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Subaru Suprime-Cam DR2

About this page

This page provides access to the JVO Subaru Suprime-Cam mosaic image archive. The purpose of this archive is to provide quick look images taken by Subaru/Suprime-Cam. Those images were processed by a pipeline developed by JVO. Older data processed by the older pipeline are available at DR1 page.

Using the data for publication

All papers which make use of data taken with Subaru Telescope facilities should include the following acknowledgment on the title page as a footnote to the title.

"This research is based [in part] on data collected at Subaru Telescope, which is operated by the National Astronomical Observatory of Japan. We are honored and grateful for the opportunity of observing the Universe from Maunakea, which has the cultural, historical and natural significance in Hawaii."

More information on publication can be found at the Subaru web site Publishing Results from Subaru .

Please also include the following sentense on the title page as a footnote to the title or in the acknowledgment of the paper.

"[Part of] the data are retrieved from the JVO portal (http://jvo.nao.ac.jp/portal) operated by the NAOJ"

News

1. Search data of which the target name starts with:

A B C D E F G H I J K L M N O P Q R S T U V W X Y Z 0-9

or

2. Search data of which the target name matches the POSIX regular expression of:

Search Result (target name starts with "" )

Search data by sky coordinates or sky ID

Number per page :

Number of datasets :

Order by :

Condition :

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# Sky ID
 		Equatorial Coords
RA (deg) ~
Dec (deg) ~
Ra Dec Rad (deg) 		# of Data Filters Target names
1 000000+000000 0.000 0.000 1

VR

DJ26,F01,F02

2 000000+002400 0.000 0.400 1

VR

DJ25,DJ26,F01

3 000000-002400 0.000 -0.400 1

VR

DJ26,DJ27,F02

4 000000+004800 0.000 0.800 1

VR

DJ24,DJ25

5 000000-004800 0.000 -0.800 2

VR,r

DJ27,DJ28,NH0601

6 000000+011200 0.000 1.200 1

VR

DJ24,DJ25

7 000000-011200 0.000 -1.200 2

VR,r

DJ27,DJ28,NH0601

8 000000+013600 0.000 1.600 1

VR

DJ23,DJ24

9 000000-013600 0.000 -1.600 1

VR

DJ28,DJ29

10 000000+020000 0.000 2.000 1

VR

DJ23

11 000000-020000 0.000 -2.000 1

VR

DJ29

12 000000+022400 0.000 2.400 1

VR

DJ22,DJ23

13 000000-022400 0.000 -2.400 1

VR

DJ29,DJ30

14 000000+024800 0.000 2.800 1

VR

DJ21,DJ22

15 000000-024800 0.000 -2.800 1

VR

DJ30

16 000000+031200 0.000 3.200 1

VR

DJ21,DJ22

17 000000+033600 0.000 3.600 1

VR

DJ21

18 000000+064800 0.000 6.800 1

N0359

Q2359_1

19 000000+071200 0.000 7.200 1

N0359

Q2359_1

20 000000-151200 0.000 -15.200 4

B,V,I,i

WLM,WLM_2,Wolf-Lundmark-Melotte

21 000000-153600 0.000 -15.600 4

B,V,I,i

WLM,WLM_2,Wolf-Lundmark-Melotte

22 000000+231200 0.000 23.200 1

U

UGC12914

23 000000+233600 0.000 23.600 1

U

UGC12914

24 000000+444800 0.000 44.800 2

V,i

AndXVIII

25 000000+451200 0.000 45.200 2

V,i

AndXVIII

26 000136+000000 0.400 0.000 1

VR

DJ26,F01,F02,F03,F04

27 000136+002400 0.400 0.400 1

VR

DJ25,DJ26,F01,F04

28 000136-002400 0.400 -0.400 1

VR

DJ26,DJ27,F02,F03

29 000136+004800 0.400 0.800 1

VR

DJ24,DJ25

30 000136-004800 0.400 -0.800 2

VR,r

DJ27,DJ28,NH0601

31 000136+011200 0.400 1.200 1

VR

DJ24,DJ25

32 000136-011200 0.400 -1.200 2

VR,r

DJ27,DJ28,NH0601

33 000136+013600 0.400 1.600 1

VR

DJ23,DJ24

34 000136-013600 0.400 -1.600 1

VR

DJ28,DJ29

35 000136+020000 0.400 2.000 1

VR

DJ23

36 000136-020000 0.400 -2.000 1

VR

DJ29

37 000136+022400 0.400 2.400 1

VR

DJ22,DJ23

38 000136-022400 0.400 -2.400 1

VR

DJ29,DJ30

39 000136+024800 0.400 2.800 1

VR

DJ21,DJ22

40 000136-024800 0.400 -2.800 1

VR

DJ30

41 000136+031200 0.400 3.200 1

VR

DJ21,DJ22

42 000136+033600 0.400 3.600 1

VR

DJ21

43 000136-060000 0.400 -6.000 2

V,i

ABELL2697

44 000136-062400 0.400 -6.400 2

V,i

ABELL2697

45 000136+064800 0.400 6.800 1

N0359

Q2359_1

46 000136+071200 0.400 7.200 1

N0359

Q2359_1

47 000139-151200 0.412 -15.200 5

B,V,R,I,i

WLM,WLM_1,WLM_2,Wolf-Lundmark-Melotte

48 000139-153600 0.412 -15.600 5

B,V,R,I,i

WLM,WLM_1,WLM_2,Wolf-Lundmark-Melotte

49 000144+231200 0.433 23.200 1

U

UGC12914

50 000144+233600 0.433 23.600 1

U

UGC12914

51 000214+444800 0.558 44.800 2

V,i

AndXVIII

52 000215+451200 0.562 45.200 2

V,i

AndXVIII

53 000312+000000 0.800 0.000 1

VR

F03,F04

54 000312+002400 0.800 0.400 1

VR

F04

55 000312-002400 0.800 -0.400 2

VR,r

39315.0,F03

56 000312-004800 0.800 -0.800 1

r

39315.0

57 000312-024800 0.800 -2.800 1

r

36143.0

58 000312-031200 0.800 -3.200 1

r

36143.0

59 000312-060000 0.800 -6.000 2

V,i

ABELL2697

60 000313-062400 0.804 -6.400 2

V,i

ABELL2697

61 000313+064800 0.804 6.800 1

N0359

Q2359_1

62 000313+071200 0.804 7.200 1

N0359

Q2359_1

63 000318-151200 0.825 -15.200 5

B,V,R,I,i

WLM,WLM_1,WLM_2,Wolf-Lundmark-Melotte

64 000319-153600 0.829 -15.600 5

B,V,R,I,i

WLM,WLM_1,WLM_2,Wolf-Lundmark-Melotte

65 000429+444800 1.120 44.800 2

V,i

AndXVIII

66 000431+451200 1.129 45.200 2

V,i

AndXVIII

67 000448-002400 1.200 -0.400 1

r

39315.0

68 000448-004800 1.200 -0.800 1

r

39315.0

69 000448-024800 1.200 -2.800 1

r

36143.0

70 000448-031200 1.200 -3.200 1

r

36143.0

71 000449-060000 1.204 -6.000 2

V,i

ABELL2697

72 000449-062400 1.204 -6.400 2

V,i

ABELL2697

73 000457-151200 1.237 -15.200 2

V,I

WLM_1,WLM_EXTERNAL

74 000458-153600 1.241 -15.600 2

V,I

WLM_1,WLM_EXTERNAL

75 000549+344800 1.454 34.800 2

V,i

AndXX

76 000551+351200 1.462 35.200 2

V,i

AndXX

77 000624-002400 1.600 -0.400 1

r

39315.0

78 000624-004800 1.600 -0.800 1

r

39315.0

79 000624-024800 1.600 -2.800 1

r

36143.0

80 000624-031200 1.600 -3.200 1

r

36143.0

81 000637-151200 1.654 -15.200 2

V,I

WLM_EXTERNAL

82 000638-153600 1.658 -15.600 2

V,I

WLM_EXTERNAL

83 000650+453600 1.708 45.600 2

V,I

Minor_15

84 000746+344800 1.941 34.800 2

V,i

AndXX

85 000748+351200 1.950 35.200 2

V,i

AndXX

86 000802+064800 2.008 6.800 1

V

24952_Oct3_8UT,24952_Oct4_8UT

87 000803+071200 2.012 7.200 1

V

24952_Oct3_8UT,24952_Oct4_8UT

88 000806-093600 2.024 -9.600 1

r

26691.0

89 000807-100000 2.029 -10.000 1

r

26691.0

90 000816-151200 2.066 -15.200 1

V

WLM_EXTERNAL

91 000817-153600 2.070 -15.600 1

V

WLM_EXTERNAL

92 000902+451200 2.258 45.200 1

V

Minor_15

93 000906+453600 2.275 45.600 1

V

Minor_14,Minor_15

94 000910+460000 2.291 46.000 1

V

Minor_15

95 000936+000000 2.400 0.000 1

VR

Rec1,Rec2

96 000936+002400 2.400 0.400 1

VR

Rec1,Rec2

97 000937-042400 2.404 -4.400 1

r

33613.0

98 000937-044800 2.404 -4.800 1

r

33613.0

99 000937-051200 2.404 -5.200 1

r

33613.0

100 000939+064800 2.412 6.800 1

V

24952_Oct3_8UT,24952_Oct4_8UT

1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53 54 55 56 57 58 59 60 61 62 63 64 65 66 67 68 69 70 71 72 73 74 75 76 77 78 79 80 81 82 83 84 85 86 87 88 89 90 91 92 93 94 95 96 97 98 99 100 101 102 103 104 105 106 107 108 109 110 111 112 113 114 115 116 117 118 119 120 121 122 Next

Criteria unchecked in the checkbox are ignored.

1. Region of Interest

Center Coords or Target Name
Sample Format :
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2. Other Search Conditions

~* : comparator to test a matche with a POSIX regular expression, case insensitive.

e.g. (1) abc : contains abc, (2) ^abc : starts with abc, (3) (abc|def) : contains abc or def, (4) abc.*def : .* matches any sequence of zero or more characters

proc_id? ~* dataset_id? ~*
data_id? ~* obs_date? >= & <
target? ~* filter? =
center_ra? >= & < center_dec? >= & <
fcov? >= & < m50? >= & <
fwhm? >= & < m90? >= & <
photo_sig? >= & < mpk? >= & <
dr? = mlimit_chi2? >= & <

  • DR2.1 was released. Images of DR2.1 were created by stacking only the CCD images taken under better (not the best) photometric condition than those used for DR2.0 images. DR2.0 images are still available from the form in the advanced search tab. (2020-10-16)

Suprime-Cam Mosaic Data Archive

  • The purpose of this archive is to provide quick look images taken by Subaru/Suprime-Cam.
  • These data were processed by an automated data reduction pipeline developed by JVO.
  • Astrometric and photometric calibration was made by using Pan-STARRS1 DR2 catalog.
  • The entire sky is divided into small patches of sky region with an area of 0.42x0.42 deg^2 and mosaic images were created at each sky region.
  • Only CCD data taken with good quality (seeing < 1.2 arcsec, number of detected sources >= 100 for each CCD etc.) were used for creating a mosaic image.
  • Flat fielding was performed by using a master flat frame which was calculated for each combination of CCD and filter by using object data taken on various dates.
  • Metadata of all the mosaic data and URLs to retrieve the data are described in mosaic-meta-201014.psv.gz.
  • Statistical information of the data set is described in "Statistical information" page. The typical FWHM of the point spread function is 1.0", astrometric accuracy is 0.13", and photometric accuracy is 0.1 mag. The photometric accuracy depends on the observed wavelength; It gets worse at shorter wavelengths, e.g. 0.5 mag for W-J-U and 0.35 for N-B-L359 etc.. .
  • Our pipeline makes use of SDFRED1, SDFRED2, FTOOLS, SExtractor, SCAMP, SWarp, and ROOT. The GUI of our archive system makes use of Aladin Lite. We would like to thank the developers of those software for making them available to the public.
  • Should you have any questions please feel free to contact us at : .

JVO Suprime-Cam HiPS service

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Image data collected by other facilities