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 | A383_FIELD_2 | 41.9447 | -3.4083 | 41.315431 | -3.616408 | 38.400744 | -18.662791 | 177.53047769 | -53.46482162 | 60.9996 | 55389.1380208333 | 2010-07-12 03:18:45 | 55390.062662037 | 2010-07-13 01:30:14 | 805063010 | 43.3415 | 40 | 43.3575 | 43.3415 | 0 | 43.3575 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 39.2589 | 39.2589 | 79.8749 | 0 | PROCESSED | 57552.6168055556 | 2016-06-13 14:48:12 | 55287 | 2010-04-01 00:00:00 | 55411.2445601852 | 2010-08-03 05:52:10 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 051115 | We propose observations of 5 clusters of galaxies to probe the cluster environment out to r200 in order to (1) determine the temperature and density profiles for a representative sample of clusters, including those apparently discrepant with numerical simulations; (2) search for azimuthal variations at these scales which may be indicative of the ongoing cluster accretion process; (3) construct the largest sample to date of clusters with accurate X-ray mass determination out to r200; and (4) provide a fiducial data set for detailed comparison with high resolution numerical simulations. These targets capitalize on our large sample of clusters surveyed with XMM and will provide a large enough data set to truly sample the properties of clusters at large radii. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | A | ERIC MILLER | USA | 5 | AO5 | THE OUTER LIMITS OF RICH CLUSTERS: SUZAKU OBSERVATIONS TO R200 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/805063010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '805063010'
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