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Planetary System DynamicsPart III Mathematics / Part III Astrophysics …
https://people.ast.cam.ac.uk/~wyatt/psd_eg2.pdf5 Nov 2023: the eccentricity of the new orbit e2. -
PowerPoint Presentation
https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_14.pdf6 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 -
Question_solutions
https://people.ast.cam.ac.uk/~gpe/Question_solutions.pdf16 Mar 2012: There are new leptoquarks which allow transitions along the rows between the coloured quark states and the colourless leptons. -
M. Pettini: Structure and Evolution of Stars EXERCISES: Set ...
https://people.ast.cam.ac.uk/~phewett/SandES2017/Examples1_2017.pdf13 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. -
https://people.ast.cam.ac.uk/~optics/cirsi/ociw/DuPontIoaTimeProposals…
https://people.ast.cam.ac.uk/~optics/cirsi/ociw/DuPontIoaTimeProposals/cirsi-dupont-bulge-gilmore-proposal.txt16 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. -
Microsoft PowerPoint - wyatt
https://people.ast.cam.ac.uk/~wyatt/wyatt_hst08.pdf7 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. -
https://people.ast.cam.ac.uk/~rgm/vhs/newsletter/VHS_Newsletter_1.txt
https://people.ast.cam.ac.uk/~rgm/vhs/newsletter/VHS_Newsletter_1.txt19 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. | |-------------------------------------------------------- -
PowerPoint Presentation
https://people.ast.cam.ac.uk/~phewett/Astro-jobs_1_2308.pdf15 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. -
PrimordialD_jun18.key
https://people.ast.cam.ac.uk/~pettini/Primordial%20D%20Jun185 Jul 2018: 1950s. AlpherGamowHermanHayashi. BBN CMB. = New Physics? BBN CMB. = New Physics? -
PowerPoint Presentation
https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_22.pdf17 Nov 2017: Historically, until last fifteen years, “objective-prism” spectra employed. • New wide-field photometric surveys allow accurate (few percent, i.e. -
LOCAL HEATING IN THE GALACTIC CENTER WESTERN ARC N. ...
https://people.ast.cam.ac.uk/~wyatt/mtpf03.pdf19 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 -
Chapter 4 - Controls Reference
https://people.ast.cam.ac.uk/~optics/cirsi/docs/pixcel/20010508/chapter4.htm16 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. -
David King's Home Page
https://people.ast.cam.ac.uk/~king/13 May 2008: Project 1640 is a new collaborative project between the IoA and the Astrophysics Group at the American Museum of Natural History. -
Chapter 5 - Tutorials
https://people.ast.cam.ac.uk/~optics/cirsi/docs/pixcel/20010508/chapter5.htm16 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. -
https://people.ast.cam.ac.uk/~rgm/cirsi/ociw/cirsi-guide-sylvie-beauli…
https://people.ast.cam.ac.uk/~rgm/cirsi/ociw/cirsi-guide-sylvie-beaulieu.txt3 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. -
McMahon
https://people.ast.cam.ac.uk/~rgm/vhs/PSP_feedback_VHS_McMahon.doc18 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. -
CASU WFCAM/VISTA Diary Page
https://people.ast.cam.ac.uk/~wfcam/diary.html24 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. -
PowerPoint Presentation
https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_16.pdf10 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 -
Debris disk dynamical theory Mark Wyatt Institute of Astronomy, ...
https://people.ast.cam.ac.uk/~wyatt/MarkWyatt_Spitzer2008Conference.pdf12 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. -
Table of Contents 2 Tides Locally familiar 2.1 Astrophysical ...
https://people.ast.cam.ac.uk/~wyatt/topics2.pdf29 Sep 2023: 2.4.3 Tidal Locking. Remember:. Note that at New Moon we only see Earth-shine. -
HAWAII SAM MICROCODE
https://people.ast.cam.ac.uk/~optics/cirsi/SAM/cirsi_sam_microcode_22dec97.html16 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. -
Astroparticle_14
https://people.ast.cam.ac.uk/~gpe/Astroparticle_14.pdf12 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. -
Observing guide for CIRSI (WFIRC) at LCO du Pont ...
https://people.ast.cam.ac.uk/~optics/cirsi/cirsi-guide-lco-0.6.html16 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). -
L187 The Astrophysical Journal, 619:L187–L190, 2005 February 1� 2005. …
https://people.ast.cam.ac.uk/~wyatt/ghwd05.pdf19 Apr 2006: ABSTRACT. New submillimeter images have been obtained of the dust disk around the nearby K2 V stare Eridani, withthe total data set now spanning 5 yr. ... 4. DISCUSSION. The new images of thee Eri dust ring confirm its structureand dimensions, and the -
https://people.ast.cam.ac.uk/~optics/cirsi/ing/proposals_public/2001/2…
https://people.ast.cam.ac.uk/~optics/cirsi/ing/proposals_public/2001/2001a/int_2001a_cirsi_sur.log16 Jun 2015: It should NOT be used for NEW documents! New documents should use Standard LaTeX conventions and start with the documentclass command. -
MATHEMATICAL TRIPOS Part III Friday, 27 May, 2016 1:30 ...
https://people.ast.cam.ac.uk/~wyatt/psd_exam2016.pdf16 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. -
L93 The Astrophysical Journal, 570:L93–L96, 2002 May 10 �� ...
https://people.ast.cam.ac.uk/~wyatt/jhkg02.pdf19 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. -
fellowships_2015
https://people.ast.cam.ac.uk/~phewett/HPeiris_fellowships_2015.pdf30 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 -
Astroparticle_16
https://people.ast.cam.ac.uk/~gpe/Astroparticle_16.pdf13 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 -
PowerPoint Presentation
https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_19.pdf16 Nov 2017: Structure & Evolution of Stars 27. New HST observations at ultraviolet wavelengths –sensitive to [Fe/H] variations. -
About the Instrumentation Group
https://people.ast.cam.ac.uk/~optics/about.htm16 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. -
ESO Public Surveys Proposal Form Phase 1 Title: The ...
https://people.ast.cam.ac.uk/~rgm/vhs/PS-VHS-v4p2-Appendix-B-PSP-Response.pdf9 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 -
3CD8ACD5-01E7-18B8
https://people.ast.cam.ac.uk/~optics/dazle/info/science.pdf16 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. -
SUBMILLIMETER OBSERVATIONS OF AN ASYMMETRIC DUST DISK AROUND…
https://people.ast.cam.ac.uk/~wyatt/hgdw03.pdf19 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 -
https://people.ast.cam.ac.uk/~pettini/canaries13/cupconf.sty
https://people.ast.cam.ac.uk/~pettini/canaries13/cupconf.sty5 Oct 2010: def@subeqnnum{{reset@fontrm (thesubequation)}} % % A new label command to refer to subequations. -
Domain walls, cosmic strings and monopoles, dark matter ...
https://people.ast.cam.ac.uk/~gpe/Astroparticle_11.pdf27 Feb 2012: With Higgs and other vacuum fields, this means that the vacuum itself drops into a new phase. ... long strings interacting will create new loops, so get population of lines and loops which tend to stable “scaling solution”. -
Index of /~optics/cirpass
https://people.ast.cam.ac.uk/~optics/cirpass/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. -
Astroparticle_1
https://people.ast.cam.ac.uk/~gpe/Astroparticle_1.pdf5 Feb 2013: Bottom b! Tau τ! Neutrino ντ!This is the new periodic table of the elements! ... Define new field H=φ-µ/λ:!Higgs acquires a mass because of the broken symmetry. -
MATHEMATICAL TRIPOS Part III Wednesday, 3 June, 2015 1:30 ...
https://people.ast.cam.ac.uk/~wyatt/psd_exam2015.pdf9 Oct 2015: v22 v21) 4(Mp/M)2ǫ21 v5pv3. Hence show that the new orbit has a semimajor axis with a corresponding ǫ2 thatsatisfies. -
PowerPoint Presentation
https://people.ast.cam.ac.uk/~phewett/IAU_1208_Journal_pres.pdf6 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. -
This is the text of the SAM microcode that ...
https://people.ast.cam.ac.uk/~optics/cirsi/SAM/cirsi_sam_microcode_code_27may98.html16 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 % -
The Dynamics of Scarlet Fever Epidemics in England and Wales in the…
https://people.ast.cam.ac.uk/~vasily/data/scarlet.pdf18 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. -
MNRAS 000, 1–6 (2020) Preprint 30November 2020 Compiled…
https://people.ast.cam.ac.uk/~wyatt/lkmw20.pdf10 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 -
The APM Sky Catalogues: Overview
https://people.ast.cam.ac.uk/~mike/apmcat/overview.html20 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 -
Project Reassessment Start Date
https://people.ast.cam.ac.uk/~optics/cirsi/docs/review/webreview.htm16 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 -
https://people.ast.cam.ac.uk/~optics/cirsi/ociw/lco1999may/eric/reduct…
https://people.ast.cam.ac.uk/~optics/cirsi/ociw/lco1999may/eric/reduction_manual16 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. -
CASU analysis of SV data for WFCAM
https://people.ast.cam.ac.uk/~wfcam/docs/reports/sv/index.html26 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 -
14667ms.dvi
https://people.ast.cam.ac.uk/~wyatt/mskp10.pdf27 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 -
https://people.ast.cam.ac.uk/~rgm/wfcsur/meetings/wfs_minutes_draft_20…
https://people.ast.cam.ac.uk/~rgm/wfcsur/meetings/wfs_minutes_draft_20000117.txt26 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. -
https://people.ast.cam.ac.uk/~wfcam/docs/ukidss02.txt
https://people.ast.cam.ac.uk/~wfcam/docs/ukidss02.txt18 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?
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