Z. H. Zhang
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View article: Observation of undepleted phosphine in the atmosphere of a low-temperature brown dwarf
Observation of undepleted phosphine in the atmosphere of a low-temperature brown dwarf Open
The atmospheres of low-temperature brown dwarfs and gas giant planets are expected to contain the phosphine molecule, PH 3 . However, previous observations have shown much lower abundances of this molecule than predicted with atmospheric c…
View article: X-SHYNE: X-Shooter spectra of young exoplanet analogs
X-SHYNE: X-Shooter spectra of young exoplanet analogs Open
Characterizing exoplanets’ spectra is a crucial step in understanding the chemical and physical processes shaping their atmospheres and constraining their formation and evolutionary history. The X-SHYNE library is a homogeneous sample of 4…
View article: Imaging-spectroscopy diagnosis of the giant sloshing spiral in the Virgo cluster with the Einstein Probe Follow-up X-ray Telescope
Imaging-spectroscopy diagnosis of the giant sloshing spiral in the Virgo cluster with the Einstein Probe Follow-up X-ray Telescope Open
We performed deep X-ray observations of the Virgo cluster using the Einstein Probe Follow-up X-ray Telescope ( EP-FXT ) with a total exposure of 295 ks. Taking advantage of the large field of view (FoV) and low particle background of EP-FX…
View article: Benchmark brown dwarfs – I. A blue M2 + T5 wide binary and a probable young [M4 + M4] + [T7 + T8] hierarchical quadruple
Benchmark brown dwarfs – I. A blue M2 + T5 wide binary and a probable young [M4 + M4] + [T7 + T8] hierarchical quadruple Open
Benchmark brown dwarfs in wide binary systems are crucial for characterizing substellar objects and calibrating atmospheric and evolutionary models. However, brown dwarf benchmarks with subsolar metallicity, very cool temperatures, or suit…
View article: GTC Optical/Near-infrared Upper Limits and NICER X-Ray Analysis of SGR J1935+2154 for the Outburst in 2022
GTC Optical/Near-infrared Upper Limits and NICER X-Ray Analysis of SGR J1935+2154 for the Outburst in 2022 Open
The Galactic magnetar SGR J1935+2154 has undergone another outburst since 2022 October 10. We present the results of searching for an optical/near-infrared (NIR) counterpart of SGR J1935+2154 before and during this outburst. No counterpart…
View article: The <i>Gaia</i> ultracool dwarf sample–IV. GTC/OSIRIS optical spectra of <i>Gaia</i> late-M and L dwarfs
The <i>Gaia</i> ultracool dwarf sample–IV. GTC/OSIRIS optical spectra of <i>Gaia</i> late-M and L dwarfs Open
As part of our comprehensive, ongoing characterization of the low-mass end of the main sequence in the Solar neighbourhood, we used the OSIRIS instrument at the 10.4 m Gran Telescopio Canarias to acquire low- and mid-resolution (R${\approx…
View article: Primeval very low-mass stars and brown dwarfs – VIII. The first age benchmark L subdwarf, a wide companion to a halo white dwarf
Primeval very low-mass stars and brown dwarfs – VIII. The first age benchmark L subdwarf, a wide companion to a halo white dwarf Open
We report the discovery of five white dwarf + ultracool dwarf systems identified as common proper motion wide binaries in the Gaia Catalogue of Nearby Stars. The discoveries include a white dwarf + L subdwarf binary, VVV 1256−62AB, a gravi…
View article: 76 T dwarfs from the UKIDSS LAS: Benchmarks, kinematics and an updated space density
76 T dwarfs from the UKIDSS LAS: Benchmarks, kinematics and an updated space density Open
We report the discovery of 76 new T dwarfs from the UKIRT Infrared Deep Sky Survey(UKIDSS) Large Area Survey (LAS). Near-infrared broad-and narrow-band photometry and spectroscopy are presented for the new objects, along withWide-field Inf…
View article: Non-equilibrium effect modeling and particle velocity estimation for particulate flow in porous media
Non-equilibrium effect modeling and particle velocity estimation for particulate flow in porous media Open
The complex dynamics of fluid and particles flowing through pore space demands some relaxation time for particles to catch up with fluid velocity, which manifest themselves as non-equilibrium (NE) effects. Previous studies have shown that …
View article: Search for gamma-ray bursts and gravitational wave electromagnetic counterparts with High Energy X-ray Telescope of <i>Insight</i>-HXMT
Search for gamma-ray bursts and gravitational wave electromagnetic counterparts with High Energy X-ray Telescope of <i>Insight</i>-HXMT Open
The High Energy (HE) X-ray telescope on board the Hard X-ray Modulation Telescope (Insight-HXMT) can serve as a wide field of view (FOV) gamma-ray monitor with high time resolution (μs) and large effective area (up to thousands cm2). We de…
View article: Discovery of the substellar transition zone of transitional brown dwarfs between stars and degenerate brown dwarfs
Discovery of the substellar transition zone of transitional brown dwarfs between stars and degenerate brown dwarfs Open
The destiny of a star is depending on the status of hydrogen fusion that it can reach after its formation. Stars have steady hydrogen fusion and can maintain their luminosity. Degenerate brown dwarfs (D-BD) have no energy supply from hydro…
View article: Primeval very low-mass stars and brown dwarfs series
Primeval very low-mass stars and brown dwarfs series Open
Primeval - I. Six new L subdwarfs, classification and atmospheric properties Primeval - II. The most metal-poor substellar object Primeval - III. The halo transitional brown dwarfs Primeval - IV. New L subdwarfs, Gaia astrometry, populatio…
View article: First discovery of an ultra-cool white dwarf benchmark in common proper motion with an M dwarf
First discovery of an ultra-cool white dwarf benchmark in common proper motion with an M dwarf Open
Ultra-cool white dwarfs are among the oldest stellar remnants in the Universe. Their efficient gravitational settling and low effective temperatures are responsible for the smooth spectra they exhibit. For that reason, it is not possible t…
View article: Primeval very low-mass stars and brown dwarfs – VII. The discovery of the first wide M + L extreme subdwarf binary
Primeval very low-mass stars and brown dwarfs – VII. The discovery of the first wide M + L extreme subdwarf binary Open
I present the discovery of the first wide M + L extreme subdwarf binary system Gaia J0452−36AB. The binary is located at a distance of 137.27 $^{+0.68}_{-0.67}$ pc with a projected separation of 15828 ± 78 au. I classified Gaia J0452−36AB …
View article: Primeval very low-mass stars and brown dwarfs – VI. Population properties of metal-poor degenerate brown dwarfs
Primeval very low-mass stars and brown dwarfs – VI. Population properties of metal-poor degenerate brown dwarfs Open
We presented 15 new T dwarfs that were selected from UKIRT Infrared Deep Sky Survey, Visible and Infrared Survey Telescope for Astronomy , and Wide-field Infrared Survey Explorer surveys, and confirmed with optical to near-infrared spectra…
View article: Primeval very low-mass stars and brown dwarfs – V. A halo L3 subdwarf with prograde eccentric orbit in the Galactic plane
Primeval very low-mass stars and brown dwarfs – V. A halo L3 subdwarf with prograde eccentric orbit in the Galactic plane Open
VVV J12564163$-$6202039 is an L subdwarf located in the Galactic plane ($b$ =\n0.831 deg) discovered by its high proper motion (1.1 arcsec yr/s). We obtained\nan optical to near-infrared spectrum of it with the X-shooter on the Very Large\…
View article: Microlens mass determination for<i>Gaia</i>’s predicted photometric events
Microlens mass determination for<i>Gaia</i>’s predicted photometric events Open
We used Gaia Data Release 2 to search for upcoming photometric microlensing\nevents, identifying two candidates with high amplification. In the case of\ncandidate 1, a spectrum of the lens (l1) confirms it is a usdM3 subdwarf with\nmass $\…
View article: The Substellar Transition Zone: A Stretched Temperature Canyon in Brown Dwarf Population due to Unsteady Hydrogen Fusion
The Substellar Transition Zone: A Stretched Temperature Canyon in Brown Dwarf Population due to Unsteady Hydrogen Fusion Open
I summarize results on transitional and degenerate brown dwarfs presented in a series titled Primeval very low-mass stars and brown dwarfs. I introduce an L subdwarf classification scheme, which classified L subdwarfs into three m…
View article: The Substellar Transition Zone: A Stretched Temperature Canyon In Brown Dwarf Population Due To Unsteady Hydrogen Fusion
The Substellar Transition Zone: A Stretched Temperature Canyon In Brown Dwarf Population Due To Unsteady Hydrogen Fusion Open
I introduce an L subdwarf classification scheme, which classified L subdwarfs into three metal subclasses. I would also like to draw your attention to transitional brown dwarfs which have unsteady hydrogen fusion in their cores to replenis…
View article: Primeval very low-mass stars and brown dwarfs – IV. New L subdwarfs, Gaia astrometry, population properties, and a blue brown dwarf binary
Primeval very low-mass stars and brown dwarfs – IV. New L subdwarfs, Gaia astrometry, population properties, and a blue brown dwarf binary Open
We present 27 new L subdwarfs and classify five of them as esdL and 22 as\nsdL. Our L subdwarf candidates were selected with the UKIRT Infrared Deep Sky\nSurvey and Sloan Digital Sky Survey. Spectroscopic follow-up was carried out\nprimari…
View article: The Science Advantage of a Redder Filter for WFIRST
The Science Advantage of a Redder Filter for WFIRST Open
WFIRST will be capable of providing Hubble-quality imaging performance over several thousand square degrees of the sky. The wide-area, high spatial resolution survey data from WFIRST will be unsurpassed for many decades into the future. Wi…
View article: Primeval very low-mass stars and brown dwarfs – III. The halo transitional brown dwarfs
Primeval very low-mass stars and brown dwarfs – III. The halo transitional brown dwarfs Open
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society. © 2018 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
View article: Ultracool dwarf benchmarks with Gaia primaries
Ultracool dwarf benchmarks with Gaia primaries Open
We explore the potential of Gaia for the field of benchmark ultracool/brown dwarf companions, and present the results of an initial search for metal-rich/metal-poor systems. A simulated population of resolved ultracool dwarf companions to …
View article: Primeval very low-mass stars and brown dwarfs – II. The most metal-poor substellar object
Primeval very low-mass stars and brown dwarfs – II. The most metal-poor substellar object Open
SDSS J010448.46+153501.8 has previously been classified as an sdM9.5\nsubdwarf. However, its very blue $J-K$ colour ($-0.15 \\pm 0.17$) suggests a\nmuch lower metallicity compared to normal sdM9.5 subdwarfs. Here, we\nre-classify this obje…
View article: Primeval very low-mass stars and brown dwarfs – I. Six new L subdwarfs, classification and atmospheric properties
Primeval very low-mass stars and brown dwarfs – I. Six new L subdwarfs, classification and atmospheric properties Open
We have conducted a search for L subdwarf candidates within the photometric\ncatalogues of the UKIRT Infrared Deep Sky Survey and Sloan Digital Sky Survey.\nSix of our candidates are confirmed as L subdwarfs spectroscopically at optical\na…
View article: 49 new T dwarfs identified using methane imaging
49 new T dwarfs identified using methane imaging Open
We present the discovery of 49 new photometrically classified T dwarfs from the combination of large infrared and optical surveys combined with follow-up TNG photometry. We used multi-band infrared and optical photometry from the UKIRT and…
View article: A large spectroscopic sample of L and T dwarfs from UKIDSS LAS: peculiar objects, binaries, and space density
A large spectroscopic sample of L and T dwarfs from UKIDSS LAS: peculiar objects, binaries, and space density Open
This is a pre-copyedited, author-produced PDF of an article accepted for publication in Monthly Notices of the Royal Astronomical Society following peer review. The version of record [F. Marocco, et al, 'A large spectroscopic sample of L a…