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This study presents a search for IR excess in the 3.4, 4.6, 12 and 22 $\mu$m bands in a sample of 216 targets, composed of solar sibling, twin and analog stars observed by the \textit{WISE} mission. In general, an infrared excess suggests…

We present the results of a search of infrared excess candidates in a comprehensive (29\,000 stars) magnitude limited sample of dwarf stars, spanning the spectral range F2-K0, and brighter than V$=$15 mag. We searched the sample within the…

Solar and Stellar Astrophysics · Physics 2015-06-17 Fernando Cruz-Saenz de Miera , Miguel Chavez , Emanuele Bertone , Olga Vega

Circumstellar debris disks are important because of their connection to planetary systems. An efficient way to identify these systems is through their infrared excess. Most studies so far concentrated on early-type or solar-type stars, but…

Solar and Stellar Astrophysics · Physics 2015-06-11 Henning Avenhaus , Hans Martin Schmid , Michael R. Meyer

Stars with excess infrared radiation from circumstellar dust are invaluable for studies of exoplanetary systems, informing our understanding on processes of planet formation and destruction alike. All-sky photometric surveys have made the…

Solar and Stellar Astrophysics · Physics 2020-03-18 Erik Dennihy , Jay Farihi , Nicola Pietro Gentile Fusillo , John H. Debes

We describe a search for infra-red excess emission from dusty circumstellar material around 180,000 stars observed by the Kepler and WISE missions. This study is motivated by i) the potential to find bright warm disks around planet host…

Earth and Planetary Astrophysics · Physics 2013-11-07 G. M. Kennedy , M. C. Wyatt

Stellar infrared excesses can indicate various phenomena of interest, from protoplanetary disks to debris disks, or (more speculatively) techno-signatures along the lines of Dyson spheres. In this paper, we conduct a large search for such…

Earth and Planetary Astrophysics · Physics 2024-09-20 Gabriella Contardo , David W. Hogg

Infrared excesses around white dwarf stars indicate the presence of various astrophysical objects of interest, including companions and debris disks. In this second paper of a series, we present follow-up observations of infrared excess…

The conclusion of the WISE mission presents an opportune time to summarize the history of using excess emission in the infrared as a tracer of circumstellar material and exploit all available data for future missions such as JWST. We have…

Solar and Stellar Astrophysics · Physics 2016-08-03 Tara H. Cotten , Inseok Song

We present results of the analysis of a sample of 22 stars of spectral types from O7 to B5 and luminosity classes I-V for which Spitzer/IRS spectra are available. The IRS spectra of these stars are examined for signs of excess infrared (IR)…

Solar and Stellar Astrophysics · Physics 2018-11-28 R. Siebenmorgen , P. Scicluna , J. Krelowski

Context: Extended circumstellar emission has been detected within a few 100 milli-arcsec around > 10% of nearby main sequence stars using near-infrared interferometry. Follow-up observations using other techniques, should they yield similar…

In this paper we present a catalog which includes 141 bright candidates ($\leq10.27$ mag, V band) showing the infrared (IR) excess at 22 $\mu$m. Of which, 38 stars are known IR excess stars or disk, 23 stars are double or multiple stars and…

Solar and Stellar Astrophysics · Physics 2013-10-10 Chao-Jian Wu , Hong Wu , Man-I Lam , Ming Yang , Xiao-Qing Wen , Shuo Li , Tong-Jie Zhang , Liang Gao

Using data from the WISE All-Sky Survey, we have found >100 new infrared excess sources around main-sequence Hipparcos stars within 75pc. Our empirical calibration of WISE photospheric colors and removal of non-trivial false-positive…

Solar and Stellar Astrophysics · Physics 2016-02-03 Rahul Patel , Stanimir Metchev , Aren Heinze , Joseph Trollo

We present sources selected from their Wide-field Infrared Survey Explorer (WISE) colors that merit future observations to image for disks and possible exoplanet companions. Introducing a weighted detection method, we eliminated the…

Instrumentation and Methods for Astrophysics · Physics 2016-07-28 Jonathon K. Zink , Damian Christian

In an earlier study we reported nearly 100 previously unknown dusty debris disks around Hipparcos main sequence stars within 75 pc by selecting stars with excesses in individual WISE colors. Here, we further scrutinize the Hipparcos 75 pc…

Solar and Stellar Astrophysics · Physics 2017-01-18 Rahul I. Patel , Stanimir Metchev , Aren Heinze , Joseph Trollo

The infrared excess from OB stars are commonly considered as contributions from ionized stellar wind or circumstellar dust. With the newly published LAMOST-OB catalog and GOSSS data, this work steps further on understanding the infrared…

Solar and Stellar Astrophysics · Physics 2022-10-31 Dingshan Deng , Yang Sun , Tianding Wang , Yuxi Wang , Biwei Jiang

White dwarfs with infrared excess emission provide a window into the late stages of stellar evolution and the dynamics of circumstellar environments. Using data from the Hobby-Eberly Telescope Dark Energy Experiment (HETDEX), we…

We present a sensitive search for WISE W3 (12um) and W4 (22um) excesses from warm optically thin dust around Hipparcos main sequence stars within 75pc from the Sun. We use contemporaneously measured photometry from WISE, remove sources of…

Solar and Stellar Astrophysics · Physics 2015-06-19 Rahul I. Patel , Stanimir A. Metchev , Aren Heinze

We investigate the nature of the mid-IR excess for 31 intermediate-mass stars that exhibit an 8 micron excess in either the Galactic Legacy Infrared Mid-Plane Survey Extraordinaire or the Mid-Course Space Experiment using high resolution…

Astrophysics · Physics 2009-11-13 B. Uzpen , H. A. Kobulnicky , D. R. Semler , T. Bensby , C. Thom

As part of a large Spitzer/MIPS GTO program, we have searched for infrared excesses due to debris disks toward 26 FGK field stars known from radial velocity (RV) studies to have one or more planets. While none of these stars show excesses…

We report the mid- and far-infrared properties of nearby M dwarfs. Spitzer/MIPS measurements were obtained for a sample of 62 stars at 24 um, with subsamples of 41 and 20 stars observed at 70 um and 160 um respectively. We compare the…

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