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1041. Catalogue of calibrator stars for LBSI
ID:
ivo://CDS.VizieR/J/A+A/393/183
Title:
Catalogue of calibrator stars for LBSI
Short Name:
J/A+A/393/183
Date:
21 Oct 2021
Publisher:
CDS
Description:
Long baseline stellar interferometry shares with other techniques the need for calibrator stars in order to correct for instrumental and atmospheric effects. We present a catalogue of 374 stars carefully selected to be used for that purpose in the near infrared. Owing to several convergent criteria with the work of Cohen et al. (1999AJ....117.1864C), this catalogue is in essence a subset of their self-consistent all-sky network of spectro-photometric calibrator stars. For every star, we provide the angular limb-darkened diameter, uniform disc angular diameters in the J, H and K bands, the Johnson photometry and other useful parameters. Most stars are type III giants with spectral types K or M0, magnitudes V=3-7 and K=0-3. Their angular limb-darkened diameters range from 1 to 3 mas with a median uncertainty as low as 1.2%. The median distance from a given point on the sky to the closest reference is 5.2{deg}, whereas this distance never exceeds 16.4{deg} for any celestial location.
1042. Catalogue of close binaries
ID:
ivo://CDS.VizieR/J/MNRAS/370/2013
Title:
Catalogue of close binaries
Short Name:
J/MNRAS/370/2013
Date:
21 Oct 2021
Publisher:
CDS
Description:
A catalogue of close eclipsing binary systems (detached and semidetached) with at least one of the components located in the delta Scuti region of the Cepheid instability strip is presented. The positions of the stars in the instability strip are determined by their accurate temperatures and luminosities. Observationally detected binaries (20 semidetached, four detached and one unclassified) with oscillating components were included in the catalogue as a separate table. The primaries of the oscillating Algols tend to be located near the blue edge of the instability strip. Using reliable luminosities and temperatures determined by recent photometric and spectroscopic studies, we have found that at least one or two components of 71 detached and 90 semidetached systems are located in the delta Scuti region of the Cepheid instability strip. In addition, 36 detached or semidetached systems discovered by the Hipparcos satellite were also given as a separate list. One of their components is seen in the delta Scuti region, according to their spectral type or BV colours. They are potential candidate binaries with the delta Scuti-type pulsating components which need further photometric and spectroscopic studies in better precision. This catalogue covers information and literature references for 25 known and 197 candidate binaries with pulsating components.
1043. Catalogue of cold cores in Perseus
ID:
ivo://CDS.VizieR/J/A+A/645/A55
Title:
Catalogue of cold cores in Perseus
Short Name:
J/A+A/645/A55
Date:
21 Oct 2021
Publisher:
CDS
Description:
The complex of star-forming regions in Perseus is one of the most studied due to its proximity (about 300pc). In addition, its regions show variation in star-formation activity and age, with formation of low-mass and intermediate-mass stars. In this paper, we present analyses of images taken with the Herschel ESA satellite from 70 um to 500 um. From these images, we first constructed column density and dust temperature maps. We then identified compact cores in the maps at each wavelength, and characterised the cores using modified blackbody fits to their spectral energy distributions (SEDs): we identified 684 starless cores, of which 199 are bound and potential prestellar cores, and 132 protostars. We also matched the Herschel-identified young stars with GAIA sources to model distance variations across the Perseus cloud. We measure a linear gradient function with right ascension and declination for the entire cloud. This function is the first quantitative attempt to derive the gradient in distance across Perseus, from east to west, in an analytical form. We derived mass and temperature of cores from the SED fits. The core mass function can be modelled with a log-normal distribution that peaks at 0.82M_{sun}_ suggesting a star formation efficiency of 0.30 for a peak in the system initial mass function of stars at 0.25M_{sun}_. The high-mass tail can be modelled with a power law of slope ~-2.32, which is close to the Salpeter's value. We also identify the filamentary structure of Perseus and discuss the relation between filaments and star formation, confirming that stars form preferentially in filaments. We find that the majority of filaments with ongoing star formation are transcritical against their own internal gravity because their linear masses are below the critical limit of 16M_{sun}_/pc above which we expect filaments to collapse. We find a possible explanation for this result, showing that a filament with a linear mass as low as 8 Msun/pc can already be unstable. We confirm a linear relationship between star formation efficiency and the slope of dust probability density function, and we find a similar relationship with the core formation efficiency. We derive a lifetime for the prestellar core phase of 1.69+/-0.52Myr for the whole Perseus complex but different regions have a wide range in prestellar core fractions, suggesting that star formation began only recently in some clumps. We also derive a free-fall time for prestellar cores of 0.16Myr.
1044. Catalogue of eclipsing binaries in the SMC
ID:
ivo://CDS.VizieR/J/MNRAS/331/609
Title:
Catalogue of eclipsing binaries in the SMC
Short Name:
J/MNRAS/331/609
Date:
21 Oct 2021
Publisher:
CDS
Description:
The catalogue lists 167 eclipsing binary stars in the Small Magellanic Cloud detected in the database of time-series photometry for 400000 SMC stars acquired by the Microlensing Observations in Astrophysics (MOA) project during 1997. Coordinates, ephemerides, magnitudes and light curves are presented. Thirty-five systems are new detections. The limiting magnitude is about 17.5. The majority of periods lie within the range 0.4 to 20 days; 6 systems are possibly eccentric while 14 are probably or certainly so. The majority of the newly-identified systems lie in the outer regions of the SMC.
1045. Catalogue of eclipsing variables
ID:
ivo://CDS.VizieR/J/A+A/446/785
Title:
Catalogue of eclipsing variables
Short Name:
J/A+A/446/785
Date:
21 Oct 2021
Publisher:
CDS
Description:
A new catalogue of 6330 eclipsing variable stars is presented. The catalogue was developed from the General Catalogue of Variable Stars (GCVS) and its textual remarks by including recently published information about classification of 843 systems and making corresponding corrections of GCVS data. The catalogue represents the largest list of eclipsing binaries classified from observations.
1046. Catalogue of eclipsing variables. Version 2
ID:
ivo://CDS.VizieR/J/AN/334/860
Title:
Catalogue of eclipsing variables. Version 2
Short Name:
J/AN/334/860
Date:
21 Oct 2021
Publisher:
CDS
Description:
A new version of the Catalogue of Eclipsing Variables is presented. The catalogue contains parameters and morphological types of light curves for some 7200 stars. Spectral classification is also given when available. Recently published information about classification of 1352 systems is included in the catalogue. The catalogue represents the largest list of eclipsing binaries with available classification.
1047. Catalogue of field contact binary stars
ID:
ivo://CDS.VizieR/V/119
Title:
Catalogue of field contact binary stars
Short Name:
V/119
Date:
21 Oct 2021
Publisher:
CDS
Description:
The catalogue of 361 galactic contact binaries is presented. Enlisted contact binaries are divided into five groups according to the type and quality of the available observations and parameters. For all systems the ephemeris for the primary minimum, minimum and maximum visual brightness and equatorial coordinates are given. If available, photometric elements, (M_1_+M_2_)*(sin)i^3^, spectral type, parallax and magnitude of the O'Connell effect are also given. Photometric data for several systems are augmented by new observations. The quality of the available data is assessed and systems requiring modern light-curve solutions are selected. Selected statistical properties of the collected data are discussed.
1048. Catalogue of Galactic high-mass X-ray binaries
ID:
ivo://CDS.VizieR/J/A+A/455/1165
Title:
Catalogue of Galactic high-mass X-ray binaries
Short Name:
J/A+A/455/1165
Date:
21 Oct 2021
Publisher:
CDS
Description:
We present a new edition of the catalogue of high-mass X-ray binaries in the Galaxy. The catalogue contains source name(s), coordinates, finding chart, X-ray luminosity, system parameters, and stellar parameters of the components and other characteristic properties of 114 high-mass X-ray binaries, together with a comprehensive selection of the relevant literature. The aim of this catalogue is to provide the reader with some basic information on the X-ray sources and their counterparts in other wavelength ranges (gamma-rays, UV, optical, IR, radio). About 60% of the high-mass X-ray binary candidates are known or suspected Be/X-ray binaries, while 32% are supergiant/X-ray binaries. Some sources, however, are only tentatively identified as high-mass X-ray binaries on the basis of their X-ray properties similar to the known high-mass X-ray binaries. Further identification in other wavelength bands is needed to finally determine the nature of these sources. In cases where there is some doubt about the high-mass nature of the X-ray binary this is mentioned. Literature published before 1 October 2005 has, as far as possible, been taken into account.
1049. Catalogue of Galactic low-mass X-ray binaries
ID:
ivo://CDS.VizieR/J/A+A/469/807
Title:
Catalogue of Galactic low-mass X-ray binaries
Short Name:
J/A+A/469/807
Date:
21 Oct 2021
Publisher:
CDS
Description:
We present a new edition of the catalogue of the low-mass X-ray binaries in the Galaxy and the Magellanic Clouds. The catalogue contains source name(s), coordinates, finding chart, X-ray luminosity, system parameters, and stellar parameters of the components and other characteristic properties of 187 low-mass X-ray binaries, together with a comprehensive selection of the relevant literature. The aim of this catalogue is to provide the reader with some basic information on the X-ray sources and their counterparts in other wavelength ranges ({gamma}-rays, UV, optical, IR, and radio). Some sources, however, are only tentatively identifed as low-mass X-ray binaries on the basis of their X-ray properties similar to the known low-mass X-ray binaries. Further identification in other wavelength bands is needed to finally determine the nature of these sources. In cases where there is some doubt about the low-mass nature of the X-ray binary this is mentioned. Literature published before 1 October 2006 has, as far as possible, been taken into account.
1050. Catalogue of galaxies observed with Hectospec
ID:
ivo://CDS.VizieR/J/ApJS/256/4
Title:
Catalogue of galaxies observed with Hectospec
Short Name:
J/ApJS/256/4
Date:
03 Dec 2021 00:37:37
Publisher:
CDS
Description:
We present redshifts for 2753 low-redshift (0.05~<z_spec_~<0.5) galaxies with 18<=r<=22 obtained with Hectospec at the Multi-Mirror Telescope (MMT). The observations targeted the XMM-LSS, ELAIS-N1 and DEEP2-3 fields, each of which covers ~1deg^2^. These fields are also part of the recently completed CFHT Large Area U-band Deep Survey (CLAUDS) and on-going Hyper Suprime-Cam deep fields surveys. The efficiency of our technique for selecting low-redshift galaxies is confirmed by the redshift distribution of our sources. In addition to redshifts, these high S/N spectra are used to measure ages, metallicities, and nuclear activity levels. In combination with the photometric catalogue in u, g, r, i, z, y down to 27 AB mag, we are able to study the galaxy population down to stellar masses of ~10^8^M_{sun}_ . This paper presents the observation strategy, the reduction procedure and properties of the galaxy sample. The catalog can be accessed through the webpage of this survey http://mips.as.arizona.edu/~cnaw/Faint_Low_z/.