J/ApJ/892/L35  He+He white dwarf SDSS J232230.20+050942.0 RVels  (Brown+, 2020)

A 1201s orbital period detached binary: the first double helium core white dwarf LISA verification binary. Brown W.R., Kilic M., Bedard A., Kosakowski A., Bergeron P. <Astrophys. J., 892, L35 (2020)> =2020ApJ...892L..35B 2020ApJ...892L..35B
ADC_Keywords: Binaries, spectroscopic; Stars, white dwarf; Radial velocities; Optical Keywords: Compact binary stars; DA stars; DC stars; Gravitational wave sources; Gravitational waves; White dwarf stars; Compact objects; Detached binary stars Abstract: We report the discovery of a 1201s orbital period binary, the third shortest-period detached binary known. Sloan Digital Sky Survey J232230.20+050942.06 contains two He-core white dwarfs orbiting with a 27° inclination. Located 0.76kpc from the Sun, the binary has an estimated Laser Interferometer Space Antenna (LISA) 4yr signal-to-noise ratio of 40. J2322+0509 is the first He+He white dwarf LISA verification binary, a source class that is predicted to account for one-third of resolved LISA ultra-compact binary detections. Description: We targeted SDSSJ232230.20+050942.06 on the basis of its Gaia parallax and Sloan Digital Sky Survey (SDSS) colors. We obtained an exploratory spectrum of J2322+0509 on UT 2018-Dec-9 to determine its stellar nature. We used the Blue Channel spectrograph on the 6.5m MMT telescope. The following year we obtained time-series MMT Blue Channel spectroscopy. Finally, on UT 2019 November 20, we obtained 1hr of MagE spectroscopy on the 6.5m Magellan Baade telescope. We obtained time-series photometry of J2322+0509 using the 8m Gemini North telescope with the Gemini Multi-Object Spectrograph on UT 2019 October 24 as part of the Director's Discretionary Time program GN-2019B-DD-201. Objects: ------------------------------------------------------------------- RA (ICRS) DE Designation(s) ------------------------------------------------------------------- 23 22 30.19 +05 09 42.2 J2322+0509 = SDSS J232230.20+050942.0 ------------------------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file fig1.dat 29 74 Radial velocities phased to the best-fit orbital solution -------------------------------------------------------------------------------- See also: II/319 : UKIDSS-DR9 LAS, GCS and DXS Surveys (Lawrence+ 2012) V/147 : The SDSS Photometric Catalogue, Release 12 (Alam+, 2015) I/345 : Gaia DR2 (Gaia Collaboration, 2018) J/ApJ/743/138 : Spectroscopic survey of bright white dwarfs (Gianninas+, 2011) J/ApJ/750/99 : The Pan-STARRS1 photometric system (Tonry+, 2012) J/A+A/557/A19 : Mass and age of extreme low-mass white dwarfs (Althaus+, 2013) J/ApJ/812/167 : The ELM survey. VI. 11 new ELM WD binaries (Gianninas+, 2015) J/A+A/595/A35 : Low-mass helium WDs evolutionary models (Istrate+, 2016) J/ApJ/848/11 : Spectroscopic and photometric analysis of WDs (Bedard+, 2017) J/ApJ/889/49 : The ELM Survey. VIII. Final double WD binaries (Brown+, 2020) Byte-by-byte Description of file: fig1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 11 F11.7 d BJD Barycentric Julian Date (TDB) at mid-exposure, BJD-2458000 13- 19 F7.2 km/s RV [-222/209] Barycentric radial velocity 21- 25 F5.2 km/s e_RV [12.9/56.3] Uncertainty in RV 27- 29 I3 s Exp [150/480] Exposure time -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Prepared by [AAS], Emmanuelle Perret [CDS] 17-Aug-2021
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line