A publishing partnership

The following article is Free article

ERRATUM: "ON INFRARED EXCESSES ASSOCIATED WITH LI-RICH K GIANTS" (2015, AJ, 150, 123)

, , , , , , , , , , , , and

Published 2016 August 4 • © 2016. The American Astronomical Society. All rights reserved.
, , Citation Luisa M. Rebull et al 2016 AJ 152 52 DOI 10.3847/0004-6256/152/2/52

Download Article PDF

Article metrics

678 Total downloads

Share this article

Author affiliations

1 Spitzer Science Center (SSC) and Infrared Science Archive (IRSA), Infrared Processing and Analysis Center (IPAC), 1200 E. California Blvd., California Institute of Technology, Pasadena, CA 91125 USA; rebull@ipac.caltech.edu

2 NASA Goddard Space Flight Center, Code 667, Greenbelt MD 20771 USA

3 Glencoe High School, 2700 NW Glencoe Rd., Hillsboro, OR 97124 USA

4 Bear Creek High School, 9800 W. Dartmouth Pl., Lakewood, CO 80227 USA

5 Millard South High School, 14905 Q St., Omaha, NE 68137 USA

6 Walden School of Liberal Arts, 4230 N. University Ave., Provo, UT 84604 USA

Author notes

7 NASA Postdoctoral Program Fellow.

ORCID iDs

Dates

  1. Received 2016 May 2
  2. Accepted 2016 May 2
  3. Published

Check for updates using Crossmark

Journal RSS
Create or edit your corridor alerts

What are corridors?opens in new tab

1538-3881/152/2/52

Export citation and abstract BibTeX RIS

Previous article in issue

The units for the flux densities in Table 1 are not Janskys as indicated, but instead milliJanskys. This affects the IRAS PSC and FSC, the Akari IRC and FIS, and the MSX flux densities. Thanks to Sylvain Guéhenneux of VizieR at CDS for finding this error.

Table 1. Contents of Online Catalog a

FormatUnitsLabelExplanations
A26⋯namename of source
F11.6decRAright ascension of source (J2000)
F11.6decDecdeclination of source (J2000)
A6⋯dlR97flag to indicate source is part of the dlR97 sample
A4⋯C12flag to indicate star is part of the C12 sample
A5⋯litflag to indicate star is selected from the literature as a Li-rich giant (but not C12 or dlR97)
A4⋯LirichLitvalue of "yes" means source is identified in the literature as a Li-rich giant
A4⋯LirichHerevalue of "yes" means source is selected here as a Li-rich giant
F7.2⋯ALiNLTE A(Li) under the assumption of NLTE from the literature
A2⋯ALiLTEllimit flag for A(Li) under the assumption of LTE from the literature
F7.2⋯ALiLTE A(Li) under the assumption of LTE from the literature
A2⋯Cratiollimit flag on 12C/13C ratio
F5.1⋯Cratio 12C/13C ratio
F5.1km s−1 vsiniprojected rotational velocity $v\sin i$ in km s−1 from the literature
I5KTeffEffective temperature from the literature
F5.1⋯logglog g from the literature
F6.2magUmagVega-based magnitude in U band
F6.2magUmerrVega-based magnitude error in U band; taken to be 20% unless specified
F6.2magBmagVega-based magnitude in B band
F6.2magBmerrVega-based magnitude error in B band; taken to be 20% unless specified
F6.2magVmagVega-based magnitude in V band
F6.2magVmerrVega-based magnitude error in V band; taken to be 20% unless specified
F6.2magRmagVega-based magnitude in R band
F6.2magRmerrVega-based magnitude error in R band; taken to be 20% unless specified
F6.2magumagAB SDSS magnitude in u band
F6.2magumerrAB SDSS magnitude error in u band
F6.2maggmagAB SDSS magnitude in g band
F6.2maggmerrAB SDSS magnitude error in g band
F6.2magrmagAB SDSS magnitude in r band
F6.2magrmerrAB SDSS magnitude error in r band
F6.2magimagAB SDSS magnitude in i band
F6.2magimerrAB SDSS magnitude error in i band
F6.2magzmagAB SDSS magnitude in z band
F6.2magzmerrAB SDSS magnitude error in z band
A22⋯2MnameName from 2MASS or 2MASX catalog
A2⋯Jlimlimit flag for 2MASS J band
F6.2magJmagVega-based magnitude in 2MASS J band
F6.2magJmerrVega-based magnitude error in 2MASS J band
A2⋯Jqual2MASS data quality flag for J (A = best)
A2⋯Hlimlimit flag for 2MASS H band
F6.2magHmagVega-based magnitude in 2MASS H band
F6.2magHmerrVega-based magnitude error in 2MASS H band
A2⋯Hqual2MASS data quality flag for H (A = best)
A2⋯Klimlimit flag for 2MASS Ks band
F6.2magKmagVega-based magnitude in 2MASS Ks band
F6.2magKmerrVega-based magnitude error in 2MASS Ks band
A2⋯Kqual2MASS data quality flag for Ks (A = best)
A18⋯DENISnameName from DENIS catalog
F6.2magImagVega-based DENIS magnitude in I band
F6.2magImerrVega-based DENIS magnitude error in I band
F6.2magJmagVega-based DENIS magnitude in J band
F6.2magJmerrVega-based DENIS magnitude error in J band
F6.2magKmagVega-based DENIS magnitude in K band
F6.2magKmerrVega-based DENIS magnitude error in K band
A26⋯WISEnameName from WISE (AllWISE) catalog or reject catalog
A2⋯W1limlimit flag for WISE-1 ([3.4])
F6.2magW1magVega-based magnitude in WISE-1 ([3.4])
F6.2magW1merrVega-based magnitude error in WISE-1 ([3.4]); value of $-9$ for those measures that are limits
A2magW1qualWISE-1 ([3.4]) data quality flag (A = best)
A2⋯W2limlimit flag for WISE-2 ([4.6])
F6.2magW2magVega-based magnitude in WISE-2 ([4.6])
F6.2magW2merrVega-based magnitude error in WISE-2 ([4.6]); value of $-9$ for those measures that are limits
A2magW2qualWISE-2 ([4.6]) data quality flag (A = best)
A2⋯W3limlimit flag for WISE-3 ([12])
F6.2magW3magVega-based magnitude in WISE-3 ([12])
F6.2magW3merrVega-based magnitude error in WISE-3 ([12]); value of $-9$ for those measures that are limits
A2magW3qualWISE-3 ([12]) data quality flag (A = best)
A2⋯W4limlimit flag for WISE-4 ([22])
F6.2magW4magVega-based magnitude in WISE-4 ([22])
F6.2magW4merrVega-based magnitude error in WISE-4 ([22]); value of $-9$ for those measures that are limits
A2magW4qualWISE-4 ([22]) data quality flag (A = best)
A27⋯SEIPnameName from SEIP source list
F6.2magI1magVega-based magnitude in IRAC-1 ([3.6])
F6.2magI1merrVega-based magnitude error in IRAC-1([3.6])
F6.2magI2magVega-based magnitude in IRAC-2 ([4.5])
F6.2magI2merrVega-based magnitude error in IRAC-2 ([4.5])
F6.2magI3magVega-based magnitude in IRAC-3 ([5.8])
F6.2magI3merrVega-based magnitude error in IRAC-3 ([5.8])
F6.2magI4magVega-based magnitude in IRAC-4 ([8])
F6.2magI4merrVega-based magnitude error in IRAC-4 ([8])
F6.2magM1magVega-based magnitude in MIPS-1 ([24])
F6.2magM1merrVega-based magnitude error in MIPS-1 ([24])
A14⋯IRASPSCnameName from IRAS Point Source Catalog (PSC)
F6.2magIRAS1PSCmagVega-based magnitude in IRAS-1 ([12]) from PSC; errors taken to be 0.22 mags
F9.2mJyIRAS1PSCfdflux density in mJy in IRAS-1 from PSC
A2magIRAS1PSCqualData quality flag for IRAS-1 from PSC (3 = best, 1 = limit)
F6.2magIRA21PSCmagVega-based magnitude in IRAS-2 ([25]) from PSC; errors taken to be 0.22 mags
F9.2mJyIRAS2PSCfdflux density in mJy in IRAS-2 from PSC
A2magIRAS2PSCqualData quality flag for IRAS-2 from PSC (3 = best, 1 = limit)
F6.2magIRAS3PSCmagVega-based magnitude in IRAS-3 ([60]) from PSC; errors taken to be 0.22 mags
F9.2mJyIRAS3PSCfdflux density in mJy in IRAS-3 from PSC
A2magIRAS3PSCqualData quality flag for IRAS-3 from PSC (3 = best, 1 = limit)
F6.2magIRAS4PSCmagVega-based magnitude in IRAS-4 ([100]) from PSC; errors taken to be 0.22 mags
F9.2mJyIRAS4PSCfdflux density in mJy in IRAS-4 from PSC
A2magIRAS4PSCqualData quality flag for IRAS-4 from PSC (3 = best, 1 = limit)
A14⋯IRASFSCnameName from IRAS Faint Source Catalog (FSC)
F6.2magIRAS1FSCmagVega-based magnitude in IRAS-1 ([12]) from FSC; errors taken to be 0.22 mags
F9.2mJyIRAS1FSCfdflux density in mJy in IRAS-1 from FSC
A2magIRAS1FSCqualData quality flag for IRAS-1 from FSC (3 = best, 1 = limit)
F6.2magIRA21FSCmagVega-based magnitude in IRAS-2 ([25]) from FSC; errors taken to be 0.22 mags
F9.2mJyIRAS2FSCfdflux density in mJy in IRAS-2 from FSC
A2magIRAS2FSCqualData quality flag for IRAS-2 from FSC (3 = best, 1 = limit)
F6.2magIRAS3FSCmagVega-based magnitude in IRAS-3 ([60]) from FSC; errors taken to be 0.22 mags
F9.2mJyIRAS3FSCfdflux density in mJy in IRAS-3 from FSC
A2magIRAS3FSCqualData quality flag for IRAS-3 from FSC (3 = best, 1 = limit)
F6.2magIRAS4FSCmagVega-based magnitude in IRAS-4 ([100]) from FSC; errors taken to be 0.22 mags
F9.2mJyIRAS4FSCfdflux density in mJy in IRAS-4 from FSC
A2magIRAS4FSCqualData quality flag for IRAS-4 from FSC (3 = best, 1 = limit)
A28⋯AKARIIRCnameName from AKARI IRC catalog, v1
F9.2mJyAKARI9fdflux density in mJy in 9 microns from AKARI IRC
F9.2mJyAKARI9fderrerror in flux density in mJy in 9 microns from AKARI IRC
F9.2mJyAKARI18fdflux density in mJy in 18 microns from AKARI IRC
F9.2mJyAKARI18fderrerror in flux density in mJy in 18 microns from AKARI IRC
A28⋯AKARIFISnameName from AKARI FIS catalog, v1
F9.2mJyAKARI65fdflux density in mJy in 65 microns from AKARI FIS
F9.2mJyAKARI65fderrerror in flux density in mJy in 65 microns from AKARI FIS
F9.2mJyAKARI90fdflux density in mJy in 90 microns from AKARI FIS
F9.2mJyAKARI90fderrerror in flux density in mJy in 90 microns from AKARI FIS
F9.2mJyAKARI140fdflux density in mJy in 140 microns from AKARI FIS
F9.2mJyAKARI140fderrerror in flux density in mJy in 140 microns from AKARI FIS
F9.2mJyAKARI160fdflux density in mJy in 160 microns from AKARI FIS
F9.2mJyAKARI160fderrerror in flux density in mJy in 160 microns from AKARI FIS
A18⋯MSXnameName from MSX catalog
F9.2mJyMsxAfdflux density in mJy in MSX Band A (7.76 μm)
F9.2mJyMsxAfderrerror in flux density in mJy in MSX Band A (7.76 μm)–as reported, may be very large
F9.2mJyMsxB1fdflux density in mJy in MSX Band B1 (4.29 μm)
F9.2mJyMsxB1fderrerror in flux density in mJy in MSX Band B1 (4.29 μm)–as reported, may be very large
F9.2mJyMsxB2fdflux density in mJy in MSX Band B2 (4.35 μm)
F9.2mJyMsxB2fderrerror in flux density in mJy in MSX Band B2 (4.35 μm)–as reported, may be very large
F9.2mJyMsxCfdflux density in mJy in MSX Band C (11.99 μm)
F9.2mJyMsxCfderrerror in flux density in mJy in MSX Band C (11.99 μm)–as reported, may be very large
F9.2mJyMsxDfdflux density in mJy in MSX Band D (14.55 μm)
F9.2mJyMsxDfderrerror in flux density in mJy in MSX Band D (14.55 μm)–as reported, may be very large
F9.2mJyMsxEfdflux density in mJy in MSX Band E (20.68 μm)
F9.2mJyMsxEfderrerror in flux density in mJy in MSX Band E (20.68 μm)–as reported, may be very large

Note.

a This catalog is available in its entirety in the online version of Table 1.

Only a portion of this table is shown here to demonstrate its form and content. A machine-readable version of the full table is available.

Download table as:  DataTypeset images: 1 2 3

10.3847/0004-6256/152/2/52