J/A+A/623/A82 HST/COS and FUSE UV spectra of Mrk 509 (Kriss+, 2019)
Multiwavelength campaign on Mrk 509.
XVI. Continued HST/COS monitoring of the far-ultraviolet spectrum.
Kriss G.A., Arav N., Edmonds D., Ely J., Kaastra J.S., Bianchi S.,
Cappi M., Costantini E., Ebrero J., Mehdipour M., Paltani S., Petrucci P.,
Ponti G.
<Astron. Astrophys. 623, A82 (2019)>
=2019A&A...623A..82K 2019A&A...623A..82K (SIMBAD/NED BibCode)
ADC_Keywords: Galaxies, Markarian ; Galaxies, Seyfert ; Galaxies, spectra ;
Spectra, ultraviolet
Keywords: galaxies: Seyfert - galaxies: nuclei -
quasars: absorption lines - galaxies: individual: Mrk 509 -
ultraviolet: galaxies - X-rays: galaxies
Abstract:
To elucidate the location, physical conditions, mass outflow rate, and
kinetic luminosity of the outflow from the active nucleus of the
Seyfert 1 galaxy Mrk 509 we used coordinated ultraviolet and X-ray
spectral observations in 2012 to followup our lengthier campaign
conducted in 2009. We observed Mrk 509 with the Cosmic Origins
Spectrograph (COS) on the Hubble Space Telescope (HST) on 2012-09-03
and 2012-10-11 coordinated with X-ray observations using the High
Energy Transmission Grating on the Chandra X-ray Observatory. Our
far-ultraviolet spectra used grating G140L on COS to cover wavelengths
from 920-2000Å at a resolving power of 2000, and gratings G130M and
G160M to cover 1160-1750Å at a resolving power of 15000. We detect
variability in the blue-shifted UV absorption lines on timescales
spanning 3-12 years. The inferred densities in the absorbing gas are
greater than logn[cm-3]∼3. For ionization parameters ranging over
logU=-1.5 to -0.2, we constrain the distances of the absorbers to
be closer than 220pc to the active nucleus. The impact on the host
galaxy appears to be confined to the nuclear region.
Description:
Ultraviolet spectra obtained with the Cosmic Origins Spectrograph
(COS) on the Hubble Space Telescope (HST) in 2009 and 2012, and with
the Far Ultraviolet Spectroscopic Explorer (FUSE) in 2000 are
presented. We include both original data, deconvolved COS spectra, and
FUSE spectra convolved to the resolution of the COS 2012 observation.
Objects:
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RA (2000) DE Designation(s)
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20 44 09.75 -10 43 24.7 Mrk 509 = SWIFT J2044.3-1045
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File Summary:
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FileName Lrecl Records Explanations
--------------------------------------------------------------------------------
ReadMe 80 . This file
g130m09o.dat 36 31268 Original COS G130M spectrum from
2009 December 10 and 11
g160m09o.dat 36 29426 Original COS G160M spectrum from
2009 December 10 and 11
lya09d.dat 36 5019 Deconvolved version of the Lyα region of
the 2009 COS spectrum
n509d.dat 36 5020 Deconvolved version of the NV region of the
2009 COS spectrum
c409d.dat 36 3106 Deconvolved version of the CIV region of the
2009 COS spectrum
g130m12o.dat 36 28364 Original calibrated COS G130M spectrum from 2012,
that is the combination of the observations
obtained on 2012 September 3 and 2012 October 11
g160m12o.dat 36 28840 Original calibrated COS G160M spectrum from 2012,
that is the combination of the observations
obtained on 2012 September 3 and 2012 October 11
g140l12o.dat 36 3453 Original calibrated COS G140L spectrum from 2012,
that is the combination of the observations
obtained on 2012 September 3 and 2012 October 11
lya12d.dat 36 5018 Deconvolved version of the Lyα region of
the 2012 COS spectrum
n512d.dat 36 2008 Deconvolved version of the NV region of the
2012 COS spectrum
c412d.dat 36 1634 Deconvolved version of the CIV region of the
2012 COS spectrum
fus1999o.dat 36 5365 Original FUSE spectrum obtained in 1999 November
fus1999c.dat 36 5364 FUSE spectrum from 1999 convolved to the
resolution of the COS 2012 spectrum
fus2000o.dat 36 5365 Original calibrated FUSE spectrum obtained in
2000 September
fus2000c.dat 36 5364 FUSE spectrum from 2000 convolved to the
resolution of the COS 2012 spectrum
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See also:
J/PAZh/23/409 : Spectrophotometry of Mrk 509 (Chuvaev+, 1997)
Byte-by-byte Description of file: *.dat
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Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 10 F10.4 0.1nm lambda Observed wavelength (Angstroms)
14- 23 E10.4 cW/m2/nm Flux Observed flux (erg/cm2/s/Å)
28- 36 E9.4 cW/m2/nm e_Flux 1-sigma error in the observed flux
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Acknowledgements:
Gerard Kriss, gak(at)stsci.edu
References:
Kriss et al., 2000ApJ...538L..17K 2000ApJ...538L..17K
Kaastra et al., Paper I 2011A&A...534A..36K 2011A&A...534A..36K
Kaastra et al., Paper II 2011A&A...534A..37K 2011A&A...534A..37K
Detmers et al., Paper III 2011A&A...534A..38D 2011A&A...534A..38D
Mehdipour et al., Paper IV 2011A&A...534A..39M 2011A&A...534A..39M
Ebrero et al., Paper V 2011A&A...534A..40E 2011A&A...534A..40E
Kriss et al., Pzper VI 2011A&A...534A..41K 2011A&A...534A..41K
Steenbrugge et al., Paper VII 2011A&A...534A..42S 2011A&A...534A..42S
Kaastra et al., Paper VIII 2012A&A...539A.117K 2012A&A...539A.117K
Pinto et al,. Paper IX 2012A&A...541A.147P 2012A&A...541A.147P
Arav et al., Paper X 2012A&A...544A..33A 2012A&A...544A..33A
Ponti et al., Paper XI 2013A&A...549A..72P 2013A&A...549A..72P
Petrucci et al., Paper XII 2013A&A...549A..73P 2013A&A...549A..73P
Boissay et al., Paper XIII 2014A&A...567A..44B 2014A&A...567A..44B
Kaastra et al., Paper XIV 2014A&A...570A..73K 2014A&A...570A..73K
Costantini et al., Paper XV 2016A&A...595A.106C 2016A&A...595A.106C
(End) Patricia Vannier [CDS] 27-Feb-2019