2013-09-27T00:12:00
100
Sasmirala: Subarcsecond mid-infrared atlas of local AGN
Asmus, D.; Hoenig, S.F.; Gandhi, P.; Smette, A.;
Duschl, W.J.
active-galactic-nuclei
seyfert-galaxies
infrared-photometry
2014MNRAS.439.1648A
ESO VLT, Gemini North & South, Subaru, Spitzer,
IRAS
VISIR, T-ReCS, Michelle, COMICS, IRAC, IRS, MIPS,
IRAS
Infrared
If you use this atlas please cite the Asmus et al. work given under
the "source" metadata item.
This catalog provides access to data and mid-infrared images obtained at
ground-based 8-meter class telescopes with public archives
(Gemini/Michelle, Gemini/T-ReCS, Subaru/COMICS, and VLT/VISIR).
The Subarcsecond mid-infrared (MIR) atlas of local active galactic nuclei
(AGN) is a collection of all available N- and Q-band images obtained at
ground-based 8-meter class telescopes with public archives
(Gemini/Michelle, Gemini/T-ReCS, Subaru/COMICS, and VLT/VISIR). It includes
in total 895 images, of which 60% are perviously unpublished. These
correspond to 253 local AGN with a median redshift of 0.016. The atlas
contains the uniformly processed and calibrated images and nuclear
photometry obtained through Gauss and PSF fitting for all objects and
filters. This also includes measurements of the nuclear extensions. In
addition, the classifications of extended emission (if present) and derived
nuclear monochromatic 12 and 18 micron continuum fluxes are available.
Finally, flux ratios with the circumnuclear MIR emission (measured by
Spitzer) and total MIR emission of the galaxy (measured by IRAS) are
presented.
//scs#pgs-pos-index
Sasmirala Basic Object Properties
Basic object properties and nuclear 12 and 18
micron continuum fluxes/ratios.
Position ICRS "raj2000" "dej2000"
[Details][Photometry Details]
Mostly redshift-based luminosity distance, corrected for the Earth's
motion relative to the cosmic microwave background reference frame
with H_0 = 67.3, Omega_m = 0.315, and Omega_vac = 0.685, or
redshift-independent distance (App. B of 2014MNRAS.439.1648A).
Nuclear morphology at subarcsecond resolution; values used include:
======== ====================================
\- point-like,
o possibly extended
? unknown extension
circ. spherical extended
ellip. elliptical and bar-like extended
spir. spiral-like extended
comp. complex extended emission
======== ====================================
2003-12-02 2011-06-151.528e-20 2.838e-206/18,650,1701,4116,4381,4439,4447,4993,5091,5116,5202,5975-5976,6098,7552,7606,7659,7869,7959,8195,8264,8299,8492,8675,8922,9770,10265,10355,10364,10454,10465,10475,10817,10839,10856,10912,10924-10925,10927,10977,11027,11029,11457,11512,12241,12306,12335,12380,13564,13707,14744,14858,16301,16434,16655,16690,16712,17075,17183,17264,17369,17525,17727,17748,17754,17795,17814,17819,17850,18017,18242,18365,18432,18484,18524,18683,18714,18838,18895,18897,18935,19283,19373,19376,19433,19611,19619,19730,19746,19932,20000,20489,21016,21036,21450,22654,22721,22890,22912,22976,23167,23269,23323,23469,24842,25035,25083,25182,25518,25610,25790,25890,25907,26028,26091,26148,26264,26292,26303,26313,26338,26365,26393,26547,26937,27030,27191,27255,27382,27426,27512,27515,27699,27714,27719,27721,27765,27767,27773,27909,27914,27945,28075,28167,28173,28184,28221,28249,28259,28495,28535,29795,30140,31080,31158,31352,33034,33716,33930,33954,33958,34099,34104,34273,34294,34318,34343,34412,34493,34531,34534,34695,34737,34881,34913,35246,35447,35608,35623,35691,35993,36005,36158,36668,36765,36785-36786,36861,36896,37650,38268,38479,38653,38704,38853,38868,38887,38948,39182,39487,39836,40221,40410,40777,40818,41586,41982,42016,42027,43233,43242,43262,43339,43625,43634,43677,43748,43806,43877,43925,44507,44551,44650,44660,45587,45735,45779,45816,45883,46079,46399,46442,46481,46568,46615,46715,46811,46987,47047,47107,47120,47154,47169,47325,47415,49042Inserts a var for the link to the info page.makeAbsoluteURL("\\schema/q/prod/qp/"+
urllib.parse.quote(@name))import_photimport_descriptionsdata/tables/table01.dat
name: 1-23
raj2000: 25-34
dej2000: 36-45
z: 47-53
d: 55-60
cls: 62-70
u_agn: 72-76
batid: 78-80
n_ext: 82-87
lim12: 89-93
flu12: 95-101
err12: 103-108
lim18: 110-114
flu18: 116-122
err18: 124-129
dunr: 131-134
rmed: 136-139
rlar: 141-146
parseBooleanLiteral(@u_agn)parseBooleanLiteral(@lim12)parseBooleanLiteral(@lim18)makeAbsoluteURL("\rdId/phot/qp/"+urllib.parse.quote(@name))
import csv
with open(os.path.join(base.getConfig("inputsDir"),
"\schema", "data/Name_conversions.txt")) as f:
fNames4objs = dict(
(b.strip(), a.strip())
for a,b in csv.reader(f, delimiter=";"))
@pathcomp = fNames4objs[@name]
Photometric parameters for all
nuclear measurements.
method, abbrev
Gauss fitting, Gauss
PSF fitting, PSF
"\schema.atlas"@FILTER(@WAVELEN-@FHWIDTH)*1e-6(@WAVELEN+@FHWIDTH)*1e-6@WAVELEN*1e-6"m"@MJD_OBS@INSTRUME"Sasmirala %s %s"%(@OBJECT, @FILTER)
unstickEat0CatRE = re.compile(
"(NGC|PKS|Mrk|Fairall|1RXS|2MASX|3C|Ark|ESO|IC"
"|LEDA|MR|UGC|IC)0*([0-9J])")
unstickKeep0CatRE = re.compile(
"(PG|IRAS|1H)([0-9])")
removeESOG0RE = re.compile("-I?G0*")
removeMCGLeadingZeroRE = re.compile("-0+")
removeLeadingZeroesMRE = re.compile("^M0+")
radioRE = re.compile("^(Cygnus|Cen|Pictor|Fornax|Hydra|"
"Superantennae)")
miscReplacements = {
'M51A': 'M51a',
'Z041-020': 'Z 41-20',
'H0557-385': 'H 0557-385',
'IZW001': 'I Zw 1',
'IIIZW035N': 'III Zw 35N',
'3C 390-3': '3C 390.3',
'4C+73-08': '4C +73.08',
'1RXS J112716-6+190914': '1RXS J112716.6+190914',
}
@OBJECT = radioRE.sub(r"\1 ",
removeLeadingZeroesMRE.sub("M",
unstickEat0CatRE.sub(r"\1 \2",
unstickKeep0CatRE.sub(r"\1 \2", @OBJECT))))
if @OBJECT.startswith("MCG"):
@OBJECT = removeMCGLeadingZeroRE.sub("-", @OBJECT)
if @OBJECT.startswith("ESO"):
@OBJECT = removeESOG0RE.sub("-", @OBJECT)
@OBJECT = miscReplacements.get(@OBJECT, @OBJECT)
Sasmirala Photometry Details
sasmirala phot
\internallink{sasmirala/q/cone/form}
name0.2
yield "%%(%s)s BETWEEN w_obs-hwidth AND w_obs+hwidth"%(
base.getSQLKey("wl", inPars["wl"], outPars))
sasmirala cone
Sasmirala Subarcsecond mid-infrared atlas of local AGN,
Cone Search
This catalog provides access to data and mid-infrared images obtained at
ground-based 8-meter class telescopes with public archives
(Gemini/Michelle, Gemini/T-ReCS, Subaru/COMICS, and VLT/VISIR).
You can also download full collections of:
* \RSTservicelink{sasmirala/q/prod/static/collection/fits.tar.gz}{mid-infrared reduced FITS images}
* \RSTservicelink{sasmirala/q/prod/static/collection/plots.tar.gz}{associated plots}
* \RSTservicelink{sasmirala/q/prod/static/collection/tables.tar.gz}{tables}
\internallink{sasmirala/q/phot/form}
338.9425
-26.050556
0.01
name0.2
Sasmirala object pages
namedata
res/objdesc.html
return ctx.tag[T.xml(data["description"])]
if os.path.exists(service.rd.getAbsPath(
"data/IRAC_MIPS/"+data["pathcomp"]+"_INT.jpg")):
return ctx.tag
else:
return ""
if os.path.exists(service.rd.getAbsPath(
"data/mid-infrared/"+data["pathcomp"]+"_HAR.jpg")):
return ctx.tag
else:
return ""
from gavo import svcs
from gavo.web import htmltable
otd = svcs.OutputTableDef.fromTableDef(
service.rd.getById("photpar"), None)
obName = data.getPrimaryTable().rows[0]["name"]
with base.getTableConn() as conn:
t = rsc.TableForDef(otd, rows=(otd.makeRowFromTuple(t)
for t in conn.query(
"SELECT * FROM sasmirala.photpar WHERE name=%(name)s",
{"name": obName})))
return htmltable.HTMLTableFragment(t, svcs.emptyQueryMeta)
SELECT
name, pathcomp, description
FROM sasmirala.objects
NATURAL JOIN sasmirala.descriptions
%s
Sasmirala Subarcsecond mid-infrared atlas of local AGN
sasmirala atlas
These FITS images were generated with the IDL package MIRphot
[Asmus2014]_ by extraction (and combination) of the sub-images from the
chopped/nodded total images from COMICS, Michelle, T-ReCS and VISIR (see
[Asmus2014]_ for details).
The FITS images contain the central ~4 arcsec of each source centered on
the (putative) nuclear position with North being up and East to the
left. The WCS registration has been performed after extraction by using
coordinates of the nucleus from other wavelengths (mostly 2MASS and
NED). The uncertainty of these reference position is usually less than 1
arcsec. In addition, the imprecision of the assignment itself is ~1px ~
0.1".
The FITS images are flux calibrated (unit is mJy) using the Gaussian 2D
fits to the corresponding STD observation (where available, otherwise
using the median conversion factor for the used instrument/filter
settings). Therefore, correction factors have to be applied in case
other flux measurement methods are applied to the images. The flux
values given in the FITS headers should be regarded as approximate
values. In particular for the instruments, VISIR and COMICS, they are
not necessarily exactly equal to the values provided in the photometry
results table, because many flux measurements were performed during the
process of combining individual subimages (all in MIRphot), instead of
in the final combined image, provided here. The used total images are
available upon request. Note, however, that these are just the products
of the observatory-delivered pipelines with default parameters.
.. [Asmus2014] Asmus D., Hoenig S.F., Gandhi P., Smette A.,
Duschl W.: The subarcsecond mid-infrared view of local active
galactic nuclei: I. The N- and Q-band imaging atlas,
`2014MNRAS.439.1648A <http://ads.ari.uni-heidelberg.de/abs/2014MNRAS.439.1648A>`_
Pointed
213.31
-3.2075
0.1
0.1
return T.a(href=f"/sasmirala/q/prod/qp/{data}",
style="white-space:nowrap")[data]
im/siap.xml
self.assertHasStrings(' value="2MASX J03565655-4041453"',
' name="Z 41-20"')
self.assertXpath("//v:TR[1]/v:TD[8]",
{None: "Sasmirala NGC5506 NEII_2"})
cone/scs.xml
row = self.getFirstVOTableRow()
self.assertEqual(row["batid"], 147)
self.assertEqual(row["name"], "NGC 7314")
self.assertEqual("/".join(row["photpar"].split("/")[3:]),
"sasmirala/q/phot/qp/NGC%207314")
self.assertAlmostEqual(row["err12"], 11.8, places=6)
phot/qp/NGC%207314',
'