OptInt PmWiki : MROI Fast Tip Tilt / Tech Meet 6 . ... Attendees: JSY, MF, ADR, XS, CAH, DMAW, EBS . ... With reference to error budgets . ... Selection of layouts and error budgets to present at CoDR . ... Dog-leg Transmissive . ... Zoom Transmissive . ... ADR: Refine selected layouts . ... Space to overhang table . ... ADR: Tolerancing of direct transmissive layout under table bending . ... Printable View of http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/pmwiki.php/MROIFastTipTilt/TechMeet6) ...

... Tonight's Sky . ... The Magazine . ... Observing . ... The double star 54 Leonis, spiral galaxy NGC 3198, and emission nebula NGC 3199 . ... Astronomy for Kids . ... Observing springtime deep-sky objects with a large telescope . ... Bright planets meet at dusk . ... Astronomy magazine subscribers can read the full article for free. ... Get instant access to subscriber content on Astronomy.com! ... Receive news, sky-event information, observing tips, and more from Astronomy's weekly email newsletter....

... User Guide ] Key: select This keyword selects the subset of the visibility data to be processed. ... If only one value is given, uvmin is taken as zero. uvnrange(uvmin,uvmax) Select visibilities with uv radius between uvmin and uvmax (in nanoseconds). If only one value is given, uvmin is taken as zero. visibility(n1,n2) Select visibilities numbered n1 to n2 inclusive. increment(inc) Select every inc'th visibility. ra(r1,r2) Select visibilities whose RA is in the range r1 to r2. ...

... GOODS unites extremely deep observations from NASA's Great Observatories, Spitzer , Hubble , and Chandra , ESA's Herschel and XMM-Newton , and from the most powerful ground-based facilities, to survey the distant universe to the faintest flux limits across the electromagnetic spectrum. ... The space-based observations are complemented by ground-based imaging and spectroscopy, including extensive commitments of ESO and NOAO observing time. ... 2010-04-10: Deep VLA 1.4 GHz data for GOODS-North . ...

... This step is done mostly interactively and uses some basic ad-hoc IDL procedures, mainly for testing and checking of the consistency of the results.Once the observations have been selected and the count spectra extracted, the available spectra of each background level are accumulated. ... Average QUALITY such that QUALITY =0|1 Exposure times are added and the total is written in the EXPOSURE keyword of the header of the output FITS file. Finally, the CCFs are built from these templates. ...

... This represents the first HI selected sample covering the core and the outskirts of a local cluster of galaxies. ... Optically selected samples miss a considerable number of low luminosity, low surface brightness galaxies underestimating by almost a factor 2 the number of HI rich galaxies present in the cluster volume. ... Right: The g band luminosity function for galaxies in the A1367 volume as obtained from the optically (circles) and HI (histogram) selected sample. ...

... The numbers of three types of compact binaries containing accreting NSs and BHs, which are most interesting from the point of view of their observational appearances, have been calculated as a function of time: i) X-ray transient source containing a NS in an eccentric orbit around a main sequence Be-star (the observed prototype: A0535+26), ii) BH The evolution of the selected types of X-ray binaries during the first 10 million years after the starburst onset is presented in Fig. ...

Next: The APM selected sample Up: Second priority candidates Previous: Second priority candidates . From the random selected subsample of second priority candidates we observed twenty six objects during the 6-m telescope runs (mainly those with R.A.< 11 h ) along with the observations of first priority targets. Altogether we found 12 emission-line objects: one appeared to be a QSO with z =3.15, and the rest are various types of ELGs. ... One object is an absorption-line galaxy. ...

... Visited 6949 times - Selected 51 months ago . ... Visited 7311 times - Selected 51 months ago . ... Visited 4085 times - Selected 52 months ago . ... Visited 4399 times - Selected 52 months ago . ... Visited 4150 times - Selected 52 months ago . ... Visited 4559 times - Selected 51 months ago . ... Visited 3961 times - Selected 52 months ago . ... Visited 9211 times - Selected 51 months ago . ... Visited 2227 times - Selected 52 months ago . ... Visited 3974 times - Selected 51 months ago . ...

These observations are aimed at fully charactering FORS1 photometric system (UBVRI zero-points, color-terms and extinction coefficients) for the Tektronix 2048x2048 pixel CCD (24µm px) . To this aim, the two Landolt/Stetson photometric fields SA95 and SA101 will be observed on a number of epochs and at different airmasses during February and March 2007. ... SA101 . ... OBs for SA101 have to be observed during evenigh twilight (exceptions are expected for the second half of March) . ...

... Accelerating black holes, spin-2/3fields and C-metric . A TOPOLOGICAL EXTENSION OF GENERAL RELATIVITY TO EXPLORE THE NATURE OF QUANTUM SPACETIME, DARK ENERGY AND INFLATION . EFFECTIVE THEORY FOR QUANTUM GRAVITY . TESTS OF GENERAL RELATIVITY AND ALTERNATIVE THEORIES OF GRAVITY USING GRAVITATIONAL WAVE OBSERVATIONS . ... THE MASS OF THE OPPENHEIMER-SNYDER-BLACK HOLE: ONLY FINITE MASS QUASI-BLACK HOLES . ... NEUTRINO MASS AND THE STANDARD MODEL . Neutrino masses and flavor mixing . ...

... In one situation, we can use light from quasars to probe the material between us and them because that light may pass through one or more galaxies or gas clouds on its way to us. The gas inside the galaxies or the intergalactic clouds acts then as a filter, absorbing selected wavelengths from the quasar light. ... Light from a quasar must pass through clouds of gas and even faint galaxies -- each leaving its imprint on the light -- before we receive it here on Earth. ... Gravitational lensing . ...

Klimov,S.I., V.V.Kopeikin, V.V. Krasnosel`skikh, A.M.Natanzon, A.E.Reznikov, M.P.Gough, S.P.Kingsley, T.A.Lachlan-Cope, H.G.Muller, L.J.C.Woolliscroft. ... Space Res., (1990), v.10, No.3-4, (3)35-(3)38. Grard,R., C.Nairn, A.Pedersen, S.Klimov, S.Savin, A.Skalsky, J.G.Trotignon. ... Space Sci., (1991), vol.39, No.1/2, pp.89-98. ... Res. ... Space Res., (1991), vol.11, No.9, pp.( ... Space Res., vol.11, No.9, p.(9)15-(9)18, 1991. ... Adv. space Res., v.11, No.9, p.19-34, 1991. ...

The K20 survey. I. Disentangling old and dusty star-forming galaxies in the ERO population", 2002, Cimatti A. et al., ... Probing the evolution of massive galaxies with the K20 survey", 2002, Cimatti A., invited contribution in the ESO/USM Workshop "The Mass of Galaxies at Low and High Redshift", Venezia (Italy), October 24-26, 2001, in press. ... The K20 survey: new light on galaxy formation and evolution", 2003, Cimatti et al., ... Old galaxies in the young Universe", 2004, Cimatti et al., ...

Next: HST Paper Products: A New Way to Look at HST Data . ... After providing on-the-fly re-calibration of HST data to archive users, ST-ECF has embarked on a new project aiming at grouping, cosmic ray cleaning and drizzling images taken by most HST instruments. ... The production of the missing jitter files combined with the extraction of additional engineering parameters will greatly enhance the homogeneity and the scientific value of the entire archive. ... 1995, HST Data Handbook, STScI, 107 . ...

... Пиджак Selected One Creed Moдель: 16046564 One SHCreed Blazer IСостав: 60% полиэстер 30% шерсть 10% другие волокна Модель: 27955519 . ... Пиджаки . ... Артикул: 93-DE-ZU-13 Цвет: металл Состав: нержавеющая сталь, стекло Описание: практичная и удобная сахарница с ложечкой будет незаменимым аксессуаром при любым семейном чаепитии. ... Кеды Woden Kasper Moдель: Kasper Low 14192 Модель: 2633504 . ...

RadioAstron AO-4 prop osal Submission dead line: 25 January 2016, 23:59 UT. ... Pro ject type: KSP Select from the fol lowing: KSP or GOT. ... Team contact name and e-mail address: Ivan Petrov (e-mail: Ivan.Petrov@gmail.com ) Total observing time request: 60 hrs Should be < 100 hours if GOT. ... Observational Strategy -- describing the methodology of observations. ... AO-4 Observations -- describing specific observations and time request for the AO-4. 5 e o r . ...

Storing and accessing the largest astronomical catalogues with the SAI CAS project S. Koposov1,2,3, O. Bartunov2, S. Karpov4 et al2. ... Why we want to build our own Catalogue Access Service The requirements for our CAS system The importance of the Database for the CAS (PostgreSQL & Q3C) The technical realization of CAS What has been already done Example of work TODO Storing and Accessing Astronomical Catalogues Existing projects CDS OpenSkyQuery CASjobs with SDSS They are all really great! ...

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... BBC Stargazing LIVE . An Creag n . Beaghmore Stone Circles . Beaghmore drawings . ... Armagh Observatory and the Northern Ireland Environment Agency (NIEA) together with An Creag n and the Omagh and Cookstown District Councils are hosting a day of free BBC Stargazing LIVE and Universe Awareness (UNAWE) activities at An Creag n and the nearby Beaghmore Stone Circles. ... Living History and Observing at Beaghmore . ...

... Equivalent widths of Ca I absorption lines at 6122?, 6162?, and 6494? and Fe I at 6103?, 6200?, and 6574? were measured for several spectral standards. ... The spectral types of the target stars were determined by comparing source line ratios to those of standard stars. ... The uncertainty in the spectral type is about one and a half sub--types. ... Northwest of the belt, again all but one source shows Li in absorption, but only one star (out of 13 = 7.7%) shows an H emission line. ...