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
|
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1 | MKW 4-OFFSET1 | 181.1304 | 2.2289 | 180.489911 | 2.507266 | 180.147119 | 2.494288 | 276.66004128 | 62.68282085 | 114.5816 | 55528.2862847222 | 2010-11-28 06:52:15 | 55530.2501967593 | 2010-11-30 06:00:17 | 805081010 | 79.4261 | 80 | 79.4261 | 79.4261 | 0 | 79.4261 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 68.2112 | 68.2112 | 169.6679 | 2 | PROCESSED | 57554.312025463 | 2016-06-15 07:29:19 | 55909 | 2011-12-14 00:00:00 | 55543.4043402778 | 2010-12-13 09:42:15 | 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/ver3.0/805081010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '805081010'
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