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12 Jul 2002: This new schema reflects the fact that the classifier is (ideally) Bayesian and up until now I have been assuming the equivalent of a deep high latitude prior (ie.

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.

17 Mar 2006: o Legacy value, Serendipity and new classes of object. o Maximising the science return from ESA missions, XMM-Newton, Planck, Herschel and GAIA.

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 Jul 1999: Here is the population model used (note that we have some new official predictions to 2005 that we will use to update these figures soon, but they make little difference to

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).

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.

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: 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

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.

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 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

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.

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

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: 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

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)?

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.

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

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

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.

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.

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. •

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

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

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

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

10 Jul 2024: FitteR for Accretion ProPErties of T Tauri stars (FRAPPE): A new approach to use Class III spectra to derive stellar and accretion properties. ... An ALMA Survey of M-dwarfs in the Beta Pictoris Moving Group with Two New Debris Disc Detections.

12 Jul 1999: Here is the population model used (note that we have some new official predictions to 2005 that we will use to update these figures soon, but they make little difference to

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.

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.

16 Jun 2015: Before you install your software. If you are using a new PC with your system, it is strongly recommended you check your PC system is functioning correctly.

16 Jun 2015: In conjunction with the improved image quality now demonstrated with new 6.5-10 m telescopes, DAZLE will be the only instrument well suited to searching for early star-forming systems

8 Jul 2000: Villafranca Station at Villafranca del Castillo, Spain VLA Very Large Array (Radio Telescope in New Mexico) VOB Vertical Optical Branch V&V Validation and Verification WAN Wide Area Network WFC Wide

11 Oct 2023: Astronomy is a collaborative endeavour. At least some fixed-term contracts can be replaced by open-ended contracts, with people moving to new funding sources as they become available. ... a3877756.html. [10]

27 Aug 2022: 4355. 91. R. MacDonald and N. Madhusudhan, HD 209458b in New Light: Detection of Nitrogen Chemistry, Patchy. ... Matsumura, T-S. Pyo, Deep Thermal Infrared Imaging of HR 8799 bcde: New.

30 Mar 2009: The new (O2)4 structure is not the lowest-energy structure at this level of theory, demonstrating the need for additional studies. ... sensitive detectors have arrived on wide-field imaging instru-ments, on a new generation of 8-metre-aper-ture telescopes

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

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

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

13 Oct 2006: New disks: >30mJy (none), 10-30mJy (5), 3-10mJy (9). • Mean flux of non-detections is 0.3mJy. • ... Expect some structures explained by current models. • For others new dynamical models will be developed.

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

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

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

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.

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

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