Guinea pig C3(Complement Component 3) ELISA Kit

Name: Guinea pig C3(Complement Component 3) ELISA Kit
SKU: DEIA7754
Rating: 5 (1 reviews)

Regulatory status: For research use only, not for use in diagnostic procedures.

COA

SDS

Datasheet

Summary

Sample

Serum, plasma, tissue homogenates and other biological fluids

Species Reactivity

Guinea pig

Detection Method

sELISA

Intended Use

C3 ELISA Kit allows for the in vitro quantitative determination of C3 concentrations in serum, plasma, tissue homogenates and other biological fluids.

Contents of Kit

Storage

2-8°C for 6 months

Precision

Intra-Assay: CV<8%
Inter-Assay: CV<10%

Detection Range

0.313-20ng/ml

Sensitivity

< 0.188ng/ml

Standard Curve

Results of a typical standard operation of a C3 ELISA Kit are listed below. This standard curve was generated at our lab for demonstration purpose only. Users shall obtain standard curve as per experiment by themselves. (N/A=not applicable)

Citations

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Documents

pdf COA

pdf SDS

pdf Datasheet

QA & Reviews

Customer Reviews

References

Multiwavelength Analysis of the Kinematics of a Long Duration Flare-CME Event on 27 January 2012

SOLAR PHYSICS

Authors: Selvarani, G.; Prasanna Subramanian, S.; Shanmugaraju, A.; Suresh, K.

Abstract

We present a detailed analysis of a long-duration flare associated with a coronal mass ejection (CME) event that occurred on 27 January 2012 in the active region (AR) 11402. We analyze the kinematics of the CME and the close relationship between the flare, radio burst, and CME. We used STEREO (Solar Terrestrial Relations Observatory)/EUVI A (Extreme Ultraviolet Imager) and white light data from STEREO (COR1 A and COR2 A) and LASCO (Large Angle and Spectrometric COronagraph) (C2/C3) coronagraphs, and X-ray data from the GOES (Geostationary Operational Environmental Satellite) spacecraft. The height of the CME is measured using the Graduated Cylindrical Shell (GCS) model. Our results show that: i) the speed of the CME (1460 km/s at 2.54 R-circle dot) is comparable to the speed of the type II radio burst (1581 km/s), ii) the height of the type II radio burst is lower than that of the CME leading edge, iii) the CME acceleration phase is found to be related to the rise time of the flare and its propagation phase is related to the decay phase of the flare, iv) the type II radio burst origin is likely to be near the CME region where a CME-streamer interaction takes place around 1.6 R-circle dot, and v) the sequence of events and the CME kinematics show a close association between the CME and type II radio emissions.

A Natural Alkaloid, beta-Carboline, as a One- and Two-Photon Responsive Fluorescent Photoremovable Protecting Group: Sequential Release of the Same or Different Carboxylic Acids

ORGANIC LETTERS

Authors: Sikder, Antara; Banerjee, Moumita; Singha, Tara; Mondal, Saugat; Datta, P. K.; Anoop, Anakuthil; Singh, N. D. Pradeep

Abstract

The beta-carboline moiety, substituted at the C1 and C3 benzylic positions with a leaving group, has been demonstrated for the first time as a photoremovable protecting group for time-dependent sequential release of two (same or different) carboxylic acids upon one- and two-photon light irradiation. Density functional theory calculations suggest that the electronic environment of the beta-carboline moiety at C1 and C3 positions plays a key role in the rate of photorelease.