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http://www.stsci.edu/hst/hst/proposing/documents/cp/9_PDF_Attachment7.html.
http://www.stsci.edu/hst/hst/proposing/documents/cp/9_PDF_Attachment7.html.
1. Proposing Overview
STScI . ... Phase I Proposing . ... Astronomer's Proposal Tool . ... STScI solicits proposals for HST Observing, Archival Theoretical Research. ... HST Cycle 24 Phase II Proposal Deadline . The Call for Proposals (CP) invites the astronomical community to propose for observing time on HST in a given cycle (nominally one year in duration). It summarizes the policies and procedures for proposing in that cycle of HST observing, including requests for funding research on archival HST data. ...
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Ссылки http://www.stsci.edu/hst/proposing/docs/proposingOverview -- 20.5 Кб -- 10.04.2016
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2. ESO - Instrumentation Development
... Science . ... Science Users Information > Observing Facilities > Instrumentation Development . ... Science Users Information . ... La Silla Paranal Observatory . ... Paranal Instrumentation . Decommissioned Instruments . ... VLT/VLTI Science Verification . ... ESO exercises strict control over the interfaces between the VLT observatory and its instruments. ... The instruments below are now maintained (and documented on the ESO web) by the Directorate of Operations/La Silla Paranal Observatory: . ...
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Ссылки http://www.eso.org/sci/facilities/develop.html -- 36.7 Кб -- 09.04.2016
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3. Calibration and Performance Control for the VLT Instrumentation
Next: The ESO VLT CCD Detectors Software . ... Up: Instrument-Specific Software . ... The framework for data calibration and analysis of the VLT instrumentation is presented, based on the concepts of a calibration plan, pipeline calibration, quality control, and archiving of calibrated data for a ground-based observatory. ... Quality Control Pipeline provides quality assessment for instrument performance data and observing conditions, and tests the results of the Reduction Pipeline. ...
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Ссылки http://www.adass.org/adass/proceedings/adass96/ballesterp.html -- 9.3 Кб -- 23.06.1998
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4. Pulsar Group Main/Psrfits
... There are compelling reasons for the pulsar community to utilise a standard data storage format. For example, standardisation of file formats significantly decreases the amount of effort required to integrate new instruments into the analysis chain. ... Accordingly, we have defined PSRFITS as a standard FITS-based format for pulsar data files. ... For example, the first line of Processing History HDU contains information about the data acquisition program and the initial structure of the file. ...
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Ссылки http://www.atnf.csiro.au/people/pulsar/index.html?n=Main.Psrfits -- 15.3 Кб -- 12.04.2016
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5. http://www.apo.nmsu.edu/Telescopes/ARCSAT/Operations/arcsat_cfp.pdf
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! ...
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Ссылки http://www.apo.nmsu.edu/Telescopes/ARCSAT/Operations/arcsat_cfp.pdf -- 48.7 Кб -- 16.06.2014
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6. http://xmm.vilspa.esa.es/sas/6.5.0/doc/calview.ps.gz
XMM-Newton Science Analysis System Page: 1 calview August 16, 2005 Abstract An interactive viewer of the XMM calibration database. 1 Instruments/Modes Instrument Mode all all 2 Use pipeline processing no interactive analysis yes 3 Description The XMM calibration database is comprised of 100 calibration datasets (the current calibration le, or CCF [1]), and a number of calibration algorithms and access functions (the calibration access layer, or cal). ... The former is described in detail in cal. ...
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Ссылки http://xmm.vilspa.esa.es/sas/6.5.0/doc/calview.ps.gz -- 76.3 Кб -- 16.08.2005
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7. HST/FOS Atlas of AGN and Quasars
As a service to the astronomical community, we are recalibrating all archival Hubble Space Telescope Faint Object Spectrograph UV and optical spectrophotometry of active galaxies and quasars in order to extract uniformly calibrated spectrophotometric data for further detailed scientific investigations. ... NGC 4151 CLOUD F . NGC 5548 . ... NGC 4395 . ... NGC 4486 . ... NGC 4486 JET KNOT-A . ... NGC 4486 CLOUD-A . ... NGC 3031 . ... NGC 1068 . ... NGC 1068 CLOUD A . ... 1413+117A . ... NGC 4151 . ...
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Ссылки http://hea-www.harvard.edu/FOSAGN/ -- 18.4 Кб -- 27.02.2014
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8. OptInt PmWiki : MROI / Science Instrument Downselect
... Workpackage Status 2006/10/12 . Proc. SPIE paper on downselect . ... Due Date . ... P4S combiner optimization . ... P4S switchyard optimization . ... P8 combiner optimization . ... P8 (internal) switchyard optimization . ... Due 2006/07/31 . 70% done . ... P4S/P8 spectrograph optimization . ... I4S combiner optimization . ... I4S switchyard optimization . ... Printable View of http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/pmwiki.php/MROI/ScienceInstrumentDownselect) ...
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Ссылки http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/pmwiki.php/MROI/ScienceInstrumentDownselect?action=print -- 14.0 Кб -- 01.03.2014
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9. http://www.naic.edu/vscience/schedule/tpfiles/KaspitagP1636tp.ps
P1636 2002-Feb-01 18:06:19 Technical Page Proposal Type: Regular General Category: Pulsars Sub-Category: Continuum Observation Category: Galactic Total Time Requested: 54 Hours Proposal Title: A Complete 1.4-GHz Search for Pulsars in Globular Clusters Using WAPP ABSTRACT: In June 2001 we obtained 1.4-GHz Arecibo pulsar search data toward 10 globular clusters using the WAPP instrument. ... Maybe Part of the observing run. ... This proposal requires coordination with GPS L3 at 1381 MHz. ...
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Ссылки http://www.naic.edu/vscience/schedule/tpfiles/KaspitagP1636tp.ps -- 92.3 Кб -- 19.04.2004
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10. Observing capabilities
... NICS will be the only infrared instrument for the first light of the TNG; as a consequence, we decided to incorporate a sufficient degree of operation flexibility by providing the instrument with six different observing modes, three aimed at imaging and three at spectroscopy: . ... It will be possible to use the narrow band filters as order sorters; this will allow to perform high resolution long-slit spectroscopy in the wavelength ranges covered by the available narrow band filters. ...
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Ссылки http://www.arcetri.astro.it/irlab/instr/nics/generale/osserv.html -- 6.1 Кб -- 28.07.2005
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