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 E2 | 158.2496 | -35.3292 | 157.682674 | -35.071089 | 176.423673 | -40.599314 | 273.48585529 | 19.50669913 | 277.9997 | 56092.2642361111 | 2012-06-14 06:20:30 | 56093.0181944444 | 2012-06-15 00:26:12 | 807067010 | 24.1741 | 23 | 24.1821 | 24.1741 | 0 | 24.1901 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 22.8534 | 22.8534 | 65.1359 | 3 | PROCESSED | 57605.6727546296 | 2016-08-05 16:08:46 | 56476 | 2013-07-03 00:00:00 | 56110.5259027778 | 2012-07-02 12:37:18 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 071521 | We propose to carry out mosaic observations (204 ks total) of the Antlia cluster, the third closest galaxy cluster highly ignored in X-ray, out to R200. It is the nearest non-cool core cluster with a similar low temperature as the cool core Virgo Cluster, allowing us to make a direct comparison to the cool core counterpart in our neighborhood. 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 | A | KA-WAH WONG | USA | 7 | AO7 | MAPPING THE NEAREST NON-COOL CORE CLUSTER OUT TO R200 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/807067010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '807067010'
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