RECONSTRUCTING THE STELLAR MASS DISTRIBUTIONS OF GALAXIES USING S4G IRAC 3.6 AND 4.5 μm IMAGES. II. THE CONVERSION FROM LIGHT TO MASS-Reference-Cited by-同舟云学术

RECONSTRUCTING THE STELLAR MASS DISTRIBUTIONS OF GALAXIES USING S4G IRAC 3.6 AND 4.5 μm IMAGES. II. THE CONVERSION FROM LIGHT TO MASS

Published:2014-06-03 Issue:2 Volume:788 Page:144
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Meidt Sharon E.,Schinnerer Eva,van de Ven Glenn,Zaritsky Dennis^ORCID,Peletier Reynier,Knapen Johan H.,Sheth Kartik,Regan Michael,Querejeta Miguel,Muñoz-Mateos Juan-Carlos,Kim Taehyun,Hinz Joannah L.^ORCID,de Paz Armando Gil,Athanassoula E.,Bosma Albert,Buta Ronald J.,Cisternas Mauricio,Ho Luis C.,Holwerda Benne,Skibba Ramin,Laurikainen E.,Salo H.,Gadotti D. A.,Laine Jarkko,Erroz-Ferrer S.,Comerón Sébastien,Menéndez-Delmestre K.,Seibert M.,Mizusawa T.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/788/i=2/a=144/pdf

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2. Stellar Mass‐to‐Light Ratios and the Tully‐Fisher Relation

3. GLIMPSE. I. AnSIRTFLegacy Project to Map the Inner Galaxy

4. Galaxy luminosities, stellar masses, sizes, velocity dispersions as a function of morphological type

5. JHKLM photometry - Standard systems, passbands, and intrinsic colors

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