J/A+AS/129/505 Effective temperatures by Infrared Flux Method (Blackwell+ 1998)
Determination of the temperatures of selected ISO flux calibration stars
using the Infrared Flux Method
Blackwell D.E., Lynas-Gray A.E.
<Astron. Astrophys. Suppl. Ser. 129, 505 (1998)>
=1998A&AS..129..505B 1998A&AS..129..505B
ADC_Keywords: Effective temperatures ; Photometry, infrared
Keywords: stars: fundamental parameters - temperatures
Abstract:
Effective temperatures for 420 stars with spectral types between A0
and K3, and luminosity classes between II and V, selected for a flux
calibration of the Infrared Space Observatory, ISO, have been
determined using the Infrared Flux Method (IRFM). The determinations
are based on narrow and wide band photometric data obtained for this
purpose, and take into account previously published narrow-band
measures of temperature.
File Summary:
--------------------------------------------------------------------------------
FileName Lrecl Records Explanations
--------------------------------------------------------------------------------
ReadMe 80 . This file
table1.dat 27 420 Total fluxes and derived temperatures for ISO Stars
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table1.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 6 I6 --- HD HD number
8- 16 E9.3 W/m2 Flux Integrated stellar flux, corrected from
interstellar absorption.
18- 21 I4 K Teff Derived stellar effective temperature
23 A1 --- r_Flux [AB] Source of infrared data (1)
25- 27 F3.1 % e_Teff Estimated probable errors of derived temperatures
--------------------------------------------------------------------------------
Note (1): The sources are:
A = Telescopio Carlos Sanchez (TCS) data
B = ESO data
--------------------------------------------------------------------------------
History:
* 11-Aug-1998: from A&AS electronic version
* 30-Jun-2011: the "Flux" column, claimed to be expressed in nW/m2
in the paper, was fixed to W/m2.
(End) Patricia Bauer [CDS] 11-Aug-1998