activity
19982023
most citedTorus and AGN properties of nearby Seyfert galaxies: Results from fitting IR spectral energy distributions and spectroscopy

236 citations · 2.9k across the 75 of their papers we have counts for

collaborators

76 papers

astro-ph.GA2023★ 26 cited

AGN feedback in action in the molecular gas ring of the Seyfert galaxy NGC7172

A. Alonso-Herrero, S. Garcia-Burillo, M. Pereira-Santaella +14

We present new ALMA observations of the CO(3-2) transition and 854micron continuum at 0.06-0.3" resolution, together with new VLT/SINFONI observations of NGC7172. This is a luminou…

astro-ph.GA2023★ 23 cited

A radio-jet driven outflow in the Seyfert 2 galaxy NGC 2110?

L. Peralta de Arriba, A. Alonso-Herrero, S. García-Burillo +16

We present a spatially-resolved study of the ionised gas in the central 2 kpc of the Seyfert 2 galaxy NGC 2110 and investigate the role of its moderate luminosity radio jet (kineti…

astro-ph.GA2023★ 1 cited

GTC/CanariCam Mid-IR Polarimetry of Magnetic Fields in Star-Forming Region W51 IRS2

Charles M. Telesco, Han Zhang, Frank Varosi +4

We present 0.4 arcsec-resolution imaging polarimetry at 8.7, 10.3, and 12.5 microns, obtained with CanariCam at the Gran Telescopio Canarias, of the central region of W51 IRS2. The…

astro-ph.GA2022★ 5 cited

Mid-Infrared Polarization of the Diffuse Interstellar Medium toward CygOB2-12

Charles M. Telesco, Frank Varosi, Christopher Wright +3

We present the first mid-IR detection of the linear polarization toward the star CygOB2-12, a luminous blue hypergiant that, with Av of ~10 mag of foreground extinction, is a bench…

astro-ph.IM2022★ 1 cited

Technology to scale up diversity in astronomy education

Carmen Fies, Chris Packham

The San Antonio Teacher Training Astronomy Academy (SATTAA) completed its fourth annual iteration in June 2021 . While the program began as a face-to-face professional development…

astro-ph.IM2021

CanariCam Mid-Infrared Drift Scanning: Improved Sensitivity and Spatial Resolution

Amílcar R. Torres-Quijano, Christopher Packham, Sergio Fernandez Acosta

Ground-based mid-infrared (MIR) astronomical observations require the removal of the fast time variable components of (a) sky/background variation and (b) array background. Typical…