BASS XLVII: 22 GHz Radio Atlas of Swift-BAT Selected AGN

Kavli Affiliate: Claudio Ricci | First 5 Authors: Macon Magno, Krista L. Smith, O. Ivy Wong, Richard Mushotzky, Stuart Vogel | Summary: We present the third phase of the largest high-frequency, high-resolution imaging survey of 231 nearby, hard X-ray selected AGN, with a very high $98 pm 1%$ detection fraction. This survey presents VLA 22 […]


Continue.. BASS XLVII: 22 GHz Radio Atlas of Swift-BAT Selected AGN

BASS XLVII: 22 GHz Radio Atlas of Swift-BAT Selected AGN

Kavli Affiliate: Claudio Ricci | First 5 Authors: Macon Magno, Krista L. Smith, O. Ivy Wong, Richard Mushotzky, Stuart Vogel | Summary: We present the third phase of the largest high-frequency, high-resolution imaging survey of 231 nearby, hard X-ray selected AGN, with a very high $98 pm 1%$ detection fraction. This survey presents VLA 22 […]


Continue.. BASS XLVII: 22 GHz Radio Atlas of Swift-BAT Selected AGN

BASS XLVII: 22 GHz Radio Atlas of Swift-BAT Selected AGN

Kavli Affiliate: Claudio Ricci | First 5 Authors: Macon Magno, Krista L. Smith, O. Ivy Wong, Richard Mushotzky, Stuart Vogel | Summary: We present the third phase of the largest high-frequency, high-resolution imaging survey of 231 nearby, hard X-ray selected AGN, with a very high $98 pm 1%$ detection fraction. This survey presents VLA 22 […]


Continue.. BASS XLVII: 22 GHz Radio Atlas of Swift-BAT Selected AGN

First Axion-Like Particle Results from a Broadband Search for Wave-Like Dark Matter in the 44 to 52 $μ$eV Range with a Coaxial Dish Antenna

Kavli Affiliate: David W. Miller | First 5 Authors: Gabe Hoshino, Stefan Knirck, Mohamed H. Awida, Gustavo I. Cancelo, Simon Corrodi | Summary: We present the results from the first axion-like particle search conducted using a dish antenna. The experiment was conducted at room temperature and sensitive to axion-like particles in the $44-52,mumathrm{eV}$ range ($10.7 […]


Continue.. First Axion-Like Particle Results from a Broadband Search for Wave-Like Dark Matter in the 44 to 52 $μ$eV Range with a Coaxial Dish Antenna

The case for large-scale AGN feedback in galaxy formation simulations: insights from XFABLE

Kavli Affiliate: Debora Sijacki | First 5 Authors: Leah Bigwood, Martin A. Bourne, Vid Irsic, Alexandra Amon, Debora Sijacki | Summary: While cosmological simulations of galaxy formation have reached maturity, able to reproduce many fundamental galaxy and halo properties, no consensus has yet been reached on the impact of `baryonic feedback’ on the non-linear matter […]


Continue.. The case for large-scale AGN feedback in galaxy formation simulations: insights from XFABLE

BASS XLV: Quantifying AGN Selection Effects in the Chandra COSMOS-Legacy Survey with BASS

Kavli Affiliate: Claudio Ricci | First 5 Authors: Yarone M. Tokayer, Michael J. Koss, C. Megan Urry, Priyamvada Natarajan, Richard Mushotzky | Summary: Deep extragalactic X-ray surveys, such as the Chandra COSMOS-Legacy field (CCLS), are prone to be biased against active galactic nuclei (AGN) with high column densities due to their lower count rates at […]


Continue.. BASS XLV: Quantifying AGN Selection Effects in the Chandra COSMOS-Legacy Survey with BASS

BASS XLV: Quantifying AGN Selection Effects in the Chandra COSMOS-Legacy Survey with BASS

Kavli Affiliate: Claudio Ricci | First 5 Authors: Yarone M. Tokayer, Michael J. Koss, C. Megan Urry, Priyamvada Natarajan, Richard Mushotzky | Summary: Deep extragalactic X-ray surveys, such as the Chandra COSMOS-Legacy field (CCLS), are prone to be biased against active galactic nuclei (AGN) with high column densities due to their lower count rates at […]


Continue.. BASS XLV: Quantifying AGN Selection Effects in the Chandra COSMOS-Legacy Survey with BASS

ATOMS: ALMA Three-millimeter Observations of massive Star-forming regions -XX. Probability distribution function of integrated intensity for dense molecular gas tracers

Kavli Affiliate: Ke Wang | First 5 Authors: C. Zhang, Tie Liu, Sihan Jiao, Feng-Yao Zhu, Z. -Y. Ren | Summary: We report the observations of J=1-0 of HCN, HCO+, H13CO+, and H13CN, HC3N (J=11-10) emission towards 135 massive star-forming clumps, as part of the ATOMS (ALMA Three-millimeter Observations of Massive Star-forming regions) Survey. We […]


Continue.. ATOMS: ALMA Three-millimeter Observations of massive Star-forming regions -XX. Probability distribution function of integrated intensity for dense molecular gas tracers

Central densities of dark matter halos in FIRE-2 simulations of low-mass galaxies with cold dark matter and self-interacting dark matter

Kavli Affiliate: Lina Necib | First 5 Authors: Maria C. Straight, Michael Boylan-Kolchin, James S. Bullock, Philip F. Hopkins, Xuejian Shen | Summary: We investigate the central density structure of dark matter halos in cold dark matter (CDM) and self-interacting dark matter (SIDM) models using simulations that are part of the Feedback In Realistic Environments […]


Continue.. Central densities of dark matter halos in FIRE-2 simulations of low-mass galaxies with cold dark matter and self-interacting dark matter

Central densities of dark matter halos in FIRE-2 simulations of low-mass galaxies with cold dark matter and self-interacting dark matter

Kavli Affiliate: Lina Necib | First 5 Authors: Maria C. Straight, Michael Boylan-Kolchin, James S. Bullock, Philip F. Hopkins, Xuejian Shen | Summary: We investigate the central density structure of dark matter halos in cold dark matter (CDM) and self-interacting dark matter (SIDM) models using simulations that are part of the Feedback In Realistic Environments […]


Continue.. Central densities of dark matter halos in FIRE-2 simulations of low-mass galaxies with cold dark matter and self-interacting dark matter