A cross-calibration between Tycho-2 photometry and HST spectrophotometry
arXiv:astro-ph/0504085 · doi:10.1086/430370
Abstract
I show that Tycho-2 photometry and HST spectrophotometry are accurate and stable enough to obtain a precise cross-calibration by analyzing a well-calibrated sample of 256 stars observed with both Hipparcos and HST. Based on this analysis, I obtain the following photometric zero points in the Vega magnitude system for Tycho-2: 0.020+-0.001 (B_T-V_T), 0.078+-0.009 (B_T), and 0.058+-0.009 (V_T).
arXiv comment11 pages, 4 figures, to appear in Publications of the Astronomical Society of the Pacific (June 2005 issue)
References in corpus (2)
Cited by in corpus (15)
- A reanalysis of the Gaia Data Release 2 photometric sensitivity curves using HST/STIS spectrophotometry
- A recalibration of optical photometry: Tycho-2, Strömgren, and Johnson systems
- The VLT-FLAMES Tarantula Survey XVI. The optical+NIR extinction laws in 30 Doradus and the photometric determination of the effective temperatures of OB stars
- The chemical abundance analysis of normal early A- and late B-type stars
- Optical-NIR dust extinction towards Galactic O stars
- Measurement of the Cosmic Optical Background using the Long Range Reconnaissance Imager on New Horizons
- Orbital and physical properties of the Ori Aa,Ab,B triple system
- Galactic extinction laws: I. A global NIR analysis with 2MASS photometry
- Gaia-ESO Survey: global properties of clusters Trumpler 14 and 16 in the Carina Nebula
- VdBH 222: a starburst cluster in the inner Milky Way
- Calibration of the photometric G passband for Gaia Data Release 1
- A reevaluation of the 2MASS zero points using CALSPEC spectrophotometry complemented with Gaia Data Release 2 parallaxes
- A Method to Measure Photometries of Moderately-Saturated UVOT Sources
- An in-depth analysis of the differentially expanding star cluster Stock 18 (Villafranca O-036) using Gaia DR3 and ground-based data
- Cross-Calibration of SMART-1 XSM with GOES and RHESSI