Target: Messier 22 Date: 2012-09-08 Time: 12:03 Telescope: CDK20S Camera: Apogee U16M Filters: UBVRI Exposure time: 100 seconds each filter; one frame each selected for RGB Observer: Rhodes Hart Processing: John Kielkopf AstroImageJ to select frames and render as composite RGB

... Note on Filters: . ... NGC 3351 is a mostly face-on late type spiral galaxy. It is marked by a bar like feature in its central regions and a strong inner ring of star formation. ... The galaxy was imaged through the A1,B1 and B5 filters over a total exposure time of 1936 seconds. ... The galaxy was imaged through the A1 filter for 450 seconds and the B1 filter for 1084 seconds. ... The galaxy was imaged through the A1 and V1 filters over a total exposure time of 1200 seconds. ...

... Near Infrared Camera and Multi-Object Spectrometer Instrument Handbook for Cycle 17 > Chapter 8: Detector Readout Modes > 8.1 Introduction . ... NICMOS has four detector readout modes that may be used to take data. ... There are three supported readout modes: . ... Multiple-accumulate Mode (MULTIACCUM). ... The BRIGHTOBJ mode is not supported for Cycle 13 and later cycles; it is, however, an available mode for the special case of acquisition of very bright targets under the coronagraphic hole. ...

Next: The APM selected sample Up: Second priority candidates Previous: Second priority candidates . From the random selected subsample of second priority candidates we observed twenty six objects during the 6-m telescope runs (mainly those with R.A.< 11 h ) along with the observations of first priority targets. Altogether we found 12 emission-line objects: one appeared to be a QSO with z =3.15, and the rest are various types of ELGs. ... One object is an absorption-line galaxy. ...

... Psrcat . Data archive . ... PSRCORR receives data from PKCCC1 , and displays, processes and archives them. ... Click on Setup and select WBA and old tape or new tape as appropriate. ... At the end of each observation the raw data files are written to the archive tape and the file details recorded in the tape log which is located in /psr1/runtime/psrcorr/db/tape.log . ... This allows you to select an archive tape and the file(s) to be archived (from PKCCC1 _1) and to write these files to the tape. ...

XMM-Newton Science Analysis System . ... Meta Index / Home Page / Description The selected function facilitates step-wise filtering of tables. Used as a sub-expression it evaluates to true for a particular row if that rows has been selected in the selection process preceding the current one. If the table undergoes selection for the very first time, selected returns true for all table rows, i.e., has no effect. ... SELECTED && PHA >= 10 . ... XMM-Newton SOC/SSC -- 2008-07-01 ...

Next: The Interaction of the ISO-SWS Pipeline Software and the ISO-SWS Interactive Analysis System . ... This paper presents the latest developments in ISOCAM data analysis with the Interactive Analysis System for ISOCAM (CIA) . ... 1. data preparation (slicing, generation of CIA prepared data structures) . ... 1997, ``Design and Implementation of CIA, the ISOCAM Interactive Analysis System", in Astronomical Data Analysis Software and Systems VI, ASP Conf. ... CIA . ...

adapted from Observe: Eclipses, published in 1979 by the Astronomical League and "Safe Solar Filters," by B. Ralph Chou, Sky and Telescope, August 1981) . ... Tape TWO pieces of film together into a sandwich, and tape this over the opening in the cardboard. ... The cardboard frame will act as a shade from the bright Sun, while you safely observe through the film sandwich. ... Undeveloped film is not safe. ... tape . ... At the end of one of the tubes, tape the aluminum foil, and make a tiny pinhole. ...

Program Id: . ... UTC End Time: . Astronomer/PI Name(s): . ... Observer Name(s): . Nightlog Day: Sunday Monday Tuesday Wednesday Thursday Friday Saturday Month: January Febuary March April May June July August September October November December Day (DD): Year (YYYY): Full Night A (First half) B (Second half) Special Schedule . ... Note: Open this weather logfile program in another browser window. Please copy and past the resultant info below at the end of the night) . ...

... Tonight's Sky . ... SUN MOON MERCURY VENUS MARS, JUPITER SATURN . ... The Magazine . News . Observing . ... Gravitational wave search provides insights into galaxy evolution and mergers . ... The double star 54 Leonis, spiral galaxy NGC 3198, and emission nebula NGC 3199 . ... Astronomy for Kids . ... Using filters . ... Get instant access to subscriber content on Astronomy.com! ... Receive news, sky-event information, observing tips, and more from Astronomy's weekly email newsletter. ...

... 22apr13: check lbw filterbank . ... They were using the 1230-1470 filter with the 1370 hipass filter. On 10apr13 we did a cable test on the 1370 hipass cable going into,out of the filter bank. ... The calRatio will show variations in Tsys caused by Ttm. ... Filter 9 (1280 hipass) shows Tsys variation (.ps) ( .pdf ): The top figure shows the fractional change in Tsys for polA (black) and polB (red) for the 10 cal off measurements that were made the first time the 1280 hipass filter was measured. ...

... example, note below the dramatic speedup in searching a 1 Gb file using an AND filter, even when one of the columns (pha) has no index : time fundisp \ huge.fits'[idx_activate=0,idx_debug=1,pha= 2348 4000 4000 1]' \ x y pha x y pha ---------- ----------- ---------- 3999.48 4000.47 2348 3999.48 4000.47 2348 3999.48 4000.47 2348 3999.48 4000.47 2348 3999.48 4000.47 2348 ... Currently, indexed filtering only works with FITS binary tables and raw event files. ...

OptInt PmWiki : Pm Wiki / Forms . ... Forms processing can be found in the Cookbook (see below). ... input text name value size= n :) (:input hidden name value :) (:input password name value :) (:input radio name value :) (:input checkbox name value :) (:input select name value label :) (:input default default-name default-value :) (:input submit name value :) (:input textarea name [=value=] rows= n cols= n :) (:input reset name label :) (:input file name label :) (:input image name "src" alt :) . ...

... The first step to improve the FORS calibration is therefore to obtain data to allow a computation of the illumination correction across the field. ... Another limitation on the calibration accuracy has been the brightness of the Landolt standards which have forced the use of extremely short exposures introducing small but non-negligible shutter-time errors and also resulting in a very small number of useful standards per frame. ...

Start with a new RGB image (white background, black foreground). Using type tool type some text. Now save the selection (while the text is still selected). Select/Save Selection.. ... Switch to second image and blur it - use gaussian blur with setting 2.0 on it. Filter/Blur/Gaussian Blur/2.0 . Rotate in 90 degrees clockwise. Image/Rotate/90 CW . Then go to Filters/Stylize/Wind... and use it with settings Wind/Right. ... Image/Rotate/90 CCW . ... Use following settings: . ...

... Visited 5572 times - Selected 51 months ago . ... Visited 6948 times - Selected 51 months ago . ... Visited 4688 times - Selected 51 months ago . ... Visited 7791 times - Selected 51 months ago . ... Visited 9271 times - Selected 51 months ago . ... Visited 7887 times - Selected 51 months ago . ... Visited 4431 times - Selected 51 months ago . ... An online resource for building customized observing lists based on a database with over 10,000 deep sky objects. http://www.virtualcolony.com/sac/ . ...

... The numbers of three types of compact binaries containing accreting NSs and BHs, which are most interesting from the point of view of their observational appearances, have been calculated as a function of time: i) X-ray transient source containing a NS in an eccentric orbit around a main sequence Be-star (the observed prototype: A0535+26), ii) BH The evolution of the selected types of X-ray binaries during the first 10 million years after the starburst onset is presented in Fig. ...

... Meade Instruments Corporation . ... Meade Pictor XT-Series CCD Autoguider/Imagers . Section 7: Camera Menu . ... allows the user to take continuous exposures using the current exposure setup. ... Exposure Time: The Pictor cameras can take exposures as short as 4ms or as long as 120min, though a practical limit on exposures time will usually be less than 20 minutes for most objects and conditions. ... The camera will then take the rest of the images and add them together to produce a single image. ...

... Exposure Time Calculator (ETC) . ... ESO - Public Surveys . ... the recommended values to use for DIT, . ... Detector on-chip integration (DIT): seconds. to your chosen value - a separate page gives recommended values to use for DIT - for modes 1 and 2 below you may wish to start with the maximum recommended values as these will minimize the effect of read noise (a total object exposure of Y secs with DIT=X secs will produce Y/X lots of read noise) and give you a lower limit on the time needed. ...

... The three optical trains for the cameras, and the pupil reimaging system, are mounted on a wheel, accurately driven by an external motor. ... The low-resolution spectroscopic mode uses the wide field camera and a suitable set of grisms and order sorting filters that are inserted in the parallel beam after the pupil. ... One of the five grisms can operate at four different orders, depending on the filter selected on the first filter wheel that acts as order sorter. ...