Plasmonic Nanosensors for the Determination of Drug Effectiveness on Membrane Receptors

2016 ◽  
Vol 9 (1) ◽  
pp. 218-223 ◽  
Author(s):  
Rubén Ahijado-Guzmán ◽  
Julia Menten ◽  
Janak Prasad ◽  
Christina Lambertz ◽  
Germán Rivas ◽  
...  
Keyword(s):  
Membrane Receptors ◽  
Drug Effectiveness

Vasodilation and glomerular binding of adrenomedullin in rabbit kidney are not CGRP receptor mediated

1997 ◽  
Vol 273 (2) ◽  
pp. R716-R724 ◽  
Author(s):  
H. Hjelmqvist ◽  
R. Keil ◽  
M. Mathai ◽  
T. Hubschle ◽  
R. Gerstberger
Keyword(s):  
Binding Sites ◽  
Membrane Receptors ◽  
Rabbit Kidney ◽  
Calcitonin Gene ◽  
Body Fluid Homeostasis ◽  
Mild Reduction ◽  
Specific Membrane ◽  
Camp Formation

The polypeptide adrenomedullin (ADM) was infused systemically to conscious rabbits to elucidate its actions on overall circulation and especially the renovascular bed and the formation and/or release of hormones important for body fluid homeostasis, including adrenocortical steroids. ADM lowered mean arterial pressure from 71.5 +/- 3.2 to 64.7 +/- 3.2 mmHg only at the highest dose of 25 pmol.min-1.kg-1 infused intravenously for 20 min and concomitantly induced tachycardia, possibly due to both baroreflex activation and direct cardiostimulatory effects. Renal blood flow (RBF) determined in rabbits chronically equipped with a perivascular ultrasonic flow probe increased from 55.4 +/- 2.1 to 67.4 +/- 2.7 and from 58.2 +/- 3.5 to 75.2 +/- 6.0 ml/min at ADM infusions of 5 and 25 pmol.min-1.kg-1, respectively. The elevation in RBF persisted even in the presence of the calcitonin gene-related peptide (CGRP1 receptor antagonist CGRP-(8-37). Of all osmoregulatory hormones tested, only corticosterone (Cort) plasma concentration increased in response to the highest ADM dose from 17.6 +/- 3.1 to 38.9 +/- 6.2 ng/ml, probably due to haroreflex activation. Subdepressor doses of ADM, however, caused a mild reduction in circulating Cort. Expression of functional high-affinity binding sites specific for ADM in vitro could be demonstrated for the renal artery and outer cortical glomeruli using 125I-labeled rat ADM as radioligand and determination of cellular adenosine 3',5'-cyclic monophosphate (cAMP) formation within the glomeruli. The ineffectiveness of CGRP-(8-37) to displace radiolabeled ADM from its binding sites, to inhibit ADM-induced glomerular cAMP formation, and to prevent ADM-induced renal vasodilation supports the hypothesis of ADM altering renal hemodynamics by interacting with ADM- and not CGRP-specific membrane receptors.

scholarly journals Spectroscopic Determination of Distinct Heme Ligands in Outer-Membrane Receptors PhuR and HasR ofPseudomonas aeruginosa

Biochemistry ◽  
2015 ◽  
Vol 54 (16) ◽  
pp. 2601-2612 ◽  
Author(s):  
Aaron D. Smith ◽  
Anuja R. Modi ◽  
Shengfang Sun ◽  
John H. Dawson ◽  
Angela Wilks
Keyword(s):  
Outer Membrane ◽  
Membrane Receptors ◽  
Spectroscopic Determination ◽  
Heme Ligands

scholarly journals Cloning and Characterization of an Outer Membrane Protein of Vibrio vulnificus Required for Heme Utilization: Regulation of Expression and Determination of the Gene Sequence

1998 ◽  
Vol 66 (7) ◽  
pp. 3134-3141 ◽  
Author(s):  
Christine M. Litwin ◽  
Burke L. Byrne
Keyword(s):  
Amino Acids ◽  
Outer Membrane ◽  
Vibrio Vulnificus ◽  
Outer Membrane Proteins ◽  
Heme Iron ◽  
Membrane Receptors ◽  
Regulation Of Expression ◽  
Reading Frame

ABSTRACT Vibrio vulnificus is a halophilic, marine pathogen that has been associated with septicemia and serious wound infections in patients with iron overload and preexisting liver disease. ForV. vulnificus, the ability to acquire iron from the host has been shown to correlate with virulence. V. vulnificus is able to use host iron sources such as hemoglobin and heme. We previously constructed a fur mutant ofV. vulnificus which constitutively expresses at least two iron-regulated outer membrane proteins, of 72 and 77 kDa. The N-terminal amino acid sequence of the 77-kDa protein purified from theV. vulnificus fur mutant had 67% homology with the first 15 amino acids of the mature protein of the Vibrio cholerae heme receptor, HutA. In this report, we describe the cloning, DNA sequence, mutagenesis, and analysis of transcriptional regulation of the structural gene for HupA, the heme receptor ofV. vulnificus. DNA sequencing of hupAdemonstrated a single open reading frame of 712 amino acids that was 50% identical and 66% similar to the sequence of V. cholerae HutA and similar to those of other TonB-dependent outer membrane receptors. Primer extension analysis localized one promoter for the V. vulnificus hupAgene. Analysis of the promoter region of V. vulnificus hupA showed a sequence homologous to the consensus Fur box. Northern blot analysis showed that the transcript was strongly regulated by iron. An internal deletion in the V. vulnificus hupA gene, done by using marker exchange, resulted in the loss of expression of the 77-kDa protein and the loss of the ability to use hemin or hemoglobin as a source of iron. ThehupA deletion mutant of V. vulnificus will be helpful in future studies of the role of heme iron in V. vulnificus pathogenesis.

Galactic orbits of stars

1966 ◽  
Vol 25 ◽  
pp. 93-97
Author(s):  
Richard Woolley
Keyword(s):  
Globular Cluster ◽  
Potential Field ◽  
High Velocity ◽  
Velocity Vector ◽  
Variable Stars ◽  
The Sun ◽  
Proper Motions ◽  
Rr Lyrae ◽  
The Galaxy

It is now possible to determine proper motions of high-velocity objects in such a way as to obtain with some accuracy the velocity vector relevant to the Sun. If a potential field of the Galaxy is assumed, one can compute an actual orbit. A determination of the velocity of the globular clusterωCentauri has recently been completed at Greenwich, and it is found that the orbit is strongly retrograde in the Galaxy. Similar calculations may be made, though with less certainty, in the case of RR Lyrae variable stars.

Distance to SN 1987A and the LMC

1999 ◽  
Vol 190 ◽  
pp. 549-554
Author(s):  
Nino Panagia
Keyword(s):  
Angular Size ◽  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
Light Curves ◽  
Distance Modulus ◽  
Absolute Size ◽  
Sn 1987A

Using the new reductions of the IUE light curves by Sonneborn et al. (1997) and an extensive set of HST images of SN 1987A we have repeated and improved Panagia et al. (1991) analysis to obtain a better determination of the distance to the supernova. In this way we have derived an absolute size of the ringRabs= (6.23 ± 0.08) x 1017cm and an angular sizeR″ = 808 ± 17 mas, which give a distance to the supernovad(SN1987A) = 51.4 ± 1.2 kpc and a distance modulusm–M(SN1987A) = 18.55 ± 0.05. Allowing for a displacement of SN 1987A position relative to the LMC center, the distance to the barycenter of the Large Magellanic Cloud is also estimated to bed(LMC) = 52.0±1.3 kpc, which corresponds to a distance modulus ofm–M(LMC) = 18.58±0.05.

International determination of the total motion of the pole

1961 ◽  
Vol 13 ◽  
pp. 29-41
Author(s):  
Wm. Markowitz
Keyword(s):  
Secular Motion ◽  
The Future

A symposium on the future of the International Latitude Service (I. L. S.) is to be held in Helsinki in July 1960. My report for the symposium consists of two parts. Part I, denoded (Mk I) was published [1] earlier in 1960 under the title “Latitude and Longitude, and the Secular Motion of the Pole”. Part II is the present paper, denoded (Mk II).

Time and Latitude in South Africa

1972 ◽  
Vol 1 ◽  
pp. 27-38
Author(s):  
J. Hers
Keyword(s):  
South Africa ◽  
Cape Town ◽  
Astronomical Observations ◽  
Royal Observatory ◽  
The Republic ◽  
Astronomical Determination ◽  
Limited Accuracy ◽  
Better Than

In South Africa the modern outlook towards time may be said to have started in 1948. Both the two major observatories, The Royal Observatory in Cape Town and the Union Observatory (now known as the Republic Observatory) in Johannesburg had, of course, been involved in the astronomical determination of time almost from their inception, and the Johannesburg Observatory has been responsible for the official time of South Africa since 1908. However the pendulum clocks then in use could not be relied on to provide an accuracy better than about 1/10 second, which was of the same order as that of the astronomical observations. It is doubtful if much use was made of even this limited accuracy outside the two observatories, and although there may – occasionally have been a demand for more accurate time, it was certainly not voiced.

Large-scale Motion of Solar Filaments

2000 ◽  
Vol 179 ◽  
pp. 205-208
Author(s):  
Pavel Ambrož ◽  
Alfred Schroll
Keyword(s):  
Magnetic Flux ◽  
Proper Motion ◽  
Time Scale ◽  
Large Scale ◽  
Accuracy Of Measurements ◽  
Solar Filaments ◽  
General Movement ◽  
Scale Motion ◽  
Velocity Scatter

AbstractPrecise measurements of heliographic position of solar filaments were used for determination of the proper motion of solar filaments on the time-scale of days. The filaments have a tendency to make a shaking or waving of the external structure and to make a general movement of whole filament body, coinciding with the transport of the magnetic flux in the photosphere. The velocity scatter of individual measured points is about one order higher than the accuracy of measurements.

Practical Realization of a Reference System for Earth Dynamics by Satellite Methods

1975 ◽  
Vol 26 ◽  
pp. 341-380 ◽  
Author(s):  
R. J. Anderle ◽  
M. C. Tanenbaum
Keyword(s):  
Reference Frame ◽  
Polar Motion ◽  
Pole Position ◽  
Control Points ◽  
Significant Information ◽  
Crustal Motion ◽  
Average Reference ◽  
Future Data ◽  
Existing Data

AbstractObservations of artificial earth satellites provide a means of establishing an.origin, orientation, scale and control points for a coordinate system. Neither existing data nor future data are likely to provide significant information on the .001 angle between the axis of angular momentum and axis of rotation. Existing data have provided data to about .01 accuracy on the pole position and to possibly a meter on the origin of the system and for control points. The longitude origin is essentially arbitrary. While these accuracies permit acquisition of useful data on tides and polar motion through dynamio analyses, they are inadequate for determination of crustal motion or significant improvement in polar motion. The limitations arise from gravity, drag and radiation forces on the satellites as well as from instrument errors. Improvements in laser equipment and the launch of the dense LAGEOS satellite in an orbit high enough to suppress significant gravity and drag errors will permit determination of crustal motion and more accurate, higher frequency, polar motion. However, the reference frame for the results is likely to be an average reference frame defined by the observing stations, resulting in significant corrections to be determined for effects of changes in station configuration and data losses.

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