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The UKIRT Infrared Deep Sky Survey (UKIDSS) is the first of a new generation of infrared surveys. Here we combine the data from two UKIDSS components, the Large Area Survey (LAS) and the Galactic Cluster Survey (GCS), with 2MASS data to…

天体物理学 · 物理学 2009-11-13 N. R. Deacon , N. C. Hambly , R. R. King , M. J. McCaughrean

We present the discovery of two z > 6 quasars, selected as i band dropouts in the VST ATLAS survey. Our first quasar has redshift, z = 6.31 \pm 0.03, z band magnitude, z_AB = 19.63 \pm 0.08 and rest frame 1450A absolute magnitude, M_1450 =…

We have conducted a kinematic study of 165 young M dwarfs with ages of <300 Myr. Our sample is composed of stars and brown dwarfs with spectral types ranging from K7 to L0, detected by ROSAT and with photometric distances of <25 pc assuming…

Aims. We present a determination of the intrinsic colors and ages of galaxies at very high redshift, in particular old galaxies (OGs) within extremely red objects (EROs). To date, the definition of EROs has been restricted to objects with…

宇宙学与河外天体物理 · 物理学 2015-06-03 N. Castro-Rodriguez , M. Lopez-Corredoira

We search for stars with proper motions in a set of deep Subaru images, covering about 0.48 square degrees to a depth of $i' \simeq 26$, taken over a span of five and a half years. We follow the methods described in \citet{Richmond2009} to…

星系天体物理 · 物理学 2015-05-14 Michael W. Richmond , Tomoki Morokuma , Mamoru Doi , Yutaka Komiyama , Naoki Yasuda , Sadanori Okamura

We present preliminary results from the first part of the LuckyCam late M-dwarf binarity survey. We survey a sample of 48 nearby ($<$40 pc) and red (M5-M9) stars with the novel high angular resolution visible light imaging technique Lucky…

天体物理学 · 物理学 2007-05-23 Nicholas M. Law , Simon T. Hodgkin , Craig D. Mackay , John E. Baldwin

Stars of all evolutionary phases have been found to have excess infrared emission due to the presence of circumstellar material. To identify such stars, we have positionally correlated the infrared MSX point source catalogue and the Tycho 2…

天体物理学 · 物理学 2008-11-26 A. J. Clarke , R. D. Oudmaijer , S. L Lumsden

We report high resolution optical speckle observations of 336 M dwarfs which result in 113 measurements of relative position of 80 systems and 256 other stars with no indications of duplicity. These are the first measurements for two of the…

太阳与恒星天体物理 · 物理学 2018-05-16 Brian D. Mason , William I. Hartkopf , Korie N. Miles , John P. Subasavage , Deepak Raghavan , Todd J. Henry

We associate 132 low-mass ultracool dwarfs in the southern hemisphere as candidate members of five moving groups using photometric and astrometric selection techniques. Of these objects, we present high resolution spectroscopy for seven…

We report the discovery of 76 new T dwarfs from the UKIDSS Large Area Survey (LAS). Near-infrared broad and narrow-band photometry and spectroscopy are presented for the new objects, along with WISE and warm-Spitzer photometry. Proper…

Observations made using TESS revealed a sample of low mass stars which show a periodic modulation on a period $<0.2$~d. Surprisingly many of these Ultra Fast Rotating (UFR) stars showed no evidence of flare activity which would be expected…

太阳与恒星天体物理 · 物理学 2022-02-23 Gavin Ramsay , Pasi Hakala , J. Gerry Doyle , Lauren Doyle , Stefano Bagnulo

In order to find the most extreme dust-hidden high-redshift galaxies, we select 196 extremely red objects in the Ks and IRAC bands (KIEROs, [Ks-4.5um](AB)>1.6) in the 0.06 deg^2 GOODS-N region. This selection avoids the Balmer breaks of…

宇宙学与河外天体物理 · 物理学 2015-05-30 Wei-Hao Wang , Amy J. Barger , Lennox L. Cowie

Carbon and oxygen abundances of eight late M dwarfs are determined based on the near IR spectra of medium resolution. Seven objects with T_eff above 2600K are analyzed with the dust-free models. The M8.5 dwarf 2MASSI J1835379+325954 whose…

太阳与恒星天体物理 · 物理学 2016-01-20 Takashi Tsuji , Tadashi Nakajima

In a volume-limited sample of 63 ultracool dwarfs of spectral type M7--M9.5, we have obtained high-resolution spectroscopy with UVES at the Very Large Telescope and HIRES at Keck Observatory. In this first paper we introduce our…

太阳与恒星天体物理 · 物理学 2014-11-20 A. Reiners , G. Basri

The paper presents the identification of the stars in the lower part of the Main Sequence among the objects of the deep survey of the equatorial region of the sky, performed by the eROSITA telescope at the SRG orbital observatory. Of the…

太阳与恒星天体物理 · 物理学 2021-09-28 Aleksey A. Shlyapnikov

We discuss the very red objects found in the first field of the Caltech Faint Galaxy Redshift Survey, for which the observations and analysis are now complete. In this field, which is 15 arcmin$^2$ and at J005325+1234 there are 195 objects…

天体物理学 · 物理学 2007-05-23 Judith G. Cohen , David W. Hogg , Roger Blandford , Michael A. Pahre , Patrick L. Shopbell

The Edinburgh-Cape Blue Object Survey is an ongoing project to identify and analyse a large sample of hot stars selected initially on the basis of photographic colours (down to a magnitude limit B~18.0) over the entire…

天体物理学 · 物理学 2019-08-17 T. C. Beers , S. Rossi , D. O'Donoghue , D. Kilkenny , R. S. Stobie , C. Koen , R. Wilhelm

We present first results from a major program of methane filter photometry for low-mass stars and brown dwarfs. The definition of a new methane filter photometric system is described. A recipe is provided for the differential calibration of…

天体物理学 · 物理学 2016-08-30 C. G. Tinney , Adam J. Burgasser , J. Davy Kirkpatrick , Michael W. McElwain

We report the discovery of an extremely red planetary-mass companion to 2MASS J22362452+4751425, a $\approx$0.6 $M_{\odot}$ late-K dwarf likely belonging to the $\sim$120 Myr AB Doradus moving group. 2M2236+4751 b was identified in…

We present optical spectra for a representative sample of 27 nearby (z < 0.2) 2MASS-selected AGN with red near-IR colours (J-K 2.0). The spectra were taken with the ISIS spectrograph on the WHT with the aim of determining the nature of the…

宇宙学与河外天体物理 · 物理学 2015-06-15 Marvin Rose , Clive Tadhunter , Joanna Holt , Javier Rodríguez Zaurín