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 | COMA CLUSTER | 194.3893 | 26.9261 | 193.783242 | 27.196084 | 181.532075 | 30.236179 | 24.84225016 | 88.62234831 | 316.4746 | 55348.2119907407 | 2010-06-01 05:05:16 | 55350.6877199074 | 2010-06-03 16:30:19 | 805079010 | 101.7805 | 100 | 101.7805 | 101.7805 | 0 | 101.7805 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 77.4308 | 77.4308 | 213.8639 | 1 | PROCESSED | 57553.0722685185 | 2016-06-14 01:44:04 | 55731 | 2011-06-19 00:00:00 | 55365.54125 | 2010-06-18 12:59:24 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 051523 | The metal-enrichment mechanism of the hot gas in clusters of galaxies is still not completely understood, particularly at large (~virial) radii where current metallicity measurements are virtually non-existent. Yet a determinaton of elemental abundances of the gas at this radius will allow us to determine which enrichment mechanism (ram pressure stripping or galactic winds) is prevalant in the outskirts of clusters. We propose a 100 kec Suzaku observation of Coma at the virial radius to determine the Fe and S abundances at this location. The ratio of these two elements will allow us to discriminate among competing models for chemical enrichment. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | A | JIMMY IRWIN | USA | 5 | AO5 | THE DETERMINATION OF THE METALLICITY OF COMA AT THE VIRIAL RADIUS | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/805079010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '805079010'
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