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A multi-wavelength study of the proto-cluster surrounding the

which predict only 1 such source in our map 32.1 13 38 29.81 −19 39 31.9 R1 (e.g. Dannerbauer et al., 2002; Dunlop et

K-band imaging of 52 B3-VLA quasars: Nucleus and host

30 quasars with 0.1 Jy S408 0.4 Jy Dunlop et al. 1993, and their updated work (iii) gaussian + r1/4 law; (iv) gaussian +

Defying jet-gas alignment in two radio galaxies at z~2 with

100 0 -100 -200 -2 -1 0 1 offset [arcsec4 of the Very Large Telescope (VLT) of ESO. 1.0 1.2 1.4 1.6 1.8 2.0 R1/4 [kpc] Fig

Star formation in luminous quasar host galaxies at z= 1–2

(McLure et al. 1999; Dunlop et al. 2003; 1.923 20.3 0.049 4C45.51 RLQ 1.992 20.6 or an r1/4 de Vaucouleurs law characteristic

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0.4 z 1 99 Fig. 2.—Distributions in McLure Dunlop 2002; Marconi Hunt 2003).archive.stsci.edu/pub/ hlsp/goods/catalog_ r1

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Selective SUMO modification of cAMP-specific

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Combining physical galaxy models with radio observations to

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Magnetostratigraphy of the Fossil-Rich Shungura Formation,

magnetization at temperatures of 100 °C to 200 corrected according to Dunlop (2002) (Fig. 3d)1 4 3 1 1 1 1 R3 Mammoth top B-2/3; (

Cleaning and recirculation of perfluorohexane (C 6 F 14 ) in

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The R1e of the General Practitioner in Obstetric Practice.

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The HST Survey of BL Lacertae Objects. II. Host Galaxies

(rms dispersion), at least one magnitude brighter(Dunlop et al. 1996; Ridgway Stockton 1997; and follow quite well a r1/4 law, so the

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Simultaneous 31P MRS of the soleus and gastrocnemius in

again, a kinetic order of 1 was not observedAm J Physiol 273: R999-R1107, 1997. Dunlop, RS, Falconer, T, Stanley, C, Ho

Direct calculation of the ring current distribution and

properties from four spacecraft measurements has been developed by Shen et 100 nT/RE (albeit for short intervals of time), only one fourth of

black hole-to-galaxy mass ratios of luminous quasars at z 4

and black hole-to-galaxy mass ratios of luminous quasars at z ≃ 4Targett, T., Dunlop, J.S., McLure, R.J.: MNRAS 420 , 3621 (2012

coactivator TIF2 and the corepressor SMRT are primary 1α,

NCoR1, nuclear corepressor 1; NR, nuclear , Volumes 89–90, May 2004, Pages 1–4Dunlop, T. W., Va¨isa¨nen, S., Frank,

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L∗; see Dunlop 2001, Percival et al. 2001)(I Zw 1 – Barvainis, Alloin Antonucci were fit better by disk profiles than r1/4

Cross-correlation of the 2-10 keV XRB with radio sources:

(r1)dV1 εb(r2) 4πrL2 2 dV2 (4-3) Dunlop Peacock (1990) with low flux cutoffs pc−3 where h = H◦/100kms−1M pc−1

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of attributes in R2, such that F K is a primary key in relation R1. Links of type 3 and 4 are special cases of types 1 and 2 above: Link