X-ray-emitting stars identified from the ROSAT all-sky survey and the sloan digital sky survey

Marcel A. Agüeros, Scott F. Anderson, Kevin R. Covey, Suzanne L. Hawley, Bruce Margon, Emily R. Newsom, Bettina Posselt, Nicole M. Silvestri, Paula Szkody, Wolfgang Voges

Research output: Contribution to journalArticle

31 Citations (Scopus)

Abstract

The ROSAT All-Sky Survey (RASS) was the first imaging X-ray survey of the entire sky. Combining the RASS Bright and Faint Source Catalogs yields an average of about three X-ray sources per square degree. However, while X-ray source counterparts are known to range from distant quasars to nearby M dwarfs, the RASS data alone are often insufficient to determine the nature of an X-ray source. As a result, large-scale follow-up programs are required to construct samples of known X-ray emitters. We use optical data produced by the Sloan Digital Sky Survey (SDSS) to identify 709 stellar X-ray emitters cataloged in the RASS and falling within the SDSS Data Release 1 footprint. Most of these are bright stars with coronal X-ray emission unsuitable for SDSS spectroscopy, which is designed for fainter objects (g > 15 [mag]). Instead, we use SDSS photometry, correlations with the Two Micron All Sky Survey and other catalogs, and spectroscopy from the Apache Point Observatory 3.5 m telescope to identify these stellar Xray counterparts. Our sample of 707 X-ray-emitting F, G, K, and M stars is one of the largest X-ray-selected samples of such stars. We derive distances to these stars using photometric parallax relations appropriate for dwarfs on the main sequence, and use these distances to calculate LX. We also identify a previously unknown cataclysmic variable (CV) as a RASS counterpart. Separately, we use correlations of the RASS and the SDSS spectroscopic catalogs of CVs and white dwarfs (WDs) to study the properties of these rarer X-ray-emitting stars. We examine the relationship between (f X/fg) and the equivalent width of the Hß emission line for 46 X-ray-emitting CVs and discuss tentative classifications for a subset based on these quantities. We identify 17 new X-ray-emitting DA (hydrogen) WDs, of which three are newly identified WDs. We report on follow-up observations of three candidate cool X-rayemitting WDs (one DA and two DB (helium) WDs); we have not confirmed X-ray emission from these WDs.

Original languageEnglish (US)
Pages (from-to)444-465
Number of pages22
JournalAstrophysical Journal, Supplement Series
Volume181
Issue number2
DOIs
StatePublished - Sep 7 2009

Fingerprint

stars
x rays
catalogs
emitters
spectroscopy
G stars
F stars
K stars
faint objects
M stars
cataclysmic variables
parallax
footprints
falling
footprint
quasars
helium
set theory
photometry
sky

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Agüeros, M. A., Anderson, S. F., Covey, K. R., Hawley, S. L., Margon, B., Newsom, E. R., ... Voges, W. (2009). X-ray-emitting stars identified from the ROSAT all-sky survey and the sloan digital sky survey. Astrophysical Journal, Supplement Series, 181(2), 444-465. https://doi.org/10.1088/0067-0049/181/2/444
Agüeros, Marcel A. ; Anderson, Scott F. ; Covey, Kevin R. ; Hawley, Suzanne L. ; Margon, Bruce ; Newsom, Emily R. ; Posselt, Bettina ; Silvestri, Nicole M. ; Szkody, Paula ; Voges, Wolfgang. / X-ray-emitting stars identified from the ROSAT all-sky survey and the sloan digital sky survey. In: Astrophysical Journal, Supplement Series. 2009 ; Vol. 181, No. 2. pp. 444-465.
@article{09923e41806544e799aaeb27e01f827c,
title = "X-ray-emitting stars identified from the ROSAT all-sky survey and the sloan digital sky survey",
abstract = "The ROSAT All-Sky Survey (RASS) was the first imaging X-ray survey of the entire sky. Combining the RASS Bright and Faint Source Catalogs yields an average of about three X-ray sources per square degree. However, while X-ray source counterparts are known to range from distant quasars to nearby M dwarfs, the RASS data alone are often insufficient to determine the nature of an X-ray source. As a result, large-scale follow-up programs are required to construct samples of known X-ray emitters. We use optical data produced by the Sloan Digital Sky Survey (SDSS) to identify 709 stellar X-ray emitters cataloged in the RASS and falling within the SDSS Data Release 1 footprint. Most of these are bright stars with coronal X-ray emission unsuitable for SDSS spectroscopy, which is designed for fainter objects (g > 15 [mag]). Instead, we use SDSS photometry, correlations with the Two Micron All Sky Survey and other catalogs, and spectroscopy from the Apache Point Observatory 3.5 m telescope to identify these stellar Xray counterparts. Our sample of 707 X-ray-emitting F, G, K, and M stars is one of the largest X-ray-selected samples of such stars. We derive distances to these stars using photometric parallax relations appropriate for dwarfs on the main sequence, and use these distances to calculate LX. We also identify a previously unknown cataclysmic variable (CV) as a RASS counterpart. Separately, we use correlations of the RASS and the SDSS spectroscopic catalogs of CVs and white dwarfs (WDs) to study the properties of these rarer X-ray-emitting stars. We examine the relationship between (f X/fg) and the equivalent width of the H{\ss} emission line for 46 X-ray-emitting CVs and discuss tentative classifications for a subset based on these quantities. We identify 17 new X-ray-emitting DA (hydrogen) WDs, of which three are newly identified WDs. We report on follow-up observations of three candidate cool X-rayemitting WDs (one DA and two DB (helium) WDs); we have not confirmed X-ray emission from these WDs.",
author = "Ag{\"u}eros, {Marcel A.} and Anderson, {Scott F.} and Covey, {Kevin R.} and Hawley, {Suzanne L.} and Bruce Margon and Newsom, {Emily R.} and Bettina Posselt and Silvestri, {Nicole M.} and Paula Szkody and Wolfgang Voges",
year = "2009",
month = "9",
day = "7",
doi = "10.1088/0067-0049/181/2/444",
language = "English (US)",
volume = "181",
pages = "444--465",
journal = "Astrophysical Journal, Supplement Series",
issn = "0067-0049",
publisher = "IOP Publishing Ltd.",
number = "2",

}

Agüeros, MA, Anderson, SF, Covey, KR, Hawley, SL, Margon, B, Newsom, ER, Posselt, B, Silvestri, NM, Szkody, P & Voges, W 2009, 'X-ray-emitting stars identified from the ROSAT all-sky survey and the sloan digital sky survey', Astrophysical Journal, Supplement Series, vol. 181, no. 2, pp. 444-465. https://doi.org/10.1088/0067-0049/181/2/444

X-ray-emitting stars identified from the ROSAT all-sky survey and the sloan digital sky survey. / Agüeros, Marcel A.; Anderson, Scott F.; Covey, Kevin R.; Hawley, Suzanne L.; Margon, Bruce; Newsom, Emily R.; Posselt, Bettina; Silvestri, Nicole M.; Szkody, Paula; Voges, Wolfgang.

In: Astrophysical Journal, Supplement Series, Vol. 181, No. 2, 07.09.2009, p. 444-465.

Research output: Contribution to journalArticle

TY - JOUR

T1 - X-ray-emitting stars identified from the ROSAT all-sky survey and the sloan digital sky survey

AU - Agüeros, Marcel A.

AU - Anderson, Scott F.

AU - Covey, Kevin R.

AU - Hawley, Suzanne L.

AU - Margon, Bruce

AU - Newsom, Emily R.

AU - Posselt, Bettina

AU - Silvestri, Nicole M.

AU - Szkody, Paula

AU - Voges, Wolfgang

PY - 2009/9/7

Y1 - 2009/9/7

N2 - The ROSAT All-Sky Survey (RASS) was the first imaging X-ray survey of the entire sky. Combining the RASS Bright and Faint Source Catalogs yields an average of about three X-ray sources per square degree. However, while X-ray source counterparts are known to range from distant quasars to nearby M dwarfs, the RASS data alone are often insufficient to determine the nature of an X-ray source. As a result, large-scale follow-up programs are required to construct samples of known X-ray emitters. We use optical data produced by the Sloan Digital Sky Survey (SDSS) to identify 709 stellar X-ray emitters cataloged in the RASS and falling within the SDSS Data Release 1 footprint. Most of these are bright stars with coronal X-ray emission unsuitable for SDSS spectroscopy, which is designed for fainter objects (g > 15 [mag]). Instead, we use SDSS photometry, correlations with the Two Micron All Sky Survey and other catalogs, and spectroscopy from the Apache Point Observatory 3.5 m telescope to identify these stellar Xray counterparts. Our sample of 707 X-ray-emitting F, G, K, and M stars is one of the largest X-ray-selected samples of such stars. We derive distances to these stars using photometric parallax relations appropriate for dwarfs on the main sequence, and use these distances to calculate LX. We also identify a previously unknown cataclysmic variable (CV) as a RASS counterpart. Separately, we use correlations of the RASS and the SDSS spectroscopic catalogs of CVs and white dwarfs (WDs) to study the properties of these rarer X-ray-emitting stars. We examine the relationship between (f X/fg) and the equivalent width of the Hß emission line for 46 X-ray-emitting CVs and discuss tentative classifications for a subset based on these quantities. We identify 17 new X-ray-emitting DA (hydrogen) WDs, of which three are newly identified WDs. We report on follow-up observations of three candidate cool X-rayemitting WDs (one DA and two DB (helium) WDs); we have not confirmed X-ray emission from these WDs.

AB - The ROSAT All-Sky Survey (RASS) was the first imaging X-ray survey of the entire sky. Combining the RASS Bright and Faint Source Catalogs yields an average of about three X-ray sources per square degree. However, while X-ray source counterparts are known to range from distant quasars to nearby M dwarfs, the RASS data alone are often insufficient to determine the nature of an X-ray source. As a result, large-scale follow-up programs are required to construct samples of known X-ray emitters. We use optical data produced by the Sloan Digital Sky Survey (SDSS) to identify 709 stellar X-ray emitters cataloged in the RASS and falling within the SDSS Data Release 1 footprint. Most of these are bright stars with coronal X-ray emission unsuitable for SDSS spectroscopy, which is designed for fainter objects (g > 15 [mag]). Instead, we use SDSS photometry, correlations with the Two Micron All Sky Survey and other catalogs, and spectroscopy from the Apache Point Observatory 3.5 m telescope to identify these stellar Xray counterparts. Our sample of 707 X-ray-emitting F, G, K, and M stars is one of the largest X-ray-selected samples of such stars. We derive distances to these stars using photometric parallax relations appropriate for dwarfs on the main sequence, and use these distances to calculate LX. We also identify a previously unknown cataclysmic variable (CV) as a RASS counterpart. Separately, we use correlations of the RASS and the SDSS spectroscopic catalogs of CVs and white dwarfs (WDs) to study the properties of these rarer X-ray-emitting stars. We examine the relationship between (f X/fg) and the equivalent width of the Hß emission line for 46 X-ray-emitting CVs and discuss tentative classifications for a subset based on these quantities. We identify 17 new X-ray-emitting DA (hydrogen) WDs, of which three are newly identified WDs. We report on follow-up observations of three candidate cool X-rayemitting WDs (one DA and two DB (helium) WDs); we have not confirmed X-ray emission from these WDs.

UR - http://www.scopus.com/inward/record.url?scp=69549083373&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=69549083373&partnerID=8YFLogxK

U2 - 10.1088/0067-0049/181/2/444

DO - 10.1088/0067-0049/181/2/444

M3 - Article

AN - SCOPUS:69549083373

VL - 181

SP - 444

EP - 465

JO - Astrophysical Journal, Supplement Series

JF - Astrophysical Journal, Supplement Series

SN - 0067-0049

IS - 2

ER -