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Related papers: A WFI survey in the Chamaeleon II dark cloud

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AIMS: With our low-resolution spectroscopic observing program for selected blue proper motion stars, we tried to find new white dwarfs (WDs) in the solar neighbourhood. METHODS: We used the LSPM catalogue with a lower proper motion limit of…

Solar and Stellar Astrophysics · Physics 2018-11-07 R. -D. Scholz , H. Meusinger , A. Schwope , H. Jahreiß , I. Pelisoli

We present near-infrared (1.0-2.4 micron) spectra confirming the youth and cool effective temperatures of 6 brown dwarfs and low mass stars with circumstellar disks toward the Chamaeleon II and Ophiuchus star forming regions. The spectrum…

We report the outcome of the deep optical/infrared photometric survey of the central region (33 X 33 arcmin or 0.9 pc^2) of the eta Chamaeleontis pre-main sequence star cluster. The completeness limits of the photometry are I = 19.1, J =…

Astrophysics · Physics 2009-11-11 A-Ran Lyo , Inseok Song , Warrick A. Lawson , M. S. Bessell , B. Zuckerman

We present criteria for the photometric selection of M-dwarfs using all-sky photometry, with a view to identifying M-dwarf candidates for inclusion in the input catalogues of upcoming all-sky surveys, including TESS and FunnelWeb. The…

Instrumentation and Methods for Astrophysics · Physics 2018-04-20 J. Bentley , C. Tinney , S. Sharma , D. Wright

We present the results of a deep CCD-based IZ photometric survey of a ~1 sq. deg area in the central region of the Pleiades Galactic open cluster. The magnitude coverage of our survey (from I~17.5 down to 22) allows us to detect substellar…

We present CFHT photometry and IRTF spectroscopy of low-mass candidate members of Serpens South and Serpens Core ($\sim$430 pc, $\sim$0.5 Myr), identified using a novel combination of photometric filters, known as the W-band method. We…

I present observations of a new faint double, 2MASS J11011926-7732383AB, toward the Chamaeleon I star-forming region. From optical and near-infrared images of the pair, I measure a separation of 1.44" and extract RIJHK_s photometry of the…

Astrophysics · Physics 2009-11-10 K. L. Luhman

We present new HST/WFPC2 observations of 20 fields centered around T Tauri stars in the Chamaeleon I star forming region. Images have been obtained in the F631N ([OI]6300A), F656N (Ha) and F673N ([SII]6716A+6731A) narrow-band filters, plus…

Solar and Stellar Astrophysics · Physics 2015-06-05 M. Robberto , L. Spina , N. Da Rio , D. Apai , I. Pascucci , L. Ricci , C. Goddi , L. Testi , F. Palla , F. Bacciotti

We present an analysis of candidate members of the Eta Cha and MBM 12A young associations. For an area of 0.7 deg^2 toward Eta Cha, we have performed a search for members of the association by combining JHK_s photometry from 2MASS and i…

Astrophysics · Physics 2009-11-10 K. L. Luhman , D. Steeghs

(Abridged). We have conducted deep photometric searches for substellar members of the Praesepe (0.5-1 Gyr) and sigma Orionis (3 Myr) star clusters using the Sloan i' and z' filters, the 3.5-m and the 5-m Hale telescopes on the Calar Alto…

We present the results of a deep wide-field near-infrared survey of 12 square degrees of the Pleiades conducted as part of the UKIDSS Deep Infrared Sky Survey (UKIDSS) Galactic Cluster Survey (GCS). We have extracted over 340 high…

Astrophysics · Physics 2011-03-10 N. Lodieu , P. D. Dobbie , N. R. Deacon , S. T. Hodgkin , N. C. Hambly , R. F. Jameson

During an imaging survey of the Chamaeleon I star-forming region with the ACS aboard HST, we have discovered a candidate substellar companion to the young low-mass star CHXR 73 (~2 Myr, M=0.35 Msun). We measure a projected separation of…

Direct imaging surveys have discovered wide-orbit planetary-mass companions that challenge existing models of both star and planet formation, but their demographics remain poorly sampled. We have developed an automated binary companion…

Solar and Stellar Astrophysics · Physics 2019-09-25 Raquel A. Martinez , Adam L. Kraus

Detailed studies of intermediate/low mass pre-main sequence (PMS) stars outside the Galaxy have so far been conducted only for small targeted regions harbouring known star formation complexes. The VISTA Survey of the Magellanic Clouds (VMC)…

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…

Astrophysics · Physics 2016-08-30 C. G. Tinney , Adam J. Burgasser , J. Davy Kirkpatrick , Michael W. McElwain

We present an RI photometric survey covering an area of 430 arcmin^2 around the multiple star Sigma Orionis. The observations were conducted with the 0.8 m IAC-80 Telescope at the Teide Observatory. The survey limiting R and I magnitudes…

Astrophysics · Physics 2015-06-24 V. J. S. Bejar , M. R. Zapatero Osorio , R. Rebolo

We present results of an optical and near-infrared (IR) 1.8 deg^2 survey in the Pleiades open cluster to search for substellar objects. From optical I-band images from the CFHT and J-band images from the 3.5 m CAHA Telescope, we identify 18…

Astrophysics · Physics 2009-11-11 G. Bihain , R. Rebolo , V. J. S. Bejar , J. A. Caballero , C. A. L. Bailer-Jones , R. Mundt

Presented are the results of a large and deep optical-near-infrared multi-epoch survey of the Praesepe open star cluster using data from the UKIDSS Galactic Clusters Survey. Multiple colour magnitude diagrams were used to select potential…

Solar and Stellar Astrophysics · Physics 2015-05-19 D. E. A. Baker , R. F. Jameson , S. L. Casewell , N. Deacon , N. Lodieu , N. Hambly

We report the outcome of a deep multi-wavelength study of the IC2391 young open cluster. We aim at uncovering new low-mass and sub-stellar members of the cluster and identifying new debris disk objects. A 30*30 square arcmin area in IC 2391…

Solar and Stellar Astrophysics · Physics 2015-05-13 L. Spezzi , I. Pagano , G. Marino , G. Leto , E. Young , N. Siegler , Z. Balog , S. Messina , E. Distefano , B. Merin , D. Barrado y Navascues

We report the first results of our ongoing campaign to discover the first brown dwarfs (BD) in NGC 2264, a young (3 Myr), populous star forming region for which our optical studies have revealed a very high density of potential candidates -…

Astrophysics · Physics 2009-11-10 T. R. Kendall , J. Bouvier , E. Moraux , D. J. James , F. Menard