... Raw science 1 . ... The rootnames of the individual exposures in an associated data set are contained in the association file, which has suffix _asn (e.g., o3tt01010_ asn.fits ). ... The association table above tells the user that the product, or data set, will have the rootname o3tt01010, that there will be two science exposures contained in the o3tt01010_raw.fits file which are CRSPLITS, and that a o3tt01010_wav.fits file should exist containing the contemporaneously obtained automatic wavecal. ...

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• B.2 Suffixes of Files Common to all Instruments
• Introduction to HST Data Handbook v8.0
• HSP Data Handbook

... PostScript . ... Calculates sky coordinates on an event-by-event basis . ... Plots 3-band colour EPIC or OM images using PGPLOT . ... Computes and plots power density spectra of EPIC source time series . ... Perl script for the EPIC MOS pipeline . ... Defines final list of events, their position and time for EPIC-MOS . ... Adds corrected source positions to the EPIC source list by cross-correlating with optical source catalogues . ... Correct RGS event positions for spacecraft pointing . ...

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• How to extract MOS background spectra from blank fields event lists

Next: Imaging Polarimetry with NICMOS Up: NICMOS Data Calibration and Previous: The Photometric Performance of . ... NICMOSlook and Calnic C . ... Extracting spectra from a large number of NICMOS grism images requires a convenient interactive tool which allows a user to manipulate direct/grism image pairs. ... NICMOSlook and Calnic-C are two programs that were designed to take advantage of the fact that the NICMOS grism mode typically consists of taking both a direct and a grism image. ...

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• The STScI NICMOS Calibration Pipeline
• NICMOS Data Calibration and Analysis
• SLITLESS (Oct97) --- ST_ECF --- SLITLESS (Oct97)

Next: Comments on Individual Sources Up: Sample Identification Previous: Sample Identification . In Figure 2, we show the spectra of the optical counterparts to 85 of 97 observed X-ray/radio sources. ... Positional information for all 85 sources for which we announce identifications herein are given in Table 3, including information from WGACAT, the PMN and Green Bank surveys, the NVSS and our ATCA survey. ... Of the 85 newly identified sources, 59 are FSRQs, and 22 are BL Lacs. ...

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• Sample Identification

... The J, H and K bands are characterized by a bright background, such a background is mainly due to the emission of atmospheric lines and of thermal radiation. ... If the source cover a large fraction of the slit, spectra off-source must be observed to adequately sample the sky background. ... The on chip integration time (time spent in each position of the slit) must not exceed 40 seconds in J and H bands and 60 seconds in K band. ... We suggest a sequence of 10 for each elementary integration time. ...

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• CHIANTI atomic database

The FITS archive & data processing pipelines . ... The archived data are broad band images (BBI) and long-slit spectra (LSS) plus their associated template and calibration files. The data in HFA can enter into the HyperLeda processing pipeline and the results can be freely downloaded. ... Definition of the file system (structure of the archive) . ... The coordinate systems must be updated when the data (pixel data, other keywords, related tables) are altered (eg. rebinning of the image). ...

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• Radio spectra of quasars.
• Culgoora catalog
• The SNR X-rays Catalog

... IDL procedure to display ; a) a region of spectrum , together with a fit , if supplied, ; b) positions and relative strengths (gf or W_lambda) of lines in ; common atomic spectra may be marked in the lower panel. ; c) lines of sleceted atoms are identified in the top panel ; ; Command arguments: ; specfile - character string - name of file containing spectrum (and fit ) ; assumed to be x,y file with 3- ... Assesses lines in linelist by the strength values "listfr". ...

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• BASIC PROPERTIES
• Observations and Data Reduction
• Armagh Observatory

... The distinguishing characteristic of VIMOS is its very high multiplex capability: in MOS mode up to 800 spectra can be acquired simultaneously, while the Integral Field Unit produces 6400 spectra to obtain integral field spectroscopy of an area approximately 1 1 arcmin in size. ... Figure 1: A block diagram scheme of the DRS spectral extraction process . ... The extraction itself is carried out following two different procedures for MOS and IFU observations. ...

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• Pipeline Processing and Quality Control for Echelle Data
• ADASS 2003 Conference Proceedings
• NICMOS Calibration Pipeline: Processing Associations of Exposures

... Einstein data for SNR are available as images on magnetic tape or diskette and as tables of counting rates. ... In seven cases, with coverage from 35% to 90%, we have calculated an HRI rate for the entire SNR by using the observed IPC data and assuming the ratio of HRI to IPC rates was the same for the observed and the unobserved parts of the remnant. ... Positions of the bright bulge sources and remnants in the galactic plane are known and the rates in table 2 are free of the effects of these. ...

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• Chandra Supernova Remnants Catalog - Format of the Catalog
• Spectroscopic Data
• ChASeM33 Source Catalog

... The requirements contained in the current National Electrical Code and NFPA Standard for Electrical Requirements for Employee Workplaces apply to all electrical equipment, installations, and usage's at APO. ... do not use defective electrical equipment. ... the Site Safety Officer is to be notified of overloaded circuits in order to replace fuses and reset circuit breakers. ... the only multiple outlet adapter, other than extension cords, allowed are those have internal circuit breakers. ...

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This section of AMPLE provides a means for identification of minor planets. ... Due to special organization of the package, AMPLE permits the identification to be reliable fulfilled THROUGHOUT the TITLE YEAR. ... In such cases the result of identification depends on where the nearest opposition of inspected planet is situated, within basic interval lasted from November of preceding year to February of subsequent one or without it. ...

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• Head Litter of Minor Planet Names

... A1904 Date Received: 2004-Jan-27 09:55:22 Technical Page Proposal Type: General Category: Sub-Category: Observation Category: Total Time Requested: Prop osal Title: ABSTRACT: Regular Astronomy Spectroscopy Extragalactic 40 Hours HI Observations of Dwarf Galaxy Candidates in the Leo I Group Region The Leo I group is a nearby density enhancement characterized by a low velo city disp ersion but containing a lo cal density enhancement that supp orts the presence of bright E/SO galaxies. ...

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• AO Spectral Line Position Search Database.
• OLD ANALYZ instruction sequences HI in galaxies
• The Arecibo User Manual for Astronomers

... Galaxies 99 Cosmic background with model of cloudy interstellar medium Yu. ... Figure 1: Averaged spectrum of the cosmic background I f in frequency range 0.25 200 MHz for the Galactic poles. ... First interpretation of the cosmic noise background spectrum at broad band frequency range 0.25 200 MHz with a model of the cloudy interstellar medium ISM is presented here. ... Synthesized background spectra I f for regions of the Galactic poles at the frequency range 0.25 200 MHz is presented in Fig. ...

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• General description of the database
• Description of database
• Pulkovo NEO Page: Observations

... LABORATORY OF RADIO ASTRONOMICAL OBSERVATIONS . Radio sources identification is one of the most important tasks of the current radio astrophysics. ... Optical idetification. ... Optical identifications of subsample of steep spectra radio sources from RC catalog using 6m SAO telescope of SAO RAS: optical observations. ... Astronomy Reports. ... Identification of radio sources with data of various radio catalogs allows one to construct continual spectrum of the object and its radio structure. ...

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• Optical spectrum of IRAS04296
• Atlas and list of identified lines
• Absorption bands identified with DIBs

... Cheers, -Mike Data Providers (e.g., data centers, archives) Provider Name: NOAO Collection: High Resolution Atlas of Arcturus Spectra - 0.92-5.36 microns Characteristics: 310 ASCII tables of wavenumber vs flux Storage Format: Text tables Available online: ftp://ftp.noao.edu/catalogs/arcturusatlas/ir Comments: Tables contain three flux values (arcturus spectrum, telluric spectrum and ratio) for both summer and winter observations. ... Linelists also available as text table ...

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THE 75th NAME-LIST OF VARIABLE STARS. ... The 75th Name-List consists of two tables. ... the literature, taken from positional catalogues, including USNO A1.0/A2.0 and GSC, or determined by the authors); the range of variability (sometimes the column Min gives, in parentheses, the amplitude of light variation; the symbol ( means that the star , in minimum light, becomes fainter, than the magnitude indicated); and the system of magnitudes used ( P are photographic ...

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• The Catalogue of Interacting Galaxies by Vorontsov-Velyaminov

Next: Reducing 3-mm ATCA observations Up: Reducing 12-mm ATCA observations Previous: Loading data into Miriad: . For 12-mm data, calibration is essentially identical to the centimetre bands. Primary flux calibration can be done using gpboot and observations of 1934-638, in much the same fashion as at the lower frequencies. 1934-638 is about 1 Jy at 12-mm wavelengths: the Miriad calibration software contains a built-in model of 1934-638's change of flux density with frequency. ...

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• Observations and Data Reduction
• casacore: casa/Containers/RecordFieldId.h Source File
• High Energy Observations

... Radio observations of the Marano Field , carried out with the Australian Telescope Compact Array at 20 and 13 cm, are presented. ... Excellent optical and X-ray data relative to this field are available. We plan to obtain a deep X-ray, optical and radio survey in order to study the nature of the sub-mJy population (a population of radio sources at very low radio fluxes) and the energy distribution and evolutionary properties of faint radio galaxies and AGNs. ... The radio data . ... 1992) ). ...

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• Dave Green: G1.9+0.3 (not Nibiru)
• A 215 to 265 GHz spectral line survey of the Sgr B2 molecular cloud
• Measurements of anisotropies in the Cosmic Microwave Background Radiation on

. This image from orbit covers an area about 1,500 feet (460 meters) across, in which carbonate minerals have been identified from spectrometer observations. Fractures and possible layers are visible in the light-toned rock exposure containing the carbonates. NASA/JPL-Caltech/Univ. of Arizona

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• First "bone" of the Milky Way identified | Astronomy.com
• The Milky Way contains at least 100 billion planets according to survey |
• Most massive binary star identified | Astronomy.com

... About half an hour after the BAT trigger, the first images were obtained with the SAO RAS Zeiss-1000 telescope in four BVRI filters (see Fig.1). ... The spectrum of the optical transient was obtained with the SAO RAS 6-m BTA telescope 1.54 hours after the burst, using the SCORPIO instrument in the spectroscopic mode (Fig.2). ... The spectrum of the optical transient GRB090726 with identified lines, obtained with the BTA 1.54 hours after the burst. ...

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