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 NGC720 28.2529 -13.7362 27.644452 -13.982164 20.9363 -23.62893 173.01572713 -70.35499124 242.5294 53734.3673611111 2005-12-30 08:49:00 53739.5627546296 2006-01-04 13:30:22 800009010 177.1929 100 177.1929 177.1929 177.1929 177.1929 2 2 2 2 1 0 0 9.6621 9.6621 47.5408 0 PROCESSED 57532.602962963 2016-05-24 14:28:16 54247 2007-05-27 00:00:00 54039.6651736111 2006-10-31 15:57:51 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001031 We propose to observe an isolated elliptical galaxy NGC720 with Suzaku. Isolated elliptical galaxies are important to probe the ISM metal abundance, since their hot gas is not affected by the amibient bright intracluster medium which often exists around X-ray bright elliptical galaxies. Suzaku is expected to measure the Oxygen abundance in the ISM bettern than XMM-Newton and constrain the origin of metals in the ISM and also ICM. Dark matter content around elliptical galaxies can also be constrained better than XMM-Newton. Such a measurement is difficult for X-ray bright galaxies due to the superposition of the cluster potential. EXTRAGALACTIC DIFFUSE SOURCES 8 A YASUSHI FUKAZAWA JAP 0 SWG OXYGEN ABUNDANCE AND DARK MATTER CONTENT AROUDN AN ISOLATED ELLIPTICAL GALAXY NGC720 XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/800009010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '800009010'

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