... One can, for instance, plot the r.m.s noise of the flat field exposures against their mean pixel value to check the general consistency of the frames. Or one may want to plot the mean temperature of the detector against the date of the exposures to check whether there are outliers.( ... Figure: Trend analysis of the detector mean temperature with Modified Julian Date . ...

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• An example of selection criteria
• List of Tables

... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Murchison Radio-astronomy Observatory . ... Parkes radio telescope . ... Mopra radio telescope . ... Visiting Parkes radio telescope . ... Parkes radio telescope webcam . ... For example, modified Newtonian dynamics (MOND) has no relativistic extension, and so makes no firm lensing predictions, but galaxy-galaxy lensing data can be used to empirically constrain the deflection law of a MONDian point-mass. ...

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• VSOP Observing Schedule
• lbaops:tidnotes:fileprep [ATNF VLBI Wiki]

... From the chain visibility point of view, it is very recommended to look at the Javascript movies , especially if the frame rate can be not regulated in your MPEG player. ... The non-CH-associated large-scale chains visible on the SOHO/EIT images at three wavelengths of 171, 195 and 284 as well as on the MLSO/HAO He I 10830 spectroheliogram of December 16, 1997. ... The SOHO/EIT movies at 171 and 195 show the chain dynamics on June 1-3, 1998. ... Javascript movie (230 KB), SOHO/EIT, 171 . ...

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• Chains and CMEs

XMM-Newton Science Analysis System . ... CORR_RATE - The count rate after the following corrections have been applied; . 1) A further point-spread function correction may be applied, to extrapolate the counts from 12 to 35 pixels (presently only done for UV observations) 2) Correction for dead-time. 3) Correction for the OM sensitivity-degradation. A key-word TDS_CORR is added to the table to record the correction value. ... XMM-Newton SOC/SSC -- 2008-07-02 ...

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• Modification of Source-axes position angles

.

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• VV29 = Arp 188 = The Chainsaw Galaxy
• Designated Observatory Application

... Observing . ... Solar Observing . ... April 3 (SUN) - Solar Observing, Central Park , Manhattan . ... APRIL'S SKY . ... Lecture Series at the American Museum of Natural History The Amateur Astronomers Association is proud to present an astronomy lecture series from October through May each year for our members and the .. ... The€аAmateur Astronomers Association of New York€аwas organized in 1927 to promote the study of Astronomy, emphasizing its cultural and inspirational value. ...

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• Deep Sky Images by Joe DiNapoli ? Amateur Astronomers Association of New York
• Observing ? Amateur Astronomers Association of New York
• Lecture Series 2015-2016 ? Amateur Astronomers Association of New York

Next: Richardson-Lucy Co-Addition . ... WFPC images offer a wide field of view but significantly undersample the PSF. A strategy to recover some of the resolution lost by undersampling is to split the exposure time into several images, which are shifted by a fraction of the pixel size. ... One of the challenges of this approach is the treatment of cosmic ray hits. ... An IRAF implementation (Freudling, 1993) was tested on both simulations and real WFPC data. ... Treatment of CR Hits . ...

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• Observing Program Email Folders
• WFC3 Data Handbook
• HST Program Implementation Cron Jobs

Next: A Checklist of Things to Have Before You Observe Up: Spectral-Line Observing Previous: Some Useful Routines for Online Data Analysis . ... Observing the Old-Fashioned Way: Gui-Free . A. Gui-Free Observing: Spectral-Line Checklist . ... C. Gui-Free Observing: Preparation of Observing Files . ... General Set-up File . First Example - a9999a.sls Spectral Line Set-up file. Second Example - a9999b.sls spectral line set-up file. ... Fourth Example - a9999d.sls spectral line set-up file. ...

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• pulsedPwrIntoAlfa
• RF observing program
• CIMA Configuration Files

Name Last modified Size Description . Parent Directory - FORS2/ 07-Apr-2016 14:47 - NACO/ 17-Apr-2013 15:23 - SINFONI/ 13-Oct-2014 14:38 - VIMOS/ 07-Apr-2016 14:56 - VISIR/ 23-Feb-2015 16:26 - preimg_FORS2.txt 11-Jun-2008 15:01 32K preimg_NACO.txt 11-Jun-2008 15:01 476 preimg_SINFONI.txt 11-Jun-2008 15:01 582 preimg_VIMOS.txt 11-Jun-2008 15:01 43K preimg_VISIR.txt 11-Jun-2008 15:01 2.7K .

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• Index of /observing/dfo/quality/public_html_qc/monitor/REPROC
• Index of /observing/dfo/quality/public_html_qc/dfos/reference
• Index of /observing/dfo/quality/public_html_qc/tqs

... We demonstrate through numerical simulations that model parameters estimated with our technique are essentially bias-free, even when the average number of counts per bin is 1. ... The IW technique avoids such biases by estimating through successive iterations, where for each iteration, j, , and the best-fit parameters are determined by minimization of . ... In our sample, we find that the minimum values and best-fit parameters converge after about 6 iterations. ...

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• The NOAO Web-based Observing Proposal System
• NICMOS Calibration Pipeline: Processing Associations of Exposures
• Organizing Observational Data at the Telescope

... This gives a nice opportunity to check the quality of the FIRPO photometry against that of TIRGO. ... The values are Program POLYFIT V 10/Jul/90 ( A.Richichi ) - 24-Aug-1997 13:38:25 File : diff_temp_jc.dat Pol. degree: 1- N = 10- [ 2786.00- 4095.00 ] - [ 0.00- 1194.00] 1 -.10304E+01 0.26412E+00 2 0.29958E-03 0.74406E-04 sdev: 0.16063E+00 chi2 :0.24486E+01 Program POLYFIT V 10/Jul/90 ( A.Richichi ) - 24-Aug-1997 13:42:59 File : diff_temp_hc.dat Pol. degree: 1- N = 10- [ 2786.00- ...

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• Aldebaran Occultations
• Extended IDL Help
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The AstroGuide . ... AstroGuide | ... AstroGuide Listing . ... See many more Astronomy Listings by: Category or Alphabet . Low cost beginner eyepieces. Send SASE for price list. ... Listed Since October 26, 2004 . ... www.astronomy.net . About Astronomy Net | Advertise on Astronomy Net | ... dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

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MAIN CHARACTERISTICS BASIC MODIFICATIONS TEST RESULTS . ... integrated drop tests in order to verify the strength of DM modified shell and equipment attachment points, functional check of new chairs and DM structure, determination of shock impacts onto the crew to verify landing safety; . ... nominal landing with the main parachute system (MPS) - drop #1 took place on December 24, 1998; . ... reduction of shock g-loads values at landing in accordance with decrease of landing speeds. MAIN | ...

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• S.P. Korolev RSC Energia - International Space Station
• S.P.Korolev RSC Energia - MIR ORBITAL COMPLEX
• S.P.Korolev RSC Energia - LAUNCHERS

... Galaxy Evolution home . Cavendish Astrophysics . Cavendish Laboratory . ... Cosmological evolution of star-forming galaxies . The origin and evolution of radio sources . Radio sources and their environments . ... Publications . ... Submitted . ... Calendar . ... Paul Alexander . P.Alexander@mrao.cam.ac.uk . ...

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• Astrophysics Group members - X Sun
• Astrophysics Group members - E Waldram
• Astrophysics Group members - S Thompson

GrIm II . ... The MC has been modified to change the way GRIM images are stored to disk when FITS format is selected. ... The solution the Grim team has come up with is to internally add a constant of 10000 to every pixel of the 'bias subtracted' grim image which makes it conform to the unsigned 16-bit number standard, in that all pixel values after this addition of 10000 are in the range 0-65535. ... We have now implemented this for storage of GRIM files in FITS format. ... filetype fits . ...

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• default
• op010411
• SDSS M1 Mechanical Collimation

Hereґs one (possible) image of Sn1998ey. It was extreamly dim to observe with our telescope so could You confirm? . Observer Marko Moilanen , Jyvaskyla, Finland. David Bishop Last modified: Mon Dec 21 09:03:45 EST 1998

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• SN1989B in M66
• Bright Supernova Bright Supernova
• Supernova 2000fb in ESO 205-G011

... The accuracy of calculation of both INTERBALL spacecraft (SC) motion has been estimated at the IKI. ... The 30 days measuring intervals were used during the Tail probe (TP) orbital data treatment, and 15 days intervals - during the Auroral probe (AP) orbit determination. ... http://www.iki.rssi.ru/vprokhor/indap.htm for the Auroral probe; . http://www.iki.rssi.ru/vprokhor/indtp.htm for the Tail probe . ... http://www.iki.rssi.ru/vprokhor/ssc.htm , or http://www.iki.rssi.ru/vprokhor/amisan.htm . ...

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• INTERBALL TAIL PROBE 1999 situation analysis during operation scheduling
• INTERBALL TAIL PROBE 1997 afterflight situation analysis
• INTERBALL AURORAL PROBE 1999 afterflight situation analysis

Geomagnetic disturbances can be monitored by ground-based magnetic observatories recording the three magnetic field components. The global Kp index is obtained as the mean value of the disturbance levels in the two horizontal field components, observed at 13 selected, subauroral stations . ... Geomagnetic activity is the occurrence of K variations. ... But K still remains a local index, describing disturbances in the vicinity of each observatory. ...

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• Geomagnetic Indices Kp, ap, Ap, Cp and C9
• Julius Bartels (1899-1964)
• Kp Index: Classification of Days

... They will undergo acceptance tests. ... Appendix (The list of used acronyms) ASC Cold Plate DC Astro Space Center of Lebedev Physical Instutute cooled LNAs and antenna feed hermetic device container (part of payload); it contains Formatter ... synthesizer, control unit and is placed under dish DM Device Module = DC + H-maser EGSE Electronic Ground Support Equipment Electronic Complex ­ all SRT electronics EM Engineering Model FC Focal Container ­ hermetic package with the ...

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• http://www.asc.rssi.ru/RadioAstron/meetings/telecon/dec13_2011.pdf
• RSOG Pre-Observation Products
• RadioAstron main page, english version

chandra_acis_ao9.par ; generate an ACIS spectrum for a source using a DEM , ; and optionally rescale the DEM to produce the same ; counts as a ROSAT / PSPC observation ; ;calling sequence ; .run initale ; @chandra_acis_ao9.par ; ;(LL/VK; modified from chandra_acis_ao5.par, Feb04) ;(LL ... density [cm^-3] T_components = [6.9, 7.4] ;log(T[K]) components in the EM EM_components = [5.1d12, 6.1d12] ;Emission Measure [cm^-3] obs_rate = 0.1 ; ROSAT / ...

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• http://hea-www.harvard.edu/PINTofALE/ardb/chandra_acis_ao7.par
• PINTofALE EXAMPLE : Simulation for Chandra ACIS-I
• Modifying the SAOtng GUI