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".

total 1

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 MKW 4-OFFSET2 181.4291 1.9058 180.78864 2.184142 180.549883 2.316727 277.53009765 62.50090006 114.4199 55530.2508101852 2010-11-30 06:01:10 55532.2286805556 2010-12-02 05:29:18 805082010 82.9361 80 82.9401 82.9361 0 82.9441 2 2 0 2 1 0 0 70.0619 70.0619 170.8541 2 PROCESSED 57554.329525463 2016-06-15 07:54:31 55910 2011-12-15 00:00:00 55544.2869328704 2010-12-14 06:53:11 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 051525 We propose a set of two 19 arcmin offset observations for the galaxy groups MKW 4 to measure spatially resolved density, temperature and iron abundance out to r_{500}. These measurements are crucial for an accurate determination of the gas mass profile and gas fraction, for probing the entropy profile near the region where the accretion shocks start to be important, and for exploring the chemical enrichment at a spatial scale which retains information of early SNII and SNIa enrichment. Due to its brightness, regularity and low temperature, the object is an ideal candidate for an offset observation of its peripheral gas by Suzaku, making an excellent use of its low background and soft X-ray sensitivity. EXTRAGALACTIC DIFFUSE SOURCES 8 B FABIO GASTALDELLO USA 5 AO5 THE OUTSKIRTS OF MKW 4 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/805082010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '805082010'

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