Spitzer Matching Survey of the UltraVISTA Ultra-deep Stripes (SMUVS): Full-mission IRAC Mosaics and Catalogs

This paper describes new deep 3.6 and 4.5 m imaging of three UltraVISTA near-infrared survey stripes within the COSMOS field. The observations were carried out with Spitzer's Infrared Array Camera (IRAC) for the Spitzer Matching Survey of the UltraVISTA Deep Stripes (SMUVS). In this work we pre...

Full description

Saved in:
Bibliographic Details
Published inThe Astrophysical journal. Supplement series Vol. 237; no. 2; pp. 39 - 51
Main Authors Ashby, M. L. N., Caputi, Karina I., Cowley, Will, Deshmukh, Smaran, Dunlop, James S., Milvang-Jensen, Bo, Fynbo, Johan P. U., Muzzin, Adam, McCracken, H. J., Fèvre, Olivier Le, Huang, Jia-Sheng, Zhang, J.
Format Journal Article
LanguageEnglish
Published Saskatoon The American Astronomical Society 01.08.2018
IOP Publishing
American Astronomical Society
Subjects
Online AccessGet full text
ISSN0067-0049
1538-4365
DOI10.3847/1538-4365/aad4fb

Cover

Abstract This paper describes new deep 3.6 and 4.5 m imaging of three UltraVISTA near-infrared survey stripes within the COSMOS field. The observations were carried out with Spitzer's Infrared Array Camera (IRAC) for the Spitzer Matching Survey of the UltraVISTA Deep Stripes (SMUVS). In this work we present our data reduction techniques, and document the resulting mosaics, coverage maps, and catalogs in both IRAC passbands for the three easternmost UltraVISTA survey stripes, covering a combined area of about 0.66 deg2, of which 0.45 deg2 have at least 20 hr of integration time. SMUVS reaches point-source sensitivities of about 25.0 AB mag (0.13 Jy) at both 3.6 and 4.5 m, with a significance of 4 , accounting for both survey sensitivity and source confusion. To this limit the SMUVS catalogs contain a total of ∼350,000 sources, each of which is detected significantly in at least one IRAC band. Because of its uniform and high sensitivity, relatively large area coverage, and the wide array of ancillary data available in COSMOS, the SMUVS survey will be useful for a large number of cosmological investigations. We make all images and catalogs described herein publicly available via the Spitzer Science Center.
AbstractList This paper describes new deep 3.6 and 4.5 μm imaging of three UltraVISTA near-infrared survey stripes within the COSMOS field. The observations were carried out with Spitzer’s Infrared Array Camera (IRAC) for the Spitzer Matching Survey of the UltraVISTA Deep Stripes (SMUVS). In this work we present our data reduction techniques, and document the resulting mosaics, coverage maps, and catalogs in both IRAC passbands for the three easternmost UltraVISTA survey stripes, covering a combined area of about 0.66 deg2, of which 0.45 deg2 have at least 20 hr of integration time. SMUVS reaches point-source sensitivities of about 25.0 AB mag (0.13 μJy) at both 3.6 and 4.5 μm, with a significance of 4σ, accounting for both survey sensitivity and source confusion. To this limit the SMUVS catalogs contain a total of ∼350,000 sources, each of which is detected significantly in at least one IRAC band. Because of its uniform and high sensitivity, relatively large area coverage, and the wide array of ancillary data available in COSMOS, the SMUVS survey will be useful for a large number of cosmological investigations. We make all images and catalogs described herein publicly available via the Spitzer Science Center.
This paper describes new deep 3.6 and 4.5 m imaging of three UltraVISTA near-infrared survey stripes within the COSMOS field. The observations were carried out with Spitzer's Infrared Array Camera (IRAC) for the Spitzer Matching Survey of the UltraVISTA Deep Stripes (SMUVS). In this work we present our data reduction techniques, and document the resulting mosaics, coverage maps, and catalogs in both IRAC passbands for the three easternmost UltraVISTA survey stripes, covering a combined area of about 0.66 deg2, of which 0.45 deg2 have at least 20 hr of integration time. SMUVS reaches point-source sensitivities of about 25.0 AB mag (0.13 Jy) at both 3.6 and 4.5 m, with a significance of 4 , accounting for both survey sensitivity and source confusion. To this limit the SMUVS catalogs contain a total of ∼350,000 sources, each of which is detected significantly in at least one IRAC band. Because of its uniform and high sensitivity, relatively large area coverage, and the wide array of ancillary data available in COSMOS, the SMUVS survey will be useful for a large number of cosmological investigations. We make all images and catalogs described herein publicly available via the Spitzer Science Center.
This paper describes new deep 3.6 and 4.5 μ m imaging of three UltraVISTA near-infrared survey stripes within the COSMOS field. The observations were carried out with Spitzer ’ s Infrared Array Camera (IRAC) for the Spitzer Matching Survey of the UltraVISTA Deep Stripes (SMUVS). In this work we present our data reduction techniques, and document the resulting mosaics, coverage maps, and catalogs in both IRAC passbands for the three easternmost UltraVISTA survey stripes, covering a combined area of about 0.66 deg 2 , of which 0.45 deg 2 have at least 20 hr of integration time. SMUVS reaches point-source sensitivities of about 25.0 AB mag (0.13 μ Jy) at both 3.6 and 4.5 μ m, with a significance of 4 σ , accounting for both survey sensitivity and source confusion. To this limit the SMUVS catalogs contain a total of ∼350,000 sources, each of which is detected significantly in at least one IRAC band. Because of its uniform and high sensitivity, relatively large area coverage, and the wide array of ancillary data available in COSMOS, the SMUVS survey will be useful for a large number of cosmological investigations. We make all images and catalogs described herein publicly available via the Spitzer Science Center.
Author Ashby, M. L. N.
Muzzin, Adam
Milvang-Jensen, Bo
Caputi, Karina I.
McCracken, H. J.
Fèvre, Olivier Le
Deshmukh, Smaran
Dunlop, James S.
Fynbo, Johan P. U.
Huang, Jia-Sheng
Zhang, J.
Cowley, Will
Author_xml – sequence: 1
  givenname: M. L. N.
  orcidid: 0000-0002-3993-0745
  surname: Ashby
  fullname: Ashby, M. L. N.
  email: mashby@cfa.harvard.edu
  organization: Cambridge Harvard-Smithsonian Center for Astrophysics, Optical and Infrared Astronomy Division, 60 Garden Street, MS-66, MA 02138, USA
– sequence: 2
  givenname: Karina I.
  orcidid: 0000-0001-8183-1460
  surname: Caputi
  fullname: Caputi, Karina I.
  organization: University of Copenhagen The Cosmic Dawn Centre, Niels Bohr Institute, Juliane Maries Vej 30, DK-2100, Copenhagen Ø, Denmark
– sequence: 3
  givenname: Will
  surname: Cowley
  fullname: Cowley, Will
  organization: University of Groningen Kapteyn Astronomical Institute, P.O. Box 800, 9700 AV Groningen, The Netherlands
– sequence: 4
  givenname: Smaran
  orcidid: 0000-0001-7264-6925
  surname: Deshmukh
  fullname: Deshmukh, Smaran
  organization: University of Groningen Kapteyn Astronomical Institute, P.O. Box 800, 9700 AV Groningen, The Netherlands
– sequence: 5
  givenname: James S.
  surname: Dunlop
  fullname: Dunlop, James S.
  organization: University of Edinburgh Institute for Astronomy, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK
– sequence: 6
  givenname: Bo
  orcidid: 0000-0002-2281-2785
  surname: Milvang-Jensen
  fullname: Milvang-Jensen, Bo
  organization: University of Copenhagen The Cosmic Dawn Centre, Niels Bohr Institute, Juliane Maries Vej 30, DK-2100, Copenhagen Ø, Denmark
– sequence: 7
  givenname: Johan P. U.
  orcidid: 0000-0002-8149-8298
  surname: Fynbo
  fullname: Fynbo, Johan P. U.
  organization: University of Copenhagen The Cosmic Dawn Centre, Niels Bohr Institute, Juliane Maries Vej 30, DK-2100, Copenhagen Ø, Denmark
– sequence: 8
  givenname: Adam
  orcidid: 0000-0002-9330-9108
  surname: Muzzin
  fullname: Muzzin, Adam
  organization: York University Department of Physics and Astronomy, 4700 Keele Street, Toronto, Ontario, MJ3 1P3, Canada
– sequence: 9
  givenname: H. J.
  orcidid: 0000-0002-9489-7765
  surname: McCracken
  fullname: McCracken, H. J.
  organization: Sorbonne Universitès Institut d'Astrophysique de Paris, UPMC Univ. Paris 6 et CNRS, UMR 7095, 98 bis bd Arago, F-75014 Paris, France
– sequence: 10
  givenname: Olivier Le
  surname: Fèvre
  fullname: Fèvre, Olivier Le
  organization: Laboratoire d'Astrophysique de Marseille, 38, rue Frédéric Joliot-Curie, F-13388 Marseille cedex 13, France
– sequence: 11
  givenname: Jia-Sheng
  surname: Huang
  fullname: Huang, Jia-Sheng
  organization: Cambridge Harvard-Smithsonian Center for Astrophysics, Optical and Infrared Astronomy Division, 60 Garden Street, MS-66, MA 02138, USA
– sequence: 12
  givenname: J.
  surname: Zhang
  fullname: Zhang, J.
  organization: Harvard University , Cambridge, MA 02138, USA
BackLink https://hal.science/hal-01703657$$DView record in HAL
BookMark eNp9kFFr2zAUhUVpoWm39z4K9rLC3F5HluXsLYR2DSQU5qav4kaWEgXX8iQlkP362bi0UOie7uVwzuHwXZDTxjWakKsUbliRiduUsyLJWM5vEavMrE_I6E06JSOAXCQA2eScXISwAwDB2WRE6rK18a_2dIlRbW2zoeXeH_SROkPjVtNVHT0-z8un6fAmldYtLaO3rQ70e7lcPZfXP-n9vq6TFxuCdQ2d_57O6NIFtCpQbCo6w4i124Qv5MxgHfTX13tJVvd3T7OHZPH4az6bLhKVcYhJxQowFdNcrwvkJuVGYzbOWS4E4yydGDYBvc4RxjzV2qiCg1JYYKW4KNYK2CW5Hnq3WMvW2xf0R-nQyofpQvYapAI6LuKQdt5vg7f17s9ehyh3bu-bbp4cMy7yDlnWN8LgUt6F4LV5q01B9vxlD1v2sOXAv4vkHyLKRowdoA6jrf8X_DEErWvfx3xq_wcMRZmV
CitedBy_id crossref_primary_10_1051_0004_6361_202243100
crossref_primary_10_3847_1538_4357_ac312a
crossref_primary_10_1093_mnras_stab3242
crossref_primary_10_1093_mnras_stab432
crossref_primary_10_3847_1538_4365_ab75ed
crossref_primary_10_1093_mnras_stac3687
crossref_primary_10_1093_mnras_staf233
crossref_primary_10_1093_mnras_stae1956
crossref_primary_10_1093_mnras_staa3714
crossref_primary_10_3847_1538_4357_ad2c0b
crossref_primary_10_3847_1538_4365_ab42da
crossref_primary_10_1093_mnras_stac524
crossref_primary_10_1051_0004_6361_202348407
crossref_primary_10_3847_1538_4357_ac2b9f
crossref_primary_10_3847_1538_4365_ac3078
crossref_primary_10_1051_0004_6361_202449385
crossref_primary_10_3847_1538_4357_ac8747
crossref_primary_10_1093_mnras_stad3578
crossref_primary_10_1051_0004_6361_202449948
crossref_primary_10_3847_1538_4357_abb819
crossref_primary_10_1093_mnras_stad1919
crossref_primary_10_3847_1538_4357_ab089b
crossref_primary_10_3847_1538_4357_adb309
crossref_primary_10_1093_mnras_stad004
crossref_primary_10_1093_mnras_stae1441
crossref_primary_10_3847_1538_3881_acd773
crossref_primary_10_3847_2041_8213_acb773
crossref_primary_10_1051_0004_6361_202243950
crossref_primary_10_3847_1538_4357_ad8b1c
crossref_primary_10_3847_1538_4365_ac2498
crossref_primary_10_3847_1538_4357_ac53a9
crossref_primary_10_3847_1538_4357_ac1bb6
crossref_primary_10_1088_1538_3873_aae796
crossref_primary_10_3847_1538_4357_aad9f5
crossref_primary_10_1038_s41550_020_1104_5
crossref_primary_10_3847_1538_4357_ad023c
crossref_primary_10_1051_0004_6361_202142361
crossref_primary_10_1093_mnras_stac2140
crossref_primary_10_1051_0004_6361_202243088
crossref_primary_10_3847_1538_4357_ace10c
crossref_primary_10_3847_1538_4357_ac4605
crossref_primary_10_1093_mnras_stab731
crossref_primary_10_3847_1538_4357_ab3792
crossref_primary_10_1093_mnras_stac2291
crossref_primary_10_3847_1538_4357_abd6c1
crossref_primary_10_3847_1538_4357_ad5e78
crossref_primary_10_3847_1538_4357_ac5a4a
crossref_primary_10_1093_mnras_staa3370
crossref_primary_10_3847_1538_4357_ad86c2
crossref_primary_10_1093_mnras_stae510
crossref_primary_10_3847_1538_4357_ac5d39
crossref_primary_10_1051_0004_6361_201935782
crossref_primary_10_1093_mnras_stac737
crossref_primary_10_1093_mnras_stae118
crossref_primary_10_1093_mnras_sty2368
crossref_primary_10_3847_1538_4357_abc7c4
crossref_primary_10_1093_mnras_stab1956
crossref_primary_10_1093_mnras_stad1300
crossref_primary_10_1093_mnras_stz1038
Cites_doi 10.1117/12.857105
10.1051/0004-6361/201321814
10.1086/498708
10.1086/175659
10.1086/516585
10.1088/0067-0049/209/2/22
10.1086/422816
10.1088/0004-637X/803/1/11
10.1051/0004-6361/201219507
10.1086/422992
10.1086/376850
10.3847/0067-0049/225/1/1
10.1088/0067-0049/218/2/33
10.1088/0004-637X/701/1/428
10.1086/319728
10.1088/0004-637X/810/1/73
10.1086/116560
10.1086/422843
10.1086/116878
10.1086/306381
10.1051/0004-6361/201321100
10.1117/12.670018
10.1088/0004-637X/769/1/80
10.1111/j.1365-2966.2010.18118.x
10.1086/588583
10.1117/12.390377
10.1086/432523
10.1117/12.2233804
10.1086/423321
10.1088/0004-637X/709/2/644
10.1088/0004-637X/752/2/113
10.1086/499493
10.1088/0004-637X/788/2/126
10.1088/0004-6256/145/2/44
10.1086/430047
10.1142/S0218271814300158
10.1086/520086
10.1086/666945
10.1088/0004-637X/727/1/1
10.1088/0067-0049/185/1/85
10.3847/0067-0049/224/2/24
10.1086/422585
10.1086/507511
10.1088/0004-637X/768/2/103
10.3847/1538-4357/aa901e
10.1111/j.1365-2966.2008.13805.x
10.1038/nature07648
10.1086/191733
10.1086/319450
10.1086/375772
10.1086/517885
10.1088/2041-8205/791/2/L25
10.3847/0067-0049/224/2/28
10.1088/0004-637X/756/1/71
10.1117/12.673134
10.1086/423206
10.1086/420885
10.1088/0004-637X/777/1/18
10.1088/2041-8205/777/2/L19
ContentType Journal Article
Copyright 2018. The American Astronomical Society. All rights reserved.
Copyright IOP Publishing Aug 2018
Attribution
Copyright_xml – notice: 2018. The American Astronomical Society. All rights reserved.
– notice: Copyright IOP Publishing Aug 2018
– notice: Attribution
DBID AAYXX
CITATION
7TG
8FD
H8D
KL.
L7M
1XC
VOOES
DOI 10.3847/1538-4365/aad4fb
DatabaseName CrossRef
Meteorological & Geoastrophysical Abstracts
Technology Research Database
Aerospace Database
Meteorological & Geoastrophysical Abstracts - Academic
Advanced Technologies Database with Aerospace
Hyper Article en Ligne (HAL)
Hyper Article en Ligne (HAL) (Open Access)
DatabaseTitle CrossRef
Aerospace Database
Meteorological & Geoastrophysical Abstracts
Technology Research Database
Advanced Technologies Database with Aerospace
Meteorological & Geoastrophysical Abstracts - Academic
DatabaseTitleList Aerospace Database


CrossRef
DeliveryMethod fulltext_linktorsrc
Discipline Astronomy & Astrophysics
Physics
DocumentTitleAlternate Spitzer Matching Survey of the UltraVISTA Ultra-deep Stripes (SMUVS): Full-mission IRAC Mosaics and Catalogs
EISSN 1538-4365
ExternalDocumentID oai_HAL_hal_01703657v1
10_3847_1538_4365_aad4fb
apjsaad4fb
GroupedDBID -~X
123
1JI
23N
4.4
6J9
85S
AAFWJ
AAGCD
AAJIO
ABCQX
ABHWH
ACBEA
ACGFO
ACGFS
ACHIP
ADACN
AEFHF
AENEX
AFPKN
AKPSB
ALMA_UNASSIGNED_HOLDINGS
ASPBG
ATQHT
AVWKF
AZFZN
CJUJL
CRLBU
E3Z
EBS
EJD
F5P
FRP
GROUPED_DOAJ
IJHAN
IOP
KOT
L7B
M~E
N5L
O3W
O43
OK1
P2P
PJBAE
RIN
RNP
RNS
ROL
SY9
T37
UPT
AAYXX
CITATION
7TG
8FD
AEINN
H8D
KL.
L7M
1XC
2WC
6TJ
ADIYS
AI.
MVM
OHT
VH1
VOH
VOOES
ID FETCH-LOGICAL-c450t-d380fd3e5eb8a5f15fea426367735319f390eb6a0251eefc850cca8adc578bc03
IEDL.DBID IOP
ISSN 0067-0049
IngestDate Sat Sep 27 06:20:32 EDT 2025
Wed Aug 13 08:17:02 EDT 2025
Thu Apr 24 23:09:04 EDT 2025
Tue Jul 01 00:17:57 EDT 2025
Wed Aug 21 03:33:56 EDT 2024
IsDoiOpenAccess true
IsOpenAccess true
IsPeerReviewed true
IsScholarly true
Issue 2
Keywords surveys
catalogs
infrared: galaxies
Language English
License Attribution: http://creativecommons.org/licenses/by
LinkModel DirectLink
MergedId FETCHMERGED-LOGICAL-c450t-d380fd3e5eb8a5f15fea426367735319f390eb6a0251eefc850cca8adc578bc03
Notes AAS08731
Galaxies and Cosmology
ObjectType-Article-1
SourceType-Scholarly Journals-1
ObjectType-Feature-2
content type line 14
ORCID 0000-0002-3993-0745
0000-0001-8183-1460
0000-0002-9489-7765
0000-0002-2281-2785
0000-0002-8149-8298
0000-0001-7264-6925
0000-0002-9330-9108
OpenAccessLink https://hal.science/hal-01703657
PQID 2357604940
PQPubID 4562442
PageCount 13
ParticipantIDs hal_primary_oai_HAL_hal_01703657v1
iop_journals_10_3847_1538_4365_aad4fb
crossref_primary_10_3847_1538_4365_aad4fb
proquest_journals_2357604940
crossref_citationtrail_10_3847_1538_4365_aad4fb
ProviderPackageCode CITATION
AAYXX
PublicationCentury 2000
PublicationDate 2018-08-01
PublicationDateYYYYMMDD 2018-08-01
PublicationDate_xml – month: 08
  year: 2018
  text: 2018-08-01
  day: 01
PublicationDecade 2010
PublicationPlace Saskatoon
PublicationPlace_xml – name: Saskatoon
PublicationTitle The Astrophysical journal. Supplement series
PublicationTitleAbbrev APJS
PublicationTitleAlternate Astrophys. J. Suppl
PublicationYear 2018
Publisher The American Astronomical Society
IOP Publishing
American Astronomical Society
Publisher_xml – name: The American Astronomical Society
– name: IOP Publishing
– name: American Astronomical Society
References Scoville (apjsaad4fbbib50) 2007; 172
Werner (apjsaad4fbbib59) 2004; 154
Labbé (apjsaad4fbbib32) 2013; 777
Caputi (apjsaad4fbbib9) 2014; 23
Cohen (apjsaad4fbbib15) 1994; 107
Ilbert (apjsaad4fbbib29) 2010; 709
Mauduit (apjsaad4fbbib40) 2012; 124
Ashby (apjsaad4fbbib3) 2009; 701
Sánchez (apjsaad4fbbib47) 2017
Cohen (apjsaad4fbbib14) 1993; 105
Zacharias (apjsaad4fbbib60) 2013; 145
Lacy (apjsaad4fbbib33) 2004; 154
Arendt (apjsaad4fbbib1) 1998; 508
Papovich (apjsaad4fbbib44) 2016; 224
Ashby (apjsaad4fbbib5) 2015; 218
Ilbert (apjsaad4fbbib28) 2013; 556
Fazio (apjsaad4fbbib25) 2004b; 154
Lonsdale (apjsaad4fbbib36) 2004; 154
Shapley (apjsaad4fbbib51) 2006; 651
Sanders (apjsaad4fbbib48) 2007; 172
Hopkins (apjsaad4fbbib27) 2006; 163
Steidel (apjsaad4fbbib61a) 2003; 592
Milvang-Jensen (apjsaad4fbbib42) 2013; 560
Stern (apjsaad4fbbib56) 2005; 631
Caputi (apjsaad4fbbib8) 2013; 768
Dalton (apjsaad4fbbib17) 2006; 6269
Steinhardt (apjsaad4fbbib55) 2014; 791
Skrutskie (apjsaad4fbbib52) 2006; 131
Fazio (apjsaad4fbbib24) 2004a; 154
Caputi (apjsaad4fbbib10) 2011; 413
Dekel (apjsaad4fbbib19) 2009; 457
Lonsdale (apjsaad4fbbib37) 2003; 115
Wainscoat (apjsaad4fbbib58) 1992; 83
Timlin (apjsaad4fbbib57) 2016; 225
Emerson (apjsaad4fbbib22) 2010; 7733
Helgason (apjsaad4fbbib26) 2012; 752
Caputi (apjsaad4fbbib13) 2014; 788
Krick (apjsaad4fbbib31) 2009; 185
Stefanon (apjsaad4fbbib54) 2015; 803
Lin (apjsaad4fbbib35) 2012; 756
Ashby (apjsaad4fbbib4) 2013b; 769
Schuster (apjsaad4fbbib49) 2006; 6270
Barmby (apjsaad4fbbib6) 2008; 177
Rowan-Robinson (apjsaad4fbbib46) 2001; 549
Damen (apjsaad4fbbib18) 2011; 727
Deshmukh (apjsaad4fbbib20) 2017
Malhotra (apjsaad4fbbib39) 2005; 626
McCracken (apjsaad4fbbib41) 2012; 544
Caputi (apjsaad4fbbib11) 2017; 849
Cohen (apjsaad4fbbib16) 1995; 444
Muzzin (apjsaad4fbbib43) 2013; 777
Fang (apjsaad4fbbib23) 2004; 154
Bell (apjsaad4fbbib7) 2001; 550
Laigle (apjsaad4fbbib34) 2016; 224
Caputi (apjsaad4fbbib12) 2015; 810
Ashby (apjsaad4fbbib2) 2013a; 209
Somerville (apjsaad4fbbib53) 2008; 391
Lowrance (apjsaad4fbbib38) 2016; 9904
Diolaiti (apjsaad4fbbib21) 2000; 4007
Koekemoer (apjsaad4fbbib30) 2007; 172
Rix (apjsaad4fbbib45) 2004; 152
References_xml – volume: 7733
  start-page: 773306
  year: 2010
  ident: apjsaad4fbbib22
  publication-title: Proc. SPIE
  doi: 10.1117/12.857105
– volume: 560
  start-page: A94
  year: 2013
  ident: apjsaad4fbbib42
  publication-title: A&A
  doi: 10.1051/0004-6361/201321814
– volume: 131
  start-page: 1163
  year: 2006
  ident: apjsaad4fbbib52
  publication-title: AJ
  doi: 10.1086/498708
– volume: 444
  start-page: 874
  year: 1995
  ident: apjsaad4fbbib16
  publication-title: ApJ
  doi: 10.1086/175659
– volume: 172
  start-page: 1
  year: 2007
  ident: apjsaad4fbbib50
  publication-title: ApJS
  doi: 10.1086/516585
– volume: 209
  start-page: 22
  year: 2013a
  ident: apjsaad4fbbib2
  publication-title: ApJS
  doi: 10.1088/0067-0049/209/2/22
– volume: 154
  start-page: 166
  year: 2004
  ident: apjsaad4fbbib33
  publication-title: ApJS
  doi: 10.1086/422816
– year: 2017
  ident: apjsaad4fbbib47
– volume: 803
  start-page: 11
  year: 2015
  ident: apjsaad4fbbib54
  publication-title: ApJ
  doi: 10.1088/0004-637X/803/1/11
– volume: 544
  start-page: A156
  year: 2012
  ident: apjsaad4fbbib41
  publication-title: A&A
  doi: 10.1051/0004-6361/201219507
– volume: 154
  start-page: 1
  year: 2004
  ident: apjsaad4fbbib59
  publication-title: ApJS
  doi: 10.1086/422992
– volume: 115
  start-page: 897
  year: 2003
  ident: apjsaad4fbbib37
  publication-title: PASP
  doi: 10.1086/376850
– volume: 225
  start-page: 1
  year: 2016
  ident: apjsaad4fbbib57
  publication-title: ApJS
  doi: 10.3847/0067-0049/225/1/1
– volume: 218
  start-page: 33
  year: 2015
  ident: apjsaad4fbbib5
  publication-title: ApJS
  doi: 10.1088/0067-0049/218/2/33
– volume: 701
  start-page: 428
  year: 2009
  ident: apjsaad4fbbib3
  publication-title: ApJ
  doi: 10.1088/0004-637X/701/1/428
– volume: 550
  start-page: 212
  year: 2001
  ident: apjsaad4fbbib7
  publication-title: ApJ
  doi: 10.1086/319728
– volume: 810
  start-page: 73
  year: 2015
  ident: apjsaad4fbbib12
  publication-title: ApJ
  doi: 10.1088/0004-637X/810/1/73
– volume: 105
  start-page: 1860
  year: 1993
  ident: apjsaad4fbbib14
  publication-title: AJ
  doi: 10.1086/116560
– volume: 154
  start-page: 10
  year: 2004b
  ident: apjsaad4fbbib25
  publication-title: ApJS
  doi: 10.1086/422843
– volume: 107
  start-page: 582
  year: 1994
  ident: apjsaad4fbbib15
  publication-title: AJ
  doi: 10.1086/116878
– volume: 508
  start-page: 74
  year: 1998
  ident: apjsaad4fbbib1
  publication-title: ApJ
  doi: 10.1086/306381
– volume: 556
  start-page: A55
  year: 2013
  ident: apjsaad4fbbib28
  publication-title: A&A
  doi: 10.1051/0004-6361/201321100
– volume: 6269
  start-page: 62690X
  year: 2006
  ident: apjsaad4fbbib17
  publication-title: Proc. SPIE
  doi: 10.1117/12.670018
– volume: 769
  start-page: 80
  year: 2013b
  ident: apjsaad4fbbib4
  publication-title: ApJ
  doi: 10.1088/0004-637X/769/1/80
– volume: 413
  start-page: 162
  year: 2011
  ident: apjsaad4fbbib10
  publication-title: MNRAS
  doi: 10.1111/j.1365-2966.2010.18118.x
– volume: 177
  start-page: 431
  year: 2008
  ident: apjsaad4fbbib6
  publication-title: ApJS
  doi: 10.1086/588583
– volume: 4007
  start-page: 879
  year: 2000
  ident: apjsaad4fbbib21
  publication-title: Proc. SPIE
  doi: 10.1117/12.390377
– volume: 631
  start-page: 163
  year: 2005
  ident: apjsaad4fbbib56
  publication-title: ApJ
  doi: 10.1086/432523
– volume: 9904
  start-page: 99045Z
  year: 2016
  ident: apjsaad4fbbib38
  publication-title: Proc. SPIE
  doi: 10.1117/12.2233804
– volume: 154
  start-page: 35
  year: 2004
  ident: apjsaad4fbbib23
  publication-title: ApJS
  doi: 10.1086/423321
– volume: 709
  start-page: 644
  year: 2010
  ident: apjsaad4fbbib29
  publication-title: ApJ
  doi: 10.1088/0004-637X/709/2/644
– volume: 752
  start-page: 113
  year: 2012
  ident: apjsaad4fbbib26
  publication-title: ApJ
  doi: 10.1088/0004-637X/752/2/113
– volume: 163
  start-page: 50
  year: 2006
  ident: apjsaad4fbbib27
  publication-title: ApJS
  doi: 10.1086/499493
– volume: 788
  start-page: 126
  year: 2014
  ident: apjsaad4fbbib13
  publication-title: ApJ
  doi: 10.1088/0004-637X/788/2/126
– volume: 145
  start-page: 44
  year: 2013
  ident: apjsaad4fbbib60
  publication-title: AJ
  doi: 10.1088/0004-6256/145/2/44
– volume: 626
  start-page: 666
  year: 2005
  ident: apjsaad4fbbib39
  publication-title: ApJ
  doi: 10.1086/430047
– volume: 23
  start-page: 1430015
  year: 2014
  ident: apjsaad4fbbib9
  publication-title: IJMPD
  doi: 10.1142/S0218271814300158
– volume: 172
  start-page: 196
  year: 2007
  ident: apjsaad4fbbib30
  publication-title: ApJS
  doi: 10.1086/520086
– volume: 124
  start-page: 714
  year: 2012
  ident: apjsaad4fbbib40
  publication-title: PASP
  doi: 10.1086/666945
– volume: 727
  start-page: 1
  year: 2011
  ident: apjsaad4fbbib18
  publication-title: ApJ
  doi: 10.1088/0004-637X/727/1/1
– volume: 185
  start-page: 85
  year: 2009
  ident: apjsaad4fbbib31
  publication-title: ApJS
  doi: 10.1088/0067-0049/185/1/85
– volume: 224
  start-page: 24
  year: 2016
  ident: apjsaad4fbbib34
  publication-title: ApJS
  doi: 10.3847/0067-0049/224/2/24
– volume: 154
  start-page: 39
  year: 2004a
  ident: apjsaad4fbbib24
  publication-title: ApJS
  doi: 10.1086/422585
– volume: 651
  start-page: 688
  year: 2006
  ident: apjsaad4fbbib51
  publication-title: ApJ
  doi: 10.1086/507511
– volume: 768
  start-page: 103
  year: 2013
  ident: apjsaad4fbbib8
  publication-title: ApJ
  doi: 10.1088/0004-637X/768/2/103
– volume: 849
  start-page: 45
  year: 2017
  ident: apjsaad4fbbib11
  publication-title: ApJ
  doi: 10.3847/1538-4357/aa901e
– volume: 391
  start-page: 481
  year: 2008
  ident: apjsaad4fbbib53
  publication-title: MNRAS
  doi: 10.1111/j.1365-2966.2008.13805.x
– volume: 457
  start-page: 451
  year: 2009
  ident: apjsaad4fbbib19
  publication-title: Natur
  doi: 10.1038/nature07648
– volume: 83
  start-page: 111
  year: 1992
  ident: apjsaad4fbbib58
  publication-title: ApJS
  doi: 10.1086/191733
– volume: 549
  start-page: 745
  year: 2001
  ident: apjsaad4fbbib46
  publication-title: ApJ
  doi: 10.1086/319450
– volume: 592
  start-page: 728
  year: 2003
  ident: apjsaad4fbbib61a
  publication-title: ApJ
  doi: 10.1086/375772
– volume: 172
  start-page: 86
  year: 2007
  ident: apjsaad4fbbib48
  publication-title: ApJS
  doi: 10.1086/517885
– volume: 791
  start-page: L25
  year: 2014
  ident: apjsaad4fbbib55
  publication-title: ApJL
  doi: 10.1088/2041-8205/791/2/L25
– volume: 224
  start-page: 28
  year: 2016
  ident: apjsaad4fbbib44
  publication-title: ApJS
  doi: 10.3847/0067-0049/224/2/28
– volume: 756
  start-page: 71
  year: 2012
  ident: apjsaad4fbbib35
  publication-title: ApJ
  doi: 10.1088/0004-637X/756/1/71
– volume: 6270
  start-page: 65
  year: 2006
  ident: apjsaad4fbbib49
  publication-title: Proc. SPIE
  doi: 10.1117/12.673134
– volume: 154
  start-page: 54
  year: 2004
  ident: apjsaad4fbbib36
  publication-title: ApJS
  doi: 10.1086/423206
– year: 2017
  ident: apjsaad4fbbib20
– volume: 152
  start-page: 163
  year: 2004
  ident: apjsaad4fbbib45
  publication-title: ApJS
  doi: 10.1086/420885
– volume: 777
  start-page: 18
  year: 2013
  ident: apjsaad4fbbib43
  publication-title: ApJ
  doi: 10.1088/0004-637X/777/1/18
– volume: 777
  start-page: L19
  year: 2013
  ident: apjsaad4fbbib32
  publication-title: ApJL
  doi: 10.1088/2041-8205/777/2/L19
SSID ssj0007539
Score 2.5720375
Snippet This paper describes new deep 3.6 and 4.5 m imaging of three UltraVISTA near-infrared survey stripes within the COSMOS field. The observations were carried out...
This paper describes new deep 3.6 and 4.5 μ m imaging of three UltraVISTA near-infrared survey stripes within the COSMOS field. The observations were carried...
This paper describes new deep 3.6 and 4.5 μm imaging of three UltraVISTA near-infrared survey stripes within the COSMOS field. The observations were carried...
SourceID hal
proquest
crossref
iop
SourceType Open Access Repository
Aggregation Database
Enrichment Source
Index Database
Publisher
StartPage 39
SubjectTerms Arrays
Astrophysics
Data reduction
Infrared cameras
infrared: galaxies
Matching
Mosaics
Physics
Polls & surveys
Sensitivity
surveys
Title Spitzer Matching Survey of the UltraVISTA Ultra-deep Stripes (SMUVS): Full-mission IRAC Mosaics and Catalogs
URI https://iopscience.iop.org/article/10.3847/1538-4365/aad4fb
https://www.proquest.com/docview/2357604940
https://hal.science/hal-01703657
Volume 237
hasFullText 1
inHoldings 1
isFullTextHit
isPrint
link http://utb.summon.serialssolutions.com/2.0.0/link/0/eLvHCXMwnV3db9MwED-tQ0i88DFAKwxkIUDswW0yx0kKT1HF1CHKJrKOPSBFdmwLRGmqJp20_fXc1WkRH5oQL9EputjJ-e58d7F_BnhuVSpCZwY8NErzCANirstAcCMTE8WYEWlN-53HH-LRJHp3Ls-34M1mL0w1b11_D0kPFOxFSPYt0Jf2VzYaiVj2lTKR0x24IegkJdq9d3yyccPYrY990RNQHOz_Uf61hV_mpM4XWhHZwd7_cM-rOefwDnxev61favKtt2x0r7z6DcjxPz_nLtxuY1GWedZ7sGVnO7Cb1VQdr75fspdsRfviR70DN088dR-m-fxrc2UXbIyenGpYLF8uLuwlqxzDiJJNps1CnR3lp5knubF2zvIGPZSt2at8PDnL918zyn85KhpV7NjRx2zIxlWtsAemZoYNfWWpfgCTw7enwxFvz23gZSSDhhuRBs4IK61OlXShdFYRLnycJIJM3olBYHWsKL2x1pWpDFCPUmVKdB-kKQ9he1bN7C4wFcRqoA9MGmDeow7MIJGYH4bGmdIYJ-Mu9NcjV5QtqDmdrTEtMLkh8RYk3oLEW3jxdmF_88TcA3pcw_sMlWHDRkjco-x9QfcIdggZk4uwCy9waIvW9OtrGttba9NPZgIbigmiJ3j0j808hlsYs6V-DeIebDeLpX2CcVGjn670H6_H4tMP_rkGsw
linkProvider IOP Publishing
linkToPdf http://utb.summon.serialssolutions.com/2.0.0/link/0/eLvHCXMwpV3db9MwELfoEIgXPgZohQEWAsQe3CZznKS8RYWqhXVUZJ32FuzYFojSRE06afvruYvTIj40IfFmRRc7Od_9cnexfybkhZEx960eMF9LxQIIiJnKPc60iHQQQkakFO53nh6H43nw_kycteecNnthirKF_h40HVGwUyH6Nwcs7Tc-GvBQ9KXUgVX9UtsOuS64iNAzJx9nWyiGoV38C2iAsbD7T_nXXn75LnW-4KrIDjzBHxDdfHdGd8jnzRO75Sbfeuta9fLL38gc_-OV7pLbbUxKEyd-j1wzy12yl1RYJS--X9BXtGm7Iki1S27MXOs-WaTl1_rSrOgUEB1rWTRdr87NBS0shciSzhf1Sp5O0pPENZk2pqRpDUhlKvo6nc5P04M3FPNgBgaHlTs6-ZQM6bSoJIxA5VLToaswVQ_IfPTuZDhm7fkNLA-EVzPNY89qboRRsRTWF9ZI5IcPo4ij61s-8IwKJaY5xtg8Fh7YUyx1DjCCFvOQ7CyLpdkjVHqhHKhDHXuQ_8hDPYgE5Im-tjrX2oqwS_qb2cvyltwcz9hYZJDkoIozVHGGKs6cirvkYHtH6Yg9rpB9DgaxFUNG7nFylOE1pB8Cwejc75KXML1ZCwHVFZ3tbyzqpzCSDoVI1eM9-sdunpGbs7ej7Ghy_OExuQVhXOyWJe6TnXq1Nk8gVKrV08YdfgDM4Asj
openUrl ctx_ver=Z39.88-2004&ctx_enc=info%3Aofi%2Fenc%3AUTF-8&rfr_id=info%3Asid%2Fsummon.serialssolutions.com&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.atitle=Spitzer+Matching+Survey+of+the+UltraVISTA+Ultra-deep+Stripes+%28SMUVS%29%3A+Full-mission+IRAC+Mosaics+and+Catalogs&rft.jtitle=The+Astrophysical+journal.+Supplement+series&rft.au=Ashby%2C+M.+L.+N.&rft.au=Caputi%2C+Karina+I.&rft.au=Cowley%2C+Will&rft.au=Deshmukh%2C+Smaran&rft.date=2018-08-01&rft.pub=The+American+Astronomical+Society&rft.issn=0067-0049&rft.eissn=1538-4365&rft.volume=237&rft.issue=2&rft_id=info:doi/10.3847%2F1538-4365%2Faad4fb&rft.externalDocID=apjsaad4fb
thumbnail_l http://covers-cdn.summon.serialssolutions.com/index.aspx?isbn=/lc.gif&issn=0067-0049&client=summon
thumbnail_m http://covers-cdn.summon.serialssolutions.com/index.aspx?isbn=/mc.gif&issn=0067-0049&client=summon
thumbnail_s http://covers-cdn.summon.serialssolutions.com/index.aspx?isbn=/sc.gif&issn=0067-0049&client=summon