... Cycle 20 Phase II Proposal Instructions . ... When you first bring up APT, you will have to convert the information in your Phase I proposal, which is an XML file, into a Phase II program format using the ?Phase I->Phase II? conversion button on the APT User Interface. ... After converting your Phase I Proposal into Phase II information, please verify that all the general information is correct and readable. ... As with the Abstract , please review this text to make certain the information is...

... Posts tagged ?Methods? ... This is a special session at the January 2010 meeting of the AAS. ... Tags: 2010 , 215 , AAS , AAS 215 , astroinformatics , astrostatistics , complex data , January , Methods , special session , Washington . ... Comment . ... If you are attending the meeting, and plan to present posters or talks that deal with astrostatistical methods or techniques, we welcome you to participate in this session. ... There is also a page for this session on the astrostat google groups site....

... Two files from two exposures (even from different observations or instruments) are taken as input. These may be EPIC event lists or two other additional files (attitude files, orbit files etc [see comments]). ... Warnings are given when the event files are deemed not entirely compatible (i.e. their INSTRUME or FILTER keywords are different). ... Given here is a summary of the current conditions whereby event files (or parts thereof [blocks/columns etc]) are or are not merged. ...

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... Hopkins: The Phoenix Deep Survey at 1.4 GHz . ... For details of the Phoenix multiwavelength deep survey, refer to MNRAS 296, p839, 1998. ... We present the first results from the Phoenix Deep Survey, a multiwavelength survey of a 2 deg diameter region. Observations in the radio continuum at 1.4 GHz carried out with the Australia Telescope Compact Array are described. The catalogue of over 1000 radio sources compiled from these observations is analysed, and the source counts are presented. ...

Proposal Identification No.: ... For these observations night-time is not needed. Begin ­ End Interval ­ Interval 1700 ­ 2200 ­ ­ ­ Days Needed at This Interval 14 Time Constraints (Must Be Justified in the Prop osal Text) In order of scheduling: 2 gridding sessions : 3.5h and 2.5h (ALFA) Starting at least a week later (L-wide or 327MHz, TBD by the gridding sessions ): 3 sessions of 3h each on successive days 1 session of 3h a week later 1 session of 3h two weeks later 11 monthly ...

Title: A New Model of the Gravitational Lens 0957+561 and a Limit on the Hubble Constant . Authors: Norman A. Grogin , Ramesh Narayan (Harvard Univ.) ... Title: ROSAT/PSPC observation of the distant cluster CL0939+472 . ... Title: Interaction in the Bimodal Galaxy Cluster A3528 . ... Title: Cosmological Implications of Galaxy Cluster Evolution . ... Title: Galaxy Cluster Virial Masses and Omega . ... Matches 201 to 222 from a total of 222 matches for the search pattern galaxy cluster . ...

Journal of Atmospheric and Solar-Terrestrial Physics Manuscript Draft Manuscript Number: ATP1021 Title: comment on the paper by Dalin , Pertsev and Romejko Significance of lunar impact on noctilucent clouds ( revised version) Article Type: Research Paper Section/Category: Keywords: Noctilucent clouds moon influence mesosphere Manuscript Region of Origin: Abstract: a critical review of the paper by Dalin , ... Reference: Dalin, P.A., N.N. Pertsev, V.A. Romejko. ...

... Natalya V. Raguzova and Sergei B. Popov . ... We present a compilative catalogue of Be/X-ray binaries and candidates in the Galaxy and in the Large and Small Magellanic Clouds. This catalogue contains 160 sources and provides information on names and spectral types of optical components, distances, on spin characteristics of neutron stars, and on orbital and X-ray properties of binary systems. ... Be/X-Ray Binaries and candidates in the Galaxy . Galactic sources: comments to the Table 1 . ...

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