... Science . ... Science Users Information > Science Publications > Science Announcements > Call for Observing Proposals for Period 95 . ... Science Users Information . Observing Facilities . ... APEX . ... Observing with ESO Telescopes . ... The Call for Proposals for observations at ESO telescopes during Period 95 (1 April - 30 September 2015) has been released. ... All technical information about the offered instruments and facilities is contained on ESO webpages that are linked from the Call . ...

HST Call for Proposals and HST Primer for Cycle 24 . ... Hubble Space Telescope Call for Proposals for Cycle 24 > Chapter 5: Data Rights and Duplications > 5.1 Data Rights . 5.1 . Data Rights . ... Submitters of Small and Medium GO Proposals who wish to request a proprietary period shorter than one year (3 or 6 months), or who are willing to waive their proprietary rights altogether, should specify this in the ?Special Requirements? section of the proposal (see Section 9.3 ). ...

... Arecibo proposals submitted for the March 3, 2016 (17 AST, 21 UTC), deadline are for telescope usage during the six-month (or in some cases one-year) period beginning July 1, 2016. ... The 2 x 7, dual-polarization, 300-MHz bandwidth, "Mock" spectrometers are available to all ALFA users. ... A SINGLE-PIXEL MODE for the Mock spectrometers is available. This can provide up to 1 GHz of contiguous spectral coverage. ... For an overview of WAPP capabilities, see WAPP spectrometer information . ...

... Observation codes for VSOP General Observing Time observations have the form . ... The first letter indicates which AO period the observation was proposed in: the letter `v' indicates the first AO period, and the letter `w' indicates the second and third AO periods. The three digits indicate the proposal number. ... For proposals with more than 26 experiments (see next item), 300 is added to the proposal code for the 27th and subsequent experiments. ...

ARCSAT Call for Proposals for Shared-Risk Observing during May-Sept 2014 Suzanne Hawley, Director and Mark Klaene, Site Manager April 18, 2014 Updated June 14, 2014 We are happy to announce that the ARCSAT upgrade project led by APO engineers Joe Huehnerhoff and Bill Ketzeback is nearly complete. ... ARCSAT proposals will be accepted as text files using the ARCSAT proposal form (available from the website) which is similar to the 3.5m proposal form. ... Remember, the time is shared-risk! ...

Next: Stars without Periods Up: Other Stars Previous: Stars with Highly . ... However, due to lower signal to noise their periods are less secure. ... This could be interpreted as a continuous distribution with statistically insignificant deviations which give the appearance of gaps or a real gap. ... When the distributions of periods greater five days are compared for the ONC stars and those near Orionis the KS test gives a 47% probability of these distributions being drawn from the same population. ...

Space VLBI Mission RadioAstron Announcement of Opportunity -- 1 for the period July 2013 ­ 30 June 2014 Key Science Program ( KSP ) Final Notes Proposals Due: 8 February 2013, 23:59 UT 1 RadioAstron KSP meeting follow-up Based on the fruitful discussions, questions and suggestions from the RadioAstron Key Science program meeting in Bonn (December 3-4, 2012), we would like to emphasize the following specific aspects for the preparation of the AO-1 ...

... The process of proposing for Hubble Space Telescope observing time has been revised, to make it simpler for proposers. We describe the simple, flexible, and robust prototype system created to handle proposal submission. ... Proposing for Hubble Space Telescope ( HST ) observing time proceeds in two phases: the scientific merits of the proposal are considered in Phase I; only accepted proposals enter Phase II, where the observations are described in complete detail. ...

... For scheduling purposes, the Compton Gamma Ray Observatory mission has been divided into phases corresponding to proposal cycles. Phase 1 lasted from 1991 April, through 1992 November, and constituted the first complete survey of the gamma-ray sky. ... Viewing periods have lasted from a few days to three weeks. ... In most cases, the gaps between viewing periods are a few hours, the time needed to re-point and stabilize the Compton Observatory. ...

Subject: Call for proposals TIRGO Oct 2003 - Mar 2004 To all TIRGO users. All observers who intend to present applications for TIRGO in the 6 months period 2003B (1 October 2003 - 31 March 2004) are kindly invited to do it before June 15th, 2003. ... The camera cryostat contains a cold filter wheel with 10% bandwith filters at 8.8, 9.8, 10.3, 11.7 and 12.5 micron, the standard broad-band N filter (8.1-13.1 micron), and a circular variable filter (CVF) between 8-14 micron with a resolution of ~3%. ...

. The International Astronomy Olympiad .

... The evolution equation presented above indicates that an accreting compact star must endeavor to attain an equilibrium state in which the resultant torque vanishes (Davidson and Ostriker, 1973[ 38 ]; Lipunov and Shakura, 1976[ 109 ]). ... Let us turn to the case of disk accretion. ... Since , the equilibrium period in the case of disk accretion is close to the critical period, , separating accretion stage A and the propeller stage P . ...

Please enter the lightcurve file name and period search parameters: . Lightcurve file: . ... Apply the Heliocentric correction and convert all dates to Terrestrial Time (TT)? ... Also, the Heliocentric correction cannot be applied to such lightcurves. ... This period search service is also available at the mirror sites: Mirror 1 , Mirror 2 , Mirror 3 , Mirror 4 . You may download the latest source code distribution and install the period search service at your own web server. ...

На главную страницу НМУ миникурс будет читаться в апреле 2014 на матфаке ВШЭ в течении 3 недель 2 раза в неделю. Brief introduction to motives, with emphasis on the Tannakian viewpoint and motivic cohomology. Discussion of multiple zeta values; the theorem of Brown that all unramified mixed Tate motives over Z are multiple zeta. Motives and periods associated to motivic cohomology. ... Занятия будут по вторникам c 15:30 в аудитории 1001. ...

... If requested ( runbackground =Y), the task creates a background lightcurve, as well as a background spectrum for the imaging modes (FF, eFF, LW, SW) using background masks. ... The background masks are created by task badpixfind using threshold parameters, appropriate for the detection of real X-ray sources. ... As the GTIs strongly depend on the intended science this screening is not performed and only background masks, the lightcurve, and a GTI file are created by epchain . ...

... 2013, Nature Pepe et al. ... HARPS-N ­ Fit offset to each night Prot = 21 days Prot = 12.4 days Extra information is needed Corot 7b Bayesian Analysis with correlations (NEW) Tuomi et al. in prep. ... No planets reported RMS 2.0 m/s over 7 years Star 3 Star 3 ... but we also got lucky :) RMS ~ 0.9 m/s Kapteyn b, P = 48.7 days, M sin I = 4.0 Mearth, Kapteyn c, P = 121.0 days, M sin I = 7.0 Mearth, ... but we also got luck/y] :)-0 [Fe H ~ .9 Age > 10 Gyrs? ... 5 AU Kapteyn's 0. 0 0. 15 b c 0. ...

Общая Астрономическая Конференция > Форумы общей направленности > Любые вопросы от новичков . Vopros po povodu nabljudenij v letnij period . ... Поиск . ... Созвездия (поиск и описание) .. Созвездия южного неба (поиск и описание) .. Осенние созвездия (поиск и описание) .. Летние созвездия (поиск и описание) .. Околополюсные созвездия (поиск и описание) .. Весенние созвездия (поиск и описание).. Зимние созвездия (поиск и описание) .. ...

Please enter the lightcurve file name and period search parameters: . Lightcurve file: . ... Apply the Heliocentric correction and convert all dates to Terrestrial Time (TT)? ... Phase range for plots: -0.5 to 1.0 0.0 to 2.0 0.0 to 1.0 . ... Also, the Heliocentric correction cannot be applied to such lightcurves. ... Two period search methods are currently implemented. ... This period search service is also available at the mirror sites: Mirror 1 , Mirror 2 , Mirror 3 , Mirror 4 . ...