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 | A1060 OFFSET | 159.5124 | -27.532 | 158.922997 | -27.271679 | 173.074389 | -33.196781 | 269.88117164 | 26.64663217 | 96.4857 | 53694.9817708333 | 2005-11-20 23:33:45 | 53696.6231365741 | 2005-11-22 14:57:19 | 800004010 | 52.4025 | 60 | 52.4025 | 53.2025 | 52.4185 | 52.5385 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 46.2039 | 46.2039 | 141.8018 | 1 | PROCESSED | 57528.0764583333 | 2016-05-20 01:50:06 | 54247 | 2007-05-27 00:00:00 | 54038.1216666667 | 2006-10-30 02:55:12 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001021 | A1060 is a bright non cD cluster and gives us a unique opportunity to study injection process of metals in the intracluster space. Reliable measurement of oxygen distribution with XIS will tell us whether the metals produced by Type-II supernova (mainly oxygen) ditributes over a different scale compared with the SN-Ia product (Fe). A1060 is the best cluster where we can directly observe distribution of metals produced by general cluster galaxies. Also, central increase of temperature by 20%, probably connected with motions of bright central galaxies, suggests that non-thermal X-rays may be produced. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | A | TAKAYA OHASHI | JAP | 0 | SWG | OXYGEN DISTRIBUTION AND CENTRAL GAS FEATURES OF A1060 | XIS | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/800004010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '800004010'
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