DARTS/Astro Query System - SQL Search -

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total 1

No.
observation_id
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
exposure
awarded_exposure
xtend_exposure
xtend_number_modes
xtend_dataclass_file1
xtend_dataclass_file2
xtend_window1_exposure
xtend_window2_exposure
xtend_window1_burst_exposure
xtend_window2_burst_exposure
xtend_code
gen_code
processing_status
processing_date
public_date
distribution_date
processing_version
caldb_version
processing_software
proposal_id
proposal_abstract
proposal_category
proposal_category_code
proposal_priority
pi_name
co_pi_name
proposal_affiliated_country
proposal_cycle
proposal_type
proposal_title
observation_status
data_access_url
ql_access_url
ql_image_url
corner1_ra
corner1_dec
corner2_ra
corner2_dec
corner3_ra
corner3_dec
corner4_ra
corner4_dec
corner1_ra_b1950
corner1_dec_b1950
corner2_ra_b1950
corner2_dec_b1950
corner3_ra_b1950
corner3_dec_b1950
corner4_ra_b1950
corner4_dec_b1950
corner1_ecliptic_lon
corner1_ecliptic_lat
corner2_ecliptic_lon
corner2_ecliptic_lat
corner3_ecliptic_lon
corner3_ecliptic_lat
corner4_ecliptic_lon
corner4_ecliptic_lat
corner1_galactic_lon
corner1_galactic_lat
corner2_galactic_lon
corner2_galactic_lat
corner3_galactic_lon
corner3_galactic_lat
corner4_galactic_lon
corner4_galactic_lat
xtend_data_mode1
xtend_data_mode2
1 201043010 A1060_CENTER 159.19217 -27.53045 158.60351 -27.27069 172.77024 -33.32464 269.61492 26.49194 279.99833 60803.29727 2025-05-08 07:08:04 60805.66880 2025-05-10 16:03:04 122.317 100.000 115.324 1 300000A0 115.324 0.000 0.000 0.000 11110 11310 PROCESSED 2025-07-13 19:01:08 2026-05-29 00:00:00 2025-05-24 14:14:39 03.02.014.010 gen20241115_xtd20241115_rsl20241115 Hea_12Mar2025_V6.35_XRISM_28Feb2025_V002 000011226 We propose XRISM observations of Abell 1060, the brightest and one of the nearest non-cool core/non-merging cluster, suggested by its nearly circular symmetric ICM. There is no strong AGN-jet-ICM interaction and the ICM is likely be "calm". Measuring its bulk flow and turbulence is very important for XRISM, because all cluster PV targets are either cool-core clusters or merging clusters. This observation will provide a baselines for ICM science. By a 100 ks observation at the center, and a 200 ks observation at ~4' offset to the east, we aim to observe a ~100 km/s level of bulk motion and turbulence to the accuracy of < 30 km/s (90% CL). Origin of the newly found soft-radio diffuse source "Flying Fox", and ISM stripping of the spiral galaxy NGC 3312 are also in the scope. EXTRAGALACTIC DIFFUSE EMISSION AND SURVEYS 2 C KAZUHIRO NAKAZAWA JAP 1 NOR HOW ``CALM'' IS THE ICM OF THE NEAREST NON COOL-CORE CLUSTER ABELL 1060? archived https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201043010/ Quick Look 158.69985 -27.83968 159.41154 -27.95093 159.53509 -27.31898 158.82646 -27.20829 158.11306 -27.58079 158.8233 -27.69078 158.94517 -27.05862 158.23794 -26.94917 172.46718 -33.7957 173.2034 -33.61436 172.98359 -32.99988 172.2512 -33.18023 269.40102 25.99307 270.05373 26.24713 269.76941 26.8359 269.1132 26.58015 WINDOW1

Used SQL

SELECT * FROM xrism_xtend_data WHERE observation_id = '201043010'

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