III/39A UV Bright Star Spectrophotometric Catalog (Jamar+, 1976)
Ultraviolet Bright Stars Spectrophotometric CATalogue
Jamar C., Macau-Hercot D., Monfils A., Thompson G.I.,
Houziaux L., Wilson R.
ADC_Keywords: Spectra, ultraviolet ; Spectrophotometry ; Stars, bright
Mission_Name: TD1
Description:
This catalogue contains observations carried out by the S2/68
Ultraviolet Sky Survey Telescope (UVSST) aboard the ESRO Satellite
TD-1, which measured the absolute ultraviolet flux distribution
between 2740A (274nm) and 1350A (135nm). The data presented in this
catalogue were obtained during the first observation period, which
lasted from 19 March 1972 to 31 October 1972, and contains the
brightest objects, for which the signal is good enough to give
valuable spectrophotometric information. The Faint Star Catalogue,
which contains the photometric data of the stars up to the limit of
detectability of the instrument, is known as the "Catalogue of
Ultraviolet Fluxes", by Thompson et al. (catalog II/59)
The S2/68 experiment has been described by Boksenberg et al.
(=1973MNRAS.163..291B 1973MNRAS.163..291B) and the absolute calibration by Humphries et
al. (=1976A&A....49..389H 1976A&A....49..389H).
See also:
II/59 : Catalogue of stellar UV fluxes (TD1) (Thompson+ 1978)
II/86 : Supplement to the UVBS Photometric Catalogue
II/91 : The Intrinsic Colours of stars in the U.V. (Carnochan 1982)
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
catalog.dat 659 1356 The spectrophotometric Catalogue
adc.txt 80 733 Documentation of the original catalog by
Theresa A. Nagy and Robert S. Hill
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Byte-by-byte Description of file: catalog.dat
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Bytes Format Units Label Explanations
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1- 4 I4 --- UVBS [1/1356] UV Bright Star number
5- 10 I6 --- HD [1/225300] Henry Draper Catalog (HD) number
11- 13 I3 --- Nsp [1/194] Number of spectra averaged
14- 19 F6.2 pW/m2/nm F1360 Flux at 1360Å (10-10erg/cm2/s/Å)
20- 25 F6.2 pW/m2/nm F1380 Flux at 1380Å (10-10erg/cm2/s/Å)
26- 31 F6.2 pW/m2/nm F1400 Flux at 1400Å (10-10erg/cm2/s/Å)
32- 37 F6.2 pW/m2/nm F1420 Flux at 1420Å (10-10erg/cm2/s/Å)
38- 43 F6.2 pW/m2/nm F1440 Flux at 1440Å (10-10erg/cm2/s/Å)
44- 49 F6.2 pW/m2/nm F1460 Flux at 1460Å (10-10erg/cm2/s/Å)
50- 55 F6.2 pW/m2/nm F1480 Flux at 1480Å (10-10erg/cm2/s/Å)
56- 61 F6.2 pW/m2/nm F1500 Flux at 1500Å (10-10erg/cm2/s/Å)
62- 67 F6.2 pW/m2/nm F1520 Flux at 1520Å (10-10erg/cm2/s/Å)
68- 73 F6.2 pW/m2/nm F1540 Flux at 1540Å (10-10erg/cm2/s/Å)
74- 79 F6.2 pW/m2/nm F1560 Flux at 1560Å (10-10erg/cm2/s/Å)
80- 85 F6.2 pW/m2/nm F1580 Flux at 1580Å (10-10erg/cm2/s/Å)
86- 91 F6.2 pW/m2/nm F1600 Flux at 1600Å (10-10erg/cm2/s/Å)
92- 97 F6.2 pW/m2/nm F1620 Flux at 1620Å (10-10erg/cm2/s/Å)
98-103 F6.2 pW/m2/nm F1640 Flux at 1640Å (10-10erg/cm2/s/Å)
104-109 F6.2 pW/m2/nm F1660 Flux at 1660Å (10-10erg/cm2/s/Å)
110-115 F6.2 pW/m2/nm F1680 Flux at 1680Å (10-10erg/cm2/s/Å)
116-121 F6.2 pW/m2/nm F1700 Flux at 1700Å (10-10erg/cm2/s/Å)
122-127 F6.2 pW/m2/nm F1720 Flux at 1720Å (10-10erg/cm2/s/Å)
128-133 F6.2 pW/m2/nm F1740 Flux at 1740Å (10-10erg/cm2/s/Å)
134-139 F6.2 pW/m2/nm F1760 Flux at 1760Å (10-10erg/cm2/s/Å)
140-145 F6.2 pW/m2/nm F1780 Flux at 1780Å (10-10erg/cm2/s/Å)
146-151 F6.2 pW/m2/nm F1800 Flux at 1800Å (10-10erg/cm2/s/Å)
152-157 F6.2 pW/m2/nm F1820 Flux at 1820Å (10-10erg/cm2/s/Å)
158-163 F6.2 pW/m2/nm F1840 Flux at 1840Å (10-10erg/cm2/s/Å)
164-169 F6.2 pW/m2/nm F1860 Flux at 1860Å (10-10erg/cm2/s/Å)
170-175 F6.2 pW/m2/nm F1880 Flux at 1880Å (10-10erg/cm2/s/Å)
176-181 F6.2 pW/m2/nm F1900 Flux at 1900Å (10-10erg/cm2/s/Å)
182-187 F6.2 pW/m2/nm F1920 Flux at 1920Å (10-10erg/cm2/s/Å)
188-193 F6.2 pW/m2/nm F1940 Flux at 1940Å (10-10erg/cm2/s/Å)
194-199 F6.2 pW/m2/nm F1960 Flux at 1960Å (10-10erg/cm2/s/Å)
200-205 F6.2 pW/m2/nm F1980 Flux at 1980Å (10-10erg/cm2/s/Å)
206-211 F6.2 pW/m2/nm F2000 Flux at 2000Å (10-10erg/cm2/s/Å)
212-217 F6.2 pW/m2/nm F2020 Flux at 2020Å (10-10erg/cm2/s/Å)
218-223 F6.2 pW/m2/nm F2040 Flux at 2040Å (10-10erg/cm2/s/Å)
224-229 F6.2 pW/m2/nm F2060 Flux at 2060Å (10-10erg/cm2/s/Å)
230-235 F6.2 pW/m2/nm F2080 Flux at 2080Å (10-10erg/cm2/s/Å)
236-241 F6.2 pW/m2/nm F2100 Flux at 2100Å (10-10erg/cm2/s/Å)
242-247 F6.2 pW/m2/nm F2120 Flux at 2120Å (10-10erg/cm2/s/Å)
248-253 F6.2 pW/m2/nm F2140 Flux at 2140Å (10-10erg/cm2/s/Å)
254-259 F6.2 pW/m2/nm F2160 Flux at 2160Å (10-10erg/cm2/s/Å)
260-265 F6.2 pW/m2/nm F2180 Flux at 2180Å (10-10erg/cm2/s/Å)
266-271 F6.2 pW/m2/nm F2200 Flux at 2200Å (10-10erg/cm2/s/Å)
272-277 F6.2 pW/m2/nm F2220 Flux at 2220Å (10-10erg/cm2/s/Å)
278-283 F6.2 pW/m2/nm F2240 Flux at 2240Å (10-10erg/cm2/s/Å)
284-289 F6.2 pW/m2/nm F2260 Flux at 2260Å (10-10erg/cm2/s/Å)
290-295 F6.2 pW/m2/nm F2280 Flux at 2280Å (10-10erg/cm2/s/Å)
296-301 F6.2 pW/m2/nm F2300 Flux at 2300Å (10-10erg/cm2/s/Å)
302-307 F6.2 pW/m2/nm F2320 Flux at 2320Å (10-10erg/cm2/s/Å)
308-313 F6.2 pW/m2/nm F2340 Flux at 2340Å (10-10erg/cm2/s/Å)
314-319 F6.2 pW/m2/nm F2360 Flux at 2360Å (10-10erg/cm2/s/Å)
320-325 F6.2 pW/m2/nm F2380 Flux at 2380Å (10-10erg/cm2/s/Å)
326-331 F6.2 pW/m2/nm F2400 Flux at 2400Å (10-10erg/cm2/s/Å)
332-337 F6.2 pW/m2/nm F2420 Flux at 2420Å (10-10erg/cm2/s/Å)
338-343 F6.2 pW/m2/nm F2440 Flux at 2440Å (10-10erg/cm2/s/Å)
344-349 F6.2 pW/m2/nm F2460 Flux at 2460Å (10-10erg/cm2/s/Å)
350-355 F6.2 pW/m2/nm F2480 Flux at 2480Å (10-10erg/cm2/s/Å)
356-361 F6.2 pW/m2/nm F2500 Flux at 2500Å (10-10erg/cm2/s/Å)
362-367 F6.2 pW/m2/nm F2520 Flux at 2520Å (10-10erg/cm2/s/Å)
368-373 F6.2 pW/m2/nm F2540 Flux at 2540Å (10-10erg/cm2/s/Å)
374-379 F6.2 pW/m2/nm F2740 Flux at 2740Å (10-10erg/cm2/s/Å)
380-382 I3 % e_F1360 RMS deviation of F1360 (1)
383-385 I3 % e_F1380 RMS deviation of F1380 (1)
386-388 I3 % e_F1400 RMS deviation of F1400 (1)
389-391 I3 % e_F1420 RMS deviation of F1420 (1)
392-394 I3 % e_F1440 RMS deviation of F1440 (1)
395-397 I3 % e_F1460 RMS deviation of F1460 (1)
398-400 I3 % e_F1480 RMS deviation of F1480 (1)
401-403 I3 % e_F1500 RMS deviation of F1500 (1)
404-406 I3 % e_F1520 RMS deviation of F1520 (1)
407-409 I3 % e_F1540 RMS deviation of F1540 (1)
410-412 I3 % e_F1560 RMS deviation of F1560 (1)
413-415 I3 % e_F1580 RMS deviation of F1580 (1)
416-418 I3 % e_F1600 RMS deviation of F1600 (1)
419-421 I3 % e_F1620 RMS deviation of F1620 (1)
422-424 I3 % e_F1640 RMS deviation of F1640 (1)
425-427 I3 % e_F1660 RMS deviation of F1660 (1)
428-430 I3 % e_F1680 RMS deviation of F1680 (1)
431-433 I3 % e_F1700 RMS deviation of F1700 (1)
434-436 I3 % e_F1720 RMS deviation of F1720 (1)
437-439 I3 % e_F1740 RMS deviation of F1740 (1)
440-442 I3 % e_F1760 RMS deviation of F1760 (1)
443-445 I3 % e_F1780 RMS deviation of F1780 (1)
446-448 I3 % e_F1800 RMS deviation of F1800 (1)
449-451 I3 % e_F1820 RMS deviation of F1820 (1)
452-454 I3 % e_F1840 RMS deviation of F1840 (1)
455-457 I3 % e_F1860 RMS deviation of F1860 (1)
458-460 I3 % e_F1880 RMS deviation of F1880 (1)
461-463 I3 % e_F1900 RMS deviation of F1900 (1)
464-466 I3 % e_F1920 RMS deviation of F1920 (1)
467-469 I3 % e_F1940 RMS deviation of F1940 (1)
470-472 I3 % e_F1960 RMS deviation of F1960 (1)
473-475 I3 % e_F1980 RMS deviation of F1980 (1)
476-478 I3 % e_F2000 RMS deviation of F2000 (1)
479-481 I3 % e_F2020 RMS deviation of F2020 (1)
482-484 I3 % e_F2040 RMS deviation of F2040 (1)
485-487 I3 % e_F2060 RMS deviation of F2060 (1)
488-490 I3 % e_F2080 RMS deviation of F2080 (1)
491-493 I3 % e_F2100 RMS deviation of F2100 (1)
494-496 I3 % e_F2120 RMS deviation of F2120 (1)
497-499 I3 % e_F2140 RMS deviation of F2140 (1)
500-502 I3 % e_F2160 RMS deviation of F2160 (1)
503-505 I3 % e_F2180 RMS deviation of F2180 (1)
506-508 I3 % e_F2200 RMS deviation of F2200 (1)
509-511 I3 % e_F2220 RMS deviation of F2220 (1)
512-514 I3 % e_F2240 RMS deviation of F2240 (1)
515-517 I3 % e_F2260 RMS deviation of F2260 (1)
518-520 I3 % e_F2280 RMS deviation of F2280 (1)
521-523 I3 % e_F2300 RMS deviation of F2300 (1)
524-526 I3 % e_F2320 RMS deviation of F2320 (1)
527-529 I3 % e_F2340 RMS deviation of F2340 (1)
530-532 I3 % e_F2360 RMS deviation of F2360 (1)
533-535 I3 % e_F2380 RMS deviation of F2380 (1)
536-538 I3 % e_F2400 RMS deviation of F2400 (1)
539-541 I3 % e_F2420 RMS deviation of F2420 (1)
542-544 I3 % e_F2440 RMS deviation of F2440 (1)
545-547 I3 % e_F2460 RMS deviation of F2460 (1)
548-550 I3 % e_F2480 RMS deviation of F2480 (1)
551-553 I3 % e_F2500 RMS deviation of F2500 (1)
554-556 I3 % e_F2520 RMS deviation of F2520 (1)
557-559 I3 % e_F2540 RMS deviation of F2540 (1)
560-562 I3 % e_F2740 RMS deviation of F2740 (1)
563-568 I6 --- HD2 Henry Draper Catalog (HD) number (repeated)
569-572 A4 --- m_HD2 Additional HD IDs (given as '/n')
573-575 I3 --- Flamsteed [1/140]? Flamsteed number prefix
576-577 A2 --- VarName Variable star letter designation
578-579 I2 --- Greek [1/24]? Greek letter coded as alpha
580 I1 --- GreekSup []? Greek letter superscript
581-582 A2 --- m_GreekSup [/2] Second component
583-585 A3 --- Const Constellation abbreviation
587-588 I2 h RAh Hours RA, B2000.0
590-593 F4.1 min RAm Minutes RA, B2000.0
595 A1 --- DE- Sign Dec, B2000.0
596-597 I2 deg DEd Degrees Dec, B2000.0
599-600 I2 arcmin DEm Minutes Dec, B2000.0
602-606 A5 --- SpType Spectral type (temperature)
608-619 A12 --- LClass Luminosity class information
620-624 F5.2 mag Vmag V magnitude in the UBV system
625 A1 --- VarFlag [V] 'V' if star confirmed to be variable
626 A1 --- n_Vmag '*' if V from HR, HD or SAO catalogues
627-631 F5.2 mag B-V B-V color in the UBV system
633-637 F5.2 mag U-B U-B color in the UBV system
639-642 F4.2 mag E(B-V) B-V color excess, E(B-V)
643 A1 --- n_E(B-V) [*] '*' if E(B-V) extrapolated
(see adc.txt)
645-647 I3 km/s v.sini ?=999 Projected rotational velocity (v sin i)
649-659 A11 --- Refs Coded reference numbers (see adc.txt)
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Note (1): RMS deviations of the observations (fields named 'e_Fnnnn')
are given as a percentage:
(100/) * SQRT[SUM((Fi-)2)/(n-1)]
where
Fi = the individual flux at wavelength λ
= the average flux at wavelength λ
n = the number of averaged observations (field Spectra)
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Historical Notes:
* Catalogue originally prepared by the author (C. Jamar) and supplied
to CDS in March 1977.
* From the "Selected Astronomical Catalogs" Vol. 1 CD-ROM (1992),
directory /spectro/uvbs.
* 03-Jan-1995: a few errors corrected for UVBS:
929 (U-B value)
1019 (misalignment of Greek letter)
1039 (E(B-V) value)
1040 (E(B-V) value)
1170 (misalignment of Greek letter)
* 09-Mar-2013: Flux units corrected (werer set at 10-14W/m2/nm
instead of 10-12W/m2/nm)
(End) Francois Ochsenbein [CDS] 03-Jan-1995