The Hipparcos and Tycho Photometric System Passbands

By M. Bessell. 2000

175 citations recorded by the source corpus.

Subfields: Atomic and Molecular Physics, and Optics, Cognitive Neuroscience, Radiation

View Paper: https://www.semanticscholar.org/paper/c83d06c0e97e94b862e04374b84f38832ce65df0

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Atomic and Molecular Physics, and Optics

1. Luca Casagrande
2. Eric Mamajek
3. Martin Asplund
4. D. Huber
5. D. Stello
6. I. Ramírez
7. D. VandenBerg
8. A. Miglio

In Cognitive Neuroscience

1. Luca Casagrande
2. Marvin L. Cohen
3. S. Megeath
4. Eric Mamajek
5. M. Meyer
6. W. Wheaton
7. J. Liebert
8. D. Huber

In Radiation

1. Luca Casagrande
2. Marvin L. Cohen
3. S. Megeath
4. Eric Mamajek
5. M. Meyer
6. W. Wheaton
7. J. Liebert
8. D. Huber

Citations in the corpus

• The Gaia–Kepler Stellar Properties Catalog. I. Homogeneous Fundamental Properties for 186,301 Kepler Stars (2020, methodology): “First, we converted Tycho B (BT) and V (VT) photometry into Johnson B and V photometry using the Table 2 from Bessell (2000).”
• The stellar association around Gamma Velorum and its relationship with Vela OB2 (2008, methodology): “These are converted from the conventional BV system to the Tycho system using formulae in Bessell (2000).”
• Gaia broad band photometry (2010, background): “Additional discussion of theHipparcos-Tycho passbands and their relationship with the Johnson system can be found in Bessell (2000).”
• THE SPITZER–WISE SURVEY OF THE ECLIPTIC POLES (2011, methodology): “Following the prescription of Bessell (2000), we convert the QE-based Wright et al. (2010) RSRs from electrons per photon to photon-counting (electrons per erg) response curves, λR(λ), by multiplying by λ and renormalizing each to a peak of unity.”
• Synthetic stellar photometry – I. General considerations and new transformations for broad-band systems (2014, background): “Because of this, one must distinguish between photon-counting (e.g., CCD) and energy-integration (e.g., photo-multiplier) detectors (e.g., Bessell 2000; Maı́z Apellániz 2006; Bessell & Murphy 2012).”
• Post-T Tauri Stars in the Nearest OB Association (2002, methodology): “To convert the Tycho photometry to the Johnson system, we fit low-order polynomials to the data in Table 2 of Bessell (2000) (relations given in Appendix C).”
• FUNDAMENTAL PROPERTIES OF STARS USING ASTEROSEISMOLOGY FROM KEPLER AND CoRoT AND INTERFEROMETRY FROM THE CHARA ARRAY (2012, methodology): “…taken from List of dropped calibrators: HD179395, HD181939, HD182487, HD184875, HD189253; “ID” refers to the ID of the target star for which the calibrator has been used (see column 3 of Table 5). the Tycho catalog and were converted into the Johnson system using the calibration by Bessell (2000).”
• An absolutely calibrated T eff scale from the infrared flux method. Dwarfs and subgiants (2010, methodology): “As for the Johnson-Cousins system, we based the absolute calibration of the Tycho2 system on Vega (Bohlin & Gilliland 2004; Bohlin 2007), adopting theBT VT zero points of Maı́z-Apellániz (2007) and the corresponding filter transmission curves of Bessell (2000).”
• Spectral Irradiance Calibration in the Infrared. XIV. The Absolute Calibration of 2MASS (2003, methodology): “The quantum efficiency–based component was converted to yield photon-counting RSRs 5 See http://www2.bc.edu/~sullivab/soft/plexus.html#Desc. by multiplying by and renormalizing, exactly as described by Bessell (2000).6 3.1.”
• THE K2 ECLIPTIC PLANE INPUT CATALOG (EPIC) AND STELLAR CLASSIFICATIONS OF 138,600 TARGETS IN CAMPAIGNS 1–8 (2015, methodology): “To ensure some homogeneity, the following quality cuts and transformations were applied to the observables: • Tycho-2: BT and VT photometry were converted into the Johnson BV by interpolating Table 2 in Bessell (2000).”
• Spectral Irradiance Calibration in the Infrared. XIII. “Supertemplates” and On-Orbit Calibrators for the SIRTF Infrared Array Camera (2003, background): “Bessell(2000)has discussed theproblem sand inadequacy ofthepublished inform ation thataccom paniesthe system response curvesofthe two Tycho bands(B T,VT)and the single Hipparcosband (H p)given in Volum eIoftheHipparcosarchivalvolum es(ESA 1997).”
• Spectroscopic parameters for 451 stars in the HARPS GTO planet search program - Stellar [Fe/H] and the frequency of exo-Neptunes (2008, methodology): “We also checked that ifHipparcos TychoBT VT magnitudes, transformed onto the Johnson system (Bessell 2000), were used instead that the differences in our results would be negligible.”
• Properties of planets in binary systems - The role of binary separation (2006, background): “The Hipparcos magnitude of the secondary transformed to the standard system following Bessell (2000) yields V = 10.76, about 2.5 mag fainter than the primary (V = 8.09, Fischer et al. 2006; see Table A.2).”
• Stellar Kinematic Groups. II. A Reexamination of the Membership, Activity, and Age of the Ursa Major Group (2003, methodology): “Their VT magnitudes and BT VT colors were transformed to Johnson V and B V by using the relations from Bessell (2000).”
• Characterization of Dusty Debris Disks: The IRAS and Hipparcos Catalogs (2006, methodology): “The standard B and V magnitudes were obtained by converting Tycho B and V magnitudes using Table 2 in Bessell (2000).”