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 1332 | 51.5732 | -21.333 | 51.017829 | -21.507123 | 42.191625 | -38.615675 | 212.17958034 | -54.36451308 | 243.6482 | 55581.2509027778 | 2011-01-20 06:01:18 | 55584.0883333333 | 2011-01-23 02:07:12 | 805095010 | 101.423 | 100 | 101.423 | 101.423 | 0 | 101.423 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 89.9683 | 89.9683 | 245.1259 | 2 | PROCESSED | 57600.7603935185 | 2016-07-31 18:14:58 | 55965 | 2012-02-08 00:00:00 | 55599.216724537 | 2011-02-07 05:12:05 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 054502 | Recent observations of relaxed galaxy groups have revealed ubiquitous abundance gradients. The broad peaks of Fe abundance indicate (turbulent) diffusion of metals possibly driven by AGN feedback. Exploiting the low background and good sensitivity of Suzaku XIS, we have found similar gradients in three lower mass (virial mass 5-10E12 Msun) elliptical galaxies, which has important implications for models of feedback and chemical enrichment. We propose to observe another two carefully chosen galaxies, thus starting to build a sample for determining the frequency and properties of such abundance gradients in early-type galaxies. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | C | PHILIP HUMPHREY | RYO NAGINO | USJ | 5 | AO5 | ABUNDANCE GRADIENTS IN EARLY-TYPE GALAXIES | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/805095010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '805095010'
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