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 NGC 4125 182.0568 65.1777 181.434624 65.455888 140.391429 57.000336 130.16762444 51.33919783 175.9017 55103.512037037 2009-09-29 12:17:20 55105.4578009259 2009-10-01 10:59:14 804047010 104.0801 100 104.0801 104.0881 0 104.0961 2 2 0 2 1 0 0 93.7257 93.7257 168.0857 0 PROCESSED 57548.726712963 2016-06-09 17:26:28 55491 2010-10-22 00:00:00 55125.5744212963 2009-10-21 13:47:10 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 041502 Recent observations of relaxed galaxy groups have revealed ubiquitous abundance gradients, indicating large-scale mixing of the gas, possibly driven by AGN feedback. Exploiting the low background and good sensitivity of Suzaku, we have found similar gradients in two lower mass, galaxy-scale systems, which has important implications for models of feedback and chemical enrichment. We propose to observe two more isolated elliptical galaxies, thus starting to building a sample for determining the frequency and properties of such abundance gradients in early-type galaxies. EXTRAGALACTIC DIFFUSE SOURCES 8 B PHILIP HUMPHREY USA 4 AO4 ABUNDANCE GRADIENTS IN EARLY-TYPE GALAXIES XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/804047010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '804047010'

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