DARTS/Astro Query System - SQL Search -

All the tables available for SQL Search and information on each table are listed in the Available Data page. Please see the User Guide for the usage of "SQL Search".

Call example

【Basic Syntax】

 SELECT {*|column, column, column,..}
 FROM table name
 [ WHERE conditions ]
 [ ORDER BY column, column,... ]
 [ LIMIT {ALL|number} ] [ OFFSET number ]
 ;

---------------------------------------------------------

This is an example query to obtain the first 10 rows of 
akari_fis_bsc_1 using radial search.

The akari_fis_bsc_1 is an catalogue, and each data has 
the coorinate position of the object. So, search the objects 
contained in the circle area you specify there.

Columns to display -> all
  Table name -> akari_fis_bsc_1
  Search condition -> radial search, 
   center position is (266.0, -28,0) and radius is 10 arcmin
  Displayed results -> from 1st to 10th

---------------------------------------------------------
Point:
  You can use functions of PgSphere(https://pgsphere.github.io/)
  on this system.

Data types:
    Point   ... spoint(coordinate, coordinate)
    Path    ... spath(spoint(), spoint(), ...)
    Circle  ... scircle(spoint(), radius)
    Polygon ... spoly(spoint(), spoint(), ...)

Operators:
    a @ b = '1' ... a contained by b
    a !@ b = '1' ... a is not contained by b
    a && b = '1' ... overlaped each other
    a !&& b = '1' ... do not overlaped each other

Ths function radians needs a parameter in degree.
  Operator '/' means division. 
  Note: integer division truncates the result.
   10.0 / 60.0 = 0.16666...
   10 / 60 = 0

---------------------------------------------------------

This is an example query to obtain the first 10 rows of 
ginga_observation_log using radial search.

The ginga_observation_log has pointing observations and 
scan observation. Each data has the coorinate of the 
observation start point and the end point, and the 
average point. So, search the pointing position contained 
in the circle area you specified, or the scan-path crossed 
over the area.

Columns to display -> all
  Table name -> ginga_observation_log
  Search condition -> radial search,
  center position is M31(10.7, 41.2) and radius is 1 degree
  Displayed results -> from 1st to 10th

---------------------------------------------------------
Point:
  You can use functions of PgSphere(https://pgsphere.github.io/)
  on this system.

Data types:
    Point   ... spoint(coordinate, coordinate)
    Path    ... spath(spoint(), spoint(), ...)
    Circle  ... scircle(spoint(), radius)
    Polygon ... spoly(spoint(), spoint(), ...)

Operators:
    a @ b  ... a contained by b
    a !@ b ... a is not contained by b
    a && b ... overlaped each other
    a !&& b ... do not overlaped each other

---------------------------------------------------------

This is an example query to obtain the data near the 
galactic center of suzaku_xis_observation_log using radial search.

The SUZAKU XIS has rectanglar field of view with 18 arcmin 
x 18 arcmin. Each data of suzaku_xis_observation_log has 
the coorinate of each corner position about field of view.
So, search the rectanglar area overlapd the circle area 
you specified.

Columns to display -> all
  Table name -> suzaku_xis_observation_log
  Search condition -> radial search,
    center position is (0.0, 0.0) with Galactic coordinates
    and radius is 1 arcmin
  Displayed results -> from 1st to 200th

---------------------------------------------------------
Point:

1. Use the column of Galactic coordinates.

2. You can use functions of PgSphere(https://pgsphere.github.io/)
   on this system.

Data types:
    Point   ... spoint(coordinate, coordinate)
    Path    ... spath(spoint(), spoint(), ...)
    Circle  ... scircle(spoint(), radius)
    Polygon ... spoly(spoint(), spoint(), ...)

Operators:
    a @ b  ... a contained by b
    a !@ b ... a is not contained by b
    a && b ... overlaped each other
    a !&& b ... do not overlaped each other

---------------------------------------------------------

This is an example query to obtain the data nearthe 
galactic center of suzaku_xis_observation_log using radial search.

The SUZAKU XIS has rectanglar field of view with 18 arcmin 
x 18 arcmin. Each data of suzaku_xis_observation_log has the 
coorinate of each corner position about field of view. 
So, search the rectanglar area overlapd the rectanglar area 
you specified.

Columns to display -> object_name, center_galactic_lon, 
   center_galactic_lat, data_access_url
  Table name -> suzaku_xis_observation_log
  Search condition -> rectanglar search,
    0.1(deg) <= Galactic Latitude <= .0.1(deg)
    and 0.1(deg) <= Galactic Latitude <= 0.1(deg)
  Displayed results -> from 1st to 100th

---------------------------------------------------------
Point:
  You can use functions of PgSphere(https://pgsphere.github.io/)
  on this system.

Data types:
    Point   ... spoint(coordinate, coordinate)
    Path    ... spath(spoint(), spoint(), ...)
    Circle  ... scircle(spoint(), radius)
    Polygon ... spoly(spoint(), spoint(), ...)

Operators:
    a @ b  ... a contained by b
    a !@ b ... a is not contained by b
    a && b ... overlaped each other
    a !&& b ... do not overlaped each other

---------------------------------------------------------

This is an example query to obtain the first 10 rows of 
akari_fis_bsc_1 using radial search.

The akari_fis_bsc_1 is an catalogue, and each data has 
the coorinate position of the object. So, search the objects 
contained in the circle area you specify there.

Columns to display -> all
  Table name -> akari_fis_bsc_1
  Search condition -> radial search, 
   center position is (266.0, -28,0) and radius is 10 arcmin
  Displayed results -> from 1st to 10th

---------------------------------------------------------
Point:
  You can use functions of PgSphere(https://pgsphere.github.io/)
  on this system.

Data types:
    Point   ... spoint(coordinate, coordinate)
    Path    ... spath(spoint(), spoint(), ...)
    Circle  ... scircle(spoint(), radius)
    Polygon ... spoly(spoint(), spoint(), ...)

Operators:
    a @ b = '1' ... a contained by b
    a !@ b = '1' ... a is not contained by b
    a && b = '1' ... overlaped each other
    a !&& b = '1' ... do not overlaped each other

Ths function radians needs a parameter in degree.
  Operator '/' means division. 
  Note: integer division truncates the result.
   10.0 / 60.0 = 0.16666...
   10 / 60 = 0

---------------------------------------------------------

This is an example query to obtain the first 10 rows of 
ginga_observation_log using radial search.

---------------------------------------------------------
Point:
  You can use functions of PgSphere(https://pgsphere.github.io/)
  on this system.

Data types:
    Point   ... spoint(coordinate, coordinate)
    Path    ... spath(spoint(), spoint(), ...)
    Circle  ... scircle(spoint(), radius)
    Polygon ... spoly(spoint(), spoint(), ...)

Operators:
    a @ b  ... a contained by b
    a !@ b ... a is not contained by b
    a && b ... overlaped each other
    a !&& b ... do not overlaped each other

---------------------------------------------------------

This is an example query to obtain the data near the 
galactic center of suzaku_xis_observation_log using radial search.

---------------------------------------------------------
Point:

1. Use the column of Galactic coordinates.

2. You can use functions of PgSphere(https://pgsphere.github.io/)
   on this system.

Data types:
    Point   ... spoint(coordinate, coordinate)
    Path    ... spath(spoint(), spoint(), ...)
    Circle  ... scircle(spoint(), radius)
    Polygon ... spoly(spoint(), spoint(), ...)

Operators:
    a @ b  ... a contained by b
    a !@ b ... a is not contained by b
    a && b ... overlaped each other
    a !&& b ... do not overlaped each other

---------------------------------------------------------

This is an example query to obtain the data nearthe 
galactic center of suzaku_xis_observation_log using radial search.

The SUZAKU XIS has rectanglar field of view with 18 arcmin 
x 18 arcmin. Each data of suzaku_xis_observation_log has the 
coorinate of each corner position about field of view. 
So, search the rectanglar area overlapd the rectanglar area 
you specified.

---------------------------------------------------------
Point:
  You can use functions of PgSphere(https://pgsphere.github.io/)
  on this system.

Data types:
    Point   ... spoint(coordinate, coordinate)
    Path    ... spath(spoint(), spoint(), ...)
    Circle  ... scircle(spoint(), radius)
    Polygon ... spoly(spoint(), spoint(), ...)

Operators:
    a @ b  ... a contained by b
    a !@ b ... a is not contained by b
    a && b ... overlaped each other
    a !&& b ... do not overlaped each other

---------------------------------------------------------

SQL query

Format

total 38

Download WgetScript

No.	object_name	center_ra	center_dec	center_ra_b1950	center_dec_b1950	center_ecliptic_lon	center_ecliptic_lat	center_galactic_lon	center_galactic_lat	roll_angle	observation_start_time_mjd	observation_start_time	observation_end_time_mjd	observation_end_time	observation_id	exposure	awarded_exposure	xis0_exposure	xis1_exposure	xis2_exposure	xis3_exposure	xis0_observation_mode	xis1_observation_mode	xis2_observation_mode	xis3_observation_mode	hxd_observation_mode	hxd_coarse_clock_rate_exposure	hxd_first_clock_rate_exposure	hxd_normal_clock_rate_exposure	hxd_all_clock_rate_exposure	hxd_wam_exposure	quantity_of_hxd_burst	processing_status	processing_date_mjd	processing_date	public_date_mjd	public_date	distribution_date_mjd	distribution_date	processing_version	processing_count	processing_software	proposal_id	proposal_abstract	proposal_category	proposal_category_code	proposal_priority	pi_name	co_pi_name	proposal_affiliated_country	proposal_cycle	observation_type	proposal_title	main_instrument	has_xis_injection	data_access_url	ql_access_url	ql_image_url
1	A1914_OFFSET4	216.4138	37.6152	215.900162	37.839927	196.47734	48.33006	66.75628519	67.60183749	330.9949	55365.2958333333	2010-06-18 07:06:00	55366.115462963	2010-06-19 02:46:16	805094010	27.2904	40	27.2904	27.3001	0	27.2944	2	2	0	2	1	0	0	25.4203	25.4203	70.816	0	PROCESSED	57552.407037037	2016-06-13 09:46:08	55769	2011-07-27 00:00:00	55403.4672106482	2010-07-26 11:12:47	3.0.22.43	2	Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22	053087	We propose four pointing observations of the merging cluster Abell 1914 with exposure of 160 ks (40 ks each). We measure temperature, electron density, and entropy distributions of the ICM out to the virial radius to study the merging history of this cluster. We determine the supra-thermal component expected by the merger with a wide-band spectroscopy using XIS and HXD-PIN, and quantify heat input to the ICM by a joint analysis with weak lensing data of Subaru telescope. Then, we aim to estimate the energy ratio of the heat input to total delivered energy through the merger.	EXTRAGALACTIC DIFFUSE SOURCES	8	A	MADOKA KAWAHARADA	ERIC MILLER	JUS	5	AO5	THERMODYNAMICS OF INTRACLUSTER MEDIUM IN THE MERGING CLUSTER ABELL 1914	XIS	Y	https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/805094010/	Quick Look
2	A1750S	202.5548	-2.1063	201.910476	-1.848597	201.643103	6.819901	322.18359807	59.30814244	293.521	55751.0328009259	2011-07-09 00:47:14	55753.0002314815	2011-07-11 00:00:20	806097010	80.1668	80	80.1668	80.1668	0	80.1668	2	2	0	2	1	0	0	67.0448	67.0448	169.9618	3	PROCESSED	57602.5725578704	2016-08-02 13:44:29	56148	2012-08-09 00:00:00	55778.4321412037	2011-08-05 10:22:17	3.0.22.44	2	Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22	063019	We observe Abell 1750 which has three clusters of galaxies in a filamentary structure of the large-scale structure, with 4 pointing observations (80 x 3 + 40 ks). We reveal global spatial structures of temperature, density, and entropy in Abell 1750 for the first time. By a correlation with a galaxy map obtained from SDSS, and a comparison between thermal pressure and total pressure required by the total mass derived from weal lensing analysis, we explore the inflow of matter and evolutionary process in this system.	EXTRAGALACTIC DIFFUSE SOURCES	8	A	MADOKA KAWAHARADA	SCOTT RANDALL	JUS	6	AO6	SUZAKU OBSERVATION OF ABELL 1750 IN THE LARGE-SCALE STRUCTURE	XIS	Y	https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/806097010/	Quick Look
3	A1914_OFFSET1	216.5507	38.0175	216.039339	38.24183	196.32687	48.734523	67.63121502	67.35438204	324.9943	55362.5248148148	2010-06-15 12:35:44	55363.4724768518	2010-06-16 11:20:22	805091010	32.2034	40	32.2034	32.2034	0	32.2034	2	2	0	2	1	0	0	27.5086	27.5086	81.876	1	PROCESSED	57552.3572569445	2016-06-13 08:34:27	55766	2011-07-24 00:00:00	55399.2609722222	2010-07-22 06:15:48	3.0.22.43	2	Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22	053087	We propose four pointing observations of the merging cluster Abell 1914 with exposure of 160 ks (40 ks each). We measure temperature, electron density, and entropy distributions of the ICM out to the virial radius to study the merging history of this cluster. We determine the supra-thermal component expected by the merger with a wide-band spectroscopy using XIS and HXD-PIN, and quantify heat input to the ICM by a joint analysis with weak lensing data of Subaru telescope. Then, we aim to estimate the energy ratio of the heat input to total delivered energy through the merger.	EXTRAGALACTIC DIFFUSE SOURCES	8	A	MADOKA KAWAHARADA	ERIC MILLER	JUS	5	AO5	THERMODYNAMICS OF INTRACLUSTER MEDIUM IN THE MERGING CLUSTER ABELL 1914	XIS	Y	https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/805091010/	Quick Look
4	A262 E3	29.2513	35.7586	28.51426	35.514871	40.102333	22.236821	137.59731231	-25.23895106	250.0003	56701.0116319444	2014-02-13 00:16:45	56701.8717939815	2014-02-13 20:55:23	808114010	38.5681	40	38.5761	38.5681	0	38.5761	2	2	0	2	0	0	0	0	0	0	0	PROCESSED	57613.8129861111	2016-08-13 19:30:42	57080	2015-02-27 00:00:00	56714.7407986111	2014-02-26 17:46:45	3.0.22.44	2	Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22	083002	We propose to observe a poor cluster, Abell 262 (kT=2.2 keV, z=0.017), out to 0.9 r180 toward directions of a filament and void. The objectives are to derive gas-mass and fe-mass-to-light ratios and entropy profiles out the virial radius and study their dependence of the system mass, and to study azimuthal dependence of the temperature, density and entropy.	EXTRAGALACTIC DIFFUSE SOURCES	8	B	KYOKO MATSUSHITA	NORBERT WERNER	JUS	8	AO8	OBSERVATIONS OF AN POOR CLUSTER OUT TO THE VIRIAL RADIUS	XIS	Y	https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/808114010/	Quick Look
5	M106	184.7117	47.2376	184.094273	47.515109	160.404745	44.085185	138.43381178	68.89762168	287.1938	53896.5413078704	2006-06-10 12:59:29	53898.7113425926	2006-06-12 17:04:20	701095010	99.8175	100	99.8815	99.8175	99.8815	99.8815	2	2	2	2	1	0	0	97.5229	97.5229	187.4839	1	PROCESSED	57534.6515393518	2016-05-26 15:38:13	54401	2007-10-28 00:00:00	53927.2308449074	2006-07-11 05:32:25	3.0.22.43	4	Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22	013151	We propose observations of the nearby Low Luminosity AGN, M81 and M106, for 100 ks for each target. We aim to detect both targets up to ~200 keV for the first time. We will determine the photon indices of the hard X-ray power-law continuum, with searching for other possible characteristics such as Compton hump around 10-20 keV and cutoff around 100-200 keV which would lead major discoveries. We will study the shape of Fe-K line(s) around 6-7 keV and their time variances. Our goal is to compare their hard X-ray spectra with those of SWG seyfert galaxies, with unprecedented accuracy, to study the accresion mechanism of LLAGN.	EXTRAGALACTIC COMPACT SOURCES	7	A	TAKESHI ITOH	CHRISTOPHER REYNOLDS	JUS	1	AO1	OBSERVATIONS OF HARD X-RAYS FROM LOW LUMINOSITY ACTIVE GALACTIC NUCLEI	HXD	N	https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/701095010/	Quick Look
6	A1914_OFFSET1	216.5784	38.0421	216.067238	38.26635	196.337734	48.766613	67.66951456	67.3249966	134.001	55565.4188194445	2011-01-04 10:03:06	55565.728599537	2011-01-04 17:29:11	805091020	11.393	10	11.401	11.393	0	11.401	2	2	0	2	1	0	0	11.3763	11.3763	25.4979	0	PROCESSED	57600.5573263889	2016-07-31 13:22:33	55995	2012-03-09 00:00:00	55627.1165625	2011-03-07 02:47:51	3.0.22.44	2	Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22	053087	We propose four pointing observations of the merging cluster Abell 1914 with exposure of 160 ks (40 ks each). We measure temperature, electron density, and entropy distributions of the ICM out to the virial radius to study the merging history of this cluster. We determine the supra-thermal component expected by the merger with a wide-band spectroscopy using XIS and HXD-PIN, and quantify heat input to the ICM by a joint analysis with weak lensing data of Subaru telescope. Then, we aim to estimate the energy ratio of the heat input to total delivered energy through the merger.	EXTRAGALACTIC DIFFUSE SOURCES	8	A	MADOKA KAWAHARADA	RYO NAGINO	JUS	5	AO5	THERMODYNAMICS OF INTRACLUSTER MEDIUM IN THE MERGING CLUSTER ABELL 1914	XIS	Y	https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/805091020/	Quick Look
7	A1914_OFFSET3	216.2252	37.8719	215.712166	38.097165	196.093912	48.482824	67.5271644	67.6467927	330.9949	55364.3811805556	2010-06-17 09:08:54	55365.2953587963	2010-06-18 07:05:19	805093010	28.5066	40	28.5066	28.5066	0	28.5066	2	2	0	2	1	0	0	26.3813	26.3813	78.9679	1	PROCESSED	57552.3531018518	2016-06-13 08:28:28	55769	2011-07-27 00:00:00	55400.3084375	2010-07-23 07:24:09	3.0.22.43	2	Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22	053087	We propose four pointing observations of the merging cluster Abell 1914 with exposure of 160 ks (40 ks each). We measure temperature, electron density, and entropy distributions of the ICM out to the virial radius to study the merging history of this cluster. We determine the supra-thermal component expected by the merger with a wide-band spectroscopy using XIS and HXD-PIN, and quantify heat input to the ICM by a joint analysis with weak lensing data of Subaru telescope. Then, we aim to estimate the energy ratio of the heat input to total delivered energy through the merger.	EXTRAGALACTIC DIFFUSE SOURCES	8	A	MADOKA KAWAHARADA	ERIC MILLER	JUS	5	AO5	THERMODYNAMICS OF INTRACLUSTER MEDIUM IN THE MERGING CLUSTER ABELL 1914	XIS	Y	https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/805093010/	Quick Look
8	A262 E4	29.5568	35.6351	28.819272	35.392091	40.300853	22.029449	137.89892988	-25.28797491	250	56701.8723148148	2014-02-13 20:56:08	56702.5974652778	2014-02-14 14:20:21	808115010	31.9389	30	31.9469	31.9389	0	31.9549	2	2	0	2	0	0	0	0	0	0	0	PROCESSED	57613.8117361111	2016-08-13 19:28:54	57080	2015-02-27 00:00:00	56714.739525463	2014-02-26 17:44:55	3.0.22.44	2	Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22	083002	We propose to observe a poor cluster, Abell 262 (kT=2.2 keV, z=0.017), out to 0.9 r180 toward directions of a filament and void. The objectives are to derive gas-mass and fe-mass-to-light ratios and entropy profiles out the virial radius and study their dependence of the system mass, and to study azimuthal dependence of the temperature, density and entropy.	EXTRAGALACTIC DIFFUSE SOURCES	8	B	KYOKO MATSUSHITA	NORBERT WERNER	JUS	8	AO8	OBSERVATIONS OF AN POOR CLUSTER OUT TO THE VIRIAL RADIUS	XIS	Y	https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/808115010/	Quick Look
9	G156.2+5.7 CENTER	74.723	51.7342	73.743251	51.658579	79.264036	28.862327	156.21466687	5.62934315	273.4473	54148.7568171296	2007-02-17 18:09:49	54149.9169444444	2007-02-18 22:00:24	501106010	51.2142	50	51.2222	51.2302	0	51.2142	1	1	0	1	1	0	0	46.482	46.482	100.1999	0	PROCESSED	57537.3992824074	2016-05-29 09:34:58	54695	2008-08-17 00:00:00	54158.4264351852	2007-02-27 10:14:04	3.0.22.43	4	Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22	013079	Recent observations revealed that about 10 shell-like supernova remnants (SNRs) exhibit power-law X-ray spectra with no emission line which are considered to be synchrotron radiation from high-energy electrons (larger than 1 TeV). However, all those samples are young SNRs (ages about 300-2000 yr). G156.2+5.7 is an old SNR (age about 10^4 year), but emits hard X-rays in addition to usual thin thermal emission (about 0.5 keV temperature). We propose a Suzaku observation on a center region of this SNR, where diffuse hard X-rays were detected with ASCA and XMM. Our primary objective is to determine whether or not the hard tail is synchrotron X-rays, and study cosmic-ray acceleration in this old SNR.	GALACTIC DIFFUSE EMISSION	5	B	MASARU UENO	ROBERT PETRE	JUS	1	AO1	REVEALING THE ORIGIN OF HARD X-RAY EMISSION FROM AN OLD SNR, G156.2+5.7	XIS	Y	https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/501106010/	Quick Look
10	KEPLER	262.6698	-21.4886	261.920525	-21.451271	263.169114	1.778808	4.51918955	6.82146946	98.2145	54514.1665393518	2008-02-18 03:59:49	54516.9793287037	2008-02-20 23:30:14	502078010	116.9636	100	116.9636	116.9636	0	116.9636	2	2	0	2	1	0	0	98.9551	98.9551	242.9956	3	PROCESSED	57541.7751388889	2016-06-02 18:36:12	54894	2009-03-04 00:00:00	54525.6176851852	2008-02-29 14:49:28	3.0.22.43	2	Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22	023074	We propose to observe the Kepler's SNR in which evidence of particle acceleration will be found. Aim of the observation is to determine power-law contribution in the hard-tail spectrum above 10 keV with HXD-PIN. If we also find the Fe-Kb and Ni-K emission lines with XIS which have not observed in any previous missions, temperature and nt parameter of a NEI model will be fixed. The determination will help to distinguish the power-law component from the thermal one. We also memtioned that the amount of Fe and Ni will be a good estimator to determine the type of Kepler's SNR.	GALACTIC DIFFUSE EMISSION	5	B	TORU TAMAGAWA	Sangwook Park	JUS	2	AO2	SEARCH FOR EVIDENCE OF COSMIC-RAY ACCELERATION IN THE KEPLER'S SNR	XIS	Y	https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/502078010/	Quick Look
11	K3/PSR J1420-6048	215.0274	-60.7627	214.105774	-60.533369	236.492647	-43.553641	313.55205119	0.26755801	90.771	54842.5598263889	2009-01-11 13:26:09	54843.8801388889	2009-01-12 21:07:24	503110010	50.269	50	50.269	50.269	0	50.269	1	1	0	1	1	0	0	50.0618	50.0618	114.0639	2	PROCESSED	57545.1792013889	2016-06-06 04:18:03	55328	2010-05-12 00:00:00	54854.3728703704	2009-01-23 08:56:56	3.0.22.43	3	Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22	033076	K3/PSR J1420-6048 is one of the TeV gamma-ray pulsar wind nebulae detected by HESS, which are thought to be main particle accelerators to the Galactic Cosmic rays. It was also detected by EGRET and its X-ray spectrum is very hard. In order to reveal the radiation mechanism, we propose to observe the extended source for 50 ksec on HXD nominal position and contamination source for 20 ksec on XIS nominal position. The main purpose of this observation is to obtain the hard X-ray spectrum up to about 40 keV.	GALACTIC DIFFUSE EMISSION	5	C	TETSUICHI KISHISHITA	ROGER ROMANI	JUS	3	AO3	SUZAKU OBSERVATION OF TEV GAMMA-RAY PWN K3/PSR J1420-6048	HXD	Y	https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/503110010/	Quick Look
12	A3667_CENTER	303.141	-56.7974	302.14092	-56.947599	291.656641	-35.82366	340.90266514	-33.39955413	74.263	53861.7363078704	2006-05-06 17:40:17	53862.3843055556	2006-05-07 09:13:24	801096010	20.8805	20	20.8885	20.8885	20.8965	20.8805	1	1	1	1	1	0	0	8.425	8.425	55.9439	1	PROCESSED	57533.6497337963	2016-05-25 15:35:37	54394	2007-10-21 00:00:00	53913.7840509259	2006-06-27 18:49:02	3.0.22.43	4	Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22	013080	We propose to observe along the north west relic of Abell 3667 cluster. The aim of this observation is to obtain a high quality hard X-ray spectra of the NW relic, utlizing the high sensitivity and norrow field of view of the HXD detector, as well as the high sensitivity of the XIS to widely diffuse souces.	EXTRAGALACTIC DIFFUSE SOURCES	8	A	KAZUHIRO NAKAZAWA	CRAIG SARAZIN	JUS	1	AO1	SUZAKU OBSERVATION OF A MERGING CLUSTER ABELL 3667	HXD	N	https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/801096010/	Quick Look
13	ABELL 262 OFFSET1	28.5344	36.2686	27.797773	36.023209	39.729024	22.927942	136.82832457	-24.90547123	69.9996	54318.8941898148	2007-08-06 21:27:38	54320.0772337963	2007-08-08 01:51:13	802079010	54.5894	48	54.5974	54.5894	0	54.6029	2	2	0	2	1	0	0	50.9123	50.9123	102.2038	1	PROCESSED	57539.4485416667	2016-05-31 10:45:54	54730	2008-09-21 00:00:00	54347.4244791667	2007-09-04 10:11:15	3.0.22.43	3	Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22	023004	We propose to observe Abell 262. The temperature of the intracluster mediums of the cluster is 2 keV and therefore this cluster is between groups of galaxies and clusters of galaxies. The purpuse of the observation is to determine the distribution of O, Mg, Si and Fe f the intracluster medium upto 0.3 r180. The exposures are 30 ks for the central pointing and 40 ks for two offset pointings and the total exposure is 110ks.	EXTRAGALACTIC DIFFUSE SOURCES	8	A	KYOKO MATSUSHITA	Fabio Gastaldello	JUS	2	AO2	O AND MG ABUNDANCES OF THE INTRACLUSTER MEDIUMS OF ABELL 262	XIS	Y	https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/802079010/	Quick Look
14	A262 E2	28.9415	35.8688	28.205018	35.624348	39.895398	22.433371	137.29682221	-25.20210685	249.9999	56695.375625	2014-02-07 09:00:54	56696.1043518518	2014-02-08 02:30:16	808113010	33.0569	32	33.0609	33.0569	0	33.0649	2	2	0	2	0	0	0	0	0	0	0	PROCESSED	57613.8024884259	2016-08-13 19:15:35	57074	2015-02-21 00:00:00	56709.7139814815	2014-02-21 17:08:08	3.0.22.44	2	Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22	083002	We propose to observe a poor cluster, Abell 262 (kT=2.2 keV, z=0.017), out to 0.9 r180 toward directions of a filament and void. The objectives are to derive gas-mass and fe-mass-to-light ratios and entropy profiles out the virial radius and study their dependence of the system mass, and to study azimuthal dependence of the temperature, density and entropy.	EXTRAGALACTIC DIFFUSE SOURCES	8	B	KYOKO MATSUSHITA	NORBERT WERNER	JUS	8	AO8	OBSERVATIONS OF AN POOR CLUSTER OUT TO THE VIRIAL RADIUS	XIS	Y	https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/808113010/	Quick Look
15	1FGL J1018.6-5856	154.7461	-58.9386	154.30337	-58.687202	196.560422	-60.861111	284.35392298	-1.67969789	308.622	56105.7124189815	2012-06-27 17:05:53	56106.6523611111	2012-06-28 15:39:24	407096010	60.4324	60	60.4324	60.4324	0	60.4324	2	2	0	2	1	0	0	53.5978	53.5978	81.2059	1	PROCESSED	57606.5124768518	2016-08-06 12:17:58	56484	2013-07-11 00:00:00	56118.0496527778	2012-07-10 01:11:30	3.0.22.44	2	Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22	073113	Recently, a modulated signal has been detected with the Fermi from the source 1FGL J1018.6-5856. The presence of a O-type star in this source, and the variable character of the signal suggested that the source is a new gamma-ray binary system. Since it is expected that X-rays in these sources has the synchrotron origin, detailed X-ray observations are very important for understanding of the processes occurring in the system. However, sensitive observations of source in the X-ray energy bands are still missing. Therefore, we propose to observe the source with Suzaku. Since a long observational campaign is planned for 2012 by the HESS collaboration, the obtained X-ray, together with TeV, data will allow a proper modeling of the physical processes behind the non-thermal emission in system.	GALACTIC POINT SOURCES	4	B	HIROKAZU ODAKA	TAKAAKI TANAKA	JUS	7	AO7	X-RAY OBSERVATION OF GAMMA-RAY BINARY 1FGL J1018.6-5856	XIS	Y	https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/407096010/	Quick Look
16	A1750C	202.6943	-1.8873	202.05036	-1.629855	201.691973	7.074913	322.57262201	59.47596371	293.5241	55766.9371064815	2011-07-24 22:29:26	55767.8814814815	2011-07-25 21:09:20	806095010	41.4893	40	41.5049	41.4893	0	41.5049	2	2	0	2	1	0	0	41.0991	41.0991	81.5778	0	PROCESSED	57602.6723148148	2016-08-02 16:08:08	56219	2012-10-19 00:00:00	55851.4572106482	2011-10-17 10:58:23	3.0.22.44	2	Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22	063019	We observe Abell 1750 which has three clusters of galaxies in a filamentary structure of the large-scale structure, with 4 pointing observations (80 x 3 + 40 ks). We reveal global spatial structures of temperature, density, and entropy in Abell 1750 for the first time. By a correlation with a galaxy map obtained from SDSS, and a comparison between thermal pressure and total pressure required by the total mass derived from weal lensing analysis, we explore the inflow of matter and evolutionary process in this system.	EXTRAGALACTIC DIFFUSE SOURCES	8	A	MADOKA KAWAHARADA	SCOTT RANDALL	JUS	6	AO6	SUZAKU OBSERVATION OF ABELL 1750 IN THE LARGE-SCALE STRUCTURE	XIS	Y	https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/806095010/	Quick Look
17	PKS 1510-089	228.2108	-9.1043	227.537329	-8.917552	228.287746	8.492539	351.2856545	40.1353659	286.8003	53949.3968634259	2006-08-02 09:31:29	53952.2544444445	2006-08-05 06:06:24	701094010	119.1577	120	119.1577	119.1577	119.1657	119.1657	2	2	2	2	1	0	0	106.2588	106.2588	246.8638	5	PROCESSED	57535.1605208333	2016-05-27 03:51:09	54394	2007-10-21 00:00:00	54018.7363194444	2006-10-10 17:40:18	3.0.22.43	3	Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22	013016	It has been a long mystery (i) how the relativistic jets are formed, and (ii) what is the composition of a jet. In the theoretical view, strong magnetic field (u_B >> u_e) is necessary to produce such outflows with baryonic matters, but observations favor opposite scenario, namely particle dominated (u_e >> u_B), leptonic jet. Such discrepancies can be resolved if moderate numbers of protons (n_e/n_p > 50) are mixed in the non-tnermal pair populations. This can be easily tested if we can observe characteristic "soft X-ray bump" produced by the bulk-Comptonization of UV photons emitted from an accretion disk. We propose a deep observation (40ksec x3) of an EGRET quasar PKS 1510-089, which shows a clear sign of soft X-ray bump in BeppoSAX, ROSAT and ASCA observations.	EXTRAGALACTIC COMPACT SOURCES	7	B	JUN KATAOKA	GRZEGORZ MADEJSKI	JUS	1	AO1	DIRECT TESTING THE JET COMPOSITION IN A POWERFUL EGRET QUASAR PKS 1510-089	XIS	N	https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/701094010/	Quick Look
18	A1914_OFFSET2	216.7383	37.763	216.226328	37.986791	196.709268	48.583272	66.87630822	67.3091462	329.9943	55363.4747569444	2010-06-16 11:23:39	55364.3800115741	2010-06-17 09:07:13	805092010	28.5462	40	28.5542	28.5542	0	28.5462	2	2	0	2	1	0	0	25.8343	25.8343	78.204	0	PROCESSED	57552.3515856482	2016-06-13 08:26:17	55766	2011-07-24 00:00:00	55399.3275231482	2010-07-22 07:51:38	3.0.22.43	2	Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22	053087	We propose four pointing observations of the merging cluster Abell 1914 with exposure of 160 ks (40 ks each). We measure temperature, electron density, and entropy distributions of the ICM out to the virial radius to study the merging history of this cluster. We determine the supra-thermal component expected by the merger with a wide-band spectroscopy using XIS and HXD-PIN, and quantify heat input to the ICM by a joint analysis with weak lensing data of Subaru telescope. Then, we aim to estimate the energy ratio of the heat input to total delivered energy through the merger.	EXTRAGALACTIC DIFFUSE SOURCES	8	A	MADOKA KAWAHARADA	ERIC MILLER	JUS	5	AO5	THERMODYNAMICS OF INTRACLUSTER MEDIUM IN THE MERGING CLUSTER ABELL 1914	XIS	Y	https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/805092010/	Quick Look
19	A1914_OFFSET4	216.4424	37.6372	215.928949	37.861845	196.491265	48.360248	66.78881215	67.57279807	134.0011	55566.4311574074	2011-01-05 10:20:52	55566.8258912037	2011-01-05 19:49:17	805094020	17.3531	12	17.3531	17.3611	0	17.3691	2	2	0	2	1	0	0	16.0606	16.0606	34.1	0	PROCESSED	57600.564375	2016-07-31 13:32:42	55995	2012-03-09 00:00:00	55627.1583333333	2011-03-07 03:48:00	3.0.22.44	2	Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22	053087	We propose four pointing observations of the merging cluster Abell 1914 with exposure of 160 ks (40 ks each). We measure temperature, electron density, and entropy distributions of the ICM out to the virial radius to study the merging history of this cluster. We determine the supra-thermal component expected by the merger with a wide-band spectroscopy using XIS and HXD-PIN, and quantify heat input to the ICM by a joint analysis with weak lensing data of Subaru telescope. Then, we aim to estimate the energy ratio of the heat input to total delivered energy through the merger.	EXTRAGALACTIC DIFFUSE SOURCES	8	A	MADOKA KAWAHARADA	ERIC MILLER	JUS	5	AO5	THERMODYNAMICS OF INTRACLUSTER MEDIUM IN THE MERGING CLUSTER ABELL 1914	XIS	Y	https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/805094020/	Quick Look
20	A3667_NW_17OFF	302.8177	-56.56	301.819585	-56.708877	291.523842	-35.547493	341.18808838	-33.22347241	74.1682	53861.293912037	2006-05-06 07:03:14	53861.7356944444	2006-05-06 17:39:24	801095010	17.2586	20	17.2826	17.2746	17.2666	17.2586	1	1	1	1	1	0	0	14.2555	14.2555	38.1519	1	PROCESSED	57533.636099537	2016-05-25 15:15:59	54735	2008-09-26 00:00:00	53913.7593518518	2006-06-27 18:13:28	3.0.22.43	4	Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22	013080	We propose to observe along the north west relic of Abell 3667 cluster. The aim of this observation is to obtain a high quality hard X-ray spectra of the NW relic, utlizing the high sensitivity and norrow field of view of the HXD detector, as well as the high sensitivity of the XIS to widely diffuse souces.	EXTRAGALACTIC DIFFUSE SOURCES	8	A	KAZUHIRO NAKAZAWA	CRAIG SARAZIN	JUS	1	AO1	SUZAKU OBSERVATION OF A MERGING CLUSTER ABELL 3667	HXD	N	https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/801095010/	Quick Look
21	A3667_NW_17OFF	302.869	-56.6666	301.869632	-56.815685	291.522519	-35.657764	341.06051648	-33.2513141	258.9342	54038.8325578704	2006-10-30 19:58:53	54039.0106944444	2006-10-31 00:15:24	801095020	11.9634	10	11.9794	11.9794	11.9634	11.9714	1	1	1	1	1	0	0	8.724	8.724	15.3839	0	PROCESSED	57535.9848032407	2016-05-27 23:38:07	54735	2008-09-26 00:00:00	54056.1858796296	2006-11-17 04:27:40	3.0.22.43	3	Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22	013080	We propose to observe along the north west relic of Abell 3667 cluster. The aim of this observation is to obtain a high quality hard X-ray spectra of the NW relic, utlizing the high sensitivity and norrow field of view of the HXD detector, as well as the high sensitivity of the XIS to widely diffuse souces.	EXTRAGALACTIC DIFFUSE SOURCES	8	A	KAZUHIRO NAKAZAWA	CRAIG SARAZIN	JUS	1	AO1	SUZAKU OBSERVATION OF A MERGING CLUSTER ABELL 3667	HXD	Y	https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/801095020/	Quick Look
22	A3667_NW_RELIC	302.5617	-56.3599	301.565299	-56.507728	291.421165	-35.317169	341.42703548	-33.08195751	74.7123	53858.7409837963	2006-05-03 17:47:01	53861.2933449074	2006-05-06 07:02:25	801094010	94.3946	95	94.4026	94.3946	94.3946	94.4026	3	3	3	3	1	0	0	56.2506	56.2506	220.489	4	PROCESSED	57533.7274074074	2016-05-25 17:27:28	54394	2007-10-21 00:00:00	53913.7574189815	2006-06-27 18:10:41	3.0.22.43	4	Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22	013080	We propose to observe along the north west relic of Abell 3667 cluster. The aim of this observation is to obtain a high quality hard X-ray spectra of the NW relic, utlizing the high sensitivity and norrow field of view of the HXD detector, as well as the high sensitivity of the XIS to widely diffuse souces.	EXTRAGALACTIC DIFFUSE SOURCES	8	A	KAZUHIRO NAKAZAWA	CRAIG SARAZIN	JUS	1	AO1	SUZAKU OBSERVATION OF A MERGING CLUSTER ABELL 3667	HXD	N	https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/801094010/	Quick Look
23	MRK 110	141.3383	52.3497	140.469294	52.565715	125.649662	35.070751	164.91808924	44.3703784	110.1475	54406.3443055556	2007-11-02 08:15:48	54408.31625	2007-11-04 07:35:24	702124010	90.8712	100	90.8712	90.8792	0	90.8792	2	2	0	2	1	0	0	86.5231	86.5231	170.3558	2	PROCESSED	57540.442037037	2016-06-01 10:36:32	54786	2008-11-16 00:00:00	54417.3880092593	2007-11-13 09:18:44	3.0.22.43	3	Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22	023012	We request a 100 ks SUZAKU observation of Mrk 110 to quantify the accretion disk geometry in this high luminosity narrow line Seyfert 1 galaxy. This is an unique low mass AGN which shows an almost featureless X-ray continuum described by a two component Comptonization model. It has shown, based on an XMM-Newton data, energy dependent delays which are consistent with the idea of a Comptonized plasma confined within 10 Schwartzschild radius of the central black hole. The proposed long observation will provide high signal-to-noise hard X-ray data, thus allowing us to extend the observed delay to higher energies and also to quantify the high energy spectral parameters like cut-off energy and reflection parameters. This will help us to identify the accretion disk geometry in this source.	EXTRAGALACTIC COMPACT SOURCES	7	C	ARIKKALA RAO	Gulab Dewangan	EUS	2	AO2	PROBING THE ACCRETION DISK GEOMETRY IN THE TYPE I SEYFERT GALAXY MRK 110	HXD	Y	https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/702124010/	Quick Look
24	A1914_OFFSET2	216.77	37.7885	216.258243	38.012199	196.723878	48.617689	66.91478771	67.27662817	134.0016	55565.7291203704	2011-01-04 17:29:56	55566.0216550926	2011-01-05 00:31:11	805092020	17.0912	12	17.0992	17.0912	0	17.1072	1	1	0	1	1	0	0	13.2058	13.2058	25.2719	0	PROCESSED	57600.5511689815	2016-07-31 13:13:41	56037	2012-04-20 00:00:00	55670.1137384259	2011-04-19 02:43:47	3.0.22.44	2	Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22	053087	We propose four pointing observations of the merging cluster Abell 1914 with exposure of 160 ks (40 ks each). We measure temperature, electron density, and entropy distributions of the ICM out to the virial radius to study the merging history of this cluster. We determine the supra-thermal component expected by the merger with a wide-band spectroscopy using XIS and HXD-PIN, and quantify heat input to the ICM by a joint analysis with weak lensing data of Subaru telescope. Then, we aim to estimate the energy ratio of the heat input to total delivered energy through the merger.	EXTRAGALACTIC DIFFUSE SOURCES	8	A	MADOKA KAWAHARADA	ERIC MILLER	JUS	5	AO5	THERMODYNAMICS OF INTRACLUSTER MEDIUM IN THE MERGING CLUSTER ABELL 1914	XIS	Y	https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/805092020/	Quick Look
25	A262 NE2	28.537	36.7219	27.798764	36.476514	39.918494	23.346467	136.69850182	-24.46778258	249.9995	56703.1881712963	2014-02-15 04:30:58	56703.8821643518	2014-02-15 21:10:19	808109010	32.9447	32	32.9527	32.9607	0	32.9447	2	2	0	2	0	0	0	0	0	0	0	PROCESSED	57613.8208564815	2016-08-13 19:42:02	57080	2015-02-27 00:00:00	56714.743275463	2014-02-26 17:50:19	3.0.22.44	2	Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22	083002	We propose to observe a poor cluster, Abell 262 (kT=2.2 keV, z=0.017), out to 0.9 r180 toward directions of a filament and void. The objectives are to derive gas-mass and fe-mass-to-light ratios and entropy profiles out the virial radius and study their dependence of the system mass, and to study azimuthal dependence of the temperature, density and entropy.	EXTRAGALACTIC DIFFUSE SOURCES	8	A	KYOKO MATSUSHITA	NORBERT WERNER	JUS	8	AO8	OBSERVATIONS OF AN POOR CLUSTER OUT TO THE VIRIAL RADIUS	XIS	Y	https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/808109010/	Quick Look
26	SWIFT J1322.2-1641	200.5819	-16.7858	199.912392	-16.524578	205.294799	-7.530887	313.4989766	45.45121448	290.037	55013.9738310185	2009-07-01 23:22:19	55014.9981365741	2009-07-02 23:57:19	704022010	41.3487	40	41.3487	41.6207	0	41.6127	2	2	0	2	1	0	0	36.2368	36.2368	88.4858	7	PROCESSED	57547.7444097222	2016-06-08 17:51:57	55393	2010-07-16 00:00:00	55027.0523148148	2009-07-15 01:15:20	3.0.22.43	2	Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22	043059	The number of Compton thick AGNs is the biggest issue in the origin of the X-ray background and AGN evolution. According to the latetest population synthesis model, its estimate is strongly coupled with the broad band spectral shape of moderately absorbed AGNs, which is only poorly understood. Recently, Swift/BAT has provided the first unbiased AGN sample above 15 keV, which includes many hard X-ray bright, absorbed AGNs that can be best followed-up with Suzaku. Here we propose to observe three of them to measure the amount of reflection component with unpreceded accuracy, a key parameter to determine the total contribution of Compton thick AGNs to the X-ray background. With these observations we can make the spectral survey of bright absorbed Swift/BAT AGNs complete.	EXTRAGALACTIC COMPACT SOURCES	7	A	YOSHIHIRO UEDA	MAURO DADINA	JEU	4	AO4	SPECTRAL SURVEY OF A COMPLETE SAMPLE OF SWIFT/BAT SELECTED AGNS AND THE ORIGIN OF THE X-RAY BACKGROUND	HXD	Y	https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/704022010/	Quick Look
27	A262 NE1	28.4051	36.5019	27.66806	36.256213	39.720751	23.183318	136.64990456	-24.70790073	250	56702.5986342593	2014-02-14 14:22:02	56703.187662037	2014-02-15 04:30:14	808108010	25.6102	24	25.6102	25.6102	0	25.6102	2	2	0	2	0	0	0	0	0	0	0	PROCESSED	57613.8178472222	2016-08-13 19:37:42	57080	2015-02-27 00:00:00	56714.742037037	2014-02-26 17:48:32	3.0.22.44	2	Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22	083002	We propose to observe a poor cluster, Abell 262 (kT=2.2 keV, z=0.017), out to 0.9 r180 toward directions of a filament and void. The objectives are to derive gas-mass and fe-mass-to-light ratios and entropy profiles out the virial radius and study their dependence of the system mass, and to study azimuthal dependence of the temperature, density and entropy.	EXTRAGALACTIC DIFFUSE SOURCES	8	A	KYOKO MATSUSHITA	NORBERT WERNER	JUS	8	AO8	OBSERVATIONS OF AN POOR CLUSTER OUT TO THE VIRIAL RADIUS	XIS	Y	https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/808108010/	Quick Look
28	A1914_OFFSET3	216.2544	37.895	215.741562	38.120181	196.10746	48.514193	67.56094175	67.61680074	134.0009	55566.0223148148	2011-01-05 00:32:08	55566.4306365741	2011-01-05 10:20:07	805093020	12.8294	12	12.8294	12.8294	0	12.8294	2	2	0	2	1	0	0	13.721	13.721	35.2699	0	PROCESSED	57600.553599537	2016-07-31 13:17:11	55995	2012-03-09 00:00:00	55627.1328009259	2011-03-07 03:11:14	3.0.22.44	2	Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22	053087	We propose four pointing observations of the merging cluster Abell 1914 with exposure of 160 ks (40 ks each). We measure temperature, electron density, and entropy distributions of the ICM out to the virial radius to study the merging history of this cluster. We determine the supra-thermal component expected by the merger with a wide-band spectroscopy using XIS and HXD-PIN, and quantify heat input to the ICM by a joint analysis with weak lensing data of Subaru telescope. Then, we aim to estimate the energy ratio of the heat input to total delivered energy through the merger.	EXTRAGALACTIC DIFFUSE SOURCES	8	A	MADOKA KAWAHARADA	ERIC MILLER	JUS	5	AO5	THERMODYNAMICS OF INTRACLUSTER MEDIUM IN THE MERGING CLUSTER ABELL 1914	XIS	Y	https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/805093020/	Quick Look
29	ABELL 262 OFFSET2	28.0598	36.4356	27.324082	36.18913	39.413922	23.227924	136.37355079	-24.84408055	69.9996	54320.0778935185	2007-08-08 01:52:10	54321.2405555556	2007-08-09 05:46:24	802080010	54.7081	48	54.7241	54.7081	0	54.7241	2	2	0	2	1	0	0	50.1788	50.1788	100.3968	1	PROCESSED	57539.4536226852	2016-05-31 10:53:13	54730	2008-09-21 00:00:00	54347.6730671296	2007-09-04 16:09:13	3.0.22.43	3	Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22	023004	We propose to observe Abell 262. The temperature of the intracluster mediums of the cluster is 2 keV and therefore this cluster is between groups of galaxies and clusters of galaxies. The purpuse of the observation is to determine the distribution of O, Mg, Si and Fe f the intracluster medium upto 0.3 r180. The exposures are 30 ks for the central pointing and 40 ks for two offset pointings and the total exposure is 110ks.	EXTRAGALACTIC DIFFUSE SOURCES	8	A	KYOKO MATSUSHITA	Fabio Gastaldello	JUS	2	AO2	O AND MG ABUNDANCES OF THE INTRACLUSTER MEDIUMS OF ABELL 262	XIS	Y	https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/802080010/	Quick Look
30	A1750N	202.8147	-1.6537	202.171177	-1.396479	201.71761	7.336429	322.93839507	59.66232121	293.5219	55744.8544444444	2011-07-02 20:30:24	55746.9911111111	2011-07-04 23:47:12	806096010	74.7134	80	74.7294	74.7134	0	74.7294	2	2	0	2	1	0	0	61.6402	61.6402	184.5979	1	PROCESSED	57602.5091435185	2016-08-02 12:13:10	56144	2012-08-05 00:00:00	55775.4134027778	2011-08-02 09:55:18	3.0.22.44	2	Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22	063019	We observe Abell 1750 which has three clusters of galaxies in a filamentary structure of the large-scale structure, with 4 pointing observations (80 x 3 + 40 ks). We reveal global spatial structures of temperature, density, and entropy in Abell 1750 for the first time. By a correlation with a galaxy map obtained from SDSS, and a comparison between thermal pressure and total pressure required by the total mass derived from weal lensing analysis, we explore the inflow of matter and evolutionary process in this system.	EXTRAGALACTIC DIFFUSE SOURCES	8	A	MADOKA KAWAHARADA	SCOTT RANDALL	JUS	6	AO6	SUZAKU OBSERVATION OF ABELL 1750 IN THE LARGE-SCALE STRUCTURE	XIS	Y	https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/806096010/	Quick Look
31	A3558 WEST OFF	201.4503	-31.5856	200.748303	-31.325817	211.928183	-20.890972	311.44383739	30.71755895	288.4754	54657.5304513889	2008-07-10 12:43:51	54660.0225	2008-07-13 00:32:24	803072010	81.8162	80	81.8162	81.8162	0	81.8162	2	2	0	2	1	0	0	67.3941	67.3941	215.2857	1	PROCESSED	57543.1016898148	2016-06-04 02:26:26	55037	2009-07-25 00:00:00	54670.5540162037	2008-07-23 13:17:47	3.0.22.43	2	Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22	033089	We aim at the first significant detection of redshifted OVII and OVIII lines from the warm-hot intergalactic medium (WHIM) in the Shapley Supercluster. The system, located at z = 0.048, shows the richest concentration of X-ray clusters in the nearby universe. Previous ROSAT observation showed enhanced soft X-ray emission along the cluster connection. We propose to observe for 80 ksec a region between A3558 (the brightest central cluster) and A3556, separated by 0.9 virial radius from both clusters and along the line of cluster connection. A 40 ksec observation is also proposed at a 2-degree offest region to measure the foreground Galactic spectrum. Based on the ROSAT flux, we expect to detect redshifted OVII and OVII lines at more than 7 sigma confidence.	EXTRAGALACTIC DIFFUSE SOURCES	8	A	TAKAYA OHASHI	MASSIMILIANO GALEAZZAI	JUS	3	AO3	SEARCH FOR WHIM IN THE SHAPLEY SUPERCLUSTER	XIS	Y	https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/803072010/	Quick Look
32	G306.3-0.9	200.4753	-63.5602	199.643661	-63.298602	230.10249	-49.420915	306.31531317	-0.88874973	306.5675	56889.7845833333	2014-08-20 18:49:48	56894.0099768518	2014-08-25 00:14:22	509072010	190.0114	200	190.0181	190.0114	0	190.0114	2	2	0	2	1	0	0	14.4515	14.4515	20.22	0	PROCESSED	57616.5396759259	2016-08-16 12:57:08	57305	2015-10-10 00:00:00	56938.2302777778	2014-10-08 05:31:36	3.0.22.44	2	Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22	093109	The origin of the distorted, inhomogeneous structure of mixed-morphology SNRs (MM SNRs) is a mystery. Recently we have discovered recombining plasma from MM SNRs. The existence of recombining plasma implies rapid cooling process in past. Recombining plasma, together with the peculiar morphologies, would indicate a new SNR evolution scenario. Our systematic analysis of recombining SNRs shows that the recombination ages are almost the same, although their dynamical ages range over an order of magnitude. Such a trend can be explained by past rapid rarefaction. This hypothesis can be tested by measuring a recombination age of a dynamically young recombining SNR. We thus propose a 100-ks Suzaku observation of G306.3-0.9, a candidate of the youngest recombining SNR ever.	GALACTIC DIFFUSE EMISSION	5	A	MAKOTO SAWADA	Reynolds,Matsumura	JUS	9	AO9	THE DYNAMICS OF MIXED-MORPHOLOGY SNRS PROBED BY THE YOUNGEST RECOMBINING PLASMA	XIS	Y	https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/509072010/	Quick Look
33	GK PER	52.8202	43.8404	51.968435	43.670553	61.500851	24.010688	151.00566373	-10.1477205	257.5144	54875.4415277778	2009-02-13 10:35:48	54876.0899884259	2009-02-14 02:09:35	403081010	30.3888	30	30.3888	30.3888	0	30.3888	2	2	0	2	1	0	0	27.3999	27.3999	55.9979	2	PROCESSED	57545.5260648148	2016-06-06 12:37:32	55330	2010-05-14 00:00:00	54893.4257407407	2009-03-03 10:13:04	3.0.22.43	3	Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22	033107	We propose observations of 5 Intermediate Polars, a subcategory of magnetic CVs, as the first step toward establishment of an averaged hard X-ray spectrum of IPs that exist near the Solar system.The averaged spectrum should be compared with that of the Galactic Diffese X-ray Emssion (GDXE), to investigate the claimed spectral resemblance between them in energies above 10 keV. If the averaged IP spectrum shows any discrepancy with that of the GDXE, the "point-source origin" explanation for the GDXE would face a lack of appropriate hard X-ray source populations. This in turn is expected to strengthen the competing "truly diffuse origin"explanation, which attributes the GDXE hard X-rays to non thermal emission from electrons being accelerated in the interstellar space.	GALACTIC POINT SOURCES	4	C	TAKAYUKI YUASA	THOMAS HARRISON	JUS	3	AO3	SURVEY OBSERVATION OF INTERMEDIATE POLARS	HXD	Y	https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/403081010/	Quick Look
34	A262 E1	28.6322	35.9862	27.896259	35.741034	39.692258	22.636644	136.99532529	-25.15665513	249.9998	56694.7928935185	2014-02-06 19:01:46	56695.3750694444	2014-02-07 09:00:06	808112010	25.9466	24	25.9546	25.9466	0	25.9626	3	3	0	3	0	0	0	0	0	0	0	PROCESSED	57613.7986226852	2016-08-13 19:10:01	57074	2015-02-21 00:00:00	56709.7127893518	2014-02-21 17:06:25	3.0.22.44	2	Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22	083002	We propose to observe a poor cluster, Abell 262 (kT=2.2 keV, z=0.017), out to 0.9 r180 toward directions of a filament and void. The objectives are to derive gas-mass and fe-mass-to-light ratios and entropy profiles out the virial radius and study their dependence of the system mass, and to study azimuthal dependence of the temperature, density and entropy.	EXTRAGALACTIC DIFFUSE SOURCES	8	B	KYOKO MATSUSHITA	NORBERT WERNER	JUS	8	AO8	OBSERVATIONS OF AN POOR CLUSTER OUT TO THE VIRIAL RADIUS	XIS	Y	https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/808112010/	Quick Look
35	A262 NE4	28.8115	37.1901	28.070704	36.945344	40.33412	23.695949	136.79382783	-23.95810874	249.9999	56704.7992476852	2014-02-16 19:10:55	56705.5321064815	2014-02-17 12:46:14	808111010	30.9305	30	30.9625	30.9305	0	30.9625	1	1	0	1	1	0	0	27.8027	27.8027	63.3119	2	PROCESSED	57613.8474652778	2016-08-13 20:20:21	57085	2015-03-04 00:00:00	56719.7343981482	2014-03-03 17:37:32	3.0.22.44	2	Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22	083002	We propose to observe a poor cluster, Abell 262 (kT=2.2 keV, z=0.017), out to 0.9 r180 toward directions of a filament and void. The objectives are to derive gas-mass and fe-mass-to-light ratios and entropy profiles out the virial radius and study their dependence of the system mass, and to study azimuthal dependence of the temperature, density and entropy.	EXTRAGALACTIC DIFFUSE SOURCES	8	A	KYOKO MATSUSHITA	NORBERT WERNER	JUS	8	AO8	OBSERVATIONS OF AN POOR CLUSTER OUT TO THE VIRIAL RADIUS	XIS	Y	https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/808111010/	Quick Look
36	A262 NE3	28.6712	36.9514	27.931716	36.706321	40.12197	23.517818	136.74540455	-24.21802206	250.0003	56703.8826388889	2014-02-15 21:11:00	56704.7987731482	2014-02-16 19:10:14	808110010	40.4903	40	40.5134	40.4903	0	40.4966	2	2	0	2	1	0	0	34.2624	34.2624	69.899	1	PROCESSED	57613.8476041667	2016-08-13 20:20:33	57081	2015-02-28 00:00:00	56715.76	2014-02-27 18:14:24	3.0.22.44	2	Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22	083002	We propose to observe a poor cluster, Abell 262 (kT=2.2 keV, z=0.017), out to 0.9 r180 toward directions of a filament and void. The objectives are to derive gas-mass and fe-mass-to-light ratios and entropy profiles out the virial radius and study their dependence of the system mass, and to study azimuthal dependence of the temperature, density and entropy.	EXTRAGALACTIC DIFFUSE SOURCES	8	A	KYOKO MATSUSHITA	NORBERT WERNER	JUS	8	AO8	OBSERVATIONS OF AN POOR CLUSTER OUT TO THE VIRIAL RADIUS	XIS	Y	https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/808110010/	Quick Look
37	A1750R	202.8691	-2.0415	202.224847	-1.784379	201.912931	6.996197	322.80853082	59.27632496	111.4517	55918.5150810185	2011-12-23 12:21:43	55918.843912037	2011-12-23 20:15:14	806098020	16.062	13	16.062	16.062	0	16.062	1	1	0	1	1	0	0	11.964	11.964	28.4079	0	PROCESSED	57604.214375	2016-08-04 05:08:42	56311	2013-01-19 00:00:00	55972.6764236111	2012-02-15 16:14:03	3.0.22.44	2	Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22	063019	We observe Abell 1750 which has three clusters of galaxies in a filamentary structure of the large-scale structure, with 4 pointing observations (80 x 3 + 40 ks). We reveal global spatial structures of temperature, density, and entropy in Abell 1750 for the first time. By a correlation with a galaxy map obtained from SDSS, and a comparison between thermal pressure and total pressure required by the total mass derived from weal lensing analysis, we explore the inflow of matter and evolutionary process in this system.	EXTRAGALACTIC DIFFUSE SOURCES	8	A	MADOKA KAWAHARADA		JUS	6	AO6	SUZAKU OBSERVATION OF ABELL 1750 IN THE LARGE-SCALE STRUCTURE	XIS	Y	https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/806098020/	Quick Look
38	A1750R	202.8633	-2.0722	202.218991	-1.815068	201.918925	6.965529	322.77954726	59.24881782	293.5198	55748.0658796296	2011-07-06 01:34:52	55750.0419097222	2011-07-08 01:00:21	806098010	66.5035	80	66.5115	66.5035	0	66.5115	3	2	0	2	1	0	0	54.7821	54.7821	170.7128	3	PROCESSED	57602.5535763889	2016-08-02 13:17:09	56311	2013-01-19 00:00:00	55795.163912037	2011-08-22 03:56:02	3.0.22.44	2	Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22	063019	We observe Abell 1750 which has three clusters of galaxies in a filamentary structure of the large-scale structure, with 4 pointing observations (80 x 3 + 40 ks). We reveal global spatial structures of temperature, density, and entropy in Abell 1750 for the first time. By a correlation with a galaxy map obtained from SDSS, and a comparison between thermal pressure and total pressure required by the total mass derived from weal lensing analysis, we explore the inflow of matter and evolutionary process in this system.	EXTRAGALACTIC DIFFUSE SOURCES	8	A	MADOKA KAWAHARADA	SCOTT RANDALL	JUS	6	AO6	SUZAKU OBSERVATION OF ABELL 1750 IN THE LARGE-SCALE STRUCTURE	XIS	Y	https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/806098010/	Quick Look

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