Article, 2024
A quasar-galaxy merger at z ∼ 6.2: Black hole mass and quasar properties from the NIRSpec spectrum
Astronomy & Astrophysics,
ISSN
0004-6361,
1432-0746,
Volume 685,
Page a121,
10.1051/0004-6361/202348535
Contributors
Loiacono, Federica
0000-0002-8858-6784
(Corresponding author)
[1]
Decarli, Roberto
0000-0002-2662-8803
[1]
Mignoli, Marco
0000-0002-9087-2835
[1]
Farina, Emanuele Paolo
0000-0002-6822-2254
[2]
Bañados, Eduardo
0000-0002-2931-7824
[3]
Bosman, Sarah E I
0000-0001-8582-7012
[3]
[4]
Eilers, Anna-Christina
[5]
Schindler, Jan-Torge
0000-0002-4544-8242
[6]
Strauss, Michael A
[7]
Vestergaard, Marianne
0000-0001-9191-9837
[8]
[9]
Wang, Feige
0000-0002-7633-431X
[9]
Blecha, Laura E
0000-0002-2183-1087
[10]
Carilli, Chris L
[11]
Comastri, Andrea
0000-0003-3451-9970
[1]
Connor, Thomas
0000-0002-7898-7664
[12]
[13]
Costa, Tiago
[14]
Dotti, Massimo
0000-0002-1683-5198
[15]
[16]
[17]
Fan, Xiao-Hui
0000-0003-3310-0131
[9]
Gilli, Roberto
0000-0001-8121-6177
[1]
Jun, Hyunsung David
0000-0003-1470-5901
[18]
Liu, Weizhe
[9]
Lupi, Alessandro
0000-0001-6106-7821
[17]
Marshall, Madeline A
0000-0001-6434-7845
[19]
[20]
Mazzucchelli, Chiara
0000-0002-5941-5214
[21]
Meyer, Romain A
0000-0001-5492-4522
[22]
Neeleman, Marcel
0000-0002-9838-8191
[11]
Overzier, Roderik Adriaan
0000-0002-8214-7617
[23]
Pensabene, Antonio
0000-0001-9815-4953
[17]
Riechers, Dominik A
[24]
Trakhtenbrot, Benny
0000-0002-3683-7297
[25]
Trebitsch, Maxime
0000-0002-6849-5375
[26]
Venemans, Bram P
0000-0001-9024-8322
[23]
Walter, Fabian
0000-0003-4793-7880
[3]
Yang, Jinyi
[9]
Affiliations
- [1]
Osservatorio astronomico di Bologna
[NORA names:
Italy; Europe, EU; OECD];
- [2]
Gemini North Observatory
[NORA names:
United States; America, North; OECD];
- [3]
Max Planck Institute for Astronomy
[NORA names:
Germany; Europe, EU; OECD];
- [4]
Heidelberg University
[NORA names:
Germany; Europe, EU; OECD];
- [5]
Massachusetts Institute of Technology
[NORA names:
United States; America, North; OECD];
(... more)
- [6]
Universität Hamburg
[NORA names:
Germany; Europe, EU; OECD];
- [7]
Princeton University
[NORA names:
United States; America, North; OECD];
- [8]
University of Copenhagen
[NORA names:
KU University of Copenhagen;
University; Denmark; Europe, EU; Nordic; OECD];
- [9]
University of Arizona
[NORA names:
United States; America, North; OECD];
- [10]
University of Florida
[NORA names:
United States; America, North; OECD];
- [11]
National Radio Astronomy Observatory
[NORA names:
United States; America, North; OECD];
- [12]
California Institute of Technology
[NORA names:
United States; America, North; OECD];
- [13]
Center for Astrophysics Harvard & Smithsonian
[NORA names:
United States; America, North; OECD];
- [14]
Max Planck Institute for Astrophysics
[NORA names:
Germany; Europe, EU; OECD];
- [15]
Brera Astronomical Observatory
[NORA names:
Italy; Europe, EU; OECD];
- [16]
INFN Sezione di Milano Bicocca
[NORA names:
Italy; Europe, EU; OECD];
- [17]
University of Milano-Bicocca
[NORA names:
Italy; Europe, EU; OECD];
- [18]
Northwestern College - Iowa
[NORA names:
United States; America, North; OECD];
- [19]
ARC Centre of Excellence for All-Sky Astrophysics
[NORA names:
Australia; Oceania; OECD];
- [20]
National Research Council Canada
[NORA names:
Canada; America, North; OECD];
- [21]
Diego Portales University
[NORA names:
Chile; America, South; OECD];
- [22]
University of Geneva
[NORA names:
Switzerland; Europe, Non-EU; OECD];
- [23]
Leiden University
[NORA names:
Netherlands; Europe, EU; OECD];
- [24]
University of Cologne
[NORA names:
Germany; Europe, EU; OECD];
- [25]
Tel Aviv University
[NORA names:
Israel; Asia, Middle East; OECD];
- [26]
University of Groningen
[NORA names:
Netherlands; Europe, EU; OECD]
(less)
Abstract
We present JWST/NIRSpec integral field data of the quasar PJ308-21 at z = 6.2342. As shown by previous ALMA and HST imaging, the quasar has two companion sources, interacting with the quasar host galaxy. The high-resolution G395H/290LP NIRSpec spectrum covers the 2.87 − 5.27 μm wavelength range and shows the rest-frame optical emission of the quasar with exquisite quality (signal-to-noise ratio ∼100 − 400 per spectral element). Based on the H β line from the broad line region, we obtain an estimate of the black hole mass M BH, H β ∼ 2.7 × 10 9 M ⊙ . This value is within a factor ≲1.5 of the H α -based black hole mass from the same spectrum ( M BH, H α ∼ 1.93 × 10 9 M ⊙ ) and is consistent with a previous estimate relying on the Mg II λ 2799 line ( M BH, MgII ∼ 2.65 × 10 9 M ⊙ ). All these M BH estimates are within the ∼0.5 dex intrinsic scatter of the adopted mass calibrations. The high Eddington ratio of PJ308-21 λ Edd, H β ∼ 0.67 ( λ Edd, H α ∼ 0.96) is in line with the overall quasar population at z ≳ 6. The relative strengths of the [O III ], Fe II , and H β lines are consistent with the empirical “Eigenvector 1” correlations as observed for low redshift quasars. We find evidence for blueshifted [O III ] λ 5007 emission with a velocity offset Δ v [O III] = −1922 ± 39 km s −1 from the systemic velocity and a full width at half maximum (FWHM) FWHM ([O III ]) = 2776 −74 +75 km s −1 . This may be the signature of outflowing gas from the nuclear region, despite the true values of Δ v [O III] and FWHM ([O III ]) likely being more uncertain due to the blending with H β and Fe II lines. Our study demonstrates the unique capabilities of NIRSpec in capturing quasar spectra at cosmic dawn and studying their properties in unprecedented detail.
Keywords
ALMA,
BH,
Dex,
Eddington,
Eddington ratio,
FWHM,
Fe II,
Fe II lines,
HST,
HST images,
II lines,
NIRSPEC,
NIRSpec spectra,
black hole mass,
black hole mass M,
blends,
broad line region,
calibration,
companion,
companion source,
correlation,
cosmic dawn,
data,
dawn,
dex intrinsic scatter,
emission,
estimation,
evidence,
exquisite quality,
factors,
field data,
galaxies,
gas,
hole mass,
host galaxies,
images,
integral field data,
intrinsic scatter,
line region,
lines,
low-redshift quasars,
m-,
mass,
mass M,
mass calibration,
merger,
nuclear region,
optical emission,
outflowing gas,
population,
properties,
quality,
quasar host galaxies,
quasar population,
quasar properties,
quasar spectra,
quasars,
range,
ratio,
redshift quasars,
region,
rest-frame optical emission,
scattering,
signature,
source,
spectra,
strength,
study,
systemic velocity,
unique capabilities,
velocity,
width
Funders
Data Provider: Digital Science