Latest Images

Normalized SED shapes of dust-obscured and unob...

Normalized SED shapes of dust-obscured and unobscured AGNs. Panels (a) and (b) show the ...

Dohyeong Kim et al, The Astrophysical Journal Supplement Series 284 1

Best-fit SED results and corresponding photomet...

Best-fit SED results and corresponding photometric data for four randomly selected type ...

Dohyeong Kim et al, The Astrophysical Journal Supplement Series 284 1

Dust-obscured AGN fraction as a function of red...

Dust-obscured AGN fraction as a function of redshift in four bolometric luminosity subsa...

Dohyeong Kim et al, The Astrophysical Journal Supplement Series 284 1

Examples of spectral fitting results for the C ...

Examples of spectral fitting results for the C IV, Mg II, Hβ, and Hα line complexes. In ...

Dohyeong Kim et al, The Astrophysical Journal Supplement Series 284 1

Redshift vs. W1-band magnitude. Filled red circ...

Redshift vs. W1-band magnitude. Filled red circles and filled blue triangles represent t...

Dohyeong Kim et al, The Astrophysical Journal Supplement Series 284 1

Distribution of BH masses and bolometric lumino...

Distribution of BH masses and bolometric luminosities. Circles represent the representat...

Dohyeong Kim et al, The Astrophysical Journal Supplement Series 284 1

Distributions of bolometric luminosity vs. reds...

Distributions of bolometric luminosity vs. redshift for dust-obscured and unobscured AGN...

Dohyeong Kim et al, The Astrophysical Journal Supplement Series 284 1

Distribution of E(B − V) values derived from SE...

Distribution of E(B − V) values derived from SED fitting. The blue and red histograms re...

Dohyeong Kim et al, The Astrophysical Journal Supplement Series 284 1

Comparison of bolometric luminosities from UV c...

Comparison of bolometric luminosities from UV continuum luminosities and those from LMIR...

Dohyeong Kim et al, The Astrophysical Journal Supplement Series 284 1

...

﹩\mathrm{log}\left({\lambda }_{{\rm{Edd}}}\right)﹩ values vs. redshifts. Filled blue tr...

Dohyeong Kim et al, The Astrophysical Journal Supplement Series 284 1

S-band total intensity images of NGC 4565. (a) ...

S-band total intensity images of NGC 4565. (a) Contours from the robust zero weighting i...

Jianghui Xu et al, The Astrophysical Journal 1001 2

Polarization properties of NGC 4565 derived fro...

Polarization properties of NGC 4565 derived from RM synthesis. Left panel: map of the po...

Jianghui Xu et al, The Astrophysical Journal 1001 2

RM distribution along the major axis of NGC 456...

RM distribution along the major axis of NGC 4565. (a) The RM map overlaid with S-band to...

Jianghui Xu et al, The Astrophysical Journal 1001 2

Distribution of magnetic field orientations in ...

Distribution of magnetic field orientations in four galactic quadrants. (Top) Map of the...

Jianghui Xu et al, The Astrophysical Journal 1001 2

Vertical profiles of the nonthermal radio conti...

Vertical profiles of the nonthermal radio continuum emission at the S-band. The top-cent...

Jianghui Xu et al, The Astrophysical Journal 1001 2

Distribution of the nonthermal spectral index d...

Distribution of the nonthermal spectral index derived by fitting a single power law to t...

Jianghui Xu et al, The Astrophysical Journal 1001 2

Magnetic field strength map of NGC 4565, comput...

Magnetic field strength map of NGC 4565, computed assuming energy equipartition. The bea...

Jianghui Xu et al, The Astrophysical Journal 1001 2

Best-fit advection (left panels) and diffusion ...

Best-fit advection (left panels) and diffusion (right panels) models in the northern par...

Jianghui Xu et al, The Astrophysical Journal 1001 2

Velocity profiles derived from the advection mo...

Velocity profiles derived from the advection model. The top and bottom panels display th...

Jianghui Xu et al, The Astrophysical Journal 1001 2

Comparison of magnetic field orientations with ...

Comparison of magnetic field orientations with multiphase gas structures in NGC 4565. Th...

Jianghui Xu et al, The Astrophysical Journal 1001 2

Scaled harmonic IR spectra of HMT+ calculated a...

Scaled harmonic IR spectra of HMT+ calculated at the UCAM-B3LYP/aug-cc-pVTZ level for bo...

Parker Crandall et al, The Astrophysical Journal 1001 2

PES spectrum of HMT (P. Crandall et al. 2024b) ...

PES spectrum of HMT (P. Crandall et al. 2024b) as a function of binding energy (top axis...

Parker Crandall et al, The Astrophysical Journal 1001 2

(a) Equilibrium C–N bond lengths (in angstroms)...

(a) Equilibrium C–N bond lengths (in angstroms) of HMT+ in the calculated stable conform...

Parker Crandall et al, The Astrophysical Journal 1001 2

(a) Total EPD spectrum of HMT+ between 29,850 a...

(a) Total EPD spectrum of HMT+ between 29,850 and 32,790 cm–1 (305–335 nm). (b) EPD spec...

Parker Crandall et al, The Astrophysical Journal 1001 2

EPD mass spectrum of HMT+ (m/z 140) observed at...

EPD mass spectrum of HMT+ (m/z 140) observed at λ = 310 nm (32,258 cm–1), revealing the ...

Parker Crandall et al, The Astrophysical Journal 1001 2

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