ARC 3.5m: Standard Stars

ARC 3.5m | Standard Stars

Bright Star Catalog - broken into smaller files for easier management by TUI:

BSC_A_V0-2	BSC_RA_0-1	BSC_RA_12-13	BSC_A_V3-4
BSC_G_V3-4	BSC_RA_1-2	BSC_RA_13-14	BSC_A_V5-6
BSC_G_V5-6	BSC_RA_2-3	BSC_RA_14-15	BSC_B_V0-2
BSC_K_V0-2	BSC_RA_3-4	BSC_RA_15-16	BSC_B_V3
BSC_K_V3	BSC_RA_4-5	BSC_RA_16-17	BSC_B_V4
BSC_K_V4	BSC_RA_5-6	BSC_RA_17-18	BSC_B_V5-6
BSC_K_V5-6	BSC_RA_6-7	BSC_RA_18-19	BSC_F_V0-2
BSC_M_V0-3	BSC_RA_7-8	BSC_RA_19-20	BSC_F_V3
BSC_M_V4	BSC_RA_8-9	BSC_RA_20-21	BSC_F_V4
BSC_M_V5-6	BSC_RA_9-10	BSC_RA_21-22	BSC_F_V5-6
BSC_O_V0-6	BSC_RA_10-11	BSC_RA_22-23	BSC_G_V0-2
BSC_Other	BSC_RA_11-12	BSC_RA_23-24

Double Star Catalog

Johnson Catalog

Landolt Catalog - broken into smaller files for easier management by TUI:

Landolt_RA_0-4	Landolt_RA_8-12	Landolt_RA_16-20
Landolt_RA_4-8	Landolt_RA_12-16	Landolt_RA_20-24

Various Standard Star Links and associated TUI Catalogs

RA ordered list from ESO. Data from which the plots were produced are also available by ftp access from the standard star pages.- specstds.tui
HST UV spectrophotometric standards. Data for 23 stars based on IUE and optical spectra and calibrated by the primary WD standards. Also data on 6 more stars with IUE and model spectra - hststds.tui
Optical spectrophotometric standards from Oke (1990). Data for 25 stars (7 to 16 mag.) from 3200 to 10200A based on Hale 5m observations - okestds.tui
White Dwarf primary spectrophotometric standards. Data archive tools at STScI - wdstds.tui
Optical spectrophotometric standards from Hamuy (1992, 1994). Data for 10 bright secondary standards and 19 fainter (10 to 14 mag.) tertiary standards over the wavelength range 3300 to about 10300A, mostly in the southern hemisphere, taken with CTIO telescopes - hamuystds.tui
Echelle Standards - echstds.tui

A.U. Landolt's standards are also available from his paper 1992 AJ 104,340.

Some of the finding charts were produced from the Digitized Sky Survey produced by STScI and based on plate material from the UK Schmidt Telescope and the Oschin Schmidt Telescope.