Access to Astronomical Catalogues

Search catalogue
obsoleted
in preparation
catalog without ftp or VizieR link
J/PASP/118/1690     Spitzer solar-type stars list            (Meyer+, 2006)

The formation and evolution of planetary systems: placing our solar system in context with Spitzer. Meyer M.R., Hillenbrand L.A., Backman D., Beckwith S., Bouwman J., Brooke T., Carpenter J., Cohen M., Cortes S., Crockett N., Gorti U., Henning T., Hines D., Hollenbach D., Kim J.S., Lunine J., Malhotra R., Mamajek E., Metchev S., Moro-Martin A., Morris P., Najita J., Padgett D., Pascucci I., Rodmann J., Schlingman W., Silverstone M., Soderblom D., Stauffer J., Stobie E., Strom S., Watson D., Weidenschilling S., Wolf S., Young E. <Publ. Astron. Soc. Pac., 118, 1690-1710 (2006)> =2006PASP..118.1690M
ADC_Keywords: Stars, G-type ; Spectral types Abstract: We provide an overview of the Spitzer Legacy Program, Formation and Evolution of Planetary Systems, that was proposed in 2000, begun in 2001, and executed aboard the Spitzer Space Telescope between 2003 and 2006. This program exploits the sensitivity of Spitzer to carry out mid-infrared spectrophotometric observations of solar-type stars. With a sample of 328 stars ranging in age from 3Myr to 3Gyr, we trace the evolution of circumstellar gas and dust from primordial planet-building stages in young circumstellar disks through to older collisionally generated debris disks. When completed, our program will help define the timescales over which terrestrial and gas giant planets are built, constrain the frequency of planetesimal collisions as a function of time, and establish the diversity of mature planetary architectures. In addition to the observational program, we have coordinated a concomitant theoretical effort aimed at understanding the dynamics of circumstellar dust with and without the effects of embedded planets, dust spectral energy distributions, and atomic and molecular gas line emission. Together with the observations, these efforts will provide an astronomical context for understanding whether our solar system and its habitable planets a common or a rare circumstance. Additional information about the FEPS project can be found on the team Web site. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 71 124 Field stars table2.dat 71 60 Open cluster stars table3.dat 71 130 Young Stars table4.dat 71 14 Pre-selected IRS High-Resolution Targets
Byte-by-byte Description of file: table*.dat
Bytes Format Units Label Explanations
1- 23 A23 --- Name Star name 24 A1 --- n_Name [abc] Note on Name (1) 26- 27 I2 h RAh Right ascension (J2000.0) 29- 30 I2 min RAm Right ascension (J2000.0) 32- 36 F5.2 s RAs Right ascension (J2000.0) 38 A1 --- DE- Declination sign (J2000.0) 39- 40 I2 deg DEd Declination sign (J2000.0) 42- 43 I2 arcmin DEm Declination sign (J2000.0) 45- 49 F5.2 arcsec DEs Declination sign (J2000.0) 51- 61 A11 --- SpType MK spectral type 63- 71 A9 --- Cluster Open Cluster name (for table2)
Note (1): Notes as follows: a = IRS high-resolution spectra were also obtained for these stars. b = These stars are also Spitzer Space Telescope calibration targets c = IRS high-resolution spectra were not obtained for these sources, due to program constraints
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 11-Jan-2008
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

catalogue service

© UDS/CNRS

Contact