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
1 A3112 49.4785 -44.2477 49.044044 -44.429449 25.501128 -58.962889 252.95565297 -56.08416767 11.0983 54609.240162037 2008-05-23 05:45:50 54611.0557638889 2008-05-25 01:20:18 803054010 67.4982 60 67.4982 67.4982 0 67.4982 2 2 0 2 1 0 0 59.0658 59.0658 156.8578 0 PROCESSED 57542.6456365741 2016-06-03 15:29:43 54988 2009-06-06 00:00:00 54620.3684490741 2008-06-03 08:50:34 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 031434 We propose to perform spatially resolved spectroscopy on the X-ray bright relaxed galaxy cluster Abell 3112, in order to characterize its soft/hard X-ray excess component. Abell 3112 is one of two clusters with very strong soft excess emission (the other being Abell S1101, observed in AO1). The indications provided by this observation will be crucial in order to assess, beyond doubt, the reality of the soft excess emission, previously observed by all soft X-ray missions since EUVE. The proposed observation will constrain the nature of the excess emitter, and address outstanding questions in observational cosmology: the {it missing baryon} problem, the density of matter in the universe and the non-thermal energy in galaxy clusters. EXTRAGALACTIC DIFFUSE SOURCES 8 B MASSIMILIANO BONAMENTE USA 3 AO3 SOFT EXCESS, HARD EXCESS AND THERMAL EMISSION IN ABELL 3112 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/803054010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '803054010'

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