Adding AGN states A&A publication.

Author: emoravec

_research/agn_states.md

@@ -12,7 +12,7 @@ Do active galactic nuclei (AGN) with different radio properties lie in distinct
 To address whether AGN jets might be related to accretion states as in XRBs, I explore whether populations of radio-AGN classified according to their radio jet morphology (FR I and II), excitation class (HERG and LERG), and radio jet linear extent (compact to giant) occupy different and distinct regions of the AGN hardness-intensity diagram (total luminosity vs. hardness). I find that (a) FR Is and IIs, (b) HERGs and LERGs, (c) FR I-LERGs and FR II-HERGs occupy distinct areas of the HID at a statistically significant level (p-value < 0.05) and no clear evidence for population distinction between the different radio jet linear extents. The separation between FR I-LERG and FR II-HERG populations is the strongest in this work. Our results indicate that radio-loud AGN occupy distinct areas of the HID depending on the morphology and excitation class, showing strong similarities to XRBs.
 
 ### Publication
-* Moravec, E. et al., [Do Radio Active Galactic Nuclei Reflect X-ray Binary Spectral States?](https://ui.adsabs.harvard.edu/abs/2022arXiv220211116M/abstract0), 2022, A&A, accepted.
+* Moravec, E. et al., [Do Radio Active Galactic Nuclei Reflect X-ray Binary Spectral States?](https://ui.adsabs.harvard.edu/abs/2022A%26A...662A..28M/abstract), 2022, A&A, 662, A28.
 
 ### Video Summary
 * A 10 minute video explaining what a radio galaxy is with the public being the intended audience: [Radio Galaxies](https://youtu.be/2_HBLgb_198)
@@ -56,6 +56,7 @@ In conclusion, I find evidence that AGN with specific radio properties occupy di
 
 #### Research Question Answer
 Q: Do AGN with different radio properties lie in distinct parts of the HID diagram reflecting XRB states?
+
 A: Radio-loud AGN do indeed occupy distinct areas of the HID depending on the morphology and excitation class, showing strong similarities to XRBs.
 
 ###### Banner image credit: Judith Croston and LOFAR Survey Team 

assets/files/Moravec_CV_webpage.pdf

@@ -55,7 +55,7 @@ __Graduate Student Fellow__, University of Florida, Gainesville, FL (August 2014
 </div>
 
 #### First Author
-* Moravec, E. et al., [Do Radio Active Galactic Nuclei Reflect X-ray Binary Spectral States?](https://ui.adsabs.harvard.edu/abs/2022arXiv220211116M/abstract0), 2022, A&A, accepted.
+* Moravec, E. et al., [Do Radio Active Galactic Nuclei Reflect X-ray Binary Spectral States?](https://ui.adsabs.harvard.edu/abs/2022A%26A...662A..28M/abstract), 2022, A&A, 662, A28.
 * Moravec, E. A. et al., [The Massive and Distant Clusters of WISE Survey. IX. High Radio-Activity in a Merging Cluster](https://ui.adsabs.harvard.edu/abs/2020ApJ...898..145M/abstract), 2020b, ApJ.
 * Moravec, E. A. et al., [The Massive and Distant Clusters of WISE Survey. VII. The Environments and Properties of Radio Galaxies in Clusters at z~1](https://ui.adsabs.harvard.edu/abs/2020ApJ...888...74M/abstract), 2020a, ApJ, 88, 74.
 * Moravec, E. A. et al., [The Massive and Distant Clusters of WISE Survey. V: Extended Radio Sources in Massive Galaxy Clusters at z~1](https://ui.adsabs.harvard.edu/abs/2019ApJ...871..186M/abstract), 2019, ApJ, 871, 186.
@@ -77,10 +77,11 @@ See ORCiD page ([https://orcid.org/0000-0001-9793-5416](https://orcid.org/0000-0
 __Observing Experience__
 * JVLA — Created scheduling blocks for continuum observations for 5 projects (L-band, C-band, X-band; A and B configurations), imaged over 50 datasets. 
 * GBT — 2 weeks in-situ observational training, 35+ hours of observing experience with MUSTANG2, certified remote observer.
+* SMA - Created scheduling blocks for continuum observations for 3 projects.
 
 __Interferometry:__ radio interferometric calibration and imaging, particularly self-calibration and wide-field, high-dynamic range imaging using multi-frequency-synthesis; multi-frequency datasets
 
-__Data Familiarity:__ VLA, VLA Surveys, Radio morphology catalogs, LoTSS, XMM SUSS, 4XMM-DR9, Swift UVOT SSC, Swift 2SXPS, Spitzer, PanSTARRS, DECaLS, HST COS spectra, MDM CCDS spectra, SDSS & BOSS spectra, WIYN IFU spectra (300 - 1000 nm), SNIFS IFU spectra from 2.2m telescope of University of Hawaii (400 - 1000 nm), Gemini GMOS Images
+__Data Familiarity:__ VLA, VLA Surveys, ALMA, SMA, Radio morphology catalogs, LoTSS, XMM SUSS, 4XMM-DR9, Swift UVOT SSC, Swift 2SXPS, Spitzer, PanSTARRS, DECaLS, HST COS spectra, MDM CCDS spectra, SDSS & BOSS spectra, WIYN IFU spectra (300 - 1000 nm), SNIFS IFU spectra from 2.2m telescope of University of Hawaii (400 - 1000 nm), Gemini GMOS Images
 
 __Astronomical Languages/Software:__ CASA, DS9, IRAF/PyRAF, IDL, Topcat