ~10^24 cm^-2,...
On the evolution of clustering of 24-μm-selected galaxies (2008)
Magliocchetti, Manuela, Cirasuolo, Michele, McLure, R.J., Dunlop, J.S., Almaini, O., Foucaud, S., ...
This paper investigates the clustering properties of a complete sample of 1041 24um-selected sources brighter than F[24um]=400 uJy in the overlapping region between the SWIRE and UKIDSS UDS surveys....
Properties of X-ray selected Broad Absorption Line Quasars (2008)
Blustin, A. J., Dwelly, T., Page, M. J., McHardy, I. M., Seymour, N., Kennea, J. A., ...
Broad absorption line quasars (commonly termed BALQSOs) contain the most dramatic examples of AGN-driven winds. The high absorbing columns in these winds, ~10^24 cm^-2, ensure that BALQSOs are...
Ihara, E., Wakasa, T., Dozono, M., Hatanaka, K., Imamura, T., Kato, M., ...
The cross-sections and analyzing powers for $(p,n)$ reactions on ${}^{3}{\rm He}$ and ${}^{4}{\rm He}$ have been measured at a bombarding energy of $T_p$ = 346 MeV and reaction angles of $\theta_{\rm...
Clements, D. L., Vaccari, M., Babbedge, T., Oliver, S., Rowan-Robinson, M., Davoodi, P., ...
We present the optical-to-submillimetre spectral energy distributions (SEDs) for 33 radio and mid-infrared (mid-IR) identified submillimetre galaxies discovered via the SHADES 850-μm SCUBA imaging...
The pulsation modes of the pre-white dwarf PG 1159-035 (2008)
Costa, J. E. S., Kepler, S. O., Winget, D. E., O'Brien, M. S., Kawaler, S. D., Costa, A. F. M., ...
Context. PG 1159-035, a pre-white dwarf with T_(eff) ≃ 140 000 K, is the prototype of both two classes: the PG 1159 spectroscopic class and the DOV pulsating class. Previous studies of PG 1159-035...
Analyzing powers Ayy, Axx, Axz and Ay in the dd->3Hen reaction at 270 MeV (2007)
Janek, M., Saito, T., Ladygin, V. P., Uesaka, T., Hatano, M., Isupov, A. Yu., ...
The data on the tensor Ayy, Axx, Axz and vector Ay analyzing powers in the dd->3Hen obtained at Td= 270 MeV in the angular range 0 - 110 degrees in the c.m. are presented. The observed negative sign...
Mardanpour, H., Amir-Ahmadi, H. R., Deltuva, A., Itoh, K., Kalantar-Nayestanaki, N., Kawabata, T., ...
High precision vector and tensor analyzing powers of elastic deuteron-proton d+p scattering have been measured at intermediate energies to investigate effects of three-nucleon forces (3NF). Angular...
The UKIRT infrared deep sky survey early data release (2006)
Dye, S., Warren, S.J., Hambly, N.C., Cross, N.J.G., Hodgkin, S.T., Irwin, M.J., ...
This paper defines the UKIRT Infrared Deep Sky Survey (UKIDSS) Early Data Release (EDR). UKIDSS is a set of five large near-infrared surveys being undertaken with the United Kingdom Infrared...
Galaxy clusters at 0.6 < z < 1.4 in the UKIDSS ultra deep survey early data release (2006)
Van Breukelen, C., Clewley, L., Bonfield, D.G., Rawlings, S., Jarvis, M.J., Barr, J.M., ...
We present the first cluster catalogue extracted from the UKIRT Infrared Deep Sky Survey (UKIDSS) Early Data Release. The catalogue is created using UKIDSS Ultra Deep Survey infrared J and K data...
Coppin, K., Chapin, E. L., Mortier, A. M. J., Scott, S. E., Borys, C., Dunlop, J. S., ...
We present the maps, source catalogue and number counts of the largest, most complete and unbiased extragalactic submillimetre survey ever undertaken: the 850-micron SCUBA HAlf Degree Extragalactic...
McLure, R. J., Cirasuolo, M., Dunlop, J. S., Sekiguchi, K., Almaini, O., Foucaud, S., ...
We have exploited the large area coverage of the combined UKIDSS Ultra Deep Survey (UDS) and Subaru/XMM-Newton Deep Survey (SXDS) to search for bright Lyman-break galaxies (LBGs) at z >= 5. Using the...
The proper motion of the isolated neutron star RX J1605.3+3249 (2005)
Motch, C., Sekiguchi, K., Haberl, F., Zavlin, V. E., Schwope, A., Pakull, M. W.
A simplified laminin nomenclature (2005)
Aumailley, M., Bruckner-Tuderman, L., Carter, W. G., Deutzmann, R., Edgar, D., Ekblom, P., ...
The Discovery of Primeval Large-Scale Structures with Forming Clusters at Redshift 6 (2004)
Ouchi, M., Shimasaku, K., Akiyama, M., Sekiguchi, K., Furusawa, H., Okamura, S., ...
We report the discovery of primeval large-scale structures (LSSs) including two proto-clusters in a forming phase at z=5.7. We carried out extensive deep narrow-band imaging in the 1 deg^2 sky of the...
Association between laminin-8 and glial tumor grade, recurrence, and patient survival (2004)
Ljubimova, J. Y., Fugita, M., Khazenzon, N. M., Das, A., Pikul, B. B., Newman, D., ...
XMM-Newton observations reveal AGN in apparently normal galaxies (2003)
Severgnini, P., Caccianiga, A., Braito, V., Della Ceca, R., Maccacaro, T., Wolter, A., ...
XMM-Newton observations reveal AGN in apparently normal galaxies (2003)
Severgnini, P., Caccianiga, A., Braito, V., Della Ceca, R., Maccacaro, T., Wolter, A., ...
An electrically powered binary star? (2002)
Wu, K., Cropper, M., Ramsay, G., Sekiguchi, K.
We propose a model for stellar binary systems consisting of a magnetic and a non-magnetic white dwarf pair which is powered principally by electrical energy. In our model the luminosity is caused by...