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16 Jun 2015: im_ - Pointer to an image created with new(). h_ - Handle.

16 Jun 2015: Parameters. The new parameters are in five groups at end of the pixcel.ini. ... RUN=0 to 9999999. A run number is inserted into the filename of each fits file written, the number is automatically incremented with each new sequence.

16 Jun 2015: The plot is updated with the pixels from the new image under the line selection. ... The histogram is updated with the data from the new image under the rectangle selection.

16 Jun 2015: vii) type 'cmd TCS USER "ENTER APERTURE 0 x y" where x & y are the new aperture 0 values. ... The boring command in section (vii) could be put into a script [rgm 20000614] (ix) NOW edit the CIRSILoadApertures script to have the new value of aperture 0.

16 Jun 2015: Then on the PLW window, go to Files->New Settings and click OK on the next few windows that pop up. ... In the Guider Control GUI, select Options->Timing and enter new rates (two sets of rates are written on the white board).

16 Jun 2015: Moshut. Woodbury, New York : American Institute of Physics, 1998. (AIP conference proceedings ; 428), p.499. ... S. Young, and D. F. Buscher. A new photon counting spectrometer for the COAST.

16 Jun 2015: Readers should be altered as soon as possible to cope with the new format. ... Cases of DATE-OBS before 1900-01-01 should always be written with the new format.

16 Jun 2015: I found a British company (now called E2V Technologies ) working on a new detector called the Charge Coupled Device (CCD).

16 Jun 2015: The CIRPASS team and the new CIRPASS plug-plate system at cassegrain.

15 Jan 2015: The dust detectoraboard New Horizons may soon detect dust in resonance.

16 Jun 2015: QUAD_SEL= "H" % Latch new quadrant mask %. CHIP_SEL= "H" % Latch new chip mask %. _SELECT = "L L" % Don't change quad or chip select%. %

16 Jun 2015: The new, definitive list of UKIRT standards will be published, more formally than the old, in due course.

16 Jun 2015: New technologies being developed for space applications such as composite or thin metal mirrors could offer a solution.

16 Jun 2015: status. commissioned WHT June and Sept 1999, foreoptics modified during 2000 to work with new WHT AO system, NAOMI.

16 Jun 2015: Check the 'Override settings for.' to make changes to settings, or check 'Store as.' for the creation of a new setting. ... To create a new sequence of single or multi image acquisition, select the Sequence tab.

19 Jan 2015: 3 School of Physics, University of New South Wales, Sydney,NSW 2052, Australia. ... 4 Australian Centre for Astrobiology, University of New SouthWales, Sydney, NSW 2052, Australia.

16 Jun 2015: The prime difficulty in moving in this direction has been the prohibitive cost of the new large arrays. ... Thus the new Keck spectra give much more promising indications of the merits of surveying for emission line galaxies in the near-infrared spectral

16 Jun 2015: New L-band data are being obtained in an approved program at the South Pole facility. ... SCUBA data are being obtained and analysed, together with new high-resolution CO data.

16 Jun 2015: It should NOT be used for NEW documents! New documents should use Standard LaTeX conventions and start with the documentclass command.

16 Jun 2015: New Select the New file icon to clear the image area to start a new image. ... Software toolbar. New file Select the New file icon to clear the image area to start a new image.

16 Jun 2015: The plot is updated with the pixels from the new image under the line selection. ... The histogram view is updated with the pixels from the new image that are contained by the rectangle selection.

16 Jun 2015: Although see NOTE, 3 points below. Edit extern.pkg to define the new package, e.g. ... Use the new install script provided at the ftp site, not the extracted one installed by default as it doesn't work!

16 Jun 2015: What has to happen is that the configuration file being used has to be edited and then re-loaded into Pixcel with the new parameters in it.

16 Jun 2015: It discusses the advantages of array detectors over single element devices and examines the differences in operation between the new generation of infrared arrays and visible CCD imagers. ... The new generation of 1024x1024 pixel arrays are only possible

9 Oct 2015: v22 v21) 4(Mp/M)2ǫ21 v5pv3. Hence show that the new orbit has a semimajor axis with a corresponding ǫ2 thatsatisfies.

16 Jun 2015: Transfer to another telescope therefore is simply a case of making a new fibre feed and making a new plate-holder unit to suit the new telescope. ... For a multislit system transfer to another telescope requires making a new collimator.

16 Jun 2015: make_masks n1 This will make new versions of the ones stored in home$wfirc/script_frames. ... It is incremented by one for each new position in an observation sequence.

16 Jun 2015: Clearing FSYNC leaves the first row only selected. Rowstart function. A similar sequence is used to start reading a new row. ... Start new frame Loop over 48 rows at top of the array i.e.

16 Jun 2015: 3.0 Sept 1996 Richard McMahon (IoA) [rgm@ast.cam.ac.uk] %% Conversion to Latex substyle %% %% 3.1 July 1997 Bill Martin and Vik Dhillon (RGO) %% Released to community for new ... AAO) %% Increased space for Section 14 - Related Applications %% %% 3.5

16 Jun 2015: The quality of the images is excellent and now that we have an effective data processing pipeline, the data produced is breaking new ground in our understanding of the most distant ... clusters of galaxies Planned upgrades to CIRSI include a new parallel

8 Jan 2015: given in Stark et al. (2014). A larger telescope can tol-erate larger zodi levels for the same integration time.Detections of warm dust will also reveal new informa-. ... U. 2000, in Allen’s Astrophysical. Quantities, ed. A. N. Cox (New York: AIP Press)

16 Jun 2015: between the filters’different properties.14, 15 As result of this consulation process two options were offered by Barr, one design basedon standard techniques and a second using an new filter ... 940–944, Sept. 1993. 13. S. D. Lord, “A New Software

14 Sep 2015: In this work we compare new ALMA high-frequency radio continuum observations of HD 142527,obtained at 700 GHz (ALMA band 9; wavelengths of0.43 mm, described in Appendix, Sec. ... Sec. A.1 presentsthe new ALMA observations, Sec. A.2 presents the newATCA

20 Jan 2015: New modeling based on Spitzer/IRS models and KIN observations also suggests a com-.

15 Jan 2015: obtained at two epochs separated by 15 years. The new images and the re-. ... ing Spectrograph, Woodgate et al. 1998) archival dataset and also introduce a new set of.

14 Sep 2015: Goodman2, A. Hoekstra2, K. J.Jek21Department of Astronomy, Yale University, New Haven, CT 06511, USA2Amateur Astronomer3Department of Physics, and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge,

24 Oct 2015: Box 23-141, Taipei, 106,Taiwan12 National Radio Astronomy Observatory, 1003 Lopezville Road, Socorro, New Mexico,87801, USA13 LESIA, Observatoire de Paris, 5 place J. ... The low frequency, high resolution,and excellent sensitivity of the ngVLA will open

10 Mar 2015: 10 March 2015. ABSTRACTWe present new observations of the Kuiper belt analogues around HD 38858 andHD 20794, hosts of super-Earth mass planets within 1 au. ... 2014). 3 DEBRIS DISC OBSERVATIONS. Here we present new observations of HD 38858 with sev-eral

15 Jan 2015: will characterise the exo-zodi luminosity functionwith sufficient detail to provide new information on the dustorigin and evolution.

2 Nov 2015: Road, Cambridge, UK9 Department of Astronomy, Yale University, New Haven, CT10 Visiting Astronomer, NASA Infrared Telescope Facility, op-. ... 2012), these additional pointing variationsrequire new data reduction solutions optimized for K2(e.g.,

16 Jun 2015: 2 European Southern Observatory, Alonso de Cordova 3107, Vitacura, Casilla 19001, Santiago, Chile3 School of Physics, University of New South Wales, NSW 2052 Sydney, Australia4 Australian Centre for Astrobiology, University of ... New South Wales, NSW