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5 Jun 2007: This required a total time of 7359hrs based on VISTA ETC(v1.1).With the new VISTA ETC(v1.3) this reduces to a total of 6750hrs. ... PSP Panel Issue 5 The Panel strongly recommends that the PI submits a new proposal whichfocused on the science that can be

10 Oct 2023: Gaia is also providing a numberof stringent new tests of general relativity and cosmology.

27 May 2010: All three stars are known disc hosts.Herschel spatially resolves the dust emissionaround all three stars (marginally, in the case ofβ UMa), providing new information about discs as close as 11

10 Oct 2023: levels.Eventually the electron will de-excite and jump down to a lower energylevel, emitting a new photon of specific frequency.

2 Sep 2010: The de-bris absorbs starlight and re-emits it at longer wavelengths,and observations since 2003 with the Spitzer space telescopehave yielded many new debris detections in the mid- to ... 3 OBSERVATIONS AND DATA REDUCTION. The eleven new stars were

19 Mar 2010: Project 1640 is a new collaborative project between the IoA and the Astrophysics Group at the American Museum of Natural History. ... Lucky Imaging We built a new four-shooter optical system to image a strip of sky at a range of scales from f/11 to f/44

16 Jun 2015: This new instrument configuration is called CIRPASS. COHSI was designed to suppress the nightsky airglow due to OH emission in the 1.0-1.8 micron region by filtering out the

16 Jun 2015: cubemean.c Assume new controler in place, loop1 not skipped Version 0.94 (November 2001) - Carine Babusiaux Add 2mass catalogue option in astrometry.pl (using 2mass.pl) Version 0.93 (20

Index of /optics/cirsi/docs/pixcel/20010508/Images. 2015-06-16 07:29. 931. 2015-06-16 07:29. 2.3K. 2015-06-16 07:29. 2.2K. 2015-06-16 07:29. 1.5K. 2015-06-16 07:29. 1.8K. 2015-06-16 07:29. 2.2K. 2015-06-16 07:29. 1.9K. 2015-06-16 07:29. 4.5K. 2015-06

9 Oct 2017: The Sun has spectral class G2. In recent years, new observations allow detection of the faintest stars and brown dwarfs, resulting in extension of the scheme to include types L and

11 Dec 2003: If this is different from that in. modin. , the code should interpolate the given model to give the new one, provided that NCH is greater than or equal to 1.

16 Jun 2015: The device is operated via simple polled transfers. New device drivers that support full DMA access have recently been received by AstroCam for Windows 95. ... A new filter wheel is under construction now. 2.6 System Testing hardware and software.

4 Jul 2013: C-x 4 0 kill buffer and window. C-x 5 2 make new frame. ... C-x v a create changelog file in gnu-style. NEWS. 8.1.2002: The first part comes here.

18 Jul 2006: The Panel strongly recommends that the PI submits a new proposal which focused on the science that can be achieved by covering the whole southern sky in JK only.

13 Jul 2010: The waste water is used to heat a swimming pool. For a while it was popular with jetsets on their way from New York to Europe.

2 Nov 2017: Follow-up Hubble Space Telescope observations in Adams et al. Existing HST precursor images (top), new 2015 images (middle) and near-infrared images (bottom).

Index of /optics/cirpass. 2015-06-16 07:28. -. 2015-06-16 07:28. -. 2015-06-16 07:28. -. 2015-06-16 07:28. -. 2015-06-16 07:28. 3.2K. 2015-06-16 07:28. 3.3K. 2015-06-16 07:28. 2.9K. 2015-06-16 07:28. 16K. 2015-06-16 07:28. 1.7K. 2015-06-16 07:28.

10 Apr 2013: cpl_table vircam_chantab_new. (. int . nord,. cpl_table. template. ). Name:. vircam_chantab_new. Purpose:. ... Returns:. The cpl_table pointer for the new channel table. Author:. Jim Lewis, CASU.

16 Jun 2015: New features. Now works on windows98 with vxd driver. Hawaii 2K devices supported.

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: Default values for new sections. [INFRARED] LINEAR=none FLIP_V=FALSE FLIP_H=FALSE ASSEMBLE=FALSE ROTATE_ORDER=0,90,180,270 ROTATE=FALSE SHIFT=0 CONSTANT=0 SUBTRACT=FALSE

16 Jun 2015: Filters that were loaded when CIRSI was shipped to LCO:. 0 Dk Dark position; metal plate 1 Jc New Carnegie J replacing Z 2 Jg J(Gemini consortium specification) 3 Hs

16 Nov 2017: more tightly constrained via observations?• From the upper end, new studies of supernovae progenitors, as in Star of the Week #2, now making progress• From the lower end, use observations of

13 Jan 2000: of Astronomy, Cambridge Observatory Building Meeting Room Note: The IOA, Hoyle Building is partially a building site while a new Lecture Theatre is completed, so reception is in the Observatory Building.

14 May 2009: I found a British company (now called E2V Technologies ) working on a new detector called the Charge Coupled Device (CCD).

16 Jun 2015: READY - Camera is able to start a new sequence, or has just finished one. ... To return the current value of a parameter send the name of the parameter, to set a new value send the name and the value separated by a space.

n"); // $filemod = filemtime("xmmssc/public_html/xidops/fields_status.txt"); $filemod = filemtime("/home/xmmssc/public_html/xidops/fields_status_new.txt"); $filemodtime = date("F j Y h:i:s A", $filemod);

18 Oct 2017: A new look at the Cosmos. The World in 1994, p144 (Economist publications). ... Daily Telegraph 13 Sept 1995. Reminiscences of S Chandrasekhar. New Scientist 30 Sept 1995.

16 Jun 2015: Enter. PCIDeviceId=0x826e. if you have a new card, ie:. It says PCI Digital Camera Interface on the top left of the card.

1 Mar 1998: This new instrument offers unique opportunities for the UK/NL communities to execute high resolution, deep, wide field optical imaging surveys.

22 Jul 2007: In July, 2007, SDSS released a new SGC stripe as part of theThis is shown in green.

14 May 2009: In addition a new detector system that allows the spectrum of the fringe pattern to be detected has been developed. ... Following that a new CCD system was built by CDM and used on the Anglo-Australian Telescope (AAT) in 1981.

15 Oct 2017: The new line-width determination scheme is the key to the project.From Clewley et al., 2002, MNRAS, 337, 87.

5 Oct 2006: If yes, explain why the need for new data. Are the data requested in this proposal on the ESO Archive (http://archive.eso.org)?

5 Dec 1999: NEW 1ST FULL LAST Dec 07 22 33 Dec 16 0 51 Dec 22 17 33 Dec 29 14 06 Jan 06 18 15 Jan 14 13 35 Jan 21 4

22 Oct 2017: Energy released given by Einstein’s formula E=mc2, where “m”=Δm the difference in mass between the constituent light nuclei and the nucleus of the new element. •

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.

5 Jun 2007: This required a total time of 7359hrs based on VISTA ETC(v1.1).With the new VISTA ETC(v1.3) this reduces to a total of 6750hrs. ... PSP Panel Issue 5 The Panel strongly recommends that the PI submits a new proposal whichfocused on the science that can be

18 Oct 2017: Bahcall and E.E. Salpeter). New Interpretation of Extragalactic Radio Sources. Nat 229, 312 (1971) (errata, p. ... Pacini). New Evidence on Long-term Behaviour of Her X-1. Nat 244, 212 (1973) (with A.C.

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.

11 Oct 2018: 3.32). The force due to this new potential is:. FΛ = VΛr.

6 Apr 2013: For example 10 objects to a. previous survey of 150 is not a major new result. ... Finding one new Algol system or quasar is. not major unless there is some peculiarity or modelling that advances the field.

25 May 2007: In my opinion working with data from more than one survey will help with some of the quality control since debugging software or classifying a new type of artifacts only has ... from the list below and/or add some new ones] Observing block preparation

16 Jun 2015: DAZLE: Dark Ages Z Lyman-alpha Explorer. This is a collection of published work with a connection to issues relating to the DAZLE project. There are two lists, one covering the theoretical background and the other relevant observational results.

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.

10 Nov 2017: Fusion in shell via p-p chain and CNO cycle becomes the new energy source for the star. •

10 Nov 2017: Note left-right excursions corresponding to core contraction and onset of new burning phase.

1 Mar 1998: Deep optical surveys combined with the renaissance of interest in large area surveys at all wavelengths are fundamental in searching for rare types of object, discovering new categories of object, and ... Quality control will be assured by a rigorous and

1 Mar 2010: already in the SM and the new ones. b) For the new gauge bosons (not in the standard model), write down their charge, colour.

5 Nov 2023: the eccentricity of the new orbit e2.