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 | ANTLIA NW4 | 156.477 | -34.4731 | 155.913183 | -34.218342 | 174.203454 | -40.552676 | 271.69853818 | 19.42589093 | 299.2985 | 57168.4177546296 | 2015-05-26 10:01:34 | 57169.4605902778 | 2015-05-27 11:03:15 | 810066010 | 6.3596 | 40 | 6.3596 | 6.8635 | 0 | 6.8635 | 3 | 2 | 0 | 2 | 1 | 0 | 0 | 6.7341 | 6.7341 | 78.0621 | 0 | PROCESSED | 57618.7963657407 | 2016-08-18 19:06:46 | 57626 | 2016-08-26 00:00:00 | 57178.2408101852 | 2015-06-05 05:46:46 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 101522 | We have measured hot gas properties of the nearest non-cool core cluster, Antlia, in the eastern direction out to R200. Our initial results suggest that its density profile is more consistent with some massive clusters, but significantly steeper than its cool core counterpart with a similar temperature (mass), Virgo. We propose to extend our program to observe two other directions to test azimuthal variation, which is likely to be significant. Physical properties such as density and temperature will be studied around the virial radius. These data can place important constraints on theoretical models of clusters and their environments. We will test models for clumping, electron-ion equipartition, and non-equilibrium ionization. The low Suzaku background allows this measurement. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | C | KA-WAH WONG | USA | 10 | AO10 | MAPPING THE NEAREST NON-COOL CORE CLUSTER OUT TO R200 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/810066010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '810066010'
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