Search Results - "LEHMER, B. D"
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A magnetar-powered X-ray transient as the aftermath of a binary neutron-star merger
Published in Nature (London) (01-04-2019)“…Mergers of neutron stars are known to be associated with short γ-ray bursts 1 – 4 . If the neutron-star equation of state is sufficiently stiff (that is, the…”
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THE EVOLUTION OF NORMAL GALAXY X-RAY EMISSION THROUGH COSMIC HISTORY: CONSTRAINTS FROM THE 6 MS CHANDRA DEEP FIELD-SOUTH
Published in The Astrophysical journal (01-07-2016)“…ABSTRACT We present measurements of the evolution of normal-galaxy X-ray emission from 0-7 using local galaxies and galaxy samples in the 6 Ms Chandra Deep…”
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A Chandra Perspective on Galaxy-wide X-ray Binary Emission and its Correlation with Star Formation Rate and Stellar Mass: New Results from Luminous Infrared Galaxies
Published in The Astrophysical journal (20-11-2010)“…We present new Chandra observations that complete a sample of seventeen (17) luminous infrared galaxies (LIRGs) with D < 60 Mpc and low Galactic column…”
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4
Black Hole Growth Is Mainly Linked to Host-galaxy Stellar Mass Rather Than Star Formation Rate
Published in The Astrophysical journal (20-06-2017)“…We investigate the dependence of black hole accretion rate (BHAR) on host-galaxy star formation rate (SFR) and stellar mass (M*) in the CANDELS/GOODS-South…”
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The deepest X-ray view of high-redshift galaxies: constraints on low-rate black hole accretion
Published in Monthly notices of the Royal Astronomical Society (21-11-2016)“…We exploit the 7 Ms Chandra observations in the Chandra Deep Field-South (CDF-S), the deepest X-ray survey to date, coupled with CANDELS/GOODS-S data, to…”
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Color-Magnitude Relations of Active and Non-active Galaxies in the Chandra Deep Fields: High-redshift Constraints and Stellar-mass Selection Effects
Published in The Astrophysical journal (01-09-2010)“…We extend color-magnitude relations for moderate-luminosity X-ray active galactic nucleus (AGN) hosts and non-AGN galaxies through the galaxy formation epoch…”
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THE 4 Ms CHANDRA DEEP FIELD-SOUTH NUMBER COUNTS APPORTIONED BY SOURCE CLASS: PERVASIVE ACTIVE GALACTIC NUCLEI AND THE ASCENT OF NORMAL GALAXIES
Published in The Astrophysical journal (10-06-2012)“…We present 0.5-2 keV, 2-8 keV, 4-8 keV, and 0.5-8 keV (hereafter soft, hard, ultra-hard, and full bands, respectively) cumulative and differential number-count…”
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On the Spatially Resolved Star Formation History in M51. I. Hybrid UV+IR Star Formation Laws and IR Emission from Dust Heated by Old Stars
Published in The Astrophysical journal (10-12-2017)“…We present Lightning, a new spectral energy distribution fitting procedure, capable of quickly and reliably recovering star formation history (SFH) and…”
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Towards a complete census of active galactic nuclei in nearby galaxies: the incidence of growing black holes
Published in Monthly notices of the Royal Astronomical Society (21-07-2010)“…We investigate the local supermassive black hole (SMBH) density function and relative mass accretion rates of all active galactic nuclei (AGNs) identified in a…”
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Young Accreting Compact Objects in M31: The Combined Power of NuSTAR, Chandra, and Hubble
Published in The Astrophysical journal (20-07-2018)“…We present 15 high-mass X-ray binary (HMXB) candidates in the disk of M31 for which we are able to infer compact object type, spectral type of the donor star,…”
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The Evolution of AGN Host Galaxies: From Blue to Red and the Influence of Large-Scale Structures
Published in The Astrophysical journal (10-03-2008)“…We present an analysis of 109 moderate-luminosity AGNs in the Extended Chandra Deep Field-South survey, which is drawn from 5549 galaxies from the COMBO-17 and…”
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The Chandra Deep Protocluster Survey: Evidence for an Enhancement of AGN Activity in the SSA22 Protocluster at z = 3.09
Published in The Astrophysical journal (20-01-2009)“…We present results from a new ultra-deep 400 ks Chandra observation of the SSA22 protocluster at z = 3.09. We have studied the X-ray properties of 234 z ~ 3…”
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INVERSE COMPTON X-RAY HALOS AROUND HIGH-z RADIO GALAXIES: A FEEDBACK MECHANISM POWERED BY FAR-INFRARED STARBURSTS OR THE COSMIC MICROWAVE BACKGROUND?
Published in The Astrophysical journal (01-12-2012)“…We report the detection of extended X-ray emission around two powerful radio galaxies at z ~ 3.6 (4C 03.24 and 4C 19.71) and use these to investigate the…”
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The Chandra Deep Protocluster Survey: point-source catalogues for a 400-ks observation of the z= 3.09 protocluster in SSA22
Published in Monthly notices of the Royal Astronomical Society (21-11-2009)“…We present X-ray point-source catalogues for a deep ≈400-ks Chandra ACIS-I (Advanced CCD Imaging Spectrometer) exposure of the SSA22 field. The observations…”
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15
Identification of the Hard X-Ray Source Dominating the E > 25 keV Emission of the Nearby Galaxy M31
Published in The Astrophysical journal (20-03-2017)“…We report the identification of a bright hard X-ray source dominating the M31 bulge above 25 keV from a simultaneous NuSTAR-Swift observation. We find that…”
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Tracing the Mass-Dependent Star Formation History of Late-Type Galaxies Using X-Ray Emission: Results from the Chandra Deep Fields
Published in The Astrophysical journal (10-07-2008)“…We report on the X-ray evolution over the last [sim]9 Gyr of cosmic history (i.e., since [image]) of late-type galaxy populations in the Chandra Deep…”
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A submillimetre galaxy at z= 4.76 in the LABOCA survey of the Extended Chandra Deep Field-South
Published in Monthly notices of the Royal Astronomical Society (01-06-2009)“…We report on the identification of the highest redshift submillimetre-selected source currently known LESS J033229.4−275619. This source was detected in the…”
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TRACKING DOWN THE SOURCE POPULATION RESPONSIBLE FOR THE UNRESOLVED COSMIC 6-8 keV BACKGROUND
Published in The Astrophysical journal (20-10-2012)“…Using the 4 Ms Chandra Deep Field-South (CDF-S) survey, we have identified a sample of 6845 X-ray-undetected galaxies that dominates the unresolved 20%-25% of…”
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The X-Ray Evolution of Early-Type Galaxies in the Extended Chandra Deep Field-South
Published in The Astrophysical journal (10-03-2007)“…We investigate the evolution over the last 6.3 Gyr of cosmic time (i.e., since z- 0.7) of the average X-ray properties of early-type galaxies within the…”
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The cosmic history of hot gas cooling and radio active galactic nucleus activity in massive early-type galaxies
Published in Monthly notices of the Royal Astronomical Society (01-05-2012)“…We study the X-ray properties of 393 optically selected early-type galaxies (ETGs) over the redshift range of z≈ 0.0-1.2 in the Chandra Deep Fields (CDFs). To…”
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