Hierarchical progressive surveys - Multi-resolution HEALPix data structures for astronomical images, catalogues, and 3-dimensional data cubes

P. Fernique; M. G. Allen; T. Boch; A. Oberto; F-X. Pineau; D. Durand; C. Bot; L. Cambrésy; S. Derriere; F. Genova; F. Bonnarel

doi:10.1051/0004-6361/201526075

Home

All issues

Volume 578 (June 2015)

A&A, 578 (2015) A114

Full HTML

Highlight

Free Access

Table 3

HiPS images.

ID^a	Data set name and description	k_tile	θ_pix	Sky
				(%)


– Gamma Ray –

P/Fermi^E^b^c^d ............	Fermi⁽¹⁾: 4 HiPS in 3–300 MeV, 300–1000 MeV,	3	6.́87	100%
	and 1–3 GeV and a colour composite (n_tile = 64)
P/EGRET^E^b^c^d ............	EGRET⁽²⁾: 12 HiPS for 100 MeV inf and sup maps, and	3	51.̋5	100%
	diffuse maps 30–50, 50–70, 70–100, 100–150, 150–300,
	300–500, 500–1000 MeV, 1–2 GeV, 2–4 GeV, 4–10 GeV


– X-ray –

P/XMM^E^e^f ............	XMM-Newton: 5 HiPS for EPIC stacked images, PN	7	3.̋22	7%
	in 0.5–1, 1–2, and 2–4.5 keV bands and PN colour
P/INTEGRAL^E^g,^c,^d ............	INTEGRAL⁽³⁾ SPI GC (20–40 keV)	3	51.̋5	17%
P/INTGAL^E^c,^d,^h ............	INTEGRAL IBIS⁽⁴⁾: 4 HiPS for 17–35, 17–60,	3	51.̋5	31%
	35–80 keV, and colour composition
P/RASS^G,^c,^d,ⁱ ............	ROSAT X-Ray All Sky Survey⁽⁵⁾	4	25.̋8	100%


– Ultraviolet –

P/GALEXGR6^E^c,^d,^j ............	GALEX⁽⁶⁾ : Colour composition of GR6 AIS	8	1.̋61	69%


– Optical –

P/DSS2^E,^c,^d,^j ............	DSS2: 2 HiPS for red band and colour composite	9	0.̋81	100%
P/SDSS9^E,^c,^d,^k ............	SDSS DR9⁽⁷⁾: 3 HiPS for r, g, and a colour composite	10	0.̋4	36%
P/Mellinger/color^E,^c,^d,^m ............	Mellinger optical survey	4	25.̋77	100%
P/CFHTLS/D^E,^c,^d,ⁿ ............	CFHTLS⁽⁸⁾ Deep : 6 HiPS for u,g,r,i,z, and colour	12	0.̋1	0.01%
P/CFHTLS/W^E,^c,^d,ⁿ ............	CFHTLS⁽⁸⁾ Wide : 6 HiPS for u,g,r,i,z, and colour	11	0.̋2	0.4%
P/HST^E,^d,^p,^q ............	HST: 17 HiPS for NICMOS, WFPC2, and ACS in	14	25.1 mas	0.044%
	F110W, F160W, F225W, F300W, F450W, F606W,
	F625W, F702W, F814W, F850LP, and GOODS⁽⁹⁾
	associations in b,v,i,z, and colour


– Infrared –

P/2MASS^E,^c,^d,^r ............	2MASS⁽¹⁰⁾: 4 HiPS for J, H, K, and colour	9	0.̋81	100%
P/2MASS6X^E,^c,^d,^r ............	2MASS6X: 3 HiPS for J, H, and K	9	0.̋81	1.32%
P/ULTRAVISTA^E
^c,^d,^s ............	VISTA Ultra Deep Survey⁽¹¹⁾: 6 HiPS for Y, J,	12	0.̋1	0.005%
	H, Ks, NB118, and colour
P/WISE^E,^c,^d,^r ............	WISE⁽¹²⁾: 5 HiPS for 3.4, 4.6, 12, 22 μm, and colour	5	12.̋9	100%
P/WISE/WSSA^E,^c,^d, ............	WSSA⁽¹³⁾ Diffuse dust emission at 12 μm	7	3.̋22	100%
P/ALLWISE^E,^c,^d,^r ............	ALLWISE⁽¹⁴⁾: 5 HiPS for 3.4, 4.6, 12, 22 μm, and colour	8	1.̋61	100%
P/DIRBE^G,^u,^v ............	DIRBE⁽¹⁵⁾: 20 HiPS for bands 1–10 and ZSMA bands 1–10	3	51.̋5	100%
P/IRIS^G,^u,^v,^r ............	IRAS-IRIS⁽¹⁶⁾: 4 HiPS for 12, 25, 60, and 100 μm	3	51.̋5	100%
P/IRIS^G,^c,^d,^r ............	IRAS-IRIS⁽¹⁶⁾: HiPS colour composition	3	51.̋5	100%
P/GLIMPSE360^E,^r,^w,^x,^z ............	GLIMPSE 360^(17,18): colour	9	0.̋81	3.1%
P/SPITZER/IRAC^c,^d,^y,^x ............	Spitzer IRAC: 5 HiPS for the 3.6, 4.5, 5.8,	9	0.̋81	1.4%
	8 μm, and colour bands
P/SPITZER/MIPS1^G,^c,^d,^y,^x ............	Spitzer MIPS1⁽²²⁾ 24 μm band	8	1.̋61	1.6%
P/SPITZER/MIPS2^G,^c,^d,^y,^x ............	Spitzer MIPS2⁽²²⁾ 70 μm band	7	3.̋22	1.6%
P/SPITZER/MIPS3^G,^c,^d,^y,^x ............	Spitzer MIPS3⁽²²⁾ 160 μm band	6	6.̋44	1.6%
P/AKARI/FIS^E,^c,^d,^α ............	AKARI⁽²³⁾ Far infrared all-sky survey: 5 HiPS for N60,	5	12.̋9	99.9%
	N160, WideS, WideL, and colour


– Sub-mm and radio –

P/SCUBA/450em^E,^c,^d,^β ............	SCUBA 450⁽²⁴⁾μm	8	1.̋61	0.3%
P/SCUBA/850em^E,^c,^d,^β ............	SCUBA 850⁽²⁴⁾μm	7	3.̋22	0.9%
P/SCUBA/850emi^E,^c,^d,^β ............	SCUBA 850^(24,47)μm extended data set	7	3.̋22	0.9%
P/SCUBA2^E,^d,^γ ............	SCUBA-2⁽²⁵⁾ : 2 HiPS for 450 and 850 μm	9	0.̋81	1.8%
P/BOLOCAM^G,^u,^v ............	Bolocam Galactic plane survey⁽²⁶⁾ (BGPS)	5	12.̋9	2%
P/WMAP^G,^c,^d,^δ ............	WMAP Year 9 results⁽²⁷⁾: 5 HiPS for W, V, Q, Ka, and K	3	6.́87	100%
	(n_tile = 64)
P/PLANCK/HFI^G,^c,^d,^ϵ ............	PLANCK⁽²⁸⁾ (2013 data release): 6 HiPS for HFI in HFI100,	3	1.́72	100%
	143, 217, 353, 545, 857 GHz, and colour (n_tile = 256)
P/PLANCK/LFI^G,^c,^d,^ϵ ............	PLANCK⁽²⁸⁾ (2013 data release): 4 HiPS for LFI in 1030,	3	3.́44	100%
	1044, 1070 GHz, and colour (n_tile = 256)
P/PLANCK/CMB^G,^c,^d,^ϵ ............	PLANCK CMB fluctuations map (SMICA inpainted)	3	1.́72	100%
	(n_tile = 256)
P/NVSS^E,^c,^d,^ζ ............	The NRAO VLA Sky Survey⁽²⁹⁾	5	12.88	84.8%
P/CHIPASS^G,^u,^v ............	CHIPASS⁽³⁰⁾ 1.4 GHz Radio continuum survey	3	51.̋5	72%
P/SUMSS^E,^c,^d ............	Sydney University Molonglo sky survey^(31,32) 843 MHz	6	6.̋44	25%
P/DWINGELOO^G,^u,^v ............	Dwingeloo 820 MHz continuum survey⁽³³⁾	3	51.̋5	57%
P/HASLAM408^G,^η^θ^d ............	Haslam 408 MHz survey: 2 HiPS for original⁽³⁴⁾	3	51.̋5	100%
	and reprocessed⁽³⁵⁾ data
P/VLSSR^E,^c,^d,^ζ ............	VLA low-frequency sky survey redux⁽³⁶⁾	5	12.̋9	75%
	(74 MHz continuum)
P/WENSS^E,^c,^d,^κ ............	Westerbork northern sky survey⁽³⁷⁾ (325 MHz)	5	12.88	26.9%


– H α –

P/Finkbeiner^G,^c,^d,^λ ............	Finkbeiner Hα composite survey⁽³⁸⁾	3	51.̋5	100%
P/SHS^E,^c,^d,^μ ............	SuperCOSMOS digitized photographic Hα Survey⁽³⁹⁾	10	0.̋4	9.8%
P/SHASSA^G,^c,^d,^ξ ............	SHASSA southern Hα sky survey atlas⁽⁴⁰⁾: 4 HiPS for	4	25.̋77	67%
	Hα, continuum, continuum-corrected, Hα
	and smoothed Hα images
P/VTSS^G,^c,^d,^π ............	Virginia Tech spectral line survey⁽⁴¹⁾: 2 HiPS for	3	51.̋5	20%
	Hα and continuum corrected Hα


– HI –

P/GASS^G,^c,^d,^ρ ............	Parkes Galactic all sky survey⁽⁴²⁾ (GASS) (n_tile = 64)	3	6.́87	53%
P/GASS/NH^G,^u,^v,^ρ ............	Parkes Galactic all sky survey⁽⁴²⁾ (GASS) (n_tile = 128)	3	3.́44	53%
P/CGPS/VGPS^G,^u,^v,^σ^τ ............	Combination CGPS⁽⁴³⁾ and VGPS⁽⁴⁴⁾: 2 HiPS for	4	25.̋8	3.9%
	1420 MHz continuum and HI


– CO –

P/CO^G,^d,^δ ............	CO composite survey⁽⁴⁵⁾	3	51.̋5	100%
P/COHRS^E,^c,^d,^δ ............	CO high resolution survey⁽⁴⁶⁾ (HARP/JCMT)	7	3.̋22	0.15%

Notes.

^(E)

Equatorial (ICRS) coordinate system HiPS;

^(G)

Galactic coordinate system HiPS;

^(a)

CDS identifier for the HiPS data set;

^(b)

Original data distributed by SkyView/HEASARC;

^(c)

HEALPixed by CDS;

^(d)

HiPS distributed by CDS;

^(e)

HEALPixed by Laurent Michel (Observatoire de Strasbourg);

^(f)

HiPS distributed by XMM-Newton science survey consortium, EC FP7 ARCHES project;

^(g)

Original data distributed by INTEGRAL Science Data Centre, Geneva;

^(h)

Original data distributed by Space Research Institute (IKI), Moscow;

⁽ⁱ⁾

Original data distributed by Max Planck Institut fur extraterrestrische Physik;

^(j)

Original data distributed by MAST at STScI;

^(k)

Original data distributed by the SLOAN Digital Sky Survey;

^(m)

Original data (c) Axel Mellinger;

⁽ⁿ⁾

Original data (c) CFH – powered by Terapix;

^(p)

Processed data from CADC;

^(q)

HEALPixed by Daniel Durand (CADC);

^(r)

Original data distributed by IPAC/NASA Infrared Science Archive (IRSA);

^(s)

Original data distributed by the UltraVISTA consortium;

^(u)

HiPS distributed by Analysis Centre for Extended Data (CADE), IRAP Toulouse;

^(v)

HEALPixed by D. Paradis, CADE, IRAP Toulouse;

^(w)

HEALPixed by Robitaille;

^(x)

Original data from Spitzer mission, JPL/NASA;

^(y)

Composite from Spitzer legacy programs: GLIMPSE (17,18), SAGE (19), SAGE-SMC (20) and SINGS (21);

^(z)

HiPS distributed by Spitzer mission, JPL/NASA;

^(α)

Original data distributed by ISAS, JAXA, Japan;

^(β)

Processed data obtained from CADC;

^(γ)

HiPS built from JCMT data via CADC archive;

^(δ)

Original data from LAMBDA;

^(ϵ)

Original data from PLANCK mission at ESA;

^(ζ)

Original data from NRAO;

^(η)

Data distributed and maintained by LAMBDA, who cite Jodrell Bank Centre for Astrophyscis as the original data source;

^(θ)

Reprocessed data described in (35) including details of various versions of the 408 MHz Haslam map;

^(κ)

Original data from WENSS at ASTRON in The Netherlands;

^(λ)

Composed by VTSS (Virginia Tech spectral line survey), SHASSA (Southern Hα sky survey atlas), WHAM (Wisconsin Hα mapper);

^(μ)

Original data courtesy of WFAU, AAO/UKST, PPARC/STFC;

^(ξ)

Original data from Swarthmore College Incorporated and available from NASA/Skyview;

^(π)

Original data from Virginia Tech Physics;

^(ρ)

Original data from CSIRO/ATNF;

^(σ)

Original VGPS data from University of Calgary and CADC;

^(τ)

Original CGPS data from Canadian Galactic plane consortium and available from CADC.

Reference. (1) Atwood et al. (2009); (2) Cillis & Hartman (2005); (3) Winkler et al. (2003); (4) Krivonos et al. (2012); (5) Voges (1992); (6) Martin et al. (2005); (7) Ahn et al. (2012); (8) see CFHTLS in the acknowledgements; (9) Giavalisco et al. (2004); (10) Skrutskie et al. (2006); (11) McCracken et al. (2012); (12) Wright et al. (2010); (13) Meisner & Finkbeiner (2014); (14) Cutri et al. (2013); (15) Miville-Deschênes & Lagache (2005); (16) Boggess et al. (1992); (17) Benjamin et al. (2003); (18) Churchwell et al. (2009); (19) Meixner (2008); (20) Gordon et al. (2011); (21) Kennicutt et al. (2003); (22) Werner et al. (2004); (23) Murakami et al. (2007); (24) Holland et al. (1999); (25) Holland et al. (2013); (26) Aguirre et al. (2011); (27) Bennett et al. (2013); (28) Planck Collaboration I (2014); (29) Condon et al. (1998); (30) Calabretta et al. (2014); (31) Mauchet al. (2003); (32) Murphy et al. (2007); (33) Berkhuijsen (1972); (34) Haslam et al. (1982); (35) Remazeilles et al. (2014); (36) Lane et al. (2012); (37) Rengelink et al. (1997); (38) Finkbeiner (2003); (39) Parker et al. (2005); (40) Gaustad et al. (2001); (41) Dennison et al. (1999); (42) McClure-Griffiths et al. (2009); (43) (Taylor et al. 2003); (44) Stil et al. (2006); (45) Dame et al. (2001); (46) Dempsey et al. (2013); (47) Di Francesco et al. (2008).

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.