Synphot Data User's Guide
A.4 The Stellar Spectral Flux Library by Pickles 1998
This library of wide spectral coverage, consists of 131 flux calibrated stellar spectra, encompassing all normal spectral types and luminosity classes at solar abundance, and metal-weak and metal-rich F-K dwarf and G-K giant components. Each spectrum in the library is a combination of several sources overlapping in wavelength coverage. Pickles has followed precise criteria to combine sources and to assemble the most reliable spectra. As part of the selection criteria prior to combination, all input sources were checked against the SIMBAD database and against the colors and line strengths as derived by the observed spectra themselves to make sure they had similar spectral types. As a result, this library provides an uniform and complete flux library of observed spectra representing normal stellar types over an uniform grid.
In the following, the list of the above mentioned input sources is given, numbered following Table 1 in the original paper.
- Sviderskiene (1988, Bull. Vilna. Astron. Obs. 80, 1)
- Heck et al. (1984, ESA SP-1052)
- Gunn and Stryker (1983, ApJS 52, 121)
- Kiehling (1987, A&A 69, 465)
- Jacobi, Hunter and Christian (1984, ApJS 56, 257)
- Silva and Cornell (1992, ApJS 81, 865)
- Pickles (1985, ApJS 59, 33)
- Pickles and van der Kruit (1990, A&A 84,421)
- Serote Roos, Boisson and Joly (1996, A&A 117, 93)
- Danks and Dennefeld (1994, PASP 106, 382)
- Lancon and Rocca-Volmerange (1992, A&A 96, 593)
- Dallier, Boisson and Joly (1996, A&A 116, 239)
- Kleinmann and Hall (1986, ApJS 62, 501)
- Cohen et al. (1995, 1996a, 1996b, AJ 110, 275; AJ 112, 241; AJ 112, 2274)
- Fluks et al. (1994, A&AS 105, 311)
Table A.8 of Pickles (1998) precisely identifies what of the above sources entered the combination to create the complete set of spectral types. The output wavelength grid was chosen to be 1150-25000 Angstrom, with a sampling interval of 5 Angstrom per pixel and resolution of ~500 Angstrom. In the end, two separate libraries were created, UVILIB and UVKLIB, that cover the spectral range 1150-10620 Angstrom, and 1150-25000 Angstrom, respectively. In fact, only half of all spectral types in the library (mainly later types of solar abundance) have longer spectral coverages available.
Table A.8 gives an idea of the spectra available. Spectra are ordered by progressive number, according to the spectral type (decreasing effective temperature) and luminosity class. The same ordering sequence is valid for both the UVILIB and the UVKLIB libraries, where the suffix "uk" differentiates between two spectra of the same spectral type but with different wavelength coverage (as described in the next section).
Table A.8: Pickles Library Spectra:
Spectrum ID no. Spectral Type and Luminosity Class 1-45 O5-M6 V 46-59 B2-K3 IV 60-105 O8-M10 III 106-113 B2-M3 II 114-131 B0-M2 I
A.4.1 The HST/CDBS Version of the Pickles Library
The library installed in CDBS and distributed within STSDAS was obtained from
http://cdsarc.u-strasbg.fr/viz-bin/ftp-index?J/PASP/110/863. This library is divided in 2 independent subdirectories, according to spectral coverage, and exactly reproducing the structure of the original library by Pickles. Subdirectory dat_uvi groups all spectra derived from all ultraviolet, optical and near infrared sources, in the wavelength range 1150-10620 Angstrom. This library has complete spectral coverage for all components over this wavelength range, and is (in the original library) referred to as UVILIB. Subdirectory dat_uvk groups all spectra that were derived by combining the UVILIB spectra with additional infrared data to a long wavelength limit of 25000 Angstrom. This is originally referred to as UVKLIB. Within each subdirectory each spectrum is given in FITS table format: the first column gives the wavelength for the given spectral range, and the second column gives the flux. Fluxes are tabulated in units of
erg s-1cm-2Å-1 and were calculated by normalizing the original fluxes in the Pickles V band to a 0 magnitude in vegamag. In the vegamag system, Vega has magnitude zero in all passbands.
For the UVILIB spectra, the names of the files are given as pickles_ttt.fits where "pickles", for Pickles, is the library identifier and "ttt" is a number ranging from 1 to 131. For the UVKLIB spectra, the names have the format pickles_uk_ttt.fits, following the same nomenclature, and with the suffix "uk" provided as to distinguish them from the shorter wavelength library.
The complete list of stars of different spectral type and luminosity class together with the corresponding Pickles file is presented in Table A.9. The effective temperature information is extracted from Table 2 of Pickles (1998). A "w" or an "r" preceding the spectral type indicates a "weak" or "rich" metallicity in respect to solar.
Table A.9: Spectral Type and Effective Temperature Corresponding to the Pickles Spectra in the Library.
FILENAME SPTYPE(K) EFF TEMP. pickles_uk_1 O5V 39810.7 pickles_uk_2 O9V 35481.4 pickles_uk_3 B0V 28183.8 pickles_uk_4 B1V 22387.2 pickles_uk_5 B3V 19054.6 pickles_uk_6 B5-7V 14125.4 pickles_uk_7 B8V 11749.0 pickles_uk_9 A0V 9549.93 pickles_uk_10 A2V 8912.51 pickles_uk_11 A3V 8790.23 pickles_uk_12 A5V 8491.80 pickles_uk_14 F0V 7211.08 pickles_uk_15 F2V 6776.42 pickles_uk_16 F5V 6531.31 pickles_uk_20 F8V 6039.48 pickles_uk_23 G0V 5807.64 pickles_uk_26 G2V 5636.38 pickles_uk_27 G5V 5584.70 pickles_uk_30 G8V 5333.35 pickles_uk_31 K0V 5188.00 pickles_uk_33 K2V 4886.52 pickles_uk_36 K5V 4187.94 pickles_uk_37 K7V 3999.45 pickles_uk_38 M0V 3801.89 pickles_uk_40 M2V 3548.13 pickles_uk_43 M4V 3111.72 pickles_uk_44 M5V 2951.21 pickles_uk_46 B2IV 19952.6 pickles_uk_47 B6IV 12589.3 pickles_uk_48 A0IV 9727.47 pickles_uk_49 A4-7IV 7943.28 pickles_uk_50 F0-2IV 7030.72 pickles_uk_51 F5IV 6561.45 pickles_uk_52 F8IV 6151.77 pickles_uk_53 G0IV 5929.25 pickles_uk_54 G2IV 5688.53 pickles_uk_55 G5IV 5597.57 pickles_uk_56 G8IV 5308.84 pickles_uk_57 K0IV 5011.87 pickles_uk_58 K1IV 4786.30 pickles_uk_59 K3IV 4570.88 pickles_uk_60 O8III 31622.8 pickles_uk_61 B1-2III 19952.6 pickles_uk_63 B5III 14791.1 pickles_uk_64 B9III 11091.8 pickles_uk_65 A0III 9571.94 pickles_uk_67 A5III 8452.79 pickles_uk_69 F0III 7585.78 pickles_uk_71 F5III 6531.31 pickles_uk_72 G0III 5610.48 pickles_uk_73 G5III 5164.16 pickles_uk_76 G8III 5011.87 pickles_uk_78 K0III 4852.89 pickles_uk_87 K3III 4365.16 pickles_uk_93 K5III 4008.67 pickles_uk_95 M0III 3819.44 pickles_uk_100 M5III 3419.79 pickles_uk_105 M10III 2500.35 pickles_uk_106 B2II 15995.6 pickles_uk_107 B5II 12589.3 pickles_uk_108 F0II 7943.28 pickles_uk_109 F2II 7328.25 pickles_uk_110 G5II 5248.07 pickles_uk_111 K0-1II 5011.87 pickles_uk_112 K3-4II 4255.98 pickles_uk_113 M3II 3411.93 pickles_uk_114 B0I 26001.6 pickles_uk_117 B5I 13396.8 pickles_uk_118 B8I 11194.4 pickles_uk_119 A0I 9727.47 pickles_uk_121 F0I 7691.30 pickles_uk_122 F5I 6637.43 pickles_uk_123 F8I 6095.37 pickles_uk_124 G0I 5508.08 pickles_uk_126 G5I 5046.61 pickles_uk_127 G8I 4591.98 pickles_uk_128 K2I 4255.98 pickles_uk_130 K4I 3990.25 pickles_uk_131 M2I 3451.44
A similar list applies for the UKVKLIB library. For these spectra the names have the format "pickles_uk_ttt.fits". A reduced form of Table A.9 can also be found in the library installed in CDBS and is named pickles.fits for the spectra in dat_uvi, and pickles_uk.fits for the spectra in dat_uvk directory. A "w" or an "r" preceding the spectral type indicates a "weak" or "rich" metallicity in respect to solar.
A.4.2 Use of the Pickles Library with Synphot
Use of these spectra should be exactly similar to other libraries already available in synphot. The desired spectrum is provided in input in any of the synphot tasks as appropriate with no particular syntax.
Table A.10 is an example of a standard header file for the spectrum pickles_uk_51.fits. This spectrum corresponds to a star of spectral type F5IV and covers a range in wavelength of 1150 to 25000 Angstrom as can be assumed by the suffix "uk", which indicates a spectrum of the UVKLIB library.
Table A.10: Header for fits file pickles_uk_51.fits.
The fluxes were extracted from the original paper and were normalized to V=0 in the Pickles' V band. In this way the spectra were provided in a synphot-friendly format and in the usual units of erg s-1 cm-2Å-1.
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