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

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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).

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