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The Taurus Spitzer Survey: New Candidate Taurus Members Selected Using Sensitive Mid-Infrared Photometry
DOI: 10.1088/0067-0049/186/2/259 Bibcode: 2010ApJS..186..259R

Stapelfeldt, K. R.; Wolf, S.; Audard, M. +31 more

We report on the properties of pre-main-sequence objects in the Taurus molecular clouds as observed in seven mid- and far-infrared bands with the Spitzer Space Telescope. There are 215 previously identified members of the Taurus star-forming region in our ~44 deg2 map these members exhibit a range of Spitzer colors that we take to defin…

2010 The Astrophysical Journal Supplement Series
XMM-Newton 259
The Extended Chandra Deep Field-South Survey: Optical Spectroscopy of Faint X-ray Sources with the VLT and Keck
DOI: 10.1088/0067-0049/191/1/124 Bibcode: 2010ApJS..191..124S

Finoguenov, A.; Lehmer, B. D.; Alexander, D. M. +26 more

We present the results of a program to acquire high-quality optical spectra of X-ray sources detected in the Extended-Chandra Deep Field-South (E-CDF-S) and its central 2 Ms area. New spectroscopic redshifts, up to z = 4, are measured for 283 counterparts to Chandra sources with deep exposures (t ~ 2-9 hr per pointing) using multi-slit facilities …

2010 The Astrophysical Journal Supplement Series
XMM-Newton eHST 130
The Atacama Cosmology Telescope (ACT): Beam Profiles and First SZ Cluster Maps
DOI: 10.1088/0067-0049/191/2/423 Bibcode: 2010ApJS..191..423H

Ade, P. A. R.; Bond, J. R.; Hernández-Monteagudo, C. +69 more

The Atacama Cosmology Telescope (ACT) is currently observing the cosmic microwave background with arcminute resolution at 148 GHz, 218 GHz, and 277 GHz. In this paper, we present ACT's first results. Data have been analyzed using a maximum-likelihood map-making method which uses B-splines to model and remove the atmospheric signal. It has been use…

2010 The Astrophysical Journal Supplement Series
XMM-Newton 119
The Chandra M101 Megasecond: Diffuse Emission
DOI: 10.1088/0067-0049/188/1/46 Bibcode: 2010ApJS..188...46K

Kuntz, K. D.; Snowden, S. L.

Because M101 is nearly face-on, it provides an excellent laboratory in which to study the distribution of X-ray-emitting gas in a typical late-type spiral galaxy. We obtained a Chandra observation with a cumulative exposure of roughly 1 Ms to study the diffuse X-ray emission in M101. The bulk of the X-ray emission is correlated with the star forma…

2010 The Astrophysical Journal Supplement Series
XMM-Newton eHST 55
An XMM-Newton Survey of the Soft X-ray Background. I. The O VII and O VIII Lines Between l = 120° and l = 240°
DOI: 10.1088/0067-0049/187/2/388 Bibcode: 2010ApJS..187..388H

Henley, David B.; Shelton, Robin L.

We present measurements of the soft X-ray background (SXRB) O VII and O VIII intensity between l = 120° and l = 240°, the first results of a survey of the SXRB using archival XMM-Newton observations. We do not restrict ourselves to blank-sky observations, but instead use as many observations as possible, removing bright or extended sources by hand…

2010 The Astrophysical Journal Supplement Series
XMM-Newton 47
Southern Cosmology Survey. II. Massive Optically Selected Clusters from 70 Square Degrees of the Sunyaev-Zel'dovich Effect Common Survey Area
DOI: 10.1088/0067-0049/191/2/340 Bibcode: 2010ApJS..191..340M

Hilton, Matt; Hughes, John P.; Kosowsky, Arthur +8 more

We present a catalog of 105 rich and massive (M>3 × 1014 M sun) optically selected clusters of galaxies extracted from 70 deg2 of public archival griz imaging from the Blanco 4 m telescope acquired over 45 nights between 2005 and 2007. We use the clusters' optically derived properties to estimate photometric red…

2010 The Astrophysical Journal Supplement Series
XMM-Newton 40