Lower limit of the bandpass (in BandPass_Unit units)Ĭharacteristic quantity for the bandpass of the image Upper limit of the bandpass (in BandPass_Unit units) Moreįields may be available for selection these would be given below The following fields are contained in the output by default. VERB=1 only returns the most important columns, VERB=2 selects the columns deemed useful to the average user, VERB=3 returns a table with all available columns. ICRS Position, RA,DEC decimal degrees (e.g., 234.234,-32.46)Įxhaustiveness of column selection. Size in decimal degrees (e.g., 0.2 or 1,0.1) Relation of image and specified Region of Interest.
(with some renderers, some of these fields may be unavailable): Name The following fields are available to provide input to the service Resource, see Information on resource 'Sasmirala: Subarcsecond mid-infrared atlas of local AGN' OverviewĪ standard SIAP interface as defined by the IVOA to access collections of celestial images SIAP clients use to access the serviceĪn interface for web browsers through an HTML form The N- and Q-band imaging atlas,įor a list of all services and tables belonging to this service's ( 1, 2) Asmus D., Hoenig S.F., Gandhi P., Smette A.,ĭuschl W.: The subarcsecond mid-infrared view of local active Of the observatory-delivered pipelines with default parameters. Note, however, that these are just the products The used total images areĪvailable upon request. In the final combined image, provided here. Process of combining individual subimages (all in MIRphot), instead of Results table, because many flux measurements were performed during the Not necessarily exactly equal to the values provided in the photometry In particular for the instruments, VISIR and COMICS, they are Values given in the FITS headers should be regarded as approximate Other flux measurement methods are applied to the images. Therefore, correction factors have to be applied in case Using the median conversion factor for the used instrument/filter The FITS images are flux calibrated (unit is mJy) using the Gaussian 2Dįits to the corresponding STD observation (where available, otherwise In addition, the imprecision of the assignment itself is ~1px ~
The uncertainty of these reference position is usually less than 1Īrcsec.
CONVERT IMAGE FORMAT ATLAS REGISTRATION
The WCS registration has been performed after extraction by usingĬoordinates of the nucleus from other wavelengths (mostly 2MASS and The (putative) nuclear position with North being up and East to the The FITS images contain the central ~4 arcsec of each source centered on
by extraction (and combination) of the sub-images from theĬhopped/nodded total images from COMICS, Michelle, T-ReCS and VISIR (see These FITS images were generated with the IDL package MIRphot
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