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13 Oct 2017: What are the new values of apparent and absolute mag-nitude? Q6c: The supernova remnant, in the shape of a ring, is expanding with aspeed v = 10, 000 km s1.

6 Nov 2017: is adjusted, to take account of the fusion processes, to give composition at t=t0δt- new composition used to solve the stellar structure equations again- sequence repeats through lifetime of the

16 Mar 2012: There are new leptoquarks which allow transitions along the rows between the coloured quark states and the colourless leptons.

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.

7 Feb 2008: Stochastic evolution of small grains and dynamical excitation. Indirect detection of planets and discovery of new phenomena. ... Indirect detection of planets and discovery of new phenomena. Constraining planet properties and comet population.

15 Aug 2023: 15/08/2023 2. Astronomy Job Opportunities for New Ph.D. Graduates. Paul Hewett. ... working environment/support compared to academia. Institute of Astronomy “astro-jobs” presentation. Astronomy Job Opportunities for New Ph.D.

5 Jul 2018: 1950s. AlpherGamowHermanHayashi. BBN CMB. = New Physics? BBN CMB. = New Physics?

19 Feb 2007: The Dark Energy Survey(DES) will use a new wide field CCD mosaic camera called DECam that is currently under construction. ... With the new VISTA ETC(v1.3) this reduces to a | | total of 6750hrs. | |--------------------------------------------------------

17 Nov 2017: Historically, until last fifteen years, “objective-prism” spectra employed. • New wide-field photometric surveys allow accurate (few percent, i.e.

19 Apr 2006: Our observations provide new information aboutthe distribution of the color temperature and optical depthstructure of this region. ... The high resolution of mid-infrared detec-tors on new large telescopes, such as Gemini, VLT, and theGTC, will permit

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.

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.

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.

3 Nov 2000: DO THE MOSAIC OFFSET INSTEAD OF PULLING THE NEW POSITION OFFSET FROM THE CATFILE i.e. ... this will open three new windows. =setup "equinox" and let the telescope operator know what you will be using.

10 Nov 2017: 2016 AJ 151 51 doi:10.3847/0004-6256/151/3/51. New, 2016, 27µm image shows extensions to the NW and SW as seen in shorter wavelength observations – Blackbody temperature

12 Jan 2009: Sub-mm. Far-IR. Mid-IR. Good news: different wavelengths see different grain sizes and different structures. ... Bad news: both spatial distribution τ1/r and temperature of far-IR dust implies mass loss of 2M/Myr.

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.

12 Mar 2012: 4. Read off the new fields and interactions needed! 5. Note conserved quantum numbers! ... Plot shows likelihood of solutions in mSUGRA parameter space, using SM electroweak data and new LHC results.

13 May 2008: Project 1640 is a new collaborative project between the IoA and the Astrophysics Group at the American Museum of Natural History.

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

29 Sep 2023: 2.4.3 Tidal Locking. Remember:. Note that at New Moon we only see Earth-shine.

24 Mar 2010: Neither JAC nor CASU have budgetted for this since the requirement is a new one. ... Monthly progress and summary reports completed. 13th September - new version of ESO WFCAM FITS header document.

16 Sep 2016: origin. Show that the new orbit of a dust grain with a given β has a semimajor axis ad andeccentricity ed given by.

19 Apr 2006: All rights reserved. Printed in U.S.A. NEW SUBMILLIMETER LIMITS ON DUST IN THE 55 CANCRI PLANETARY SYSTEM. ... 2000), which was already a factor of 100 below. L96 NEW SUBMILLIMETER OBSERVATIONS OF 55 CNC Vol.

30 Sep 2015: While you may have many ideas and projects from your PhD to continue in your first postdoc, don’t let this stop you from developing new collaborations with people at your

13 Mar 2012:  New data from Planck, LHC will directly address major questions in particle physics, cosmology and the connections between them. ...  New experiments searching for dark matter, neutrino masses, anomalous gravitations effects etc are reaching

16 Nov 2017: Structure & Evolution of Stars 27. New HST observations at ultraviolet wavelengths –sensitive to [Fe/H] variations.

9 Oct 2006: 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

26 Jan 2006: The good news is these artefacts are non-astronomical in appearance and do not "talk" across the detector quadrant boundaries, or between detectors; the bad news is that they do not ... Darks. The darks, including new improved residual reset anomaly now

16 Jun 2015: this regime can we expect to discover and open up new astrophysics in the early universe. ... Either result would be very important and open up new parameter space in observational cosmology.

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).

19 Apr 2006: Received 2002 April 17; accepted 2002 September 20. ABSTRACT. New submillimeter images of the cold dust emission around the nearby main-sequence star Fomalhaut arepresented. ... object. 5. CONCLUSIONS. We have presented new, high signal-to-noise ratio sub

16 Jun 2015: 2. HgCdTe arrays for making deep NIR surveys. As part of our spectroscopy program we are also designing new spectrographs for 8-m telescopes which employ digital and hardware OH suppression.

5 Oct 2010: def@subeqnnum{{reset@fontrm (thesubequation)}} % % A new label command to refer to subequations.

6 Apr 2013: adding 10 objects to a previous survey of 150 is not a significant new result. • ... Brightness temperature for 166 radio sources. NSV 11154 is a New R Coronae Borealis Star.

26 Feb 2004: The images clearly show that while a large number of the dust particles seen on 20031008 are still present a month and a half later, there are now many new particles,

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: The command will not create a new image if an existing image has the same name. ... Note that new images can be initialsed to any value when they are created with the imcreate command.

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.

26 Feb 2000: The campaign successfully found ten new SN in the required red-shift range. ... Put seeing statistics, new flats, fringe frames etc. on too and more detailed filter responses with correct overall QE.

25 Oct 2018: This is alsoreferred to as the ‘quantum gravity limit’ because it involves new physicallaws that unify quantum physics (which describes the strong and weaknuclear forces and the electromagnetic force) and gravity

16 Jun 2015: Attempted to install new modes, but unsuccessfully 8/6/97 4.08: Installed Shutter control mode selection: type 2 = single line multiple repeat type 4 = normal type 8 = read-reset-read ... L H" % Chip 4 only % CHIPALL = "H H H H" % All Chips active %

18 Dec 2002: different seeing, PSF etc.). [For suggested set see new parameter list on diary web page] Simulations needed perhaps - get someone keen to do them. ... MJI will check with JRL (plus wants some software modules/code). FITS headers: Any news?

18 Oct 2020: We use information technology and tools to increase productivity and facilitate new forms of scholarship. ... Famine and human development: The Dutch hunger winter of 1944-45. New York, Oxford: Oxford University Press, 1975.

10 Feb 2021: In 2 we providea summary of the NO Lup system, and introduce new X-Shooterobservations. ... We note furtherwork to explore the nature of this detection, such as new highresolution imaging of the continuum,measurements for the neutralCI gas, and

2 Nov 2006: taken roughly in the middle of the night (and as it happens also taken within 4 days of new moon).

6 Nov 2018: In both cases, we find no evidence for. new physics. The Planck results for base CDM are in good agreement with baryon acoustic oscillation data and with the JLA sample of

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

20 Apr 2012: The APM Sky Catalogues: Overview. Over the last few years we have used the APM facility to measure the first epoch Palomar O and E sky survey plates, with the aim of constructing a readily accessible Northern sky optical catalogue (see Gemini No. 37

19 Apr 2006: Here we present new mid-IR observations of the Vega-likestar HD 141569 (B9.5 Ve).