RESOLVING THE INNER JET STRUCTURE OF 1924-292 WITH THE EVENT HORIZON TELESCOPE by Fish, Vincent L., Weintroub, Jonathan, Bower, Geoffrey C., Freund, Robert, Friberg, Per, Ho, Paul T. P., Honma, Mareki, Inoue, Makoto, Krichbaum, Thomas P., Marrone, Daniel P., Moran, James M., Oyama, Tomoaki, Plambeck, Richard, Primiani, Rurik, Shen, Zhi-Qiang, Tilanus, Remo P. J., Wright, Melvyn, Young, Ken H., Ziurys, Lucy M., Zensus, J. Anton, Lu, Rusen, Doeleman, Sheperd Samuel

“…We present the first 1.3 mm (230 GHz) very long baseline interferometry model image of an active galactic nucleus (AGN) jet using closure phase techniques with a four-element array. …”
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EXTENDED, DUSTY STAR FORMATION FUELED BY A RESIDUAL COOLING FLOW IN THE CLUSTER OF GALAXIES SERSIC 159-03 by Werner, N., Oonk, J. B. R., Veilleux, S., McDonald, Michael A.

“…While the cooling of the hot intracluster medium (ICM) in the cores of galaxy clusters is mostly counteracted by heating from the central active galactic nucleus (AGN), the balance is not perfect. …”
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FAR-INFRARED FINE-STRUCTURE LINE DIAGNOSTICS OF ULTRALUMINOUS INFRARED GALAXIES by Farrah, D, Lebouteiller, V, Spoon, H, Bernard-Salas, J, Pearson, C, Rigopoulou, D, Smith, H, Gonzalez-Alfonso, E, Clements, D, Efstathiou, A, Cormier, D, Afonso, J, Petty, S, Harris, K, Hurley, P, Borys, C, Verma, A, Cooray, A, Salvatelli, V

“…We do not find relationships between far-IR line properties and several other parameters: active galactic nucleus (AGN) activity, merger stage, mid-IR excitation, and SMBH mass. …”

THE WFC3 INFRARED SPECTROSCOPIC PARALLEL (WISP) SURVEY by Atek, H, Malkan, M, McCarthy, P, Teplitz, H, Scarlata, C, Siana, B, Henry, A, Colbert, J, Ross, N, Bridge, C, Bunker, A, Dressler, A, Fosbury, R, Martin, C, Shim, H

“…These first fields show high equivalent width sources, active galactic nucleus, and post-starburst galaxies. The median observed star formation rate (SFR) of our Hα-selected sample is 4 M⊙ yr-1. …”

The e-MERGE Survey (e-MERLIN Galaxy Evolution Survey): overview and survey description by Muxlow, TWB, Thomson, AP, Radcliffe, JF, Wrigley, NH, Beswick, RJ, Smail, I, McHardy, IM, Garrington, ST, Ivison, RJ, Jarvis, MJ, Prandoni, I, Bondi, M, Guidetti, D, Argo, MK, Bacon, D, Best, PN, Biggs, AD, Chapman, SC, Coppin, K, Chen, H, Garratt, TK, Garrett, MA, Ibar, E, Kneib, J-P, Knudsen, KK, Koopmans, LVE, Morabito, LK, Murphy, EJ, Njeri, A, Pearson, C, Perez-Torres, MA, Richards, AMS, Rottgering, HJA, Sargent, MT, Serjeant, S, Simpson, C, Simpson, JM, Swinbank, AM, Varenius, E, Venturi, T

“…We combine the long baselines of e-MERLIN (providing high angular resolution) with the relatively closely packed antennas of the VLA (providing excellent surface brightness sensitivity) to produce a deep 1.5-GHz radio survey with the sensitivity (⁠∼1.5μ Jy beam−1), angular resolution (0.2–0.7 arcsec) and field-of-view (∼15 × 15 arcmin2) to detect and spatially resolve star-forming galaxies and active galactic nucleus (AGN) at z ≳ 1. The goal of e-MERGE is to provide new constraints on the deep, sub-arcsecond radio sky which will be surveyed by SKA1-mid. …”

A far-infrared spectroscopic survey of intermediate redshift (ultra) luminous infrared galaxies by Magdis, G, Rigopoulou, D, Hopwood, R, Huang, J, Farrah, D, Pearson, C, Alonso-Herrero, A, Bock, J, Clements, D, Cooray, A, Griffin, M, Oliver, S, Perez Fournon, I, Riechers, D, Swinyard, B, Scott, D, Thatte, N, Valtchanov, I, Vaccari, M

“…Using our sample to bridge local and high-z [C II] observations, we find that the majority of galaxies at all redshifts and all luminosities follow an L C II –L FIR relation with a slope of unity, from which local ULIRGs and high- z active-galactic-nucleus-dominated sources are clear outliers. …”

VERY STRONG EMISSION-LINE GALAXIES IN THE WFC3 INFRARED SPECTROSCOPIC PARALLEL SURVEY AND IMPLICATIONS FOR HIGH-REDSHIFT GALAXIES by Atek, H, Siana, B, Scarlata, C, Malkan, M, McCarthy, P, Teplitz, H, Henry, A, Colbert, J, Bridge, C, Bunker, A, Dressler, A, Fosbury, R, Hathi, N, Martin, C, Ross, N, Shim, H

“…After estimating the active galactic nucleus fraction in the sample, we show that the high-EW galaxies have higher sSFR than normal star-forming galaxies at any redshift. …”

The 2dF galaxy redshift survey: clustering properties of radio galaxies by Magliocchetti, M, Maddox, S, Hawkins, E, Peacock, J, Bland-Hawthorn, J, Bridges, T, Cannon, R, Cole, S, Colless, M, Collins, C, Couch, W, Dalton, G, de Propris, R, Driver, S, Efstathiou, G, Ellis, R, Frenk, C, Glazebrook, K, Jackson, C, Jones, B, Lahav, O, Lewis, I, Lumsden, S, Norberg, P, Peterson, B

“…Different results are instead obtained if we only consider sources that present signatures of active galactic nucleus (AGN) activity in their spectra. These objects are shown to be very strongly correlated, with r 0 = 10.9 -1.2+10 Mpc and γ = 2 ± 0.1, a steeper slope than has been claimed in other recent works. …”

Observations of the Hubble deep field south with the Infrared space observatory - II. Associations and star formation rates by Mann, R, Oliver, S, Carballo, R, Franceschini, A, Rowan-Robinson, M, Heavens, A, Kontizas, M, Elbaz, D, Dapergolas, A, Kontizas, E, Granato, G, Silva, L, Rigopoulou, D, Gonzalez-Serrano, J, Verma, A, Serjeant, S, Efstathiou, A, van der Werf, P

“…(Paper I): eight of them are identified as stars, one is definitely an active galactic nucleus (AGN), a second seems likely to be an AGN too, while the remaining 22 appear to be normal spiral or starburst galaxies. …”

Quiescent Low-mass Galaxies Observed by JWST in the Epoch of Reionization by Viola Gelli, Stefania Salvadori, Andrea Ferrara, Andrea Pallottini, Stefano Carniani

“…As supernova feedback can only act on a longer timescale (≳30 Myr), this implies that the observed abrupt quenching must be caused by a faster physical mechanism, such as radiation-driven winds from young massive stars and/or an active galactic nucleus.…”
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The Star Formation Across Cosmic Time (SFACT) Survey. I. Survey Description and Early Results from a New Narrowband Emission-line Galaxy Survey by John J. Salzer, David J. Carr, Jennifer Sieben, Samantha W. Brunker, Alec S. Hirschauer

“…One of the key attributes of the SFACT survey is that the ELGs are detected in discrete redshift windows that will allow us to robustly quantify the properties of the star-forming and active galactic nucleus populations as a function of redshift to z = 1 and beyond. …”
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Ejecta–Circumstellar Medium Interaction in High-density Environment Contribution to Kilonova Emission: Application to GRB 191019A by Suo-Ning Wang, Hou-Jun Lü, Yong Yuan, Hao-Yu Yuan, Jared Rice, Meng-Hua Chen, En-Wei Liang

“…The nearby long-duration GRB 191019A recently detected by Swift lacks an associated supernova and belongs to a host galaxy with little star formation activity, suggesting that the origin of this burst is the result of a merger of two compact objects with dynamical interactions in a high-density medium of an active galactic nucleus. Given the potential motivation of this event, and given that it occurs in such a high-density environment, the ejecta–circumstellar medium (CSM) interaction cannot be ignored as possibly contributing to the kilonova emission. …”
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Discovery of A Large-scale Bent Radio Jet in the Merging Cluster A514 by Wonki Lee, John ZuHone, M. James Jee, Kim HyeongHan, Ruta Kale, Eunmo Ahn

“…The radio emission originates from the two radio lobes of the active galactic nucleus (AGN) located near the center of the southern subcluster and extends toward the southern outskirts with multiple bends. …”
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The Origins of Gas Accreted by Supermassive Black Holes: The Importance of Recycled Gas by Ena Choi, Rachel S. Somerville, Jeremiah P. Ostriker, Michaela Hirschmann, Thorsten Naab

“…Considering the presence of various other gas triggers for active galactic nucleus (AGN) activity alongside this time delay, the association between AGNs and mergers may not always be obvious.…”
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Deep Chandra Observation of the Remarkable Ionization Cones of NGC 5252 by Chen Wang, Junfeng Wang, Mauro Dadina, Giuseppina Fabbiano, Martin Elvis, Stefano Bianchi, Matteo Guainazzi

“…Seyfert galaxy NGC 5252 harbors enormously extended ionization cones that have been previously detected in the optical and X-ray band, offering a unique opportunity to investigate the interaction between the central active galactic nucleus (AGN) and the surrounding gas in the AGN host galaxy. …”
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Host Galaxy and Nuclear Properties of IR-selected AGNs with and without Outflow Signatures by Gabriel A. Oio, Y. Sophia Dai, C. G. Bornancini, Zi-Jian Li

“…Active galactic nucleus (AGN) driven outflows can have a significant impact on the evolution of the host galaxy. …”
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A Search for Kilonova Radio Flares in a Sample of Swift/BAT Short Gamma-Ray Bursts by Avery Eddins, Kyung-Hwan Lee, Alessandra Corsi, Imre Bartos, Zsuzsanna Márka, Szabolcs Márka

“…We found one radio candidate counterpart for one of the GRBs in our sample, GRB 111126A, though an origin related to emission from star formation or from an active galactic nucleus in its host galaxy cannot be excluded without further observations.…”
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A New Galaxy Cluster Merger Capable of Probing Dark Matter: A56 by David Wittman, Rodrigo Stancioli, Kyle Finner, Faik Bouhrik, Reinout van Weeren, Andrea Botteon

“…We also present deep GMRT 650 MHz data revealing extended emission, 420 kpc long, which may be an active galactic nucleus (AGN) tail but is potentially also a candidate radio relic. …”
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Chandra and JVLA Observations of HST Frontier Fields Cluster MACS J0717.5+3745 by van Weeren, R. J., Ogrean, G. A., Jones, C., Forman, W. R., Andrade-Santos, F., Pearce, Connor J. J., Bonafede, A., Brüggen, M., Clarke, T. E., Churazov, E., David, L., Dawson, W. A., Donahue, M., Goulding, A., Kraft, R. P., Mason, B., Merten, J., Mroczkowski, T., Nulsen, P. E. J., Rosati, P., Roediger, E., Randall, S. W., Sayers, J., Umetsu, K., Vikhlinin, A., Zitrin, A., Bulbul, Gul E

“…The steep spectrum tails of this active galactic nucleus lead into the large radio relic where the radio spectrum flattens again. …”
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Spatially Resolved Patchy Lyα Emission Within the Central Kiloparsec of a Strongly Lensed Quasar Host Galaxy at z = 2.8 by Sharon, Keren, Acharyya, Ayan, Gladders, Michael D., Rigby, Jane R., Bian, Fuyan, Runnoe, Jessie, Dahle, Hakon, Kewley, Lisa, Florian, Michael, Johnson, Traci, Paterno-Mahler, Rachel, Bayliss, Matthew B, Bordoloi, Rongmon

“…Spectroscopic follow-up clearly reveals extended Lyα in emission between two images of the central active galactic nucleus (AGN). We reconstruct the lensed quasar host galaxy in the source plane by applying a strong lens model to HST imaging and resolve spatial scales as small as ∼200 pc. …”
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