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 | 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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