J/A+A/558/A12       M5 (NGC5904) UBVRI photometry                 (Viaux+, 2013)

Particle-physics constraints from the globular cluster M5: neutrino dipole moments. Viaux N., Catelan M., Stetson P., Raffelt G., Redondo J., Valcarce A., Weiss A. <Astron. Astrophys. 558, A12 (2013)> =2013A&A...558A..12V 2013A&A...558A..12V
ADC_Keywords: Clusters, globular ; Photometry, UBVRI Keywords: globular clusters: general - globular clusters: individual: M5 - stars: evolution - stars: interiors - neutrinos - Hertzsprung-Russell and C-M diagrams Abstract: Stellar evolution is modified if energy is lost in a "dark channel" similar to neutrino emission. Comparing modified stellar evolution sequences with observations provides some of the most restrictive limits on axions and other hypothetical low-mass particles and on non-standard neutrino properties. In particular, a putative neutrino magnetic dipole moment µν enhances the plasmon decay process, postpones helium ignition in low-mass stars, and therefore extends the red-giant branch (RGB) in globular clusters (GCs). The brightness of the tip of the RGB (TRGB) remains the most sensitive probe for µν and we revisit this argument from a modern perspective. Based on a large set of archival observations, we provide high-precision photometry for the Galactic GC M5 (NGC 5904) and carefully determine its TRGB position. Description: We have carried out crowded-field, point-spread function (PSF) photometry for M5 using the DAOPHOT II/ALLFRAME suite of programs (Stetson 1987PASP...99..191S 1987PASP...99..191S, 1994PASP..106..250S 1994PASP..106..250S). The current corpus of observations for M5 consists of 2840 CCD images obtained during 40 observing runs on 12 telescopes over a span of 27 years (1984-2011) File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file photm5.dat 93 83351 UBVRI photometry of NGC 5904 (M5) -------------------------------------------------------------------------------- See also: J/AJ/106/1524 : Proper motions in M5 (Rees, 1993) J/PAZh/21/509 : Identification and coordinates in M5 (Evstigneeva,+ 1995) J/ApJ/611/323 : BVI photometry of M5 giant branch stars (Sandquist+, 2004) J/ApJ/632/266 : WFPC2 photometry of the globular cluster M5 (Layden+, 2005) J/ApJ/648/1026 : HST photometry of M5 blue stragglers (Warren+, 2006) J/ApJ/663/267 : M5 globular cluster blue straggler population (Lanzoni+, 2007) J/AJ/139/2289 : Abundances of five red giants in M5 (Koch+, 2010) J/AJ/141/62 : M5 chemical abundances for evolved stars (Lai+, 2011) J/A+A/549/A41 : Horizontal branch stars in 47 Tuc and M5 (Gratton+, 2013) Byte-by-byte Description of file: photm5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 h RAh Right ascension (J2000) 4- 5 I2 min RAm Right ascension (J2000) 7- 11 F5.2 s RAs Right ascension (J2000) 13 A1 --- DE- Declination sign (J2000) 14- 15 I2 deg DEd Declination (J2000) 17- 18 I2 arcmin DEm Declination (J2000) 20- 23 F4.1 arcsec DEs Declination (J2000) 25- 30 F6.3 mag Umag ?=99.999 U magnitude (1) 32- 37 F6.4 mag e_Umag ?=9.9999 rms uncertainty on Umag 39- 44 F6.3 mag Bmag ?=99.999 B magnitude (1) 46- 51 F6.4 mag e_Bmag ?=9.9999 rms uncertainty on Bmag 53- 58 F6.3 mag Vmag ?=99.999 V magnitude (1) 60- 65 F6.4 mag e_Vmag ?=9.9999 rms uncertainty on Vmag 67- 72 F6.3 mag Rmag ?=99.999 R magnitude (1) 74- 79 F6.4 mag e_Rmag ?=9.9999 rms uncertainty on Rmag 81- 86 F6.3 mag Imag ?=99.999 I magnitude (1) 88- 93 F6.4 mag e_Imag ?=9.9999 rms uncertainty on Imag -------------------------------------------------------------------------------- Note (1): magnitudes reduced to the Landolt system -------------------------------------------------------------------------------- Acknowledgements: Nicolas Viaux, nviaux(at)astro.puc.cl
(End) Nicolas Viaux [PUC], Patricia Vannier [CDS] 28-Aug-2013
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