M
Mercedes Gomez
Researcher at National Scientific and Technical Research Council
Publications - 49
Citations - 3423
Mercedes Gomez is an academic researcher from National Scientific and Technical Research Council. The author has contributed to research in topics: Stars & Young stellar object. The author has an hindex of 26, co-authored 49 publications receiving 3277 citations. Previous affiliations of Mercedes Gomez include National University of Cordoba & Association of Universities for Research in Astronomy.
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Journal ArticleDOI
A Catalog of Extended Green Objects in the GLIMPSE Survey: A New Sample of Massive Young Stellar Object Outflow Candidates
Claudia Cyganowski,B. A. Whitney,E. Holden,Ella K. Braden,Crystal L. Brogan,Ed Churchwell,Remy Indebetouw,D. F. Watson,Brian Babler,Robert A. Benjamin,Mercedes Gomez,Marilyn R. Meade,Matthew S. Povich,Thomas P. Robitaille,C. Watson +14 more
TL;DR: In this paper, a catalog of extended green objects (EGOs) is presented, including integrated flux density measurements at 3.6, 4.5, 5.8, 8.0, and 24 μm from the Spitzer Galactic Legacy Infrared Mid-Plane Survey Extraordinaire (GLIMPSE).
Journal ArticleDOI
A Catalog of Extended Green Objects (EGOs) in the GLIMPSE Survey: A new sample of massive young stellar object outflow candidates
Claudia Cyganowski,B. A. Whitney,E. Holden,Ella K. Braden,Crystal Brogan,Ed Churchwell,Remy Indebetouw,D. F. Watson,Brian Babler,Robert A. Benjamin,Mercedes Gomez,Marilyn R. Meade,M. S. Povich,Thomas Robitaille,C. Watson +14 more
TL;DR: In this paper, the authors identified more than 300 extended 4.5 micron sources (abbreviated EGO, Extended Green Object, for the common coding of the [4.5] band as green in 3-color composite IRAC images).
Journal ArticleDOI
UBVRI Light Curves of 44 Type Ia Supernovae
Saurabh Jha,Saurabh Jha,Robert P. Kirshner,Peter Challis,Peter M. Garnavich,Thomas Matheson,Alicia M. Soderberg,Genevieve J. Graves,Malcolm Hicken,João Alves,Héctor G. Arce,Zoltan Balog,Pauline Barmby,Elizabeth J. Barton,Perry Berlind,Ann Bragg,Cesar Briceno,Warren R. Brown,J. H. Buckley,Nelson Caldwell,Michael L. Calkins,B. J. Carter,Kristi Dendy Concannon,R. Hank Donnelly,Kristoffer A. Eriksen,Daniel G. Fabricant,Emilio E. Falco,Fabrizio Fiore,Michael R. Garcia,Mercedes Gomez,Norman A. Grogin,Ted Groner,Paul J. Groot,Karl E. Haisch,Lee Hartmann,Carl Hergenrother,Matthew J. Holman,John P. Huchra,Ray Jayawardhana,D. Jerius,Sheila J. Kannappan,Dong-Woo Kim,Jan T. Kleyna,Christopher S. Kochanek,Daniel M. Koranyi,M. Krockenberger,Charles J. Lada,Kevin Luhman,Jane Luu,Lucas M. Macri,J. Mader,Andisheh Mahdavi,Massimo Marengo,Brian G. Marsden,Brian McLeod,Brian R. McNamara,S. Thomas Megeath,Dan Moraru,A. Mossman,August Muench,J. A. Muñoz,James Muzerolle,Orlando Naranjo,Kristin Nelson-Patel,Michael A. Pahre,Brian M. Patten,J. Peters,Wayne Peters,John C. Raymond,Kenneth J. Rines,Rudolph E. Schild,Gregory J. Sobczak,Timothy Spahr,John R. Stauffer,Robert P. Stefanik,Andrew Szentgyorgyi,Eric V. Tollestrup,Petri Vaisanen,Alexey Vikhlinin,Zhong Wang,S. P. Willner,Scott J. Wolk,Joseph Zajac,Ping Zhao,Krzysztof Z. Stanek +84 more
TL;DR: In this article, the authors present UBVRI photometry of 44 Type Ia supernovae (SNe Ia) observed from 1997 to 2001 as part of a continuing monitoring campaign at the Fred Lawrence Whipple Observatory of the Harvard-Smithsonian Center for Astrophysics.
Journal ArticleDOI
SN 1991bg - A type Ia supernova with a difference
Bruno Leibundgut,Robert P. Kirshner,Mark M. Phillips,Mark M. Phillips,L. Wells,L. Wells,Nicholas B. Suntzeff,Nicholas B. Suntzeff,Mario Hamuy,Mario Hamuy,Robert A. Schommer,Robert A. Schommer,Alistair R. Walker,Alistair R. Walker,L. E. Gonzalez,L. E. Gonzalez,P. Ugarte,P. Ugarte,Robert Williams,Robert Williams,G. Williger,G. Williger,Mercedes Gomez,R. O. Marzke,Brian P. Schmidt,Barbara A. Whitney,Nelson Caldwell,Jan Peters,Frederic H. Chaffee,Craig B. Foltz,Daniel M. Rehner,L. Siciliano,Thomas G. Barnes,K. P. Cheng,P. Hintzen,Yong-Cheol Kim,José Maza,J. Wm. Parker,A. C. Porter,P. C. Schmidtke,George Sonneborn +40 more
TL;DR: The spectral evolution of SN 1991bg is also unique but not unrecognizable; nevertheless, the peculiarities associated with this event complicate the fundamental question as to whether the Ia SNs make good standard candles as mentioned in this paper.
Journal ArticleDOI
On the spatial distribution of pre-main-sequence stars in Taurus
TL;DR: In this paper, a power-law form for the two-point angular correlation function (with index −1.2) reproduces the overall shape of the actual pre-main-sequence distribution in Taurus at small angular scales (∼0.3°).