HI spectral-line observations of galaxies (Karen O'Neil) . Measuring the width, flux, etc. of the HI profile of two galaxies, using some combination of : dwarf emission line, HVC emission line, spiral emission line, and spiral absorption line. This project was designed to demonstrate the fundamentals of spectral line observing and position switching. ... The types of galaxies observed in this project are being kept open and will be determined when the project LST is known. ...

... Bad Astronomy . ... Bad Astronomy : The Moon appears larger on the horizon than overhead because you are comparing it to foreground objects. Good astronomy : The Moon does appear larger on the horizon, but it is because of the way we perceive the sky. ... The most common misconception is that it is because you are unconsciously comparing the Moon to foreground objects like trees and houses, or even the horizon itself, and that makes the Moon look bigger than when it is all alone in the sky. ...

Modules | ... Apache HTTP Server Version 2.2 . ... User authentication using an SQL database . ... Please note that you need to load an authorization module , such as mod_authz_ user , to get it working. # mod_dbd configuration DBDriver pgsql DBDParams dbname=apacheauth user = apache password =xxxxxx DBDMin 4 DBDKeep 8 DBDMax 20 DBDExptime 300 Directory /usr/www/myhost/private # core authentication and mod_auth_basic configuration # for mod_authn_dbd AuthType Basic AuthName My ...

Easy DMT: Using the chInterface Class to Create/Upgrade DMT Monitors Rauha Rahkola, Univ. of Oregon LSC Meeting, August 19-22, 2002 LIGO Hanford Observatory Richland, WA LIGO-G020349-00-Z Easy DMT Introduction to the chInterface utility class ! ... Run through the data 1. for each channel, either: ! ... Final report LSC Meeting, August 19-22, 2002 Hanford 3 LIGO-G020349-00-Z Easy DMT The chInterface Model ! ... No Yes Yes Defaults to RMS of data addChannel addFilter New channel? ...

... Apache HTTP Server Version 2.2 . Apache > HTTP Server > Documentation > Version 2.2 > Modules . ... User authentication using an SQL database . ... Database Management #Use the PostgreSQL driver DBDriver pgsql #Connection string: database name and login credentials DBDParams dbname=htpasswd user = apache password =xxxxxx #Parameters for Connection Pool Management DBDMin 1 DBDKeep 2 DBDMax 10 DBDExptime 60 #Authentication Section Directory ... SQL query to look up a password for a user . ...

... You can boot Linux either from a floppy or from the hard disk. ... When booting Linux from a floppy disk, the boot sector contains code that just reads the first few hundred blocks (depending on the actual kernel size, of course) to a predetermined place in memory. On a Linux boot floppy, there is no filesystem, the kernel is just stored in consecutive sectors, since this simplifies the boot process. ... For example, when I boot, I it looks like this: љ љ љ љ LILO boot: Loading linux. ...

... Donate to Support Science Literacy . ... 2016 Annual Awards . The ASP is accepting nominations for the organizationтАЩs national annual awards which recognize special achievements in astronomy research, technology, education, and public outreach. ... Shop the AstroShop . ... The Astronomical Society of the Pacific (ASP) is accepting nominations for the organizationтАЩs national annual awards which recognize special achievements in astronomy research, technology, education, and public outreach.. ...

... casa . casa::MSFieldIndex . ... Class to handle lookup or indexing into a MS FIELD subtable. ... MSFieldIndex (const MSField &field) . ... Vector < Int > . matchFieldNameOrCode (const String &name) . ... Vector < Int > casa::MSFieldIndex::maskFieldIDs . ... Vector < Int > casa::MSFieldIndex::matchFieldCode . ... Vector < Int > casa::MSFieldIndex::matchFieldCodeRegexOrPattern . ... Vector < Int > casa::MSFieldIndex::matchFieldIDGT . ... Vector < Int > casa::MSFieldIndex::matchFieldIDGTAndLT . ...

... ebadpixupdate (ebadpixupdate-1.10) [xmmsas_20070708_1801-7.1.0] . ... Standard run (get bad pixels from the CCF) over all CCDs: ebadpixupdate eventset=P0123700101PNS003PIEVLI0000.FIT . ... Take additional bad pixels from another event list and the CCF, for CCDs 2 and 3: ebadpixupdate eventset=P0123700101M2S002MIEVLI0000.FIT ccds='2 3' \ badpixtables='P0111090301M2S002MIEVLI0000.FIT:BADPIX02 \ P0111090301M2S002MIEVLI0000.FIT:BADPIX03' . ...

Next: A Plea to Up: Some Problems of Practical Previous: Problems of Fourier . I would like to spend the rest of my time showing an example of the kind of dilemma one can get into when doing restorations. In this particular case we were dealing with an FOC ultraviolet image of the center of M31, and a PC V -band image of the same region, scaled, rotated, and aligned. We wanted to take the quotient of the two images, to look for color effects. ... Image A has low , while B has high . ...

Marc White . ... Here you'll find a list of things that I find useful. ... CSS font stack: http://cssfontstack.com/ . ... E marc.white@anu.edu.au . ... F www.facebook.com/marc.white.au . L au.linkedin.com/pub/marc-white/84/460/84a/ . S marc.christopher.white . G github.com/marc-white . Design copyright Marc White 2014 . Header image taken from Old World Auctions . Title/header font is Kreon by Julia Petretta. Available at Google Fonts. Design v1.32. ...

Here are a set of pictures which progress from the original through a couple intermediary images to the final, rather 60ish looking final image. This is the original image, created using some PD fonts and some mucking around with the BCG plug-in. The original logo has been extruded a bit using the displace plug-in. A web is created by using the wave plug-in, duplicating it and rotating it 180 degrees, and adding the two pieces together. The original logo is then placed over that. ...

... Also, you have to case reverse of a spell. Example: If the OPEN spell is ECED you would use DECE in order to get the reverse effect. look leaf goto elder's tent - story - get distaff look egg write down OPEN sound cast OPEN on egg - story - look loom write down SWAN sound goto grave look thorns goto screen that has trees and knotholes look at all 4 trees write down LIGHT sound goto tent with gold ...

... Basic time functions . ... Example 2: Set a random number seed . ... Uses of time functions include: . ... time_t time(time_t *tloc) -- returns the time since 00:00:00 GMT, Jan. 1, 1970 , measured in seconds. ... timer.c */ #include <stdio.h> #include <sys/types.h> #include <time.h> main() { int i; time_t t1,t2; (void) time(&t1); for (i=1;i<=300;++i) printf(``%d %d %d n'',i, i*i, i*i*i); (void) time(&t2); printf(`` n Time to do 300 squares and cubes= %d seconds n'', (int) t2-t1); } . ...

CCD Forum Message . Forums: . ... Looking For $2500 Monochrome Camera . ... At the end of the day, you might be better off looking at something like the Starlight MX916, and writing a driver yourselves (some people have done individual Linux drivers for the Starlight cameras). ... www.astronomy.net . About Astronomy Net | Advertise on Astronomy Net | ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

. Look at these examples of how local C and TC shell variables can be used. Safeguarding your files . Setting the prompt variable .

Theory of filtering and time series processing L. Zotov Laboratory work ?6 Purpose: Studying singular spectral analysis SSA. We use Matlab software (look into the Lab N1). 1) Download the program and additional module for the lab from http://lnfm1.sai.msu.ru/grav/english/lecture/filtering/ Study the SSA package on examples. 2) Download and install program from http://www.gistatgroup.com/cat/cat33.exe Study it. Visit http://www.gistatgroup.com/gus/examples.html

Next: Pipeline Calibration for STIS . ... Previous: HST Paper Products: A New Way to Look at HST Data . ... This simplifies enormously the data reduction procedure and allows the user to interpret high-quality data correctly. ... This may result in confusion about basic instrumental parameters, the precision of the set-up, the amount and distribution of calibration frames which are required and finally the assumptions on which the data reduction procedure should rely. ...

... We received the SASS output for the HRI observation of 3C 120 (a highly variable radio galaxy with a prominent jet leaving the core at PA ) and smoothed the data with a Gaussian of FWHM = 3 '' ( Figure 13.1 ). ... The results are shown in Figure 13.2 . ... The FWHM of the original data ( Figure 13.1 ) is 11.8 (PA ); after dewobbling ( Figure 13.2 ) the width of the 50% contour is 7.6 . ... Figure 13.1 : The original data, smoothed with a Gaussian of FWHM = 3 . ...

OptInt PmWiki : Pm Wiki / Page List Templates . ... template first:) . ... template last ...:) sections to specify output for the first or last page in the list or a group. ... template]] (:template defaults order=name:) (:template first:) Pages ordered by group (:template first {=$Group}:) Pages in group [[{=$Group}/]] (:template each:) * [[{=$FullName}]] (:template last {=$Group}:) {=$Group} contains {$$GroupPageCount} pages. (:template last:) {$$PageCount} pages total. [[#templateend]] . ...