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This may seem like a somewhat silly exercise, but a little glitz and showmanship can go a long way toward uniting a project team A simple mockup such as this one shows the customers something tangible early on that they can understand Database models and relational designs are your eventual goal, but they are too abstract to generate much excitement with all but the nerdliest customers Putting a customer s face on a mockup will almost certainly grab and hold their attention After lunch, you present your mockup and let Charlie and Sveta suggest improvements That may be as far as you get during this session Before the next session, you build an improved mockup with Sveta s picture so she doesn t feel left out and to show that you listened to their suggestions and made appropriate changes.

For nearby objects z 1 and so d1um ~ dphys ie the objects really are just as far away as they look But more distant objects appear further away (dl um > d phys ) than they really are If the geometry is not flat, this gives an additional effect which can either enhance this trend (hyperbolic geometry) or oppose it (spherical geometry) - see Problem A22 Provided there is no cosmological constant, there are useful analytic forms for the luminosity distance as a function of redshift, related to an equation known as the Mattig equation, but once a cosmological constant is introduced calculations have to be done numerically A detailed account can be found in Peacock's textbook (see Bibliography) Before we can use the luminosity distance in practice, there is a problem to overcome.

The following list describes a few things to consider when you build this kind of mockup: Decide what tool you want to use Use a tool that you nd comfortable I used Visual Basic to build the form shown in Figure 11-1 (you can download the free Express Edition at wwwmicrosoftcom/express/vb) but you should use whatever tool you nd comfortable If you ve programmed before, you can use a programming tool If you like building Web pages, build one If you are experienced with Microsoft Word or some other word processor, use it Use drawing tools or even paper and colored markers Whatever is easiest for you Put an image or graphic on the form Graphics make a form more interesting, so add some graphics to your mockup.

The luminosity we have described is the total luminosity of the source across all wavelengths (called the bolometric luminosity), but in practice a detector is sensitive only to a particular range of wavelengths The redshifting of light means that the detector is seeing light emitted in a different part of the spectrum, as compared to nearby objects If enough is known about the emission spectrum of the object, a correction can be applied to allow for this which is known as the K-correction, though often its application is an uncertain business The luminosity distance depends on the cosmological model we have under discussion and hence can be used to tell us which cosmological model describes our Universe In particular we can plot the luminosity distance against redshift for different cosmologies, as in Figure A23 (see Problem A2A to find out how to obtain these curves).

Some of these include TCP UDP ICMP There are a few versions of IP in use today IP version 4 (IPv4) is the most commonly used version, but a proposed standard, IP version 6 (IPv6), is in use and.

Use familiar images such as the customers pictures, company logos, or relevant clipart (a dog leaping to catch a disc or a cat stalking a mouse would work for The Pampered Pet) You can add interest with a special font for the company s name and with colors Don t go overboard, though You want the graphics to tie the form to the customer, not to distract from the form s purpose..

Unfortunately, however, the observable quantity is the radiation flux density received from an object, and this can only be translated into a luminosity distance if the absolute luminosity of the object is known There are no distant astronomical objects for which this is the case This problem can however be circumvented if there are a population of objects at different distances which are believed to have the same luminosity: even if that luminosity is not known, it will appear merely as an overall scaling factor Such a population of objects is Type Ia supernovae These are believed to be caused by the core collapse of white dwarf stars when they accrete material to take them over the Chandrasekhar limit Accordingly the progenitors of such supernovae are expected to be very similar, leading to supernovae of a characteristic brightness This already gives a.

ysm (g/g) 0.024 0.026 0.014