Search Publications

On the AGN Nature of Two UV-bright Sources at zspec ∼ 5.5 in the CANDELS Fields: An Update on the AGN Space Density at M1450 ∼ -22.5
DOI: 10.3847/1538-4357/ab99a3 Bibcode: 2020ApJ...897...94G

Dickinson, M.; Fiore, F.; Grazian, A. +8 more

It is widespread opinion that hydrogen reionization is mainly driven by primeval star-forming galaxies, with high-z active galactic nuclei (AGNs) having a minor role. Recent observations, however, challenge this notion, indicating a number of issues related to a galaxy-driven reionization scenario. We provide here an updated assessment of the spac…

2020 The Astrophysical Journal
eHST 34
Delay Time Distributions of Type Ia Supernovae from Galaxy and Cosmic Star Formation Histories
DOI: 10.3847/1538-4357/ab6a97 Bibcode: 2020ApJ...890..140S

Pacifici, Camilla; Graur, Or; Strolger, Louis-Gregory +2 more

We present analytical reconstructions of SN Ia delay time distributions (DTDs) by way of two independent methods: by a Markov Chain Monte Carlo best-fit technique comparing the volumetric SN Ia rate history to today's compendium cosmic star formation history, and second through a maximum likelihood analysis of the star formation rate histories of …

2020 The Astrophysical Journal
eHST 34
A Systematic Study of the Dust of Galactic Supernova Remnants. I. The Distance and the Extinction
DOI: 10.3847/1538-4357/ab75ef Bibcode: 2020ApJ...891..137Z

Jiang, Biwei; Chen, Bingqiu; Zhao, He +3 more

By combining the photometric, spectroscopic, and astrometric information of the stars in the sightline of supernova remnants (SNRs), the distances to and the extinctions of 32 Galactic SNRs are investigated. The stellar atmospheric parameters are from the Sloan Digital Sky Survey-DR14/Apache Point Observatory Galaxy Evolution Experiment and Large …

2020 The Astrophysical Journal
Gaia 34
Hot Dust-obscured Galaxies with Excess Blue Light
DOI: 10.3847/1538-4357/ab9814 Bibcode: 2020ApJ...897..112A

Stern, D.; Bauer, F. E.; Díaz-Santos, T. +10 more

Hot dust-obscured galaxies (Hot DOGs) are among the most luminous galaxies in the universe. Powered by highly obscured, possibly Compton-thick, active galactic nuclei (AGNs), Hot DOGs are characterized by spectral energy distributions that are very red in the mid-infrared yet dominated by the host galaxy stellar emission in the UV and optical. An …

2020 The Astrophysical Journal
eHST 33
Very Long Baseline Astrometry of PSR J1012+5307 and its Implications on Alternative Theories of Gravity
DOI: 10.3847/1538-4357/ab8f27 Bibcode: 2020ApJ...896...85D

Deller, Adam T.; Kaplan, David L.; Lazio, T. Joseph W. +4 more

PSR J1012+5307, a millisecond pulsar in orbit with a helium white dwarf (WD), has been timed with high precision for about 25 yr. One of the main objectives of this long-term timing is to use the large asymmetry in gravitational binding energy between the neutron star and the WD to test gravitational theories. Such tests, however, will be eventual…

2020 The Astrophysical Journal
Gaia 33
X-shooter Spectroscopy and HST Imaging of 15 Massive Quiescent Galaxies at z ≳ 2
DOI: 10.3847/1538-4357/ab5af4 Bibcode: 2020ApJ...888....4S

Conselice, Christopher J.; Gallazzi, Anna; Zibetti, Stefano +23 more

We present a detailed analysis of a large sample of spectroscopically confirmed massive quiescent galaxies (MQGs; log(M */M ) ∼ 11.5) at z ≳ 2. This sample comprises 15 galaxies selected in the COSMOS and UDS fields by their bright K-band magnitudes and followed up with Very Large Telescope (VLT) X-shooter spectroscopy and H…

2020 The Astrophysical Journal
eHST 33
Introducing the Search for Intermediate-mass Black Holes in Nearby Galaxies (SIBLING) Survey
DOI: 10.3847/1538-4357/ab5f5b Bibcode: 2020ApJ...889..113M

Plotkin, Richard M.; Martínez-Palomera, Jorge; Lira, Paulina +2 more

Intermediate-mass black holes (IMBHs) have masses between 102 and 106 M and are key to our understanding of the formation of massive black holes. The known population of IMBHs remains small, with a few hundred candidates and only a handful of them confirmed as bona fide IMBHs. Until now, the most widely used selec…

2020 The Astrophysical Journal
XMM-Newton 33
Revisiting the Impact of Dust Production from Carbon-rich Wolf-Rayet Binaries
DOI: 10.3847/1538-4357/ab9cb5 Bibcode: 2020ApJ...898...74L

Sakon, Itsuki; Williams, Peredur M.; Lau, Ryan M. +3 more

We present a dust spectral energy distribution (SED) and binary stellar population analysis revisiting the dust production rates (DPRs) in the winds of carbon-rich Wolf-Rayet (WC) binaries and their impact on galactic dust budgets. DustEM SED models of 19 Galactic WC "dustars" reveal DPRs of ${\dot{M}}_{d}\sim {10}^{-10}\mbox{--}{10}^{-6}$ M⊙…

2020 The Astrophysical Journal
Gaia ISO 33
Discovery of Two Pulsating Extremely Low-mass Pre-white Dwarf Candidates in the TESS Eclipsing Binaries
DOI: 10.3847/1538-4357/ab584c Bibcode: 2020ApJ...888...49W

Zhang, Xiaobin; Wang, Kun; Dai, Min

We report the discovery of two new pulsating extremely low-mass pre-white dwarf (pre-ELMV) candidates in the Transiting Exoplanet Survey Satellite (TESS) eclipsing binaries, TIC 149160359 and TIC 416264037. Their light curves show a typical feature of EL CVn-type binaries. The light-curve modeling indicates that they are both detached systems with…

2020 The Astrophysical Journal
Gaia 33
Cosmological Insights into the Early Accretion of r-process-enhanced Stars. I. A Comprehensive Chemodynamical Analysis of LAMOST J1109+0754
DOI: 10.3847/1538-4357/abbc13 Bibcode: 2020ApJ...903...88M

Zhao, Gang; Beers, Timothy C.; Placco, Vinicius M. +11 more

This study presents a comprehensive chemodynamical analysis of LAMOST J1109+0754, a bright (V = 12.8), extremely metal-poor ([Fe/H] = -3.17) star, with a strong r-process enhancement ([Eu/Fe] = +0.94 ± 0.12). Our results are based on the 7D measurements supplied by Gaia and the chemical composition derived from a high-resolution (R ∼ 110,000), hig…

2020 The Astrophysical Journal
Gaia 33